|
m1 |
m2 |
ρ |
θ |
Year |
|
Coordinates (J2000) |
|
★★
|
STF2308 |
40/41 Dra |
AB |
5m7 |
6m0 |
18.7'' |
232° |
2019 |
Dra |
18h00m09.07s |
+80°00'13.70" |
|
|
|
|
AC |
5m7 |
8m3 |
225.3'' |
129° |
2017 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
8x44 |
2020-06-27: The pair AB split, but very tight with components of equal brightness. In acute angle far apart the component C was also visible. |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
AB: Clearly split, brighter component seems bluish. One of the finest doubles for 15x, hence my two-star rating. In 10x42 a difficult split at the limit. |
|
René Merting
Drachhausen (Germany) |
16x70 |
ein schön eng stehendes Pärchen, die Himmelsrichtungen erschließen sich mir hier leider nicht, aber die Komponenten sind beide ähnlich hell und weiß - schöner Anblick im Fernglas |
|
Christopher Hay
Seeheim (Germany) |
50mm (8x) |
AB: An elongated figure-8 very close to splitting |
|
Christopher Hay
Seeheim (Germany) |
80mm (30x) |
AB: Very clearly split, dominates the 2.5° FOV, with interesting sprinkling of fainter stars throughout the field. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (28x) |
Very nice, slightly uneven pair. Components appeared yellowish-white. Beautiful surroundings. On the sketch the components A, B and C are visible. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (100x) |
AB: =40/41 Dra. Auffallend |
|
Christopher Hay
Seeheim (Germany) |
140mm (75x) |
AB: Wide apart, the pair absolutely dominates the field of view, with attractive sprinkling of fainter stars to the west. Very delicate colour contrast that was hard to grasp in 3-inch scope now becomes clear, component B (40 Dra) is bluish, component A (41 Dra) yellowish. |
|
|
|
|
STF2271 |
|
AB |
8m2 |
9m2 |
3.5'' |
267° |
2019 |
Dra |
18h00m18.74s |
+52°51'15.40" |
|
|
|
|
AC |
8m2 |
13m0 |
160.8'' |
17° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 64x ist eine kleine 8 erkennbar - bei 107x sind beide Komponenten sicher trennbar - B ist eine dreiviertel Größenklasse schwächer |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Dull white A and pale yellow B, ~1.5 delta mag, wide ~4" |
|
|
|
|
A1375 |
|
|
9m6 |
10m6 |
1.8'' |
92° |
2018 |
Her |
18h00m24.40s |
+21°11'36.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Fine equal pair, well separated, points with seeing. |
|
|
|
★
|
H6 2, 67 Oph |
|
AC |
4m0 |
8m1 |
54.7'' |
143° |
2019 |
Oph |
18h00m38.72s |
+02°55'53.70" |
René Merting
Drachhausen (Germany) |
10x35 |
zwischen beide Sterne passt maximal ein halbes Blatt Papier - C im Südosten kommt mir entgegen aller früheren Erfahrungen nicht so schwach vor wie sonst, ich würde hier nur auf maximal eine Größenklasse schätzen, eigenartig |
|
René Merting
Drachhausen (Germany) |
10x50 |
ein einfacher Doppelstern - Komponente C steht mit gutem Abstand südöstlich von A - Komponente A ist gleißend weiß, C wirkt dagegen richtiggehend grau-braun |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
AC: Stabilised binoculars, handheld. Components wide apart, almost too wide to appear as a double star. Secondary a fine speck of light beside the primary, which is >4mag brighter. According to Stelledoppie a true physical pair at a distance of 1230 light years. It is interesting to contemplate that at this distance in space the companion still looks so separate. “H“ in the catalogue name means that this double star is listed in the catalogue of W. Herschel. The 6 in the name means that it is a double star of the 6th Class [separation 1’ or larger] in Herschel’s system. |
|
René Merting
Drachhausen (Germany) |
16x70 |
auf den ersten Blick bin ich enttäuscht, weil ich nur einen hell strahlenden Stern erkennen kann - dann aber mit etwas Konzentration ist südöstlich von der Leuchtgranate ein ganz schwacher Begleiter zu erkennen - ein sehr ungleiches Paar mit geschätzt 4 Größenklassen Unterschied - Komponente C wirkt rotbraun und steht ordentlich getrennt von A |
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
der helle ist gelb-weiß |
|
Christopher Hay
Seeheim (Germany) |
25x80 |
Very far apart, almost so far as to appear to not belong together. However, in the 3° field of view 70 Ophiuchi, which is also a physical double, is seen to be also split. Thus a very attractive field overall.
67 Oph and 70 Oph are the left and right nostrils of the bull in the old constellation Taurus Poniatowski (Poniatowski’s Bull). 68 Oph (the tip of the bull’s nose) and 73 Oph (the bull’s right eye) are also double stars, but can’t be split at 25x. All four doubles – 67, 68, 70 and 73 Oph – are physical, a rare assemblage! |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x großer Abstand zwischen beiden Sternen - weil Komponente A so gleißend hell strahlt, fehlt der mindestens um 3 Größenklassen schwächeren Komponente C im SO die Farbe, eher gräulich |
|
|
|
|
LDS6413 |
|
|
7m1 |
13m1 |
88.1'' |
105° |
2015 |
Her |
18h00m38.89s |
+29°34'18.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
A star is a pretty orange star A. B is 13th mag 88" -- not likely seen though there are several very faint stars about. |
|
|
|
|
ES640 |
|
|
9m5 |
10m1 |
8.4'' |
77° |
2018 |
Dra |
18h00m42.85s |
+54°52'38.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
~1 delta mag, wide ~4" |
|
|
|
|
STF2263 |
|
|
8m7 |
9m9 |
7.7'' |
158° |
2018 |
Her |
18h00m55.43s |
+26°32'57.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Wide ~1 delta mag, white-blue A and dull orange B |
|
|
|
|
STF3129 |
|
|
7m6 |
10m6 |
30.8'' |
168° |
2015 |
Her |
18h01m07.16s |
+45°21'03.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
White and wide separation, 2 delta mag fainter orange B. |
|
|
|
|
STF2264, 95 Her |
|
|
4m8 |
5m2 |
6.4'' |
257° |
2019 |
Her |
18h01m30.41s |
+21°35'44.80" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x mein erster Eindruck ist, dass zwei annähernd gleichhelle sehr eng stehende Sterne mich wie zwei Augen anschauen, das unmittelbare Sternumfeld passt schön und verleiht dem Doppel eine hervorgehobene Stellung - Komponente B im Westen ist nur minimal schwächer als A - in guten Momenten ist die Trennung sehr eindeutig erkennbar |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x zwei helle, knapp getrennte Sterne - die schwächere westliche Komponente zeigt ein schönes, helles Gelb und wirkt dadurch leicht schwächer - zurück auf 32x ist eine 8 mit deutlicher Einschnürung erkennbar - der Farbunterschied ist ebenfalls deutlich |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
|
|
Karsten Kopp
Köln (Germany) |
140mm (94x) |
Konnte erst mit 94-facher Vergrößerung gut getrennt wahrgenommen werden. |
|
Sarah Gebauer
Germany |
150mm (54x) |
zwei enge, hübsche Glanzpünktchen, die ich zuvor ziemlich lange in dem hellen Sterntrapez gesucht habe |
|
Robert Zebahl
Leipzig (Germany) |
152mm (49x) |
2020-06-23: At 49x eye catching double star, relatively tight with rather small difference in brightness. Beautiful color impression, which was even better visible at 69x: yellowish and yellowish-orange. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
95 Her. Orange and blue, wide, bright. |
|
Karsten Kopp
Köln (Germany) |
600mm (135x) |
Sehr einfaches und auffälliges Objekt. Kein Helligkeitsunterschied erkennbar. |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
close DS |
|
|
|
|
STF2267 |
|
|
8m4 |
8m8 |
0.4'' |
281° |
2018 |
Her |
18h01m41.17s |
+40°10'41.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
|
|
COU811 |
|
|
11m2 |
11m7 |
2.2'' |
153° |
2015 |
Her |
18h01m58.10s |
+30°47'16.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Faint but more cleanly split than at 20" due to seeing. 8" limited to 11th mag in poor transparency. |
|
|
|
★
|
BU1127 |
|
AB |
7m3 |
9m2 |
0.7'' |
39° |
2018 |
Her |
18h02m30.89s |
+44°14'02.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very tough but a small point of a star resolved at the rim of the diffraction ring at both 553x & 885x, using kind of a partial averted vision. |
|
|
|
|
STF2278 |
|
AB |
7m8 |
8m1 |
36.3'' |
29° |
2019 |
Dra |
18h02m52.88s |
+56°25'40.30" |
|
|
|
|
AC |
7m8 |
8m5 |
33.6'' |
39° |
2017 |
|
|
|
|
|
|
|
AD |
7m8 |
10m2 |
198.2'' |
189° |
2015 |
|
|
|
|
|
|
|
BC |
8m1 |
8m5 |
6.0'' |
147° |
2018 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
A und BC sind getrennt zu erkennen, sehr dicht zusammen stehend, unauffällig - B und C kann ich nicht trennen |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Pretty white-blue stars, in a 2+1 set. Not physical |
|
|
|
|
STF2262, tau Oph |
|
AB |
5m3 |
5m9 |
1.5'' |
290° |
2019 |
Oph |
18h03m04.91s |
-08°10'48.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (240x) |
getrennt |
|
|
|
|
STF2277 |
|
AB |
6m2 |
8m9 |
26.8'' |
129° |
2018 |
Her |
18h03m08.87s |
+48°27'51.30" |
|
|
|
|
AC |
6m2 |
10m2 |
99.7'' |
297° |
2015 |
|
|
|
|
|
|
|
BC |
8m9 |
10m2 |
126.4'' |
300° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ein weit getrenntes Pärchen mit schönem Farbkontrast - Komponente A weiß-gelb, B grau-orange - auch bei 20x ist noch ordentlich Luft zwischen beiden Sternen |
|
|
|
|
STTA164 |
|
|
8m3 |
9m3 |
50.8'' |
0° |
2015 |
Oph |
18h03m12.41s |
+07°54'34.60" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x sehr weit getrennt - schöner Farbkontrast, Komponente A strahlt weiß und B kupferrot und nicht viel schwächer als A, Helligkeitsunterschied nach meinem Empfinden eine halbe Größenklasse |
|
|
|
|
ES470 |
|
|
9m4 |
10m7 |
8.3'' |
208° |
2018 |
Her |
18h03m15.08s |
+27°50'40.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Can hold B direct after foveal coaxing, it's very faint ~1 delta and wide |
|
|
|
|
SLE88 |
|
|
12m2 |
13m3 |
3.8'' |
339° |
2015 |
Her |
18h03m51.56s |
+25°58'17.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
A star steady direct vision, B flashes into view with averted and slowly fades to invisibility. Close, about 4" and one and one half delta mag. [not physical, disappointingly] |
|
|
|
|
HO426 |
|
|
7m0 |
12m0 |
11.7'' |
229° |
2015 |
Her |
18h03m54.11s |
+26°39'05.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Pretty yellow star, about 7th magnitude, with a much fainter 5 delta mag, very widely separated companion [not physical] |
|
|
|
|
S698 |
|
AB |
7m2 |
8m5 |
29.7'' |
316° |
2015 |
Sgr |
18h04m12.64s |
-22°30'03.20" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x die beiden hellsten Vertreter im Sternhaufen M 21, weit getrennt - Komponente B west-nordwestlich ist eine knapp Größenklasse schwächer und grau - der Doppelstern fällt nicht besonders auf in der Sternhaufenumgebung, aber es ist ok |
|
|
|
|
TDT664 |
|
|
11m2 |
11m8 |
0.6'' |
232° |
1991 |
Her |
18h04m29.33s |
+22°54'44.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Marginal, I only get an elongation. Very tight |
|
|
|
|
STF2279 |
|
|
9m9 |
10m3 |
13.3'' |
180° |
2015 |
Dra |
18h04m33.72s |
+50°52'48.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Near equal, wide, white. Physical |
|
|
|
|
ES471 |
|
AC |
7m2 |
10m2 |
24.3'' |
44° |
2015 |
Her |
18h04m39.08s |
+27°06'54.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Much fainter B star, 3 delta mag, wide separation. Direct vision, but faint. |
|
|
|
|
STT534 |
|
|
8m5 |
10m5 |
2.3'' |
269° |
2015 |
Her |
18h04m59.56s |
+21°26'31.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
One star definitely brighter by at least one mag than the other. Well separated |
|
|
|
|
70 Oph, P Oph, STF2272 |
|
AB |
4m2 |
6m2 |
6.6'' |
122° |
2019 |
Oph |
18h05m27.37s |
+02°29'59.30" |
|
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
nicht einfach; der helle ist gelb |
|
Christopher Hay
Seeheim (Germany) |
25x80 |
Clean split, component A appears yellowish.
70 Oph is the left nostril of the bull in the old constellation Taurus Poniatowski (Poniatowski’s Bull). On the connections to 67, 68 and 73 Oph see the entry on 67 Oph. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x wirkt der Stern nicht rund, sondern ein wenig nach SO verschmiert - bei 64x dann eindeutig ein knapp getrenntes schön anzusehendes Pärchen - Komponente A hell-gelb, B orange-gelb |
|
Jörg S. Schlimmer
Germany |
127mm (136x) |
easy to split |
|
Sarah Gebauer
Germany |
150mm (85x) |
ein ganz leicht goldener Farbeindruck des Sternpaares, die Sterne stehen recht dicht beisammen und sind dennoch schön getrennt |
|
Robert Zebahl
Leipzig (Germany) |
200mm (80x) |
Conditions in the target region: SQM-L 20.1
Well split at 80x. Brighter component appeared white, fainter one slightly orange. |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
difficult DS |
|
|
|
|
STF2276 |
|
AB |
7m1 |
7m4 |
7.1'' |
257° |
2017 |
Oph |
18h05m43.30s |
+12°00'13.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Beautiful near equal well separated, yellowish, in nice field of stars. |
|
|
|
★
|
STT341 |
|
AB |
7m4 |
8m8 |
0.1'' |
86° |
2019 |
Her |
18h05m49.72s |
+21°26'45.60" |
|
|
|
|
AB-C |
7m2 |
10m6 |
28.2'' |
171° |
2015 |
|
|
|
|
|
|
|
AB-D |
7m2 |
10m5 |
39.5'' |
99° |
2009 |
|
|
|
|
|
|
|
AB-E |
7m2 |
10m2 |
66.5'' |
38° |
2018 |
|
|
|
|
|
|
|
AB-F |
7m2 |
11m5 |
111.6'' |
357° |
2009 |
|
|
|
|
|
|
|
AB-G |
7m2 |
7m6 |
132.5'' |
239° |
2018 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB-C: bei 32x ist Komponente C weit getrennt südlich von AB als Hauch von einem Stern erkennbar
AB-D: bei 32x ist Komponente D im Osten von AB ist ähnlich schwach erkennbar wie C im Süden - D ist etwas weiter weg als C
AB-E: bei 32x ist Komponente E im NO von AB ähnlich schwach erkennbar wie C im Süden und D im Osten - Entfernung zu A doppelt so weit wie AB-C
AB-F: bei 64x ist F im Norden von AB in vierfacher Entfernung AB-C erkennbar - im Grunde spiralen die vier schwachen Komponenten von Süden kommend von Osten nach Norden aus |
|
|
|
|
STF2282 |
|
AB |
7m9 |
9m4 |
2.7'' |
83° |
2017 |
Her |
18h06m30.47s |
+40°21'39.60" |
|
|
|
|
AC |
7m9 |
9m4 |
2.7'' |
80° |
2008 |
|
|
|
|
|
|
|
BC |
9m4 |
9m4 |
0.2'' |
48° |
2008 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 64x ploppen zwei kleine Perlchen auf, die dicht beieinander stehen - Komponente B im Osten ist nur unwesentlich schwächer (eigenartig, laut Stelle Doppie sollen beide Sterne 1.5 Größenklassen Helligkeitsunterschied haben) - bei 107x ist die Trennung dann eindeutig, aber immer noch sehr knapp |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Faint yellow white, 3", half delta mag. |
|
|
|
★
|
AC15, 99 Her |
|
AB |
5m1 |
9m0 |
1.4'' |
331° |
2018 |
Her |
18h07m01.61s |
+30°33'42.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
99 Her.Very nice. B star resolves just outside first diffraction ring when that ring has faded with good seeing, a very fine faint point. large delta mag. There are many other pairings in this system, including 0.2" for the A star] |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
99 Her: ! Bright yellow star, suspected double at 277x but needed 553x to resolve a 9th mag orange B when seeing stilled, resolved as a point just outside where the diffraction ring was. CDSA notes: "Local, solar type binary, faint field. AB system 1.8 solar mass, p=56 y orbit r = 17 AU, e = 0.77, apastron 2025" |
|
|
|
|
STT524 |
|
|
7m9 |
8m9 |
0.5'' |
207° |
2018 |
Her |
18h07m29.52s |
+19°39'59.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Suspected hairline with 333x, nice clean split at 533x, white stars, significant magnitude difference, ~0.5". 686 year period |
|
|
|
★★
|
STF2280, 100 Her |
|
AB |
5m8 |
5m8 |
14.3'' |
183° |
2019 |
Her |
18h07m49.56s |
+26°06'04.40" |
René Merting
Drachhausen (Germany) |
10x35 |
ein 8, eine Einschnürung ist ab und an erkennbar - Trennung nicht möglich |
|
René Merting
Drachhausen (Germany) |
10x50 |
zwei extrem dicht stehende helle Sterne - noch nicht getrennt, aber schön als 8 erkennbar |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-05: Very nice, rather isolated double star. Striking. Similar bright component, both white. |
|
René Merting
Drachhausen (Germany) |
18x70 |
perfekt für 18-fache Vergrößerung - zwei gleich helle, dicht zusammen stehende Sterne - reinweiß und sehr auffällig, weil keine ähnlich hellen Sterne im Umfeld zu sehen sind |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein schönes, enges Pärchen zweier gleichheller Sterne - beide gleich hell und reinweiß - zurück auf 20x zeigen sich beide Protagonisten weiterhin ganz knapp getrennt - Komponente B im Süden wirkt leicht gelblich und schwächer |
|
Uwe Pilz
Leipzig (Germany) |
105mm (26x) |
Weiß-orangeweiß |
|
Robert Zebahl
Leipzig (Germany) |
120mm (40x) |
Conditions in the target region: SQM-L 20.5
Very nice, evident double star with equally bright components. |
|
Karsten Kopp
Köln (Germany) |
140mm (94x) |
Doppelstern ist einfach zu trennen. Das besondere ist hier, dass die beiden Sterne recht alleine zu stehen scheinen. Beide erscheinen weiß. |
|
Sarah Gebauer
Germany |
150mm (54x) |
zwei hübsche Glanzpünktchen, die mich an ein Knöpflein mit zwei Löchern erinnern, der "typische" DS für mich: nicht zu eng, nicht zu weit, gleich hell, sehr nett |
|
Robert Zebahl
Leipzig (Germany) |
152mm (22x) |
Beautiful view. Easy to separate with components of the same brightness. It is noticeable that there are no brighter stars in the immediate vicinity, so that the double star stands out very well. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
100 Her. Bright equal wide yellow-white stars. [not physical] |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
easy DS |
|
|
|
|
COU812 |
|
|
10m8 |
10m8 |
0.7'' |
265° |
2016 |
Her |
18h09m09.93s |
+31°29'10.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Elongation, marginal notch, but a bit too hazy to make a good observation |
|
|
|
|
HU926 |
|
|
9m9 |
9m9 |
3.9'' |
265° |
2016 |
Dra |
18h09m31.81s |
+64°14'02.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Nice equal mag, wide ~4", white. Not physical |
|
|
|
|
STF2281, 73 Oph |
|
AB |
6m0 |
7m5 |
0.8'' |
283° |
2019 |
Oph |
18h09m33.86s |
+03°59'35.80" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
als 8 zu sehen, schwierig |
|
|
|
★★
|
HU674 |
|
|
7m7 |
8m6 |
0.7'' |
214° |
2018 |
Her |
18h09m40.64s |
+50°24'07.40" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt, ähnlich hell |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Split with seeing at 333x, near equal white. |
|
|
|
|
STF2289 |
|
|
6m7 |
7m2 |
1.2'' |
218° |
2019 |
Her |
18h10m08.69s |
+16°28'35.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Just split in 20" at 205x, but flaring. 333x had messy diffraction. 8" mask at 333x gave clean disks, split, ~0.7". Dull yellow and yellow-red colors. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
Hauptstern gelb, Begleiter scheint bläulich |
|
|
|
|
HO81 |
|
|
8m2 |
11m1 |
3.3'' |
215° |
2019 |
Her |
18h10m26.23s |
+32°21'10.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
With the 8" mask, the B star appears with averted vision as a bluish smear at the right PA and ~3" separation. In the 20" the A star is more diffracted and a brighter yellow, and B is a direct obvious blue small glow resolving to point with seeing. |
|
|
|
|
S700 & ABH94 |
S700 |
AB |
8m3 |
9m7 |
18.8'' |
291° |
2018 |
Ser |
18h10m33.56s |
-16°44'57.40" |
|
|
|
S700 |
AC |
8m3 |
8m6 |
28.6'' |
353° |
2018 |
|
|
|
|
|
|
ABH94 |
AD |
8m3 |
14m2 |
47.7'' |
348° |
2015 |
|
|
|
|
|
|
ABH94 |
AE |
8m3 |
13m5 |
58.0'' |
65° |
2015 |
|
|
|
|
|
|
ABH94 |
AF |
8m3 |
13m1 |
99.2'' |
49° |
2015 |
|
|
|
|
|
|
S700 |
AG |
8m3 |
11m3 |
35.6'' |
297° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AC: Komponente C ist nördlich von A eng stehend, aber gut getrennt zu sehen - beide Komponenten sind fast gleich hell - irgend etwas im Westen von A stört die Harmonie (Komponente B?), aber ich kann es nicht mit Gewissheit sagen |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: wenn man bei 32x genau hinschaut, ploppt westlich von A in halbem Abstand AC ein schwacher Lichtpunkt aus, das ist Komponente B … ohne Farbe, weil sehr schwach - auch 64x verbessert die Sichtbarkeit von B nicht wirklich
AC: bei 32x fallen die fast gleich hellen Komponenten A und C (nördlich von A) des Dreifachsystems auf |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
AB: Komponente B ist sehr schwach und nur halb so weit entfernt wie der Abstand AC
AC: A und C nehmen sich helligkeitstechnisch nicht viel - zusammen mit B entsteht ein flaches Dreieck |
|
|
|
|
ES185 |
|
|
9m9 |
11m0 |
12.3'' |
284° |
2015 |
Her |
18h11m04.08s |
+32°58'22.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Obvious pair, wide, bluish stars, half delta mag [not physical] |
|
|
|
|
HU317 |
|
|
9m6 |
9m7 |
1.5'' |
205° |
2015 |
Her |
18h11m20.44s |
+17°13'17.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Light orange stars, well separated, near equal. |
|
|
|
|
STF2292 |
|
|
8m3 |
8m6 |
0.8'' |
276° |
2016 |
Her |
18h12m06.74s |
+27°38'35.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Very fine split, white stars, slight mag difference ~0.5 delta. Very fine at this magnification |
|
|
|
|
BU131 & FOX221 |
BU131 |
AB |
7m5 |
9m3 |
3.2'' |
277° |
2005 |
Ser |
18h13m35.49s |
-15°35'54.10" |
|
|
|
BU131 |
AC |
7m5 |
11m8 |
9.2'' |
300° |
2015 |
|
|
|
|
|
|
FOX221 |
AD |
7m5 |
12m5 |
40.8'' |
34° |
2015 |
|
|
|
|
|
|
BU131 |
BC |
9m3 |
11m8 |
6.2'' |
310° |
2005 |
|
|
|
René Merting
Drachhausen (Germany) |
320mm (144x) |
BU131 (AB): bei 144x ist Komponente B knapp getrennt westlich von A zu erkennen und bestimmt 1,5 bis 2 Größenklassen schwächer - B wirkt grau gegen den weißen A |
|
|
|
★★
|
mu Sgr, Polis |
H5 7 |
AB |
3m9 |
10m5 |
16.9'' |
258° |
2013 |
Sgr |
18h13m45.81s |
-21°03'31.80" |
|
|
|
BU292 |
AC |
3m9 |
12m8 |
25.5'' |
119° |
2008 |
|
|
|
|
|
|
HJ2822 |
AD |
3m9 |
10m0 |
48.2'' |
312° |
2013 |
|
|
|
|
|
|
HJ2822 |
AE |
3m9 |
9m2 |
50.2'' |
114° |
2013 |
|
|
|
|
|
|
SLV7 |
BD |
10m5 |
10m0 |
40.9'' |
331° |
1998 |
|
|
|
|
|
|
SLV7 |
BE |
10m5 |
9m2 |
64.6'' |
106° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AD: bei 32x Komponente A gleißend hell im Zentrum und Komponente D gut abgesetzt sehr schwach im NW
AE: bei 32x auf der entgegengesetzten Seite im SW zeigt sich Komponente E in gleichem Abstand und mit gleicher Lichtschwäche - die beiden schwachen Komponenten D und E haben A voll in der Flügelzange - das Ganze funktioniert auch bei 20x, aber das sind die beiden schwachen Komponenten nahe der Sichtbarkeitsgrenze |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
AD: bei 45x ist D wunderbar als schwacher Begleiter in ordentlichem Abstand nordwestlich von A erkennbar
AE: E zeigt sich auf der entgegengesetzten Seite in gleichem Abstand - mit AD zusammen ein schickes Trio |
|
|
|
★
|
BU1274 |
|
BC |
9m8 |
10m6 |
1.0'' |
144° |
2017 |
Dra |
18h14m31.41s |
+56°34'26.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Super challenging. A-BC is bright white A and BC is blue widely separated. Near to BC is BD, which is near equal to BC and ~6". BC is faint and split with seeing, hairline, significant mag difference |
|
|
|
|
GII110 |
|
CD |
9m4 |
11m9 |
0.8'' |
302° |
2016 |
Her |
18h14m37.03s |
+23°35'01.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
With seeing, very significant delta mag ~2 delta mag, white stars, very tight but split. Suspected @ 333x. [Discoverer is amateur Rene Gili, who observes with the large refractors at the Nice Observatory, this pair was discovered in 2016 via CCD-- the discovery measure is the only one in WDS so far] |
|
|
|
|
POU3366 |
|
|
11m0 |
11m0 |
13.7'' |
238° |
2015 |
Her |
18h14m49.24s |
+23°13'54.60" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Easy near equal wide pair |
|
|
|
|
STT346 |
|
|
8m3 |
9m0 |
5.2'' |
329° |
2019 |
Her |
18h15m25.05s |
+19°46'13.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Nice pale yellow-white stars, >1 delta mag, >4" separation |
|
|
|
★
|
ES1651, TZ Lyr |
|
|
11m2 |
12m4 |
2.5'' |
5° |
2015 |
Lyr |
18h15m49.67s |
+41°06'37.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Challenging! Faint elongated star with direct vision. With averted vision it flashes a split, half delta mag, just split. |
|
|
|
|
STF2305 |
|
AB |
9m2 |
10m8 |
5.1'' |
334° |
2018 |
Dra |
18h16m13.17s |
+51°19'46.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A and >1 delta mag ruddy B, wide |
|
|
|
|
STTA167 |
|
|
8m0 |
9m1 |
53.0'' |
74° |
2016 |
Oph |
18h16m13.87s |
+04°34'02.90" |
René Merting
Drachhausen (Germany) |
10x50 |
ordentlich getrennt und mangels Konkurrenz im Umfeld leicht auffindbar - Komponente A ist schwach, B ist nochmal eine Größenklasse schwächer, aber noch problemlos erkennbar |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x leicht zu trennen - Komponente B im NW ich gut eine Magnitude schwächer, deutlich dumpfer und gräulicher, Komponente A dagegen strahlt weiß |
|
|
|
|
SHJ264 |
|
AB-C |
6m9 |
7m6 |
17.2'' |
51° |
2019 |
Sgr |
18h18m43.26s |
-18°37'10.80" |
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x ein schön getrennter Doppelstern mit leichtem Farbkontrast - B im Nordosten ist eine halbe bis dreiviertel Größenklasse schwächer |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x ein ordentlich getrenntes Pärchen, auffällig im Umfeld - Komponente AB im SW ist weiß-blau, Komponente C ist 0.75 mag schwächer und weiß-gelblich - 20x reichen ebenso, dann eng getrennt |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ein schön anzusehendes Sternpaar - gut getrennt und doch eng zusammen stehend - B im NO ist gut eine halbe Magnitude schwächer |
|
|
|
|
AG221 |
|
AB |
9m9 |
9m9 |
1.8'' |
12° |
2015 |
Her |
18h20m02.24s |
+21°20'00.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Fine near equal, split ~2" |
|
|
|
|
STF2309 |
|
|
9m3 |
9m9 |
3.4'' |
352° |
2018 |
Her |
18h20m06.84s |
+25°31'53.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Wide ~4", white stars, ~1 delta mag. Not physical |
|
|
|
|
STF2310 |
|
|
6m8 |
10m0 |
5.1'' |
235° |
2017 |
Her |
18h20m38.67s |
+22°47'50.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Bright white A and faint dull wide B, ~3 delta mag, wide ~6" |
|
|
|
|
STT353, phi Dra |
|
AB |
4m5 |
5m9 |
0.5'' |
266° |
2011 |
Dra |
18h20m45.44s |
+71°20'15.80" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
STF2312 |
|
|
9m3 |
9m9 |
1.7'' |
341° |
2015 |
Her |
18h21m09.08s |
+28°20'03.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very fine white stars, >1 delta mag, ~1.5" |
|
|
|
|
COU505 |
|
|
11m0 |
11m3 |
1.1'' |
318° |
2015 |
Her |
18h21m16.17s |
+24°09'06.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very faint pair, ~1 delta mag, split firmly with seeing, ~1" separation |
|
|
|
|
HO430 |
|
|
9m6 |
10m7 |
2.5'' |
194° |
2018 |
Her |
18h21m37.31s |
+20°30'11.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A and dull white B, ~2 delta, wide ~2". Nice looking pair [not physical] |
|
|
|
★★★
|
BU641 |
|
|
7m0 |
8m7 |
0.8'' |
341° |
2015 |
Her |
18h21m48.44s |
+21°30'27.90" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
sehr schwierig |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Extraordinary! Moderately bright A and very much fainter B, 4-5 delta mag, <1" separation. Seeing needs to still. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
V989 Her. Seen as a snowman dot to bright white A @ 333x, split with 533x, inside first diffraction ring. Need A's disk to be perfectly tight for B to resolve with seeing. Very nice. 1" at discovery 1878 with Dearborn 18.5-inch |
|
|
|
★
|
HU581 |
|
|
8m8 |
9m4 |
0.4'' |
122° |
2016 |
Her |
18h22m54.84s |
+14°58'11.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Snowman at 533x & 667x, clean split at 1067x & apodising mask, one delta mag. Amazing. Coalesces into two points, can easily tell orientation & magnitude difference for sketch. At apastron, it is on a nearly edge on orientation, will close rapidly within the next ten years to be too close for me to detect. |
|
|
|
|
STF2314 |
|
|
9m0 |
10m3 |
2.7'' |
331° |
2018 |
Her |
18h23m25.75s |
+23°27'19.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Fine pair, wide ~2.5", ~1 delta mag |
|
|
|
|
ES187 |
|
AB |
9m3 |
9m4 |
2.5'' |
207° |
2018 |
Dra |
18h23m45.03s |
+51°38'55.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Near equal, ~2", slightly ruddy stars. Nice pair |
|
|
|
★
|
STF2323, 39 Dra |
|
AC |
5m1 |
8m0 |
88.9'' |
20° |
2017 |
Dra |
18h23m54.65s |
+58°48'02.10" |
|
|
|
|
AB |
5m1 |
8m1 |
3.8'' |
348° |
2018 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
AC: Pretty wide, unequal pair. Die brighter A component appeared white. |
|
Robert Zebahl
Leipzig (Germany) |
55mm (71x) |
AB: Very nice. The B component seemed to be comparable faint as the C component. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: 39 Dra. Brilliant white A and slightly ruddy B, ~3 delta mag, ~4" sep. 3962.5 year period. |
|
|
|
★
|
STF2315 |
|
AB |
6m6 |
7m8 |
0.6'' |
117° |
2018 |
Her |
18h24m58.46s |
+27°23'41.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
als 8 zu sehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
! Hairline split @ 553x near equal mag. Suspected elongation at 277x. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Barely split with seeing, resolves to two disks, more than hairline but almost 2 delta mag, very tough, need perfect seeing. 2094 year period |
|
|
|
|
AG361 |
|
|
10m7 |
11m0 |
3.8'' |
13° |
2015 |
Her |
18h25m07.89s |
+26°54'09.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal white stars, wide ~4", in a busy field [not physical] |
|
|
|
|
BU134 |
|
|
8m0 |
9m7 |
1.0'' |
126° |
2015 |
Lyr |
18h25m17.50s |
+46°53'07.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
~2" separation, considerably fainter B, 2-3 delta mag, need the seeing to still |
|
|
|
|
STT351 & HU66 |
HU66 |
AB |
7m9 |
8m4 |
0.2'' |
197° |
2016 |
Dra |
18h25m18.20s |
+48°45'42.50" |
|
|
|
STT351 |
AC |
7m9 |
8m2 |
0.8'' |
26° |
2019 |
|
|
|
|
|
|
HU66 |
BC |
8m4 |
8m2 |
0.8'' |
26° |
2019 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (305x) |
STT351 (AC): Split, better with seeing, light orange stars, significant mag difference. Did not notice HU 66 AB, 7.9/8.4 0.1" or HU 66 BC, 8.40/8.25 0.9 -- need to go back to this one! |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
HU66 (BC): getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
HU66 (BC): Very fine near equal pair, yellowish A and blue-white B. ~1" or less. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
STT351 (AC): Orange stars, noticeable magnitude difference ~0.5, separated just less than ~1". What's curious is the AB pair is HU 66 AB listed as 7.90/8.40 0.1" currently, with HU 66 BC as 8.40/8.25 0.9". So my question is, if AC is physical, and if BC are physical too, why is AC uncertain? It would seem they should all be sharing orbits? Perhaps it just cries out for additional measures -- AB is grade 4 and BC is grade 5, so they are confident of physicality but there's not enough data to nail it down. |
|
|
|
|
STF2317 |
|
BC |
12m5 |
12m7 |
1.4'' |
315° |
2008 |
Her |
18h25m19.45s |
+26°04'45.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Very challenging. AB is obvious, A a bright light orange, B is blue and faint -- with careful examination I do get a scintillating small balls separated ~1" and near equal -- averted vision brightens these to pinpoints but I can't hold that resolution direct. Stelle Doppie says first measure of this pair is in 1901, so it's not a Struve discovery, likely Aitken or Hussey with the Lick 36-inch |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
BC much cleaner on this night of better seeing, blue stars very close and faint |
|
|
|
|
HO85 |
|
AB |
8m7 |
12m0 |
4.9'' |
196° |
2015 |
Her |
18h25m20.37s |
+28°04'59.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A and slightly red B, wide, ~3 delta. Did not notice HDS 2604 Aa-Ab, 0.7", 11.3 mag (though I probably could not have resolved it anyway). |
|
|
|
|
COU815 |
|
|
9m0 |
11m3 |
1.6'' |
144° |
2015 |
Her |
18h25m44.22s |
+26°39'25.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
B is a faint light orange star but is clearly separated from white A. Tough little pair |
|
|
|
|
STT352 |
|
|
7m9 |
9m4 |
24.2'' |
221° |
2019 |
Lyr |
18h26m24.42s |
+46°48'32.20" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ist B schön abgesetzt südwestlich von A erkennbar - Helligkeitsunterschied 1.5 mag - bei 64x zeigt sich A reinweiß, B ist grau |
|
Mark McCarthy
Fremont (California/USA) |
152mm (175x) |
Wide one delta mag |
|
|
|
|
HO634 |
|
|
8m2 |
12m2 |
3.3'' |
269° |
1998 |
Her |
18h26m34.71s |
+24°22'12.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice light yellow-orange star with very faint B, just direct vision & wide, but obviously tied to A [not physical!] |
|
|
|
|
BU1326 |
|
AB |
6m5 |
12m1 |
5.5'' |
107° |
2015 |
Her |
18h26m40.93s |
+26°26'57.20" |
|
|
|
|
AC |
6m5 |
9m6 |
61.8'' |
60° |
2015 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: B star is extremely faint 5" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: C star is extremely faint and much further out, ~50" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB: Extremely faint star ~4" distant from the A, 5 delta mag. |
|
|
|
|
SLE177 |
|
|
10m7 |
12m3 |
9.9'' |
186° |
2015 |
Her |
18h27m07.43s |
+23°05'42.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
2 delta mag wide pair, slightly blue B. |
|
|
|
|
STF2316, 59 Ser |
|
AB |
5m4 |
7m6 |
3.9'' |
322° |
2018 |
Ser |
18h27m12.51s |
+00°11'46.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x knappe Trennung - Komponente B zeigt sich wie ein kleines schwaches Anhängsel von A - mehr als 2 Größenklassen Helligkeitsunterschied |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Close but easily split, ~2", 2 delta mag, both yellow white. |
|
|
|
★
|
TDT886 |
|
|
11m0 |
11m3 |
0.5'' |
24° |
1991 |
Her |
18h27m27.80s |
+24°17'10.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Extremely fine. At first it seems not split, but in best moments B stretches out and pops out from B, 0.5" and 1 delta mag. |
|
|
|
|
AG223 |
|
|
10m3 |
11m1 |
2.6'' |
51° |
2018 |
Her |
18h27m34.56s |
+24°22'40.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice white near equal, white, well split ~2.5" [not physical] |
|
|
|
|
STF2319 |
|
AB |
8m4 |
8m2 |
5.3'' |
190° |
2019 |
Her |
18h27m43.94s |
+19°17'43.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Yellow-white near equal wide stars, in a plus one which is ~1 delta fainter wide perpendicular PA (this is the AC pair) |
|
|
|
★
|
STF2320 |
|
|
7m1 |
8m9 |
0.9'' |
1° |
2015 |
Her |
18h27m45.89s |
+24°41'50.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
V994 Her. Seen with the 20", but used the 8" mask to clean up the images. Two delta mag, ~1" very nice pair. [eclipsing binary of Algol type--surely not seeing the eclipsing star? In fact, both A & B each are eclipsing binaries, the first such system to be discovered in the whole sky!] |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Nice! Blue-white stars, 1", 2 delta mag. |
|
|
|
|
POU3411 |
|
AB |
10m6 |
12m4 |
9.9'' |
34° |
2015 |
Her |
18h27m47.84s |
+24°14'48.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Chain of three stars like an eyebrow, about 1 delta mag between them. AB & AC seen, with A in the middle. I noticed this asterism while observing TDT 886, it was in the same field. [not physical] |
|
|
|
|
POU3410 |
|
|
11m6 |
12m0 |
8.2'' |
259° |
2015 |
Her |
18h27m49.26s |
+23°56'22.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Seems more near equal than SkyTools data. Wide. [not physical] |
|
|
|
|
SLE180 |
|
|
13m1 |
13m5 |
6.4'' |
247° |
2015 |
Her |
18h28m06.90s |
+23°59'22.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
More of an equal pair, 13th mag, than the two delta in SkyTools. |
|
|
|
|
TDT896 |
|
|
10m6 |
11m4 |
8.8'' |
152° |
2015 |
Dra |
18h28m16.85s |
+49°30'16.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Faint but easy pair, wide, <1 delta mag. Not physical. |
|
|
|
|
STTA168 |
|
AB |
7m7 |
8m8 |
47.2'' |
162° |
2016 |
Ser |
18h28m33.52s |
+04°50'55.20" |
|
|
|
|
AC |
7m7 |
9m3 |
244.2'' |
217° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
10x50 |
AB: ordentlich getrenntes Sternpaar - Komponente B im Süden ist schon relativ schwach, aber ohne Mühe erkennbar - das Sternpaar steht schön isoliert, da keine vergleichbar hellen Sterne im unmittelbaren Umfeld sichtbar sind |
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: ein sehr entspannter Doppelstern - kein auffallendes Sternpaar - Komponente B steht komfortabel getrennt im Südosten von A und ist 1 bis 1.5 Magnituden schwächer - leichter Farbkontrast |
|
|
|
|
HN 125 |
|
|
8m2 |
8m5 |
2.7'' |
108° |
2016 |
Sgr |
18h28m56.75s |
-25°02'34.50" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x ist das Sternpaar nur in guten Momenten knapp getrennt zu sehen - Komponente B im Osten ist nur knapp schwächer |
|
René Merting
Drachhausen (Germany) |
320mm (144x) |
bei 144x kann ich den DS trennen - knapp, aber ok - beide Sterne sind gleichen sich wie ein Ei dem anderen, d.h. gleich hell und die gleiche Farbe |
|
|
|
|
WNO6 |
|
|
6m7 |
8m0 |
41.8'' |
182° |
2018 |
Sgr |
18h28m57.36s |
-26°34'55.50" |
René Merting
Drachhausen (Germany) |
18x70 |
ein komfortabel getrenntes Sternpaar - Komponente B im Süden ist eine dreiviertel Größenkasse schwächer - insgesamt ein schönes Sternumfeld mit den beiden ebenso hellen Sternen südwestlich |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x sehe ich ein weit auseinander stehendes Pärchen - Komponente A im Norden weiß, Komponente B ist eine Größenklasse schwächer und grau-blau |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ein weit getrenntes Paar - B im Süden ist eine knappe Größenklasse schwächer - leichter Farbkontrast durch den Helligkeitsunterschied |
|
|
|
|
STF2328 |
|
AB |
9m0 |
9m5 |
3.6'' |
71° |
2019 |
Lyr |
18h29m27.87s |
+29°55'27.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
near equal, ~4", light orange. |
|
|
|
|
TDT908 |
|
|
11m1 |
12m2 |
1.8'' |
8° |
2015 |
Her |
18h29m29.45s |
+23°29'14.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
~1 delta mag, fairly wide, white stars, B seen direct but brightens with averted vision. |
|
|
|
|
STF2338, KP Lyr |
|
AB |
9m3 |
11m2 |
12.1'' |
301° |
2017 |
Lyr |
18h30m54.75s |
+38°39'33.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Split in finder. In the scope one splits into a near equal pair. |
|
|
|
|
STF2324 |
|
AB |
9m0 |
9m4 |
2.4'' |
149° |
2018 |
Ser |
18h30m58.45s |
+01°23'30.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Very well split white stars, half delta mag |
|
|
|
|
STF2333 |
|
AB |
7m8 |
8m6 |
6.3'' |
333° |
2019 |
Lyr |
18h31m06.94s |
+32°14'43.40" |
|
|
|
|
AC |
7m8 |
12m9 |
164.1'' |
35° |
2015 |
|
|
|
|
|
|
|
AD |
7m8 |
13m7 |
85.8'' |
339° |
2015 |
|
|
|
|
|
|
|
BC |
8m6 |
12m9 |
161.1'' |
37° |
2015 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
AB: 2020-05-15: Clearly separated with a noticeable difference in brightness. All in all rather faint double star without visible colors. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (49x) |
AB: 2020-06-24: At 22x clearly elongated and almost separated. A difference in brightness can be seen. At 49x clearly separated with slight color difference: whitish and white-bluish. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 1 delta mag, wide. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
AB: wide separated yellow and orange, 2 delta mag. (several other pairings not seen) |
|
|
|
|
HU932 |
|
|
7m3 |
10m8 |
2.0'' |
76° |
2010 |
Dra |
18h31m19.01s |
+62°32'16.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
B appears with foveal coaxing, but can hold it direct. ~3 delta mag to bright light yellow A, ~2" |
|
|
|
|
STF2325 |
|
|
5m8 |
9m3 |
12.4'' |
257° |
2005 |
Sct |
18h31m25.69s |
-10°47'45.00" |
René Merting
Drachhausen (Germany) |
18x70 |
A ist sehr hell und überstrahlt sein unmittelbares Umfeld ordentlich - ab und an meine ich, B im Südwesten erkennen zu können, aber das ist zu unsicher oder mehr Wunschtraum |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
bei 45x zeichnet es sich ab, dass westlich außerhalb des Halos der gelblich strahlenden A-Komponente ein schwacher Lichtpunkt erkennbar ist - so richtig sicher war ich mir aber nicht, 72x bringt dann aber die Gewissheit, B steht schön abgesetzt, ist deutlich schwächer und wirkt grauweiß |
|
|
|
|
STF2329 |
|
|
8m2 |
9m4 |
4.3'' |
43° |
2016 |
Oph |
18h31m26.49s |
+06°27'36.90" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x entsteht schon die Ahnung von einem Begleitstern im NO von A - bei 64x sind beide Komponenten erkennbar, meist kleben sie noch zusammen und nur in guten Momenten ist eine knappe Trennung sichtbar - bei 107x ist die Trennung weiterhin knapp, aber eindeutig (soll heißen, man muss sich nicht mehr auf Momente besonderer Luftruhe verlassen) |
|
|
|
|
ES784 |
|
|
10m0 |
10m5 |
7.2'' |
65° |
2018 |
Dra |
18h31m51.82s |
+51°10'47.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
~1 delta mag, fairly wide white stars. Not physical |
|
|
|
|
POU3419 |
|
|
7m9 |
12m1 |
11.5'' |
240° |
2015 |
Her |
18h32m02.77s |
+25°04'01.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy pair, white stars, wide separation, ~3 delta mag |
|
|
|
|
RST5450 |
|
|
10m3 |
10m3 |
0.7'' |
253° |
2016 |
Ser |
18h32m32.53s |
+00°36'06.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
At very best moments, which are fleeting, I see very tight but nicely split pair, 1 delta mag, both faint. Resolves from a haze. Nice. |
|
|
|
|
STTA171 |
|
AB |
7m0 |
8m1 |
150.1'' |
328° |
2017 |
Lyr |
18h32m51.48s |
+38°49'59.80" |
René Merting
Drachhausen (Germany) |
18x70 |
ein weit auseinander stehendes Paar - B im Nordwesten ist halb so hell - mehr gibt es nicht zu sagen |
|
|
|
|
STF2357 |
|
|
9m3 |
9m9 |
4.7'' |
271° |
2018 |
Dra |
18h32m53.86s |
+63°42'33.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Wide ~1 delta mag white |
|
|
|
|
POU3427 |
|
|
10m1 |
10m4 |
6.8'' |
81° |
2018 |
Her |
18h32m58.78s |
+24°19'49.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy wide near equal stars |
|
|
|
|
STT356 |
|
AB |
7m3 |
9m2 |
28.3'' |
302° |
2019 |
Lyr |
18h33m14.62s |
+40°09'34.20" |
|
|
|
|
AC |
7m3 |
10m9 |
48.1'' |
9° |
2015 |
|
|
|
|
|
|
|
BC |
9m2 |
10m9 |
45.6'' |
45° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ein weit getrenntes Pärchen - Komponente B im NW ist sehr schwach und mindestens 2, wenn nicht sogar 3 Größenklassen schwächer als A - zurück auf 20x zeigt sich STT356 ordentlich getrennt und Komponente B ist nicht ganz so schwach wie der der gut 5° östlich stehende ähnlich aussehende Doppelstern STF2431 |
|
|
|
|
COU204 |
|
AB |
10m2 |
10m7 |
11.9'' |
130° |
2018 |
Her |
18h33m31.63s |
+21°02'00.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy wide, ~1 delta mag. Not physical |
|
|
|
|
STF2339 |
|
AB-CD |
7m5 |
8m7 |
1.7'' |
277° |
2018 |
Her |
18h33m45.62s |
+17°43'55.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
White and dull white B. Close but well separated, ~1" (AB-CD seen. AB is Hu 322 1 delta mag 0.2", good to try again at 20") |
|
|
|
|
A1377 & STF2348 & SLE216 |
A1377 |
AB |
6m2 |
6m4 |
0.2'' |
131° |
2014 |
Dra |
18h33m56.69s |
+52°21'12.60" |
|
|
|
STF2348 |
AB-C |
5m5 |
8m7 |
25.7'' |
271° |
2012 |
|
|
|
|
|
|
SLE216 |
AB-D |
5m5 |
11m2 |
93.7'' |
338° |
2005 |
|
|
|
|
|
|
SLE216 |
AB-E |
5m5 |
12m2 |
109.1'' |
232° |
2005 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STF2348 (AB-C): bei 32x ein auffälliges, klar getrenntes Sternpaar - A strahlt gelblich, B im Westen ist weißgrau und mindestens 2 Größenklassen schwächer - zurück auf 20x ist B ebenfalls knapp erkennbar |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
STF2348 (AB-C): Very pretty yellow-orange A and yellow-blue B, well separated. |
|
|
|
|
TDT939 |
|
|
10m8 |
10m8 |
0.6'' |
8° |
1991 |
Her |
18h34m15.05s |
+21°01'05.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Beautiful clean split, half delta mag, white stars, very close |
|
|
|
|
TDT938 |
|
|
11m5 |
11m8 |
0.6'' |
74° |
1991 |
Her |
18h34m18.40s |
+22°58'27.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Very faint, exceptionally fine, split with seeing and B is slightly brighter with averted vision. |
|
|
|
★
|
STF2337 |
|
AB |
8m1 |
9m1 |
16.6'' |
297° |
2018 |
Sct |
18h34m55.15s |
-14°42'10.60" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x gut trennbar, Helligkeitsunterschied zwischen A und B gut eine halbe Magnitude - bei 32x noch einfacher, und Verstärkung des schönen Farbkontrastes, Komponente A im SO ist weiß-bläulich und Komponente B zinnober-rot |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ist das Paar gut getrennt - B steht im NW von A und - A wirkt weiß und B … farbiger |
|
|
|
|
COU205 |
|
|
9m4 |
10m7 |
0.3'' |
152° |
1996 |
Her |
18h35m17.64s |
+21°44'36.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Notched elongation, I have the impression of significant delta mag |
|
|
|
★★
|
STT359 |
|
|
6m3 |
6m6 |
0.7'' |
3° |
2019 |
Her |
18h35m30.40s |
+23°36'19.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
2020-11-10: Clearly elongated with slight notching and little difference in brightness. I estimated the position angle to 0°. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (198x) |
leicht eingekerbt, Abstand 0“75 |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Kissing 8" 333x, hairline split 667x. Near equal white A and bluish white B. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Nice! ~0.8" equal yellow-orange stars. |
|
Uwe Pilz
Leipzig (Germany) |
320mm (388x) |
ein sehr ruhiger Abend gestattete die Nutzung von 12 Zoll |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Light yellow near equal split, very close. 219 year period |
|
|
|
|
STF2345 |
|
|
9m1 |
10m5 |
12.3'' |
226° |
2018 |
Her |
18h35m31.17s |
+21°04'27.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
V998 Her. Wide one delta [The A star is variable is an eclipsing binary but the eclipsing component is apparently only detectable with speckle interferometry. The Struve pair is not physical] |
|
|
|
|
BU643 & STF2342, FR Ser |
BU643 |
AB |
6m5 |
12m5 |
13.7'' |
325° |
2015 |
Ser |
18h35m36.48s |
+04°56'09.80" |
|
|
|
STF2342 |
AC |
6m5 |
9m6 |
33.6'' |
0° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
STF2342 (AC): das war eine schwere Geburt, Komponente A ist schon sehr hell und C im Norden so schwach, dass sie gerade so zu sehen ist |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STF2342 (AC): bei 20x weit getrenntes Pärchen, Komponente C im Nord-NO sehr schwach, mindestens 2 Größenklassen schwächer - Komponente A weißlich, C durch den großen Farbunterschied ohne Strahlkraft und deshalb kupfern |
|
|
|
★★
|
STT358 |
|
AB |
6m9 |
7m1 |
1.7'' |
146° |
2019 |
Her |
18h35m53.22s |
+16°58'32.50" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (110x) |
fast gleich hell, deutlich trennbar |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Pretty, near equal white, perfect disks. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Yellow-white stars, half delta mag, well split. 380 year period |
|
|
|
|
TDT952 |
|
|
11m4 |
11m6 |
0.7'' |
178° |
1991 |
Her |
18h35m54.54s |
+25°41'33.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
B appears with seeing within A's first diffraction, very faint, significant delta mag |
|
|
|
|
A249 |
|
|
10m1 |
10m2 |
1.0'' |
278° |
2016 |
Her |
18h36m03.12s |
+24°51'49.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Fine pair, equal white, nicely split ~1" |
|
|
|
★
|
STF2351 |
|
|
7m6 |
7m6 |
5.0'' |
161° |
2019 |
Lyr |
18h36m12.00s |
+41°16'41.20" |
Robert Zebahl
Leipzig (Germany) |
70mm (67x) |
2021-08-15: Beautifully separated with similar bright components. Mild but beautiful color contrast: light yellow/orange & light blue. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x sind zwei Sterne zu erkennen, die sich noch berühren - bei 64x zeigt sich dann nein knapp getrenntes Pärchen - fast kein Helligkeitsunterschied, ich habe Komponente A für die schwächere der beiden in etwas gleich hellen Sterne gehalten - Komponente B ist warm-weiß |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright yellow-orange equal pair, wide. |
|
|
|
|
A355 |
|
|
9m4 |
10m9 |
1.3'' |
143° |
2017 |
Ser |
18h36m19.32s |
+05°15'37.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Tough for tonight's conditions, poor transparency and a nearly full moon. Very faint star with very close companion like two smudges |
|
|
|
|
STF2349 |
|
AB |
5m4 |
9m4 |
7.2'' |
204° |
2016 |
Lyr |
18h36m37.34s |
+33°28'08.50" |
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
Easy to split with a clear difference in brightness. The companion only appeared as a tiny star. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
viel schwieriger, als es die Daten vermuten lassen (7") |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Bright white and faint ruddy B, fairly close ~4". |
|
|
|
★★
|
alpha Lyr, 3 Lyr, Vega |
H5 39 |
AB |
0m1 |
9m5 |
83.7'' |
184° |
2017 |
Lyr |
18h36m56.33s |
+38°47'01.20" |
|
|
|
STFB9 |
AC |
0m1 |
11m0 |
76.0'' |
255° |
2012 |
|
|
|
|
|
|
STFB9 |
AE |
0m1 |
9m5 |
86.6'' |
39° |
2017 |
|
|
|
Jörg S. Schlimmer
Germany |
127mm (203x) |
um Vega mehrere Beugungsringe sowie Speckles sichtbar, B leicht zu sehen, E nicht sichtbar |
|
Jörg S. Schlimmer
Germany |
127mm (203x) |
verschiedene Vergrößerungen zwischen 40 und 203 fach, Komponente E zeitweise bei indirektem Sehen sichtbar, da Himmel heute klarer ist |
|
|
|
|
STT363 |
|
|
7m5 |
8m1 |
0.6'' |
336° |
2018 |
Dra |
18h37m23.92s |
+77°41'12.40" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
als 8 zu sehen |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
STF2347 |
|
|
8m1 |
9m8 |
3.4'' |
259° |
2001 |
Ser |
18h37m56.63s |
-00°23'09.10" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x ist Komponente B sehr schwer und ganz knapp getrennt südwestlich von A erkennbar, bei 64x hatte ich nur eine Ahnung davon, kein Zuckerschlecken |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Orange and light blue, pretty without diffraction, wide separation, 2 delta mag. (not physical) |
|
|
|
|
STF2362 |
|
|
7m5 |
8m7 |
4.4'' |
187° |
2015 |
Lyr |
18h38m25.70s |
+36°03'11.30" |
Robert Zebahl
Leipzig (Germany) |
70mm (67x) |
2021-08-15: Clearly separated, distinct difference in brightness at still rather small angular distance. As a double star well visible. The primary component appeared white-yellowish. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x eine kleine Andeutung nach Süden, bei 64x dann der Beweis und knappe Trennung zwischen A und B - ein schönes enges Pärchen - B ist halb so hell |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
White-orange A, lighter orange B, 1-2 delta mag, well split. |
|
|
|
★★
|
STF2358 |
|
|
9m8 |
10m2 |
2.5'' |
224° |
2015 |
Lyr |
18h38m35.04s |
+30°43'20.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint near equal <2", another brighter / wider pair nearby. Nice! |
|
|
|
|
STT360 |
|
|
6m9 |
9m1 |
1.7'' |
282° |
2015 |
Ser |
18h38m39.84s |
+04°51'17.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Lovely orange stars, two delta mag, used the 8 inch mask to clean up the image, very nice |
|
|
|
|
A1379 |
|
|
9m7 |
10m3 |
2.1'' |
211° |
2015 |
Dra |
18h38m43.02s |
+52°43'27.60" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Faint pair, resolved with seeing, B is flickering between direct and averted vision. |
|
|
|
|
STF2368 |
|
AB |
7m6 |
7m8 |
1.9'' |
321° |
2017 |
Dra |
18h38m51.27s |
+52°20'38.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Brilliant white near equal stars, nicely separated ~2" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal white, close, ~1". Hair split at 205x. |
|
|
|
|
COU207 |
|
|
9m2 |
10m6 |
1.6'' |
298° |
2010 |
Her |
18h38m54.97s |
+22°21'58.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Light yellow A and light orange B, nicely split, ~2 delta mag. |
|
|
|
|
STF2360 |
|
|
8m0 |
9m2 |
2.4'' |
358° |
2011 |
Her |
18h39m19.16s |
+20°55'58.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Fainter white and 1 delta mag bluish B, ~4" nice pair. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White, ~2 delta mag, wide ~3" |
|
|
|
|
ES787 |
|
|
8m9 |
11m7 |
8.2'' |
37° |
2015 |
Dra |
18h39m56.26s |
+51°05'34.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
V410 Dra. B noticed with averted vision then held direct as a faint point, ~3 delta mag and wide, white stars. Not physical |
|
|
|
|
S704 |
|
|
8m5 |
9m1 |
58.1'' |
264° |
2019 |
Oph |
18h40m21.03s |
+09°41'50.60" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x zwei weit auseinander stehende Sterne - Komponente A im Osten weiß, B im Westen braun-orange kaum schwächer - zurück auf 20x sehe ich beide Komponenten ebenfalls weit getrennt |
|
|
|
|
BU1328 |
|
|
9m0 |
9m9 |
2.1'' |
284° |
2018 |
Ser |
18h40m57.82s |
+03°01'36.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Two orange stars, 1 delta mag, well split. |
|
|
|
|
STF2367 |
|
AB |
7m7 |
8m0 |
0.4'' |
74° |
2019 |
Lyr |
18h41m16.36s |
+30°17'40.90" |
|
|
|
|
AB-C |
7m0 |
8m8 |
14.1'' |
192° |
2019 |
|
|
|
|
|
|
|
AB-D |
7m0 |
12m0 |
21.9'' |
84° |
2007 |
|
|
|
|
|
|
|
AB-E |
7m0 |
11m0 |
151.7'' |
341° |
2002 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB-C: bei 32x einfach zu trennen - A-Komponente leicht gelblich, Komponente C südlich ist deutlich schwächer und strahlt zinnober |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: nicht als DS gesehen |
|
|
|
|
HU754 |
|
|
8m4 |
11m5 |
1.3'' |
93° |
1991 |
Dra |
18h41m44.99s |
+51°07'33.60" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Very fine B, a tiny point outside brilliant white A's diffraction. ~3 delta at least. |
|
|
|
|
STF2372 |
|
AB |
6m5 |
7m7 |
25.0'' |
82° |
2019 |
Lyr |
18h42m08.09s |
+34°44'46.70" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x weit getrennt, bei 64x noch weiter getrennt :-D, Komponente B halb so hell wie A und deshalb gräulicher |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
weiß und blaugrün, erkennbar bei 21x |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Yellow-green A and slightly blue-white B. 1 delta mag, very wide. |
|
|
|
|
STF2371 |
|
|
9m7 |
10m0 |
10.0'' |
56° |
2018 |
Lyr |
18h42m12.44s |
+27°38'32.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Half delta mag, wide light orange and blue-white pair. |
|
|
|
|
STF2398 |
|
AB |
9m1 |
10m0 |
11.3'' |
182° |
2019 |
Dra |
18h42m46.69s |
+59°37'49.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Very light orange stars, ~1 delta mag, wide. 408 year period |
|
|
|
|
STF2380 |
|
|
7m3 |
8m7 |
25.5'' |
8° |
2015 |
Lyr |
18h42m55.42s |
+44°55'30.90" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x einfach zu trennen - Komponente A strahlt gelblich, Komponente B im Norden wirkt eher grau und ist gut 1.5 Größenklassen schwächer - zurück auf 20x wird das Paar etwas attraktiver, weil beide Sterne nun enger zusammen stehen, A ist noch dominanter |
|
|
|
|
BU645 |
|
|
7m3 |
12m1 |
9.3'' |
305° |
2015 |
Her |
18h43m14.48s |
+19°27'59.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Pretty cream yellow-white A and slightly orange B, wide ~10", very large delta mag, >4 delta. |
|
|
|
|
STI2383 |
|
|
11m1 |
11m2 |
14.5'' |
342° |
2015 |
Dra |
18h43m19.16s |
+56°36'55.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Faint near equal stars, wide, seems to be in a small cluster. Physical pair. |
|
|
|
|
STF2378 |
|
AB |
8m9 |
9m9 |
11.5'' |
190° |
2018 |
Lyr |
18h43m21.93s |
+35°32'55.30" |
René Merting
Drachhausen (Germany) |
10x50 |
beide Sterne sind nebeneinander stehend erkennbar, aber noch nicht getrennt, schwache Einschnürung nur in guten Momenten |
|
|
|
|
STF2376 |
|
AB |
8m7 |
9m3 |
22.3'' |
63° |
2015 |
Lyr |
18h43m42.26s |
+30°24'16.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Triple? 1 delta mag between each, forms a triangle, wide separations. |
|
|
|
|
STT361 |
|
|
8m2 |
9m4 |
22.6'' |
172° |
2015 |
Ser |
18h43m42.36s |
+05°38'59.80" |
René Merting
Drachhausen (Germany) |
18x70 |
das Pärchen lässt sich schön trennen - B im Süden ist eine Größenklasse schwächer als die auch schon schwach wirkende A-Komponente |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x zeigen sich zwei schwache Sterne weit getrennt, Komponente B im Süden - bei 32x interessanter Farbkontrast, Komponente A dunkelgelb, B ockerbraun |
|
|
|
|
STI2384 |
|
|
11m8 |
11m8 |
3.8'' |
142° |
2015 |
Dra |
18h43m58.14s |
+55°58'31.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Very faint, barely there, averted vision hardly helps, but there are two hazy points, wide ~4". Not physical |
|
|
|
|
STF2403 |
|
|
6m2 |
8m3 |
1.1'' |
278° |
2011 |
Dra |
18h44m18.25s |
+61°02'53.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very tough. B is a brightening or condensation on A's diffraction ring, when A settles down with seeing. |
|
|
|
★
|
HU325 |
|
|
10m2 |
10m8 |
0.3'' |
7° |
2008 |
Her |
18h44m18.57s |
+20°52'17.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Hairline split, ~1 delta mag, very fine pair |
|
|
|
★★★
|
epsilon Lyr |
STFA37 |
AB-CD |
4m7 |
4m6 |
209.5'' |
172° |
2016 |
Lyr |
18h44m20.34s |
+39°40'12.40" |
|
|
|
STFA37 |
AI |
5m2 |
10m1 |
149.5'' |
137° |
2015 |
|
|
|
|
|
|
STF2382, 4 Lyr, epsilon 1 Lyr |
AB |
5m2 |
6m1 |
2.2'' |
345° |
2019 |
|
|
|
|
|
|
STF2383, 5 Lyr, epsilon 2 Lyr |
CD |
5m2 |
5m4 |
2.4'' |
74° |
2019 |
|
|
|
|
|
Christopher Hay
Seeheim (Germany) |
naked eye |
While waiting for Comet Neowise at 3 in the morning in July 2020 surprised myself with my first naked-eye separation of Alpha1 und Alpha2 Capricornis (observing site at 50° northern latitude, Alpha1/2 passing through meridian). Encouraged by this, I lay down and had a close look at Epsilon Lyrae, without really expecting to be able to split it naked-eye, having never succeeded previously. At first Epsilon Lyrae appeared as a very short dash of light. Then the dash resolved into two pinpoints. After 15 years in the hobby and at age 60, at last got Eps Lyr split! No precise prior PA knowledge. After memorising PA as seen naked-eye carefully, confirmed it with binoculars. Eps Lyr is the third-easiest physical double in the (northern hemisphere) summer sky for the naked eye, after Zeta UMa (much easier) und Alpha Lib (marginally easier). |
|
Christopher Hay
Seeheim (Germany) |
2x54 |
AB-CD: Clean split. Actually more pleasant than in 4x10 binoculars, presumably due to more steady handheld view. |
|
Robert Zebahl
Leipzig (Germany) |
55mm (59x) |
STF2382 (AB): At 42x slightly elongated, at 59x elongated and obviously notched. |
|
Robert Zebahl
Leipzig (Germany) |
55mm (59x) |
STF2383 (CD): At 42x clearly elongated, but without any visible notch. At 59x split with touching diffraction disks. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
STF2382 (AB): Obviously seen as figure '8'. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
STF2383 (CD): Split, but extremely tight with almost touching diffraction disks. |
|
René Merting
Drachhausen (Germany) |
76mm (95x) |
AB-CD: bei 29x schön getrennt erkennbar, ohne dass sich AB und CD schon trennen lassen
AB: bei 57x leicht länglich mit kleiner Einschnürung - bei 95x schön eng getrennt, B nördlich wirkt etwas schwächer- bei 127x wunderschön, das Sternpaar hat zwei Beugungsscheibchen, die wie ein Heiligenschein um die beiden Sterne stehen
CD: bei 57x eine 8 - bei 95x ein schön eng getrenntes Pärchen gleichheller Sterne - bei 127x wunderschön, das Sternpaar hat zwei Beugungsscheibchen, die wie ein Heiligenschein um die beiden Sterne stehen
EF und I: bei 127x sind alle drei Sterne (I 10.1 mag / E 12.3 mag / F 12.7 mag) erkennbar |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 64x ist das Sternpaar mit leichter Einschnürung und Nord-Süd-Ausdehnung erkennbar - beide Sterne stehen minimal enger zusammen als das südlichere Paar CD - bei 107x knappe Trennung, Komponente B nördlich ist mindestens eine halbe Größenklasse schwächer als A
CD: bei 64x als 8 mit Ost-West-Ausdehnung erkennbar - bei 107x knapp getrennt, beide Komponenten sind etwa gleich hell |
|
Sarah Gebauer
Germany |
100mm (136x) |
ein Test mit dem neuen Refraktor, um einen Vergleich zum 6''-Newton zu ziehen: bei 136x schon astrein getrennt, natürlich ziemlich eng und ganz fein getrennt, aber dennoch ein überraschend positives Ergebnis |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
Stunning view of the components A-D and I! |
|
Uwe Pilz
Leipzig (Germany) |
105mm (26x) |
bei 22x nicht trennbar |
|
Jörg S. Schlimmer
Germany |
127mm (203x) |
easy to split |
|
Sarah Gebauer
Germany |
150mm (250x) |
August 2019 zum ersten Mal die nah beieinanderstehenden Komponenten sauber getrennt, ein grandioser Doppel-Doppel-Anblick |
|
Winfried Kräling
Marburg (Germany) |
152mm (175x) |
|
|
René Merting
Drachhausen (Germany) |
320mm (144x) |
bei 144x sind die Komponenten von AB und CD gerade so getrennt voneinander erkennbar, sie tanzen wie wild miteinander - mit Arperturmaske und Abblendung auf 120 mm zeigen die vier nun deutlich schwächeren Sterne schöne Beugungsscheibchen und sind besser getrennt voneinander sichtbar |
|
Uwe Pilz
Leipzig (Germany) |
320mm (200x) |
7 Komponenten!! A-B-C-D-E-F-I |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
Double-Double |
|
|
|
★
|
STFA38, zeta Lyr, zeta 1/2 Lyr |
|
AD |
4m3 |
5m6 |
43.7'' |
150° |
2018 |
Lyr |
18h44m46.36s |
+37°36'18.40" |
Christopher Hay
Seeheim (Germany) |
10x42 |
Clearly separated. Colour contrast between bluish A and orangish D is there if one knows it, but not as striking as in 15x45 binoculars. |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
Component A clear blue-white, component D very pale tangerine orange. Wide split. Colour contrast seems even greater than that of nearby Delta 1/2 Lyrae. Physical double. |
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x ein schön getrenntes Pärchen - D im Südosten ist 1.5 Magnituden schwächer und wirkt blaugrau gegen die weißgelbe A-Komponente |
|
Mark McCarthy
Fremont (California/USA) |
80mm (13x) |
Zeta 2 Lyr. Slightly greenish-white stars. Best view in finder, cleaner. Wide, 1 delta mag. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x weit getrennt, Komponente A weißlich, D leicht gelblich |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
weiß-orange |
|
Sarah Gebauer
Germany |
150mm (85x) |
weit getrennt, unspektakulär |
|
Mark McCarthy
Fremont (California/USA) |
152mm (175x) |
Wide, white-yellow stars, one delta |
|
Winfried Kräling
Marburg (Germany) |
152mm (175x) |
|
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
ES1424 |
|
|
8m4 |
13m0 |
7.9'' |
90° |
2015 |
Lyr |
18h44m57.58s |
+44°21'32.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
A is a light orange & bright, B seen easily as a dull pin point, wide ~5", large delta mag. |
|
|
|
|
COU1792 |
|
|
11m0 |
12m0 |
1.1'' |
347° |
2007 |
Lyr |
18h45m01.28s |
+40°51'28.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very faint but just split with seeing when haze reduces to points, one slightly brighter than the other |
|
|
|
|
ES2020 |
|
|
10m3 |
12m0 |
3.5'' |
342° |
2015 |
Lyr |
18h45m09.42s |
+37°56'11.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
B star flashes into view with averted vision, three delta mag, >3", can hold direct intermittently with seeing and transparency |
|
|
|
|
STF2392 |
|
AC |
9m2 |
10m5 |
23.8'' |
173° |
2015 |
Lyr |
18h45m09.99s |
+39°13'32.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Obvious slightly blue stars, well split, 2 delta mag. Part of a two plus one with the other much further split and a little fainter than B (AC. There is a BC pair, 11th mag, 26") |
|
|
|
★
|
STF2393 |
|
AB |
7m8 |
10m4 |
18.2'' |
24° |
2015 |
Lyr |
18h45m10.84s |
+38°18'54.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty light orange and light blue! Wide separation, 1.5 delta mag. |
|
|
|
|
COU1608 |
|
|
11m5 |
13m6 |
1.0'' |
224° |
2009 |
Lyr |
18h45m17.02s |
+38°55'51.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Using averted vision, can stretch the haze around B and barely resolve a point ~1" separated. Extremely faint, at limit |
|
|
|
|
ROE50 |
|
AB |
10m8 |
11m7 |
4.7'' |
282° |
2015 |
Lyr |
18h45m19.87s |
+40°04'58.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
A is a light blue and B is much fainter orange color, wide ~5" |
|
|
|
★
|
STF2375 |
|
AB |
6m3 |
6m7 |
2.6'' |
120° |
2019 |
Ser |
18h45m28.36s |
+05°30'00.40" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x sehe ich zwei sehr dicht stehende Sterne, mit etwas Geduld wird ab und an eine knappe Trennung deutlich - beide sind in gleich hell (ich habe sogar A und B falsch zugeordnet, weil ich B knapp heller fand) und strahlen um die Wette in weiß |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
'Tweedledum' and 'Tweedledee', recognizable as double star at 68x, clearly split at 102x, components equally bright, quadruple, visual double |
|
|
|
|
STF2394 |
|
|
9m6 |
10m0 |
6.9'' |
203° |
2018 |
Lyr |
18h45m28.48s |
+42°02'07.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty wide near equal white. |
|
|
|
|
POU3532 |
|
|
12m3 |
12m4 |
9.8'' |
211° |
2015 |
Her |
18h45m31.49s |
+23°16'26.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Not visible with 8" so removed mask. Wide separation pair, in middle of two other stars forming a line [not physical] |
|
|
|
|
POU3533 |
|
|
12m7 |
12m8 |
12.5'' |
328° |
2015 |
Her |
18h45m36.33s |
+23°57'28.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide separated, half delta mag faint pair. Picked out fairly easily in crowded field. [not physical] |
|
|
|
|
BU51 |
|
BC |
11m9 |
12m9 |
6.0'' |
297° |
2015 |
Lyr |
18h45m39.17s |
+39°40'45.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
A is light orange & bright, BC is and obvious blue pair ~1 delta mag between B and C, wide ~3-4". Nice! Burnham: "Unimportant triple a short distance from Epsilon Lyrae, noted with 6-inch." |
|
|
|
|
SLE120 |
|
|
11m6 |
11m7 |
6.9'' |
115° |
2015 |
Lyr |
18h45m49.38s |
+31°13'17.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Fairly wide, about half delta mag, 7". Plain stars [not physical] |
|
|
|
|
MLB1079 |
|
BC |
11m2 |
12m5 |
7.4'' |
279° |
2015 |
Dra |
18h45m49.76s |
+59°22'27.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
A-BC is relatively bright white A, wide separation. The B of BC is easily but C is more difficult, fainter, but yet a steady point with seeing |
|
|
|
★
|
STF2390 |
|
|
7m4 |
8m6 |
4.3'' |
155° |
2016 |
Lyr |
18h45m49.83s |
+34°31'06.60" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ploppt Komponente B knapp getrennt auf, vorher war sie unsichtbar - Farben Fehlanzeige |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Orange and very wide separation B, 2x fainter B, bluish. |
|
|
|
|
STF2373 |
|
|
7m4 |
8m4 |
4.3'' |
336° |
2018 |
Sct |
18h45m51.33s |
-10°29'34.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ist Komponente B nördlich oberhalb von A knapp getrennt erkennbar - Helligkeitsunterschied mehr als eine Größenklasse, aber kein Farbkontrast |
|
|
|
|
SLE366 |
|
|
10m6 |
12m4 |
10.0'' |
337° |
2015 |
Lyr |
18h46m04.64s |
+27°34'17.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Faint orange and blue, pretty pair, wide about 9", almost one delta mag |
|
|
|
|
MLR7 |
|
|
9m9 |
11m0 |
1.1'' |
303° |
2010 |
Dra |
18h46m07.33s |
+61°21'10.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Extremely fine, ~1 delta, ~1" separation, resolved only with seeing when stars harden to points. |
|
|
|
|
HU937 |
|
|
8m8 |
9m9 |
1.0'' |
333° |
2015 |
Dra |
18h46m13.38s |
+64°11'44.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Hairline split at 205x, more definite split with 333x, ~1 delta mag. A is yellow-white, B is a deeper yellow-orange. 225.53 year period |
|
|
|
|
TDT1045 |
|
|
11m7 |
11m8 |
0.9'' |
301° |
1991 |
Aql |
18h46m18.10s |
+08°20'43.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very marginal. very faint star feels not round |
|
|
|
|
POU3541 |
|
|
11m7 |
12m5 |
12.1'' |
289° |
2015 |
Her |
18h46m18.80s |
+24°15'38.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Another faint pair, easily picked out in the field, one delta mag, wide. [not physical] |
|
|
|
|
TDT1047 |
|
|
11m5 |
11m7 |
0.7'' |
242° |
1991 |
Lyr |
18h46m24.73s |
+28°15'24.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Seeing not supporting steady view, but suspected elongation and notch at 553x, and at 1067x the image is soft but certainly a pair of stars in haze flashing brighter with averted vision |
|
|
|
|
STF2379, 5 Aql |
|
AB |
5m9 |
7m0 |
12.5'' |
121° |
2019 |
Aql |
18h46m28.58s |
-00°57'41.90" |
|
|
|
|
AC |
5m9 |
11m3 |
21.8'' |
156° |
2017 |
|
|
|
|
|
|
|
BC |
7m0 |
11m3 |
13.4'' |
172° |
2017 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x und etwas Geduld erkenne ich am Stern in Richtung SO knapp getrennt einen schwächeren Begleiter - bei 32x sind beide Sterne ordentlich getrennt, Komponente B gut eine Magnitude schwächer |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
AB: Wide triple. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
AC: I had strong visual color response, though the disks were somewhat bloated with seeing: A was blue-white, B was yellow-white, and C red-orange. Colors were the same at 100x but the disks smaller. With an 8-inch mask at 205x, the disks were tight and overall everything was fainter. C was less red, more grey, and much fainter, so the color was not so strong and maybe would not be described as orange |
|
|
|
|
TDT1049 |
|
|
11m2 |
11m5 |
1.3'' |
0° |
2015 |
Lyr |
18h46m29.75s |
+44°16'01.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Faint pair split with seeing at 205x, more definite with 333x. Slight mag difference. |
|
|
|
|
HU1191 |
|
|
8m7 |
9m4 |
0.2'' |
258° |
2008 |
Lyr |
18h46m34.62s |
+38°21'04.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
V595 Lyr. Very tough! In unsettled seeing it is an elongation or lopsided at all powers. However at best moments it tightens enough to show a very subtle notch & also different brightness and color, A being light orange-yellow, and ~1 delta mag B a deeper orange. Discovered in 1902 at 0.2, it has only a 14.64 year period, it will make a rapid circuit to the other side by 2026 (though only 0.1"), and "widen" to 0.2" again by 2030. Should be fun to observe! |
|
|
|
|
COU1153 |
|
|
10m4 |
10m7 |
0.4'' |
118° |
2011 |
Lyr |
18h46m34.77s |
+34°14'58.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Snowman at best moments, slight mag difference. Seems more difficult than a typical 0.4" |
|
|
|
|
HU935 |
|
|
9m9 |
10m6 |
3.0'' |
153° |
2015 |
Lyr |
18h46m38.12s |
+32°10'02.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Easy pair, ~3", one detla mag, yellow white stars. well split [not physical] |
|
|
|
|
BRT261 |
|
|
10m3 |
11m2 |
4.7'' |
18° |
2015 |
Lyr |
18h46m48.48s |
+30°53'55.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Quite easy pair, almost one delta mag, wide about 4-5" |
|
|
|
|
STF2410 |
|
|
8m6 |
8m8 |
1.7'' |
86° |
2018 |
Dra |
18h46m56.67s |
+59°19'52.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White, ~1 delta mag, well split ~2" |
|
|
|
|
STF2397 |
|
|
7m5 |
9m1 |
3.9'' |
269° |
2017 |
Lyr |
18h47m13.09s |
+31°24'20.20" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x klebt B noch an der A-Komponente - bei 107x können A und B in guten Momenten knapp getrennt erkannt werden - B ist deutlich schwächer |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Light orange and blue, pretty pair, two delta mag, wide ~5" |
|
|
|
★
|
COU1154 |
|
|
11m1 |
11m0 |
0.6'' |
55° |
2010 |
Lyr |
18h47m38.65s |
+32°47'28.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Suspect notch at 553x, 1067x too hazy, but great clean split at 667x, very small, near equal. What a great sight. |
|
|
|
|
POU3551 |
|
|
11m0 |
12m2 |
7.0'' |
157° |
2015 |
Her |
18h47m39.21s |
+24°11'33.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide ivory and blue stars, two delta mag [not physical] |
|
|
|
|
ALI142, EZ Lyr |
|
|
11m4 |
11m6 |
12.7'' |
127° |
2016 |
Lyr |
18h47m40.34s |
+35°59'34.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint pair, near equal to half a delta mag, light orange and a wide separation ~10". |
|
|
|
|
A255 |
|
|
9m2 |
12m9 |
4.9'' |
69° |
2017 |
Her |
18h48m21.20s |
+25°44'15.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice pair, yellow and slightly red, wide, B is pretty faint but easily seen |
|
|
|
|
ES2023 |
|
|
8m7 |
12m0 |
6.4'' |
246° |
2017 |
Lyr |
18h48m24.10s |
+36°11'41.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Bright white A, B is seen with averted vision and then can hold direct, ~7" |
|
|
|
|
TDT1063 |
|
|
11m5 |
11m5 |
0.6'' |
299° |
1991 |
Lyr |
18h48m38.18s |
+31°32'09.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Suspected at 553x, with 667x can observe elongation, and with averted vision it flashes definite elongation and at times split. Need to avert vision for the B star to be seen and to split but can hold if seeing steadies. |
|
|
|
|
STF2391 |
|
AB |
6m5 |
9m6 |
37.7'' |
332° |
2016 |
Sct |
18h48m39.49s |
-06°00'15.50" |
René Merting
Drachhausen (Germany) |
10x50 |
Komponente B ist extrem schwach nordwestlich von A zu erkennen, knapp getrennt - ich vermute, das schafft man mit der Öffnung nur stativgestützt … und mit einem richtig guten Fernglas |
|
René Merting
Drachhausen (Germany) |
18x70 |
Komponente B ist gut abgesetzt nordwestlich von A zu erkennen - großer Helligkeitsunterschied |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x ist Komponente B im NW von A unheimlich schwach erkennbar, mindestens 2 Größenklassen Helligkeitsunterschied - gewohnter Farbkontrast aufgrund der unterschiedlichen Helligkeiten |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
v.easy DS |
|
|
|
|
STF2401 |
|
AB |
7m3 |
9m3 |
4.1'' |
38° |
2017 |
Her |
18h48m57.83s |
+21°10'01.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Not difficult, reddish A and blue B, ~5", 1 delta mag. |
|
|
|
|
J1208 |
|
|
11m5 |
12m1 |
4.7'' |
334° |
2015 |
Lyr |
18h49m14.79s |
+28°34'47.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Easy white near equal, wide, about 5". May be another double in filed, which has a brighter A star but much fainter B, around 6" separation |
|
|
|
|
STF2402 |
|
|
8m9 |
9m3 |
1.5'' |
208° |
2015 |
Aql |
18h49m44.14s |
+10°40'35.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Lovely near equal, tight but well split. Forms a perfect triangle with two other stars |
|
|
|
|
HO440, nu 2 Lyr |
|
|
5m2 |
12m7 |
18.4'' |
175° |
2015 |
Lyr |
18h49m52.92s |
+32°33'03.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright white and very faint, very wide B. |
|
|
|
★★
|
STF2406 |
|
|
7m1 |
11m2 |
4.6'' |
4° |
2018 |
Lyr |
18h49m55.77s |
+26°25'30.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright white, 3-4 delta mag, B is averted vision only and delicate, with seeing. Wow! |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
White star no split at 8" 333x and 667x, but needed the 20" to see the well separated B star. |
|
|
|
|
HJ1352 |
|
|
7m6 |
11m3 |
13.5'' |
251° |
2015 |
Lyr |
18h50m03.28s |
+29°48'55.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
2 delta mag, wide. |
|
|
|
★
|
A256 |
|
|
9m0 |
11m2 |
2.9'' |
59° |
2009 |
Lyr |
18h50m03.54s |
+31°48'48.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Orange pair, about 2 delta mag, wide 4-5". Nice pair. |
|
|
|
★★
|
beta Lyr, 10 Lyr, Sheliak |
STFA39 |
AB |
3m6 |
6m7 |
45.7'' |
149° |
2017 |
Lyr |
18h50m04.79s |
+33°21'45.60" |
|
|
|
BU293 |
AE |
3m6 |
10m1 |
67.2'' |
317° |
2015 |
|
|
|
|
|
|
BU293 |
AF |
3m6 |
10m6 |
86.0'' |
18° |
2015 |
|
|
|
Christopher Hay
Seeheim (Germany) |
10x42 |
AB: Stabilised binoculars, handheld. B is well apart from A and distinct. Very pretty! |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
At 22x and 57x the components A, B, E and F were easily seen. The B component appeared slightly bluish-silver at 22x, but at 57x the color was difficult to tell. All four components form a slightly curved 'Y' with the bright A component in the center. |
|
René Merting
Drachhausen (Germany) |
76mm (18x) |
AB: bei 18x sind die beiden Sterne gut getrennt voneinander zu erkennen
EF: beide Komponenten zeigen sich bei 18x sehr schwach |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x sind die Komponenten A und B weit getrennt, B ist deutlich schwächer
EF: ebenfalls bei 32x machen zwei gleichhelle Fühlersterne (E und F) nördlich von Komponente A das System interessanter - sie sind noch schwächer als B - Farbe konnte ich bei keinem der vier Sterne erkennen |
|
Robert Zebahl
Leipzig (Germany) |
102mm (62x) |
Components A, B, E and F are easily visible. The two southern stars on the drawing do not belong to the system. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (139x) |
AB: Begleiter ist tiefrot; die Natur des Systems ist unsicher |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
schon sichtbar bei 26x, aber schwierig. A blauweiß, B orange. |
|
Jörg S. Schlimmer
Germany |
127mm (108x) |
easy to split |
|
Sarah Gebauer
Germany |
150mm (85x) |
AB: weit getrennt, viele helle Feldsterne |
|
|
|
★
|
BU265 |
|
|
7m4 |
9m2 |
1.5'' |
227° |
2018 |
Aql |
18h50m14.94s |
+11°31'21.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Very tremulous B star appears with seeing, surprisingly difficult for the mag, maybe because so close. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very faint but resolved B at outer diffraction ring when seeing stills. Yellow A, bluish B. |
|
|
|
★
|
STF2404 |
|
|
6m9 |
7m8 |
3.7'' |
181° |
2019 |
Aql |
18h50m45.55s |
+10°58'35.20" |
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
Already at 22x the double star is striking due to its orange color. At 44x split, but rather tight with a clear difference in brightness. At 100x the primary component appears in a bright orange, the secondary component shows a bluish tint. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Light orange and light blue, pretty. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
beide gelblich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
well split, yellow A and yellow-orange B. |
|
|
|
★
|
RST4605 |
|
|
11m2 |
11m6 |
0.9'' |
141° |
1995 |
Aql |
18h50m58.96s |
-02°38'02.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very, very fine, faint, split, quarter delta mag. Very tough considering proximity to nearly full moon with poor transparency. Nice! |
|
|
|
|
COU1012 |
|
|
9m6 |
10m9 |
0.4'' |
239° |
2009 |
Lyr |
18h51m49.06s |
+31°05'00.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Split best moments at 667x, suspect elongation 553x. Always elongated but needs seeing to still for split. Noticeable difference in mag, about one delta mag, but the stars are so close together is hard to tell. |
|
|
|
|
STI865 |
|
|
11m6 |
12m1 |
3.7'' |
179° |
2018 |
Dra |
18h51m54.46s |
+59°48'56.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Faint but well seen, nicely split ~4", nice hard points |
|
|
|
|
STF2408 |
|
|
8m5 |
9m4 |
2.3'' |
91° |
2019 |
Aql |
18h51m58.05s |
+10°46'48.90" |
René Merting
Drachhausen (Germany) |
100mm (142x) |
bei 107x berühren sich die beiden Sterne noch - bei 142x ist es immer noch nicht sehr einfach, aber in guten Momenten sehe ich beide Sterne ganz knapp getrennt - B im Osten ist deutlich schwächer |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
With seeing, 1.5 delta mag well split pair, nice. (not physical) |
|
|
|
★
|
HU199 |
|
|
9m1 |
9m5 |
0.9'' |
345° |
2015 |
Aql |
18h52m07.48s |
+11°47'54.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Wow! With seeing very tight very faint but split near equal. very cool. |
|
|
|
|
STF2411 |
|
AB |
6m6 |
9m6 |
13.3'' |
95° |
2019 |
Her |
18h52m18.63s |
+14°32'08.00" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x und mit etwas Geduld wird östlich vom Hauptstern ein sehr schwacher Begleiter sichtbar, knapp getrennt - Komponente A gelblich, Komponente B ziert sich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty orange A with 2 delta mag fainter B, ~7". |
|
|
|
|
COU1311 |
|
|
11m7 |
12m4 |
1.3'' |
223° |
2008 |
Lyr |
18h52m18.70s |
+37°13'21.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very faint, B needed foveal coaxing to come out then I could hold it, very tough. Suspected at 205x. |
|
|
|
|
HDS2677 |
|
Aa-Ab |
8m3 |
12m1 |
1.0'' |
81° |
2018 |
Lyr |
18h52m27.43s |
+26°32'05.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Pale yellow star resolved as a point on the first diffraction, very faint, only when seeing tightens |
|
|
|
|
ES1746 |
|
|
10m5 |
11m1 |
1.8'' |
114° |
2015 |
Dra |
18h52m50.17s |
+58°14'48.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Fairly faint, slight mag difference, well split ~2" |
|
|
|
|
TDT1106 |
|
|
10m6 |
10m9 |
0.5'' |
257° |
1991 |
Aql |
18h52m50.94s |
+08°10'34.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Marginal, maybe a smear but too tentative. |
|
|
|
|
TDT1116 |
|
|
11m1 |
11m3 |
0.6'' |
330° |
1991 |
Lyr |
18h53m38.40s |
+40°28'13.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Notched elongation only. Seeing not supporting more. |
|
|
|
|
TDT1118 |
|
|
11m3 |
11m4 |
0.6'' |
161° |
1991 |
Lyr |
18h53m39.35s |
+30°08'06.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Averted vision flashes elongation, but this one is very tough. Without AV I see a tight notched rod, very small, with notable difference in brightness. |
|
|
|
★
|
BU137 |
|
AB |
8m7 |
9m0 |
1.5'' |
169° |
2015 |
Lyr |
18h53m57.56s |
+37°22'49.70" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fine near equal light orange, ~2". Rich finder field. In Steph 1 open cluster. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice bright white near equal stars, 1.5", in a two plus one system with much fainter farther C. (AC 12th mag 23.6") |
|
|
|
★
|
HU1294 |
|
|
9m6 |
10m6 |
1.6'' |
118° |
2014 |
Lyr |
18h54m14.83s |
+32°14'12.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Well split, 1.5 delta mag, 2" sep, light orange and blue stars. pretty. |
|
|
|
|
HO90 |
|
|
8m7 |
12m7 |
4.0'' |
228° |
2017 |
Lyr |
18h54m27.98s |
+37°18'45.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Light orange star, B shows up only with averted vision, appears out of the haze as a brightening. |
|
|
|
★
|
delta 2 Lyr, 12 Lyr, delta Lyrae Cluster, Stephenson 1 |
ES2028 |
AB |
4m3 |
11m2 |
86.3'' |
349° |
2014 |
Lyr |
18h54m30.29s |
+36°53'55.00" |
|
|
|
ES2028 |
BC |
11m2 |
11m6 |
2.1'' |
135° |
2008 |
|
|
|
|
|
|
SMR13 |
AD |
4m5 |
8m8 |
193.1'' |
210° |
2014 |
|
|
|
|
|
|
SMR13 |
AE |
4m5 |
10m3 |
400.6'' |
238° |
2014 |
|
|
|
|
|
|
SMR13 |
AF |
4m5 |
8m8 |
369.4'' |
245° |
2014 |
|
|
|
|
|
|
SMR13 |
AG |
4m5 |
9m8 |
335.9'' |
261° |
2014 |
|
|
|
|
|
|
SMR13 |
AH |
4m5 |
8m7 |
229.4'' |
284° |
2014 |
|
|
|
|
|
|
SMR13 |
AJ |
4m3 |
12m0 |
279.5'' |
249° |
2014 |
|
|
|
|
|
|
SMR13 |
AK |
4m3 |
12m0 |
304.2'' |
236° |
2014 |
|
|
|
|
|
|
SMR13 |
HI |
8m7 |
12m9 |
26.1'' |
251° |
2015 |
|
|
|
Jörg S. Schlimmer
Germany |
305mm (94x) |
easy to split |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
ES2028 (BC): Delta 2 Lyr. ! Very cool. A is bright light orange, and BC are blue pinpoints, ~2" with a slight mag difference. Clearly and cleanly seen. |
|
|
|
★
|
STTA176 |
|
AB |
7m5 |
7m5 |
94.3'' |
112° |
2018 |
Aql |
18h54m30.59s |
+01°53'51.50" |
|
|
|
|
AC |
7m5 |
10m8 |
155.5'' |
4° |
2015 |
|
|
|
|
|
|
|
BD |
7m5 |
11m0 |
150.2'' |
358° |
2015 |
|
|
|
|
|
|
|
CD |
10m8 |
11m0 |
82.0'' |
119° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: trotz des riesigen Abstandes zwischen den beiden Sternen sieht dieses Paar richtig schick aus - beide Sterne sind gleich hell und haben kaum Konkurrenz im unmittelbaren Umfeld - wie zwei Augen, die einen beobachten |
|
|
|
|
STF2415 |
|
|
7m1 |
8m7 |
2.0'' |
290° |
2015 |
Her |
18h54m32.84s |
+20°36'55.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice pair, 2 delta mag, well separated. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Two delta mag, ~2". Used the 8" mask to clean up the star images, but the view in the 20" was more colorful, yellow A and bluish B. |
|
|
|
|
L41 |
|
|
9m7 |
10m7 |
1.7'' |
32° |
2000 |
Lyr |
18h54m34.41s |
+36°59'48.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
B reveals itself with averted vision, and as its haze fades can hold a tiny point well separated, 3 delta mag. |
|
|
|
|
BRT3335 |
|
AB |
11m9 |
11m7 |
10.0'' |
69° |
2015 |
Lyr |
18h54m35.26s |
+27°54'16.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Easy near equal, wide. These are the central stars of an arc of four. [not physical. DAL 5 AC is likely one of these additional stars in the arc, 12.07 26.2".] |
|
|
|
|
COU1932 |
|
|
10m3 |
10m4 |
0.9'' |
297° |
2016 |
Lyr |
18h54m51.24s |
+44°36'56.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Suspect at 205x, nice clean split with 333x. white stars, slight mag difference |
|
|
|
|
ES2029 |
|
|
10m0 |
11m4 |
5.1'' |
207° |
2015 |
Lyr |
18h54m51.46s |
+36°10'49.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easy wide pair, slightly blue-white. B is more blue, since fainter. 2 delta mag. (not physical) |
|
|
|
★
|
HO270 |
|
AB |
5m4 |
12m6 |
8.4'' |
300° |
2013 |
Lyr |
18h54m52.18s |
+41°36'09.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
! Bright yellow A and very faint B seen with averted vision then held direct, with another faint star one ninety degrees different PA and three times farter out (this is AC). There is a streak of grainy stars across the field, very rich. |
|
|
|
★★
|
STT525 & SHJ282 |
STT525 |
AB |
6m1 |
9m1 |
1.8'' |
130° |
2015 |
Lyr |
18h54m52.52s |
+33°58'06.90" |
|
|
|
SHJ282 |
AC |
6m1 |
7m6 |
45.4'' |
350° |
2018 |
|
|
|
|
|
|
SHJ282 |
AD |
6m1 |
11m0 |
214.8'' |
295° |
2015 |
|
|
|
Christopher Hay
Seeheim (Germany) |
10x42 |
SHJ282 (AC): Stabilised binoculars, handheld. Wide split, the A component yellowish. Alias South 282. According to Stelledoppie a physical double. |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
SHJ282 (AC): 2020-07-06: Easy, striking with reasonably apparent color contrast: yellowish to slightly orange & bluish. |
|
Christopher Hay
Seeheim (Germany) |
60mm (15x) |
SHJ282 (AC): Wide split. Blue colour of C component much more striking than the orange colour of the A component. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
SHJ282 (AC): Fairly bright and wide pair. The double star was conspicuous, especially in regard to its color: A appeared orange, C rather grey-bluish. It could be observed together with Messier 57 and beta & gamma Lyrae. Very nice. |
|
René Merting
Drachhausen (Germany) |
76mm (18x) |
SHJ282 (AC): bei 18x ist das Pärchen schon sehr auffällig - A ist hellgelb mit schönem Kontrast zur nördlich stehenden, gut getrennten B-Komponente - bei 57x präsentiert sich B in einem zarten stahlblau |
|
Uwe Pilz
Leipzig (Germany) |
105mm (21x) |
SHJ282 (AC): Orange und türkis |
|
Uwe Pilz
Leipzig (Germany) |
105mm (180x) |
STT525 (AB): gelbweiß-blau |
|
Christopher Hay
Seeheim (Germany) |
125mm (23x) |
SHJ282 (AC): Widely split, dominates the field of view, very attractive. A component is tangerine orange, C component ice blue. An echo of Albireo. A true physical pair. |
|
Christopher Hay
Seeheim (Germany) |
180mm (200x) |
SHJ282 (AC): A is very distant from C but the two are still a fine pair. Colour of C is more striking than that of A, in a manner similar to my simultaneous observation with 60mm at 15x, but not quite as pronounced.
C has a companion set off from it by a hair of black. I estimate PA from C at approx. 80°, separation very roughly 2". Surprisingly can't find this companion in the double star catalogues. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
STT525 (AB): 3er System, sehr schwierig wegen Helligkeitsunterschied |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
SHJ282 (AC): Wide separation orange and blue, 2 delta mag. |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
STT525 (AB) |
|
Claus-Dieter Jahn
Leipzig (Germany) |
|
SHJ282 (AC): TS APQ 65/420mm, ZWO ASI 178mc, Livestack with Sharpcap, Exposure time: 1600x 0.6s |
|
|
|
|
A258 |
|
|
8m9 |
9m9 |
0.3'' |
236° |
2016 |
Lyr |
18h54m59.91s |
+30°52'45.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very tough. I get elongation at 553x, and more clear elongation at 667x, but no split, not even notching, more like an unevenly illuminated rod. Seeing not support higher power. |
|
|
|
|
TDT1125 |
|
|
10m9 |
11m1 |
0.5'' |
345° |
1991 |
Lyr |
18h55m04.61s |
+36°11'08.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
In same field as L 41. Very fine, hairline split only with seeing elongated otherwise. |
|
|
|
|
ES1657 |
|
|
10m4 |
11m0 |
3.9'' |
355° |
2015 |
Lyr |
18h55m22.99s |
+40°52'12.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White A and light red B, ~1 delta mag, wide ~4" |
|
|
|
★
|
COU511 |
|
Aa-Ab |
9m7 |
9m9 |
0.7'' |
190° |
2016 |
Her |
18h55m23.68s |
+23°24'00.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
! Wow great pair. A star rather bright with B very close-in, ~1 delta mag, the tiniest pin prick <1" separated from A |
|
|
|
|
STF2419 |
|
|
9m1 |
9m4 |
3.4'' |
178° |
2018 |
Lyr |
18h55m28.52s |
+29°13'35.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal white, ~5" |
|
|
|
★
|
A2193 |
|
|
8m8 |
9m2 |
1.0'' |
357° |
2017 |
Ser |
18h55m51.23s |
+03°22'30.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Pair of white stars, half delta mag. found very quickly slew to. Nice pair. Very clean split. |
|
|
|
★
|
STF3130 & STT365 |
STT365 |
AB |
7m2 |
8m3 |
0.2'' |
359° |
2016 |
Lyr |
18h55m57.14s |
+44°13'41.90" |
|
|
|
STF3130 |
AB-C |
7m0 |
10m5 |
2.6'' |
257° |
2016 |
|
|
|
|
|
|
STF3130 |
AB-D |
7m0 |
12m0 |
181.2'' |
310° |
2003 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
152mm (175x) |
STF3130 (AB-C): Very fine, B very much fainter and red color. B appears with seeing, very close (AB is 0.4" and doable with 20-inch) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF3130 (AB-C): Extremely faint but present direct vision, white A and blue B, 4" 3-4 delta mag. Did not see AB 0.4". Nearby R Lyr which is a pretty orange. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STT365 (AB): Very fine, white and blue stars, ~4", 3 delta mag. Nice! |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
STF3130 (AB-C): Very nice bright white A and slightly red B well split from A, three delta mag. Did not notice the 0.4" AB pair STT 365 |
|
|
|
|
STF2421 |
|
|
8m1 |
9m3 |
24.6'' |
57° |
2015 |
Lyr |
18h56m01.68s |
+33°47'08.10" |
René Merting
Drachhausen (Germany) |
76mm (57x) |
bei 57x ein eher unauffälliges, ordentlich getrenntes Sternpaar - Komponente B im Nordwesten ist eine Magnitude schwächer |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
orange und blaugrün |
|
Uwe Pilz
Leipzig (Germany) |
105mm (137x) |
recht weit, einfach |
|
|
|
★
|
STF2417, theta Ser, 63 Ser, Alya |
|
AB |
4m6 |
4m9 |
22.4'' |
106° |
2019 |
Ser |
18h56m13.18s |
+04°12'12.90" |
|
|
|
|
AC |
4m6 |
6m8 |
421.0'' |
58° |
2007 |
|
|
|
René Merting
Drachhausen (Germany) |
10x35 |
AB: wunderschön für diese Vergrößerung - zwei helle dicht beieinander stehende Sterne, knapp getrennt - die hellsten Sterne im Umfeld |
|
René Merting
Drachhausen (Germany) |
10x50 |
AB: zwei helle schneeweiße Sterne, knapp getrennt - B im Osten ist nur knapp schwächer - ein schönes enges Pärchen |
|
René Merting
Drachhausen (Germany) |
16x70 |
AB: ein gut getrennt zu sehendes Pärchen - beide Sterne stahlen weiß, Komponente B im Osten ist keine halbe Größenklasse schwächer |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x ein auffälliges gut getrenntes Sternpaar - Komponente B östlich ist nur leicht schwächer und strahlt ein wenig warm-weißer |
|
Sarah Gebauer
Germany |
100mm (73x) |
AB: die mit deutlichem Abstand bei 73x getrennten Doppelsterne liegen wie in einem U aus recht gleich hellen Sternen und bilden dabei im Süden den unteren Bereich des Buchstabens |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
AB: wide pair, hardly any difference in brightness, wonderful field, double stars looks like an embedded pair of eyes |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
AB: easy DS |
|
|
|
|
TDS955 |
|
|
10m5 |
11m1 |
0.9'' |
146° |
2007 |
Dra |
18h56m21.13s |
+58°54'26.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very fine, resolved with seeing, ~1 delta mag ~1", pretty difficult. |
|
|
|
|
HJ1356 |
|
AB |
8m4 |
9m3 |
29.3'' |
342° |
2015 |
Lyr |
18h56m22.13s |
+45°30'25.40" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x zeigen sich zwei schwache ordentlich getrennte Sterne - Komponente A im Süden ist dabei doppelt so hell wie B, eine Größenklasse Helligkeitsunterschied |
|
|
|
|
TDT1139 |
|
|
10m8 |
11m8 |
2.9'' |
242° |
2016 |
Lyr |
18h56m32.12s |
+26°51'50.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Faint pair not quite equal, wide ~4". Seems an elongated haze behind it, as if in front of galaxy , or unresolved stars [Checked DSS, no galaxy behind it, and not particularly dense with stars] |
|
|
|
|
ES2422, OQ Lyr |
|
|
9m0 |
12m0 |
5.6'' |
179° |
2017 |
Lyr |
18h56m51.24s |
+31°12'03.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange with very faint, very wide, averted vision. |
|
|
|
|
BU648 |
|
AB |
5m3 |
8m0 |
1.3'' |
243° |
2015 |
Lyr |
18h57m01.61s |
+32°54'04.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Orange A and a just split, very small, very faint B, seen only with 285x --175x suspected, 456x image quality not good. Short period pair, it will make a half revolution by 2045 |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Tigher pair (AB) 3 delta mag, at first diffraction, needed critical focus and seeing. Second pair (AB-C) very wide, rather much fainter. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
277x an orange not quite round disk, suspected a close pair. At 553x it splits with seeing, 0.8", 3 delta mag, in diffraction. |
|
|
|
★★
|
STF2422 |
|
|
7m9 |
8m2 |
0.8'' |
68° |
2018 |
Her |
18h57m07.83s |
+26°05'45.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Excellent hairline split at 333x with eight inch. Near equal white stars. Picked them out in a crowded field, suspected elongation right away, split with seeing as I centered it in eyepiece, and from then it was a steady split |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwieriger wegen schwacher Sterne |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very tight, <0.8", equal light orange, pretty faint. |
|
|
|
|
STF2438 |
|
|
7m0 |
7m4 |
0.8'' |
357° |
2019 |
Dra |
18h57m28.47s |
+58°13'30.00" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
leicht; beide gleich hell |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Hairline split, white stars, near equal. 261.6 year period, look how fast it will move in the years 2150-2160! |
|
|
|
|
A260 |
|
|
9m2 |
9m6 |
0.9'' |
247° |
2017 |
Lyr |
18h57m34.07s |
+32°09'20.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
At 8", small and faint suspected split at 333x: 8" 667x stars are hazy. At 20" 667x got a clean wide split two hard paints of stars. |
|
|
|
|
HJ5505 |
|
|
9m4 |
9m5 |
14.4'' |
122° |
2019 |
Aql |
18h57m42.01s |
+09°42'01.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Near equal wide white stars. |
|
|
|
★
|
A587 |
|
BC |
10m6 |
11m5 |
1.8'' |
188° |
2017 |
Lyr |
18h57m55.98s |
+44°07'00.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Excellent 2+1 pair, bright A, BC wide and 1 delta mag, well split ~2" |
|
|
|
|
AG366 |
|
|
8m5 |
8m7 |
1.4'' |
185° |
2018 |
Lyr |
18h58m03.46s |
+47°11'30.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal yellow-white easy split |
|
|
|
|
ES2670 |
|
AB |
9m4 |
12m4 |
11.2'' |
71° |
2015 |
Lyr |
18h58m13.92s |
+30°10'52.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide two delta mag |
|
|
|
|
HO91, FF Aql |
|
AB |
5m4 |
10m1 |
7.0'' |
146° |
2015 |
Aql |
18h58m14.75s |
+17°21'39.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
FF Aql. Yellow light star but no pair seen with mask, but the pair is obvious when I used full 20" aperture, sitting just above the primary, well split, 4 delta mag. |
|
|
|
|
STF2429 |
|
|
8m4 |
10m0 |
5.5'' |
289° |
2017 |
Lyr |
18h58m26.49s |
+36°25'33.10" |
René Merting
Drachhausen (Germany) |
76mm (57x) |
bei 57x ist B sehr schwach und leicht abgesetzt westlich von A erkennbar - B ist wie ein Geist von A - bei 95x ist B dann besser sichtbar und noch mehr abgesetzt |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x knapp getrennt, der Begleiter west-nordwestlich ist sehr schwach |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide three delta mag white and very light orange. easy |
|
|
|
|
COU1797 |
|
|
10m1 |
11m8 |
1.2'' |
180° |
2007 |
Lyr |
18h58m28.31s |
+42°14'34.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy close split, ~1 delta. Nice |
|
|
|
|
TDT1158 |
|
|
10m6 |
10m9 |
8.3'' |
229° |
2018 |
Lyr |
18h58m36.54s |
+29°04'07.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Quite faint pair, transparency poor so extinction not helping, but wide and near equal. There is a third star about the same distance ninety degrees from this PA, assume is part of the pair (not physical) |
|
|
|
|
COU817 |
|
|
11m3 |
11m3 |
1.0'' |
198° |
2009 |
Lyr |
18h58m42.66s |
+27°45'01.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very tight but fairly well split near equal stars, transparency and seeing not cooperating, but can split when seeing allows |
|
|
|
|
STF2431 |
|
|
6m2 |
9m6 |
19.0'' |
236° |
2013 |
Lyr |
18h58m46.59s |
+40°40'45.10" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x zeigt sich ein gut getrenntes sehr ungleiches Paar - Komponente A im NO strahlt creme-weiß, Komponente B dagegen ist nur knapp erkennbar und leicht bräunlich - Helligkeitsunterschied 3-4 Größenklassen - zurück auf 20x ist B auch noch gerade so zu erkennen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Easy wide yellow-white & bluish pair. |
|
|
|
|
TDT1161 |
|
|
11m4 |
11m6 |
1.5'' |
1° |
2015 |
Lyr |
18h58m52.26s |
+42°18'25.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
In same field as COU 1797 and with a similar PA. Faint, near equal, easy split |
|
|
|
|
BU649 |
|
|
8m7 |
11m9 |
0.9'' |
2° |
2007 |
Lyr |
18h58m53.75s |
+32°28'32.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Not difficult, showed right away on edge of field as an elongated smear which resolved with seeing and in the center of field, used averted vision to bring out B star |
|
|
|
|
AGC9, gam Lyr |
|
AB |
3m2 |
12m1 |
13.5'' |
307° |
2015 |
Lyr |
18h58m56.62s |
+32°41'22.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Sulafat. B star immediately picked out of A's glow like a piece of debris suspended in the explosion, a planet almost hanging in the halo. |
|
|
|
|
HU332 |
|
|
9m7 |
9m6 |
0.5'' |
267° |
2016 |
Vul |
18h59m03.72s |
+22°30'03.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Beautiful close split, a little more than hairline, light orange stars near equal |
|
|
|
|
STF2424, 11 Aql |
|
AB |
5m3 |
9m3 |
20.8'' |
304° |
2019 |
Aql |
18h59m05.73s |
+13°37'21.20" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ist nordwestlich von Komponente A deutlich getrennt ein ganz schwacher Begleiter erkennbar - Komponente A zeigt keinen Farbstich, durch den großen Helligkeitsunterschied wirkt B dumpf, kein echter Farbkontrast, aber immer wieder schön anzusehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Orange star with very much fainter B, nearly AV only. Very wide separation. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
11 Aql. Yellow and very much fainter blue B, wide separation. |
|
|
|
|
TDT1168 |
|
|
9m6 |
11m5 |
1.8'' |
250° |
2002 |
Dra |
18h59m17.70s |
+59°28'45.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Nice white and blue pair, easily seen, ~2 delta ~2" |
|
|
|
|
A1387 |
|
AB |
9m1 |
10m0 |
0.3'' |
351° |
2011 |
Dra |
18h59m20.43s |
+54°50'12.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Notched elongation, white stars. Seeing not good enough to split |
|
|
|
|
STF2430 |
|
|
9m1 |
9m2 |
1.5'' |
187° |
2015 |
Lyr |
18h59m22.10s |
+29°36'11.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fine near equal ~1.5" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easy pair, hard white points, near equal mag, well separated |
|
|
|
|
ES1844 |
|
AB |
9m6 |
10m5 |
3.0'' |
19° |
2015 |
Dra |
18h59m30.05s |
+63°47'34.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Faint pair, significant mag difference, B noticed with averted vision before holding direct, well split ~3" |
|
|
|
|
ENG65, 13 Aql |
|
AB |
4m1 |
10m6 |
122.0'' |
184° |
2014 |
Aql |
18h59m37.39s |
+15°04'06.50" |
|
|
|
|
AC |
4m1 |
11m2 |
142.9'' |
159° |
2014 |
|
|
|
|
|
|
|
BC |
10m6 |
11m2 |
59.8'' |
102° |
2015 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Bright star and very wide separated, very much fainter B. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
BC: Two very faint stars, about half delta mag, wide separation. |
|
|
|
|
ES1748 |
|
|
9m4 |
10m8 |
6.6'' |
55° |
2018 |
Dra |
18h59m44.10s |
+55°43'25.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy ~1 delta mag wide pair |
|
|
|
|
STF2428 |
|
AB |
8m2 |
10m3 |
6.9'' |
287° |
2019 |
Aql |
18h59m56.53s |
+14°54'39.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
3 delta mag, wide yellow and blue. |
|
|
|
|
STF2426 |
|
AB |
7m5 |
9m0 |
16.5'' |
261° |
2019 |
Aql |
18h59m58.76s |
+12°53'24.10" |
|
|
|
|
BC |
9m0 |
13m5 |
4.2'' |
173° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ein gut getrenntes Pärchen, wobei die östliche Komponente A gelblich strahlt, Komponente B eher gräulich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Near equal orange, very wide separation. |
|
|
|
|
COU1798 |
|
|
11m5 |
11m8 |
0.6'' |
349° |
1995 |
Lyr |
18h59m59.58s |
+41°00'54.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Hairline split at best moments, noticeable mag difference. |
|
|
|
|
ES2236 |
|
|
9m2 |
13m2 |
7.3'' |
179° |
2015 |
Lyr |
19h00m12.11s |
+34°48'24.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
B seen averted vision only, fades to point in its after glow--like an old tube tv turning off. Wide split, big delta mag |
|
|
|
|
ES1326 |
|
|
9m3 |
10m4 |
2.4'' |
228° |
2016 |
Lyr |
19h00m21.32s |
+44°59'51.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Nicely split pair, noticeable mag difference ~1", white |
|
|
|
|
TDT1178 |
|
|
10m5 |
10m8 |
0.9'' |
336° |
2015 |
Lyr |
19h00m29.20s |
+27°16'12.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very fine pair, very tight, splits with seeing a little more than half a disk, almost one delta mag |
|
|
|
|
ES1429 |
|
AB |
9m7 |
11m1 |
6.1'' |
12° |
2015 |
Lyr |
19h00m29.30s |
+43°13'14.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy wide ~2 delta mag light yellow pair |
|
|
|
|
STF2425 |
|
|
7m9 |
8m6 |
29.5'' |
177° |
2018 |
Aql |
19h00m33.93s |
-08°06'31.80" |
René Merting
Drachhausen (Germany) |
10x50 |
ein sehr schwaches knapp getrenntes Sternpaar - die hellere Komponente steht im Norden |
|
René Merting
Drachhausen (Germany) |
18x70 |
ein einfacher Doppelstern - beide Komponenten sind komfortabel getrennt voneinander zu erkennen, im Sternumfeld wirken sie dennoch schön eng zusammen stehend - die südliche Komponente wirkt kühler, bläulicher und ist maximal eine halbe Größenklasse schwächer |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x fällt neben der gelb strahlenden Komponente A weit getrennt südlich ein weiß-oranger Begleiter auf, Komponente B nur gering schwächer - zurück auf 20x ein schönes eng stehendes Pärchen, auffällig im sonst recht farblosen Umfeld wegen des schönen Farbkontrastes |
|
|
|
★
|
COU1156 |
|
|
11m1 |
11m2 |
0.7'' |
111° |
2016 |
Lyr |
19h00m34.25s |
+33°01'24.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Near qual small and at best moments a clean split, still, just nice points. great star |
|
|
|
★
|
HO92 |
|
|
10m6 |
10m8 |
1.3'' |
40° |
2015 |
Lyr |
19h00m59.89s |
+32°33'11.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Beautifully well split, had an instant of perfect images. White pair near equal. |
|
|
|
|
J1280 |
|
|
11m7 |
12m0 |
3.9'' |
108° |
2016 |
Vul |
19h01m00.47s |
+22°05'34.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Faint pair slight mag difference, wide ~3". Not physical |
|
|
|
|
ALI382 |
|
|
12m0 |
11m7 |
14.7'' |
78° |
2017 |
Lyr |
19h01m15.00s |
+36°20'50.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Widely separated faint stars, I wonder how thought it was a double: similar mag, proper motion, spectra? (not physical) |
|
|
|
|
HJ1362, 16 Lyr |
|
AB |
5m0 |
10m6 |
46.9'' |
289° |
2003 |
Lyr |
19h01m26.36s |
+46°56'06.10" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x steht B westlich ganz schwach leicht außerhalb des Halos von A - bei 64x umkreisen insgesamt 5 schwache Sterne die A-Komponente, deshalb wirkt AB nicht wie ein klassisches Doppelsternpaar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
16 Lyr. Faint star at edge of direct vision, fairly well separated. |
|
|
|
|
STF2432 |
|
AB |
6m8 |
10m4 |
14.8'' |
87° |
2015 |
Aql |
19h01m48.60s |
+12°32'27.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
White and 3-4 delta mag B, very wide separation. |
|
|
|
★
|
STF2437 |
|
|
8m4 |
8m8 |
0.6'' |
1° |
2019 |
Sge |
19h01m53.16s |
+19°10'11.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Small faint, notched peanut when seeing stills. Orange. |
|
|
|
|
ES1965 |
|
|
10m7 |
12m5 |
7.5'' |
245° |
2015 |
Lyr |
19h02m04.33s |
+36°39'47.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easily picked out, 2 delta mag, wide separated stars, pretty |
|
|
|
|
STF2450 |
|
A-BC |
6m5 |
9m5 |
5.1'' |
298° |
2017 |
Dra |
19h02m07.04s |
+52°15'40.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Bright yellow and fainter yellow orb for B. 2-3 delta mag, ~5". |
|
|
|
|
ES1430 |
|
|
10m7 |
11m7 |
1.6'' |
109° |
2010 |
Lyr |
19h02m23.15s |
+42°30'26.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Delicate pair, good with seeing, >0.5 delta mag. |
|
|
|
|
STF2441 |
|
AB |
7m8 |
9m8 |
6.2'' |
264° |
2015 |
Lyr |
19h02m41.26s |
+31°23'58.50" |
|
|
|
|
AC |
7m8 |
11m2 |
101.2'' |
135° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
AB: bei 64x zeigt sich Komponente B knapp getrennt westlich von A - Komponente B ist deutlich schwächer |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 2 delta mag, ~10" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
AB: White and slightly greenish, wide, 2 delta mag. (AC very widely separated) |
|
|
|
|
STF2434 |
|
A-BC |
8m4 |
8m9 |
27.8'' |
88° |
2019 |
Aql |
19h02m44.38s |
-00°42'40.40" |
René Merting
Drachhausen (Germany) |
76mm (18x) |
bei 29x einfach, A und BC stehen ordentlich auseinander und haben einen ordentliche Farbkontrast, der aber immer hin und her zu springen scheint - zurück auf 18x ist das Pärchen noch immer gut getrennt zu erkennen - der Doppelstern ist schön anzusehen, er wird im Westen von einer gebogenen Kette aus sechs Sternen flankiert, die sich wie eine Schnecke einkringeln (ein großer Bogen, der immer enger wird) |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein auffallendes, schön zusammen stehendes Sternpaar mit einem Farbkontrast, der nicht richtig greifbar ist - B wirkt kühler in der Farbe und ist vielleicht eine viertel Größenklasse schwächer |
|
Robert Zebahl
Leipzig (Germany) |
120mm (18x) |
Easily split with similar brightness. |
|
|
|
|
ES480 |
|
AB |
10m3 |
11m3 |
2.4'' |
273° |
2015 |
Lyr |
19h02m55.78s |
+27°42'26.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice pair, wide split, bluish, half delta mag. (I should try again, WAK 3 AC is 11.65 1.1") |
|
|
|
★
|
A589 |
|
|
9m5 |
10m1 |
0.7'' |
6° |
2017 |
Lyr |
19h03m01.81s |
+42°32'45.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
! Exceedingly fine pair, split with seeing, ~1 delta mag, white A and blue B. In the same field with ES 1430. |
|
|
|
|
A2991 |
|
|
10m4 |
10m8 |
0.7'' |
82° |
2016 |
Vul |
19h03m23.53s |
+25°11'19.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Suspect elongation with 205x. B has a significant mag difference than A, maybe half delta, very closely separated <1" |
|
|
|
|
ALI613 |
|
|
13m3 |
13m6 |
9.0'' |
237° |
2015 |
Lyr |
19h03m36.82s |
+37°24'49.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide separation, near equal faint stars. Can see it direct vision. Averted vision needed at thirteenth magnitude if close to another star. Not a challenge at all (not physical) |
|
|
|
|
ARG33, BH Dra |
|
|
8m5 |
9m2 |
10.6'' |
57° |
2018 |
Dra |
19h03m39.54s |
+57°27'25.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
BH Dra. White stars, ~1 delta mag, wide |
|
|
|
|
STF2448 |
|
|
8m8 |
8m8 |
2.5'' |
191° |
2019 |
Lyr |
19h03m39.66s |
+35°44'34.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal white, 3-4" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easy near equal white, 2" |
|
|
|
|
STF2442 |
|
AB |
8m5 |
9m8 |
9.9'' |
210° |
2019 |
Aql |
19h03m42.21s |
+16°57'57.80" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ist A schwach und orange, B südlich ist gut getrennt erkennbar, noch schwächer und farblich nur noch als "dunkel" zu bezeichnen, dadurch aber ein auffälliger Farbkontrast -runter auf 20x kann ich B leider nicht orten - der Doppelstern bildet mit einigen 7-9 mag hellen Sternen nördlich ein markantes Muster wie ein Angelhaken (oder einer Häkelnadel, wenn man bedenkt, wie eng der Bogen südlich geschwungen ist) - STF2442 bildet dabei die Spitze der Rundung des Hakens - sehenswert innerhalb dieses Musters |
|
|
|
|
BU1285 |
|
AB |
7m3 |
12m8 |
11.2'' |
289° |
2018 |
Lyr |
19h03m55.60s |
+34°09'04.60" |
|
|
|
|
AC |
7m3 |
10m7 |
41.8'' |
208° |
2018 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: White A and wide faint B. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
AB: Thirteenth mag B easily picked out within the very bright A's glow. |
|
|
|
★
|
COU1935 |
|
|
10m6 |
11m1 |
1.1'' |
41° |
2015 |
Lyr |
19h04m11.37s |
+38°58'47.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very fine near equal, well split, 1", white. Verified on chart. |
|
|
|
|
BRD4 |
|
|
9m2 |
9m6 |
2.6'' |
310° |
2018 |
Lyr |
19h04m15.19s |
+32°45'16.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Near equal white, wide |
|
|
|
|
DA9 |
|
|
7m0 |
10m2 |
2.0'' |
172° |
1991 |
Lyr |
19h04m15.72s |
+43°52'49.50" |
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Suspected with 175x, solid split and resolution of B with 285x. Very faint B condenses with seeing. A is light blue color |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint but perfect star images showing. 3 delta mag, ~5". |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Used apodising mask to clean up A's disk image. B appears as a light blue disk nicely separated, diamond ring to white A. Nice |
|
|
|
|
J1209 |
|
|
11m5 |
12m3 |
4.4'' |
155° |
2017 |
Lyr |
19h04m25.08s |
+34°06'19.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easy pair, wide, bluish, two delta mag |
|
|
|
|
STF2445 |
|
AB |
7m2 |
8m6 |
12.4'' |
262° |
2015 |
Vul |
19h04m38.50s |
+23°19'45.50" |
|
|
|
|
AC |
7m2 |
8m5 |
143.8'' |
108° |
2015 |
|
|
|
|
|
|
|
BC |
8m6 |
8m5 |
155.1'' |
106° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x Trennung eindeutig - gut 1.5 Magnituden Helligkeitsunterschied, Komponente B wirkt trotzdem erstaunlich weiß-grau im Vergleich zur weißen A-Komponente - bei 20x ist B mit etwas Konzentration auch schon knapp getrennt westlich von A erkennbar |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Wide separated ~1.5 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
AB: Lovely wide pair, ~2 delta mag, light yellow A and dull B |
|
|
|
|
ES2237 |
|
|
10m3 |
10m6 |
9.9'' |
218° |
2018 |
Lyr |
19h04m40.41s |
+33°34'26.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide near equal pair, white, easily picked out |
|
|
|
|
TDT1213 |
|
|
10m4 |
11m4 |
2.2'' |
255° |
2015 |
Lyr |
19h04m50.67s |
+29°44'15.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Picked out at edge of field, a nice two delta mag pair, 2", could be a two plus one system |
|
|
|
|
COH1 |
|
|
10m8 |
11m1 |
9.4'' |
315° |
2015 |
Lyr |
19h04m55.99s |
+28°28'27.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide separation half delta mag, easy pair |
|
|
|
★★
|
15 Aql, SHJ286 |
|
|
5m5 |
7m0 |
39.6'' |
211° |
2019 |
Aql |
19h04m57.67s |
-04°01'53.10" |
René Merting
Drachhausen (Germany) |
8x30 |
beide Sterne zeigen sich gut getrennt, wobei B im Süden lediglich dunkler wirkt, Farben sind nicht wirklich erkennbar |
|
René Merting
Drachhausen (Germany) |
10x50 |
sehr auffälliges dicht zusammen stehendes Sternpaar - Komponente A im Norden ist hellgelb, B grau-orange, schöner Farbkontrast |
|
René Merting
Drachhausen (Germany) |
12x50 |
ein ordentlich getrenntes Sternpaar - A im NO ist weißgelb, B wirkt gelborange |
|
René Merting
Drachhausen (Germany) |
16x70 |
ein wunderschönes ordentlich getrenntes Sternpaar - Komponente A im NO samtgelb, B dagegen apricot-orange und gut 1.5 Magnituden schwächer als A - zudem ein interessanter Farbvergleich möglich zu dem mit im Gesichtsfeld stehenden V Aql gut 1.7° weiter südlich, der farblich noch eine Schippe drauf legen kann mit einem kräftigen zinnober-orange |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
Striking, pretty wide, uneven pair. Primary component gleamed in shiny orange, the companion appeared slightly orange. |
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x ein weit getrenntes Pärchen, B ist eine Größenklasse schwächer - A ist buttergelb, B wirkt noch etwas dunkelgelblicher |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x weit getrennt, Komponente A hellgelb, B dagegen orangefarben - sehenswert |
|
Sarah Gebauer
Germany |
150mm (125x) |
gut gefunden, beide Sterne stehen in weitem Abstand zueinander |
|
Robert Zebahl
Leipzig (Germany) |
200mm (37x) |
Conditions in the target region: SQM-L 19.9
Easy to split, evident. Both components appeared slightly orange colored. |
|
|
|
|
BU359 |
|
AB |
8m8 |
9m8 |
4.6'' |
81° |
2019 |
Vul |
19h05m09.69s |
+23°25'57.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
In the same field as STF 2445, and is a smaller and flipped analog of it. It's the opposite PA dimmer but with similar mag difference, just smaller scale. Not physical |
|
|
|
|
ALI614 |
|
|
12m7 |
12m8 |
10.1'' |
90° |
2015 |
Lyr |
19h05m10.34s |
+38°03'25.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Fainter pair of a double-double in field, both about the same wide separation (AG 227 the other pair) |
|
|
|
|
TDS964 |
|
|
9m9 |
11m2 |
1.3'' |
73° |
2015 |
Lyr |
19h05m11.00s |
+40°22'20.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very nice yellow A and fainter B, 1", 1.5-2 delta mag. Fine pair |
|
|
|
|
AG227 |
|
|
10m7 |
11m2 |
7.1'' |
31° |
2015 |
Lyr |
19h05m22.05s |
+38°03'20.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
This is the brighter pair of the double-double pair mentioned in last entry (ALI 614). White stars, brilliant, wide separation |
|
|
|
|
BU287, zet Aql |
|
AB |
3m0 |
12m0 |
7.2'' |
46° |
2009 |
Aql |
19h05m24.61s |
+13°51'49.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Deneb el okab. B quite easily seen as a faint companion to brilliant white A, wide ~7", very large delta mag. Burnham discovered it with the 26-inch at the USNO in 1874 during a short stint there -- at 5.53" so it was tougher and probably needed that aperture to discover |
|
|
|
|
STF2446 |
|
AB |
7m0 |
8m9 |
9.5'' |
153° |
2019 |
Aql |
19h05m47.70s |
+06°32'49.20" |
|
|
|
|
AC |
7m0 |
11m2 |
37.2'' |
347° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ein gut getrenntes Pärchen, Begleiter südöstlich schwach - aufgrund des Helligkeitsunterschiedes Farbunterschied wahrnehmbar, Komponente A strahlt weiß mit einem Stich ins gelbliche, B eher wie ein Kupferkessel in der Nacht von innen - STF2446 ist ein schönes Doppel-Doppel zusammen mit dem 37' nördlich stehenden STF2449, wo die Komponenten einen ähnlichen Abstand haben |
|
|
|
|
TDS965 |
|
|
11m0 |
11m4 |
1.4'' |
165° |
2015 |
Lyr |
19h05m57.44s |
+33°54'17.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Seeing very briefly hardened and these split to distinct points out of an elongated smear. |
|
|
|
|
STF2463 |
|
AB |
9m1 |
10m8 |
9.7'' |
0° |
2015 |
Lyr |
19h06m01.16s |
+45°48'50.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Light orange-yellow A and light blue B, wide, ~1 delta. Not physical |
|
|
|
|
COU1614 |
|
|
9m9 |
9m9 |
0.5'' |
117° |
2016 |
Lyr |
19h06m03.06s |
+35°48'45.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very tough given the conditions, but getting a suspect elongation at 667x and at 1067x I get moments of a notch within the haze, and a definite magnitude difference. Marginal. Transparency and seeing not cooperating. |
|
|
|
|
TDT1223 |
|
|
11m3 |
11m7 |
2.5'' |
41° |
2015 |
Lyr |
19h06m04.39s |
+33°35'25.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easier to see than last pair (TDS 965), wider split, half delta mag |
|
|
|
|
STF2454 |
|
AB |
8m3 |
9m7 |
1.3'' |
291° |
2016 |
Lyr |
19h06m09.37s |
+30°26'18.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fine yellowish pair, ~1.5" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice well split 2 delta mag, white A reddish B. (DRD 2 AC is 13.50 mag and 31.3") |
|
|
|
|
EHR16, lambda Aql, 16 Aql |
|
AB |
3m5 |
7m5 |
12.5'' |
30° |
2009 |
Aql |
19h06m14.95s |
-04°52'56.40" |
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
2020-07-29: The companion can be seen to some extent as an elongated brightening in the first diffraction ring of the primary component. It still appears intermittently as a fragment of the diffraction ring. |
|
|
|
★
|
STF2449 |
|
|
7m2 |
7m7 |
8.0'' |
289° |
2015 |
Aql |
19h06m23.04s |
+07°09'20.10" |
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
At 22x well separable, but quite close together. Some fainter and similarly bright stars in the immediate surrounding. At 57x small difference in brightness. Main component looked white-bluish, companion slightly orange. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein knapp getrenntes Pärchen - B-Komponente westlich nur unwesentlich schwächer - beide Sterne heiraten in weiß - STF2449 ist ein schönes Doppel-Doppel zusammen mit dem 37' südlich stehenden STF2446, wo die Komponenten einen ähnlichen Abstand haben |
|
|
|
|
HO97 |
|
AB |
9m9 |
9m8 |
0.8'' |
15° |
2016 |
Lyr |
19h06m25.55s |
+31°44'24.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Clean split with seeing, white, half delta mag. Nice. |
|
|
|
|
STF2447 |
|
AB |
6m8 |
9m6 |
14.1'' |
343° |
2019 |
Aql |
19h06m35.11s |
-01°20'46.00" |
|
|
|
|
AC |
6m8 |
14m0 |
12.9'' |
192° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
AB: bei 29x ist B nordwestlich von A knapp abgesetzt erkennbar - B ist extrem schwach - bei 57x dann ordentliche Trennung und B ist weiterhin sehr schwach |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x zeigt sich B knapp getrennt nordwestlich von A und ist deutlich schwächer - A präsentiert sich weiß, B ist grauweiß - ein eher unauffälliges Paar |
|
|
|
|
S710 |
|
|
6m1 |
8m4 |
6.4'' |
0° |
2016 |
Sgr |
19h06m52.12s |
-16°13'45.40" |
René Merting
Drachhausen (Germany) |
76mm (57x) |
bei 57x zeigt sich B genau nördlich von A wie so eine kleine Bommel - ein sehr ungleiches Paar, ich schätze 3 Größenklassen Helligkeitsunterschied (2.32 mag lt. Stelle Doppie) - A strahlt weiß und B … naja … was bleibt der schwachen Komponente anderes übrig, als grau zu schimmern |
|
|
|
|
WFC217 |
|
|
10m2 |
11m1 |
7.7'' |
335° |
2015 |
Lyr |
19h06m52.15s |
+34°10'02.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Easy yellow and blue, wide, one delta mag |
|
|
|
|
STF2458 |
|
AB |
9m7 |
10m4 |
11.3'' |
227° |
2015 |
Lyr |
19h06m52.39s |
+27°45'09.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal pretty wide. |
|
|
|
★★
|
STF2455 |
|
AB |
7m4 |
9m4 |
9.6'' |
28° |
2015 |
Vul |
19h06m53.00s |
+22°10'21.50" |
|
|
|
|
AC |
7m4 |
12m3 |
99.6'' |
20° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x noch dicht beieinander, bei 64x gut getrennt - wie STF2455 und der nahe STF2457 (25' südlicher) sich gegenüberstehen und die jeweils schwächere Komponente in Richtung des anderen Doppelsterns vor sich herschiebt, das hat was - als ob die beiden Fußball spielen (die jeweilige Komponente A hat einen Ball vor den Füßen) - zwischen den beiden Doppelsternen steht ein schwacher Stern, vermutlich der verwirrte Schiedsrichter |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Yellow and yellow-orange, 1 delta mag, very wide. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
AB: Wide ~2 delta mag, light yellow-white A and dull B. Not physical |
|
|
|
|
HEI568, 18 Aql |
|
|
5m4 |
6m4 |
0.3'' |
257° |
2015 |
Aql |
19h06m58.60s |
+11°04'16.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (410x) |
18 Aql. The A star is elongated / smeared but 410x does not resolve, seeing not good enough. |
|
|
|
|
STT369 |
|
|
7m8 |
7m9 |
0.7'' |
5° |
2018 |
Dra |
19h07m06.37s |
+72°04'26.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
zeitweilig gut erkennbar |
|
|
|
★★
|
STF2457 |
|
|
7m5 |
9m5 |
10.2'' |
201° |
2015 |
Vul |
19h07m08.02s |
+22°35'03.70" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x gut getrennt, bei 64x schon ein ordentlicher Abstand - wie STF2457 und der nahe STF2455 (25' nördlicher) sich gegenüberstehen und die jeweils schwächere Komponente in Richtung des anderen Doppelsterns vor sich herschiebt, das hat was - als ob die beiden Fußball spielen (die jeweilige Komponente A hat einen Ball vor den Füßen) - zwischen den beiden Doppelsternen steht ein schwacher Stern, vermutlich der verwirrte Schiedsrichter |
|
Christopher Hay
Seeheim (Germany) |
150mm (96x) |
Widely split. Attractive together in 0.8-degree FOV with Struve 2455AB a little less than half a degree south. The secondaries of the two doubles point towards each other, a nice sort of double-double. According to Stelledoppie 2457 is a physical double, while 2455AB is not. In 2457 the brightness of both components is less than those of 2455AB, their separation greater, and their colour contrast (itself hard to define) is greater. In 2455AB focussing on the A-component precisely is hard to achieve, perhaps due to an unresolved field star very close to it? |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Pale yellow stars, wide separation, 1.5 delta mag. |
|
|
|
|
STF2459 |
|
|
9m1 |
10m1 |
13.8'' |
232° |
2015 |
Lyr |
19h07m22.01s |
+25°58'23.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Easy wide, ~1 delta |
|
|
|
★
|
STF2461, 17 Lyr |
|
AB |
5m3 |
9m1 |
3.2'' |
281° |
2017 |
Lyr |
19h07m25.58s |
+32°30'06.20" |
René Merting
Drachhausen (Germany) |
100mm (142x) |
nichts zu holen für mich bis 142x, vermutlich verhindert der große Helligkeitsunterschied die Trennung |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
At 129x clearly split. The B component was just visible as pretty faint, tiny star. At 270x much easier visible. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
17 Lyr. Yellow and red, much fainter B ~3 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
17 Lyr. Huge delta mag. B is obvious in 20", though A's diffraction was horrible. Used mask to clean it up but the B star momentarily disappeared, though I could eventually pull it back out with seeing and critical focus. 4 delta mag. |
|
|
|
|
STF2469 |
|
AB |
7m9 |
9m1 |
1.3'' |
126° |
2015 |
Lyr |
19h07m47.60s |
+38°55'41.60" |
Uwe Pilz
Leipzig (Germany) |
105mm (130x) |
nicht trennbar, Begleiter zu schwach |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Split when seeing stills. <1", ~1 delta mag. |
|
|
|
|
A704 |
|
|
10m3 |
10m5 |
1.2'' |
280° |
2018 |
Lyr |
19h07m53.09s |
+46°52'06.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very fine split, white near equal, ~1" |
|
|
|
|
STF2466 |
|
AB |
8m6 |
9m0 |
2.3'' |
104° |
2018 |
Lyr |
19h07m53.72s |
+29°48'02.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal 3" light orange |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Hard white points, well separated, one delta mag., white (surprised it is not physical) |
|
|
|
|
STF2467 |
|
|
10m1 |
10m3 |
10.5'' |
262° |
2015 |
Lyr |
19h08m05.79s |
+30°47'34.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal pretty wide, yellowish |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Wide separated white, near equal, 10x10th mag, 10" |
|
|
|
|
TDT1243 |
|
|
11m5 |
11m6 |
2.2'' |
232° |
2015 |
Lyr |
19h08m16.62s |
+36°08'04.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Faint but easily split pair, near equal white |
|
|
|
|
COU420 |
|
|
8m7 |
10m8 |
1.2'' |
97° |
2008 |
Lyr |
19h08m17.42s |
+25°55'25.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Finely split, <2 delta mag, bluish B. |
|
|
|
|
TDT1245 |
|
|
11m7 |
11m7 |
0.7'' |
24° |
1991 |
Lyr |
19h08m21.23s |
+29°04'18.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Marginal very barely split or rather a notched double haze. Very small and faint. |
|
|
|
|
TDT1246 |
|
|
11m2 |
11m6 |
0.7'' |
97° |
1991 |
Lyr |
19h08m30.59s |
+47°27'36.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Same field as A 704. Very fine B seen and split with seeing as a fine point, ~1 delta mag |
|
|
|
★★
|
STF2470 |
|
|
7m0 |
8m4 |
13.8'' |
267° |
2017 |
Lyr |
19h08m45.20s |
+34°45'37.10" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-06: Striking with well visible brightness difference. Very nice together with STF2474, which gives a similar view. A double-double for binoculars. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x knapp getrennt - wunderschönes Synchrontänzer-Doppel-Doppel zusammen mit STF2474 unmittelbar 10' südlich, weil A und B bei beiden Paaren mit gleichen Helligkeiten und Positionswinkel strahlen - A-Komponente von STF2470 knapp schwächer als A-Komponente von STF2470 |
|
Robert Zebahl
Leipzig (Germany) |
102mm (40x) |
Striking, especially with STF 2474 in one visual field. The color of the components was not clearly visible. Worthwhile! Sketch see STF 2474. |
|
Sarah Gebauer
Germany |
150mm (85x) |
nach mehreren Anläufen dann gefunden und bei 85x wie ein Doppel-Doppel im Bild, sehr sehenswert, auch der Abstandsunterschied (13,8'' bei STF 2470 und 15,9'' bei STF 2474) ist zu erkennen |
|
|
|
|
TDT1250 |
|
|
11m9 |
12m1 |
1.2'' |
172° |
2015 |
Lyr |
19h08m51.33s |
+26°03'04.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very finely split, faint blue pair, half delta mag. |
|
|
|
★★
|
STF2474 |
|
AB |
6m8 |
7m9 |
16.0'' |
263° |
2019 |
Lyr |
19h09m04.35s |
+34°35'59.90" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-06: Striking with well visible brightness difference. Very nice together with STF2470, which gives a similar view. A double-double for binoculars. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x knapp getrennt - wunderschönes Synchrontänzer-Doppel-Doppel zusammen mit STF2470 unmittelbar 10' nördlich, weil A und B bei beiden Paaren mit gleichen Helligkeiten und Positionswinkel strahlen - A-Komponente von STF2474 knapp heller als A-Komponente von STF2470 - bei 64x Komponente A ein wenig gelblich |
|
Robert Zebahl
Leipzig (Germany) |
102mm (40x) |
Pretty conspicuous, easy double star. Especially attractive with the nearby double star STF 2470, as both are very similar in brightness, distance and position angle. The color of both components appeared slightly yellowish-orange. |
|
Sarah Gebauer
Germany |
150mm (85x) |
nach mehreren Anläufen dann gefunden und bei 85x wie ein Doppel-Doppel im Bild, sehr sehenswert, auch der Abstandsunterschied (13,8'' bei STF 2470 und 15,9'' bei STF 2474) ist zu erkennen |
|
Christopher Hay
Seeheim (Germany) |
150mm (96x) |
Widely separated. Component A yellowish, B light ice-blue. A true physical pair in 171 LY distance. Very attractive in field of view together with Struve 2470 about 10 arcseconds north. The components of each of the two Struves have almost the same position angles, similar separations and very similar delta-magnitudes. Struve 2470 is like an echo of 2474 but with no definite colour impression. |
|
|
|
|
HO444 |
|
|
8m7 |
10m5 |
1.3'' |
67° |
2016 |
Lyr |
19h09m13.70s |
+26°56'07.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Close split <1", significant magnitude difference >1 delta. White stars |
|
|
|
|
TDS972 |
|
|
11m1 |
11m3 |
0.7'' |
311° |
2008 |
Lyr |
19h09m37.79s |
+26°40'32.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Faint, finely split, slight mag difference |
|
|
|
|
TDT1262 |
|
|
12m1 |
12m3 |
0.7'' |
92° |
1991 |
Lyr |
19h09m42.80s |
+27°14'41.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Very faint, B is difficult, split and resolved with seeing, helped with foveal coaxing and I can hold it direct after. Noticeable magnitude difference, <1 delta. |
|
|
|
|
COU2279 |
|
|
10m3 |
10m6 |
0.7'' |
125° |
2008 |
Lyr |
19h10m01.22s |
+42°24'37.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Nice firm split with seeing, white near equal |
|
|
|
|
STF2471 |
|
|
7m5 |
10m6 |
8.6'' |
122° |
2015 |
Aql |
19h10m56.93s |
+08°07'17.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Detected B with averted vision. Wide and white, can hold B directly when I know where it is. |
|
|
|
|
STF2481 |
|
A-BC |
8m4 |
8m3 |
4.8'' |
18° |
2019 |
Lyr |
19h11m07.90s |
+38°46'48.40" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x kann ich zwei gleich helle dicht aneinander stehende Sterne mit Einschnürung erkennen - in guten Momenten berühren sich die Sterne nur leicht - bei 64x dann ein knapp getrenntes Pärchen, die nördliche stehende Komponente mit zartem Gelbstich |
|
Uwe Pilz
Leipzig (Germany) |
105mm (130x) |
gleichhell, einfach |
|
Mark McCarthy
Fremont (California/USA) |
152mm (175x) |
Light orange stars, near equal, well separated. (I need to try this with the 20-inch, BC is 0.2" and only one delta mag.) |
|
|
|
|
AG373 |
|
|
10m4 |
11m1 |
3.0'' |
328° |
2018 |
Lyr |
19h11m20.45s |
+27°05'28.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Light yellow-white A and deeper yellow B, ~2 delta mag, wide |
|
|
|
|
A151 |
|
|
8m6 |
9m6 |
0.6'' |
158° |
2016 |
Sge |
19h11m22.81s |
+21°15'39.20" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
|
|
J1263 |
|
BC |
12m9 |
14m0 |
8.6'' |
40° |
2015 |
Lyr |
19h11m28.70s |
+29°53'10.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
AB is the easy bright light orange star and the very wide blue pair of BC, which are wide and ~1 delta mag. Not physical |
|
|
|
|
STF2480 |
|
|
7m7 |
10m2 |
15.1'' |
23° |
2015 |
Lyr |
19h11m45.03s |
+26°14'57.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
2 delta mag, very wide yellow-white and blue. |
|
|
|
★
|
STF2486 |
|
AB |
6m5 |
6m7 |
7.1'' |
204° |
2019 |
Cyg |
19h12m05.03s |
+49°51'20.70" |
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-03: Fine split, but very tight with equally bright components. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
At 22x barely split with a slight difference in brightness. At 44x the primary looked orange. I could not determine the color of the companion. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal yellow pair. |
|
|
|
|
STF2483 |
|
AB |
8m0 |
9m1 |
10.0'' |
317° |
2015 |
Lyr |
19h12m23.60s |
+30°20'51.90" |
|
|
|
|
AC |
8m0 |
9m7 |
71.2'' |
236° |
2015 |
|
|
|
|
|
|
|
BC |
9m1 |
9m7 |
70.4'' |
228° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 20x zeigt sich nordöstlich am Hauptstern eine Andeutung von einer Lichtquelle - bei 32x dann ein fein säuberlich getrenntes Pärchen, wobei B nur unwesentlich schwächer scheint - der Doppelstern bildet mit drei schwächeren Sternen ein längliches Südost-Nordwest verlaufendes Parallelogramm |
|
Robert Zebahl
Leipzig (Germany) |
152mm (49x) |
2020-06-24: At 22x, all three components are well visible and form a prominent, acute-angled triangle with the dim C component at the apex. At 49x color differences become visible: A appears white-yellowish, B slightly bluish and C rather orange. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
AB: Easy wide A is greenish yellow-white, and B is ice blue. |
|
|
|
|
WFC218 |
|
|
9m8 |
10m2 |
9.5'' |
352° |
2016 |
Lyr |
19h12m29.46s |
+44°47'18.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Nice near equal white |
|
|
|
★
|
BU139 & STTA177, V338 Sge |
BU139 |
AB |
7m1 |
8m0 |
0.6'' |
136° |
2017 |
Sge |
19h12m34.45s |
+16°50'47.20" |
|
|
|
STTA177 |
AC |
7m1 |
8m0 |
98.4'' |
276° |
2017 |
|
|
|
|
|
|
BU139 |
AE |
7m1 |
11m2 |
28.8'' |
101° |
2015 |
|
|
|
|
|
|
BU139 |
CD |
8m0 |
11m2 |
138.9'' |
269° |
2015 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
80mm (13x) |
STTA177 (AC): Near equal wide pair split in finder |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
BU139 (AB): At the very best moments of seeing, which were fleeting, saw kissing disks to hairline split. Suspected elongation at 205x & 333x. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
BU139 (AB): getrennt, schwierig, 0,6"? |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
BU139 (AB): V338 Sge. Overlapping airy disks. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STTA177 (AC): Very wide orange-yellow and blue, ~2-3 delta mag. |
|
|
|
|
SHJ289 |
|
|
8m0 |
8m7 |
39.2'' |
56° |
2015 |
Lyr |
19h13m29.33s |
+39°02'15.90" |
Uwe Pilz
Leipzig (Germany) |
105mm (130x) |
einfach |
|
|
|
|
STF2487, eta Lyr, 20 Lyr, Aladfar |
|
AB |
4m4 |
8m6 |
28.4'' |
81° |
2017 |
Lyr |
19h13m45.49s |
+39°08'45.50" |
|
|
|
|
AC |
4m4 |
11m4 |
161.5'' |
151° |
2014 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 64x ein weit getrenntes Pärchen, Komponente B ist deutlich schwächer - zurück bis auf 20x, auch da ist B knapp getrennt östlich vom Hauptstern erkennbar - der starke Glow von A reicht nicht aus, um B zu überstrahlen - die Annäherung an diesen Doppelstern ist besser von höheren Vergrößerungen kommend |
|
|
|
|
STF2484 |
|
|
7m9 |
9m5 |
2.1'' |
242° |
2017 |
Sge |
19h14m15.66s |
+19°03'50.30" |
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
bis 142x probiert, keine Chance, Komponente B zeigt sich nicht |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close, ~2", orange, 1.5 delta mag. |
|
|
|
|
A98 |
|
AB |
6m7 |
11m0 |
22.5'' |
128° |
2015 |
Aql |
19h14m15.99s |
-08°43'08.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very faint but direct vision B is a point. Very wide. |
|
|
|
★★
|
STF2496 |
|
AB |
6m5 |
10m0 |
2.1'' |
81° |
2015 |
Cyg |
19h15m19.18s |
+50°04'16.00" |
|
|
|
|
AC |
6m5 |
11m2 |
186.1'' |
242° |
2003 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
AB: In steadier moments, the much fainter companion can be seen near the first diffraction ring of the primary component. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Very much fainter B, a pin prick when seeing stills. 3 delta mag, ~2" |
|
|
|
|
STTA178 |
|
|
5m7 |
7m6 |
89.6'' |
267° |
2018 |
Aql |
19h15m20.09s |
+15°05'01.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Wide finder split, yellowish A, ~1 delta mag. |
|
|
|
|
BRT1923 |
|
|
10m2 |
10m3 |
3.8'' |
187° |
2015 |
Lyr |
19h15m21.46s |
+43°21'31.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal white, ~4". Not physical |
|
|
|
★
|
STT371 |
|
AB |
7m0 |
7m5 |
0.9'' |
161° |
2018 |
Lyr |
19h15m56.96s |
+27°27'21.40" |
|
|
|
|
AB-C |
7m0 |
9m8 |
47.2'' |
269° |
2019 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB-C: bei 20x ist Komponente C im Westen schwach erkennbar in einem ordentlichen Abstand zu Komponente AB |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
2021-08-20: At 28x the much fainter C component is clearly visible at quite a large separation. The tight pair AB showed up at 160x and 187x clearly elongated, partially as an '8'. A small difference in brightness could be guessed. Higher magnifications did not yield any gain. The air was only moderately steady (seeing 3/5). |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Bright pair showed best masked down to 8-inches. Near equal, white stars, perfect! |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: getrennt |
|
|
|
|
STT368 |
|
AB |
7m5 |
8m5 |
1.1'' |
219° |
2017 |
Aql |
19h16m01.84s |
+16°09'39.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Very fine 1 delta mag, ~1" split, white. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Definite split, 1/2 an airy disk width, near equal brightness. |
|
|
|
|
STF2491 |
|
|
8m6 |
9m7 |
1.4'' |
230° |
2016 |
Lyr |
19h16m11.63s |
+28°16'50.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
A is white, B is slightly bluish, ~1.5 delta mag, ~1" |
|
|
|
|
STF2489 |
|
AB |
5m7 |
9m3 |
8.3'' |
347° |
2013 |
Aql |
19h16m26.78s |
+14°32'40.60" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ist Komponente B gut getrennt nördlich von A zu erkennen - der Helligkeitsunterschied zu ist A enorm, bestimmt mehr als 3 Größenklassen, deshalb wirkt B nicht wie ein Lichtpunkt, sondern eher wie ein bräunlicher kleiner Fleck |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright white and considerably fainter B. B rose up to view with averted vision, but was able to hold direct. ~5" |
|
|
|
|
BU140 |
|
AB |
6m9 |
11m7 |
49.0'' |
307° |
2015 |
Aql |
19h16m52.12s |
-10°58'18.50" |
|
|
|
|
BC |
10m4 |
10m6 |
7.9'' |
213° |
2018 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Two faint stars in about the same PA. 3 delta mag. to the A star, AB is the closer pair |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
BC: Two faint stars in about the same PA. 3 delta mag. to the A star, BC is the two fainter stars as a binary |
|
|
|
|
CSN12 |
|
AN |
4m7 |
5m8 |
9.1'' |
285° |
2000 |
Aql |
19h16m55.23s |
+05°10'07.10" |
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
2019-07-03: Absolutely no star with the given magnitude visible at this position. An error in the WDS or is this a variable one? |
|
|
|
|
STT370, V342 Aql |
|
AB |
8m3 |
8m7 |
19.5'' |
14° |
2015 |
Aql |
19h17m03.16s |
+09°20'19.60" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ist Komponente B nordöstlich nur unwesentlich schwächer - schönes Farbenspiel, Komponente A mit einem Stich ins kupferfarbene, Komponente B dagegen blass-orange |
|
|
|
|
A267 |
|
AB |
10m0 |
10m4 |
0.4'' |
181° |
2007 |
Lyr |
19h17m31.08s |
+26°37'33.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
White stars hairline split, ~1 delta mag. Notched elongation at 533x. |
|
|
|
★★
|
S715 |
|
|
7m1 |
7m9 |
8.4'' |
17° |
2018 |
Sgr |
19h17m39.96s |
-15°58'01.70" |
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x auffällig, ein schönes enges, knapp getrenntes Paar - B im NW ist eine halbe Größenklasse schwächer -ein schönes Doppel-Doppel zusammen mit dem nur 6' östlich stehenden S 716 |
|
|
|
|
BU248, 2 Vul |
|
AB |
5m4 |
8m8 |
1.8'' |
128° |
2015 |
Vul |
19h17m43.64s |
+23°01'32.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
2 Vul. White A and light blue B, split outside first diffraction ~1.5" really pretty. Burnham discovered in 1876 with his 6-inch at 1.86", "a fine pair with a moderate aperture" |
|
|
|
★★
|
S716 |
|
|
8m4 |
8m6 |
5.0'' |
196° |
2018 |
Sgr |
19h18m05.55s |
-15°57'13.40" |
René Merting
Drachhausen (Germany) |
76mm (57x) |
bei 29x sind beide Komponenten zu erkennen, können aber noch nicht getrennt werden - bei 57x dann gelingt die Trennung - ein deutlich schwächeres Par als das unmittelbar westlich stehende Sternpaar S 715, beide zusammen bilden aber ein schönes Doppel-Doppel - sie tanzen sogar synchron, wenn auch der Positionswinkel um 180° gedreht ist |
|
|
|
|
HJ881 |
|
AB |
7m8 |
9m8 |
32.0'' |
340° |
2015 |
Aql |
19h18m07.10s |
-05°25'24.50" |
|
|
|
|
BC |
9m8 |
10m5 |
7.4'' |
307° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: Komponente B wird mit etwas Geduld ganz schwach nordwestlich von A sichtbar - Helligkeitsunterschied 2 Größenklassen - Trennung ordentlich |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ist die Komponente B gut abgesetzt im Norden von A erkennbar - sehr unauffällig - auf Komponente C gut 7" weiter nordwestlich von B habe ich leider nicht geachtet |
|
|
|
|
COU322 |
|
|
10m4 |
10m5 |
0.5'' |
25° |
2008 |
Vul |
19h18m11.69s |
+22°31'06.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Near equal white stars, nice, split more than hairline, slight delta mag. |
|
|
|
|
STF2492, 23 Aql |
|
AB |
5m3 |
8m3 |
3.2'' |
2° |
2011 |
Aql |
19h18m32.49s |
+01°05'06.30" |
|
|
|
|
AC |
5m3 |
13m5 |
10.1'' |
70° |
1999 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
AB: bei 107x klebt B noch an A und schimmert im Beugungsscheibchen von A - bei 142x ist B in guten Momenten ganz knapp getrennt erkennbar und kämpft gegen das erste Beugungsscheibchen von A an - Helligkeitsunterschied geschätzt 3 Größenklassen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 23 Aql. well split, a large difference in magnitudes. A bright orange, B bluish. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: Faint star much further out was the AC, 13th mag ~10". |
|
|
|
|
STF2499 |
|
|
8m8 |
9m1 |
2.6'' |
325° |
2018 |
Vul |
19h18m33.52s |
+21°56'51.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White stars, near equal, wide |
|
|
|
|
HO575 |
|
|
8m0 |
11m7 |
5.8'' |
10° |
2015 |
Aql |
19h18m47.20s |
-05°46'20.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Best star images using 20" and 333x of 6" separated pair with 4 detla mag. I also tried a variety of combinations for this one: 8" 205x, Light orange star, no double seen. 8" 410x: no double seen. 8" 667x: Still none -- A is steady & round. 20" 667x: Light orange A messy by airy disk is there, the B star reveals itself, 6" and a hazy blue color. 20" 410x: Disks are smaller, B more clearly resolved. 20" 333x: Best star images. Observation made during poor transparency |
|
|
|
|
STFA40, 24 Aql |
|
AB |
6m5 |
6m8 |
423.5'' |
316° |
2015 |
Aql |
19h18m50.94s |
+00°20'20.40" |
|
|
|
|
AC |
6m5 |
13m2 |
49.5'' |
163° |
2015 |
|
|
|
|
|
|
|
BD |
6m8 |
11m6 |
60.4'' |
298° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: 24 Aql ist eigentlich eine FG-Empfehlung … nein, nicht wirklich schön - der Abstand zwischen den beiden Sternen ist soooo groß, die machen keinen Eindruck auf mich als Sternpaar - B im Nordwesten ist knapp schwächer - einen Farbunterschied kann ich nicht erkennen |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: eine Empfehlung aus dem Buch von Sissi Haas - ich kann diesem Paar nicht wirklich etwas abgewinnen, der Abstand ist einfach zu groß - es gibt noch einige ähnlich helle Sterne im Umfeld - B im NW ist unmerklich schwächer - A samtgelb, B weiß, dadurch leichter Farbkontrast |
|
|
|
|
ES1562 |
|
AB |
9m4 |
9m8 |
6.2'' |
325° |
2016 |
Lyr |
19h19m16.98s |
+42°17'02.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Easy wide ~6", ~1 delta |
|
|
|
|
S717, 28 Aql |
|
AB |
5m5 |
9m0 |
60.7'' |
175° |
2015 |
Aql |
19h19m39.34s |
+12°22'28.80" |
|
|
|
|
AC |
5m5 |
13m3 |
73.6'' |
107° |
2015 |
|
|
|
|
|
|
|
BC |
9m0 |
13m3 |
75.9'' |
59° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: die B-Komponente ist schwach schimmernd weit abgesetzt im Süden von A erkennbar - mindestens 3 Größenklassen Helligkeitsunterschied -A ist reinweiß, bei B bin ich froh, den Stern erkennen zu können |
|
|
|
★
|
STF2505 |
|
AB |
8m3 |
9m5 |
10.9'' |
315° |
2015 |
Lyr |
19h19m52.83s |
+35°32'16.60" |
|
|
|
|
AC |
8m3 |
13m3 |
20.8'' |
224° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x gut getrenntes Pärchen - Komponente B ist nur leicht schwächer als A - Komponente A ist nicht ganz weiß, mehr wie ein zarter Stich ins gelbliche |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Orange and blue, looks like Alberio, but fainter. Wide separation. |
|
|
|
★
|
STF2497 |
|
|
7m7 |
8m5 |
29.3'' |
356° |
2019 |
Aql |
19h20m01.09s |
+05°35'15.70" |
René Merting
Drachhausen (Germany) |
10x50 |
ein wenig Geduld war notwendig, aber dann zeigte sich Komponente B leicht abgesetzt nördlich von A - geringer Helligkeitsunterschied |
|
René Merting
Drachhausen (Germany) |
18x70 |
bei 18x ein ausgesprochen schickes Sternpaar - B zeigt sich nördlich von A gut getrennt, aber trotzdem noch eng seinem Partner stehend - Helligkeitsunterschied eine Dreiviertel Größenklasse - sonst gibt es kaum vergleichbare Sterne im Umfeld, so dass sich das Sternpaar schön prominent präsentieren kann |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x einfach trennbar, auffällig - das Sternpaar steht schön isoliert - B im Norden ist eine dreiviertel Größenklasse schwächer und grau, A dagegen ist strahlend weiß - zurück auf 20x ist der Doppelstern auch noch gut getrennt mit eingängigerem Farbkontrast |
|
Sarah Gebauer
Germany |
100mm (45x) |
auf der Suche nach dem PN NGC 6781 zufällig entdeckt, steht recht isoliert im 1,8° großen Gf. und ist bei 45x sehr deutlich getrennt, zwei feine Pünktchen beieinander |
|
|
|
|
STF2494 |
|
|
7m0 |
10m4 |
25.7'' |
89° |
2006 |
Aql |
19h20m02.80s |
-06°37'40.80" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x steht B gut abgesetzt östlich von der Hauptkomponente - B ist sehr schwach, bestimmt 3 Magnituden Helligkeitsunterschied |
|
|
|
|
STTA181 |
|
AB |
7m4 |
7m5 |
62.7'' |
0° |
2018 |
Lyr |
19h20m07.47s |
+26°38'41.60" |
|
|
|
|
AC |
7m4 |
12m8 |
31.6'' |
170° |
2018 |
|
|
|
|
|
|
|
BD |
7m5 |
12m1 |
94.0'' |
43° |
2018 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (22x) |
AB: 2020-06-24: Widely separated, small difference in brightness and beautiful color contrast: subtle orange and white-bluish. |
|
|
|
|
ES2489, U Lyr |
|
AB |
10m2 |
13m0 |
10.4'' |
190° |
2015 |
Lyr |
19h20m09.15s |
+37°52'36.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint A and very faint B, wide pair. Needed averted to detect, then could hold direct vision. |
|
|
|
★
|
COU1023 |
|
|
9m5 |
9m5 |
0.3'' |
146° |
2007 |
Lyr |
19h20m23.74s |
+26°30'58.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Hairline split, very definite and consistent, near equal |
|
|
|
|
STF2511 |
|
AB |
7m5 |
11m1 |
7.2'' |
53° |
2015 |
Cyg |
19h20m31.45s |
+50°20'24.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange and very much fainter star could be B, wide separation, 3 delta mag, ~10" |
|
|
|
|
STF2504 & WAL111 |
STF2504 |
AB |
7m0 |
9m0 |
8.6'' |
282° |
2015 |
Sge |
19h20m59.85s |
+19°08'43.40" |
|
|
|
WAL111 |
AC |
7m0 |
12m2 |
91.8'' |
101° |
2015 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
STF2504 (AB): Yellow and slight orange, 1.5 delta mag, well separated. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF2504 (AB): Yellow and slightly red, 2 delta mag, 10". Third star opposite PA, 2x the separation. (AB the first, second is AC, WAL 111) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
WAL111 (AC): Yellow and slightly red, 2 delta mag, 10". Third star opposite PA, 2x the separation. (AB the first, second is AC, WAL 111) |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
STF2504 (AB): easy DS |
|
|
|
|
ES483, Z Vul |
|
|
7m3 |
12m0 |
13.8'' |
3° |
2015 |
Vul |
19h21m39.11s |
+25°34'29.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Z Vul. Pale yellow A with slightly red color wide faint companion. Not physical |
|
|
|
|
BU141 |
|
AB |
7m6 |
9m2 |
0.9'' |
84° |
2015 |
Vul |
19h21m57.26s |
+22°30'23.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Very finely split, ~2 delta mag, pale white A and light blue B. Burnham discovered in 1875 with his 6-inch |
|
|
|
|
STF2501 |
|
AB |
7m8 |
9m7 |
20.0'' |
21° |
2015 |
Aql |
19h22m03.68s |
-04°44'20.00" |
René Merting
Drachhausen (Germany) |
18x70 |
puh, da habe ich lange gebraucht, bis ich B entdeckt habe - ich habe immer gedacht, das ist eine Unschärfe von A - B steht extrem knapp getrennt nördlich von A und ist deutlich schwächer |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x gut getrenntes Pärchen, Komponente A nördlich strahlt weiß, B nördlich strahlt … schwächer |
|
|
|
★
|
TDT1416 |
|
|
10m5 |
11m1 |
0.7'' |
298° |
1991 |
Vul |
19h23m28.49s |
+22°34'19.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Exceptionally fine, split with seeing, very faint ~1 delta mag. B resolves at first diffraction, light orange stars |
|
|
|
|
2 Sge |
HDS2753 |
Aa-Ab |
6m3 |
10m3 |
0.4'' |
138° |
2002 |
Sge |
19h24m22.08s |
+16°56'15.90" |
|
|
|
STFA41 |
AB |
6m3 |
6m9 |
342.3'' |
78° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: ein extrem weites Pärchen - B im Osten wirkt leicht gelblich, A ist reinweiß - Größenklassenunterschied maximal eine halbe Größenklasse - beide Sterne sind die hellsten im Sternumfeld, aber der weite Abstand vermindert den Doppelsterneindruck |
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Aa-Ab: Component of STFA 41. Snowman at all powers through 1067x, but it should really separate if 0.4" as WDS says. Seeing is not up to the task, or the delta mag is too large |
|
|
|
|
STF2515 |
|
AB |
8m4 |
10m3 |
6.2'' |
141° |
2015 |
Vul |
19h24m33.33s |
+21°30'57.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A and ~2 delta light orange B, wide. Not physical |
|
|
|
|
HO448 |
|
|
8m5 |
10m7 |
7.7'' |
0° |
2015 |
Vul |
19h24m44.82s |
+23°36'56.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Light yellow stars, ~3 delta mag, wide |
|
|
|
|
WSI22 |
|
|
10m3 |
10m5 |
15.0'' |
272° |
2015 |
Vul |
19h24m53.90s |
+21°26'29.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal, wide. Not physical |
|
|
|
|
HU339 |
|
|
9m4 |
9m5 |
0.9'' |
246° |
2016 |
Sge |
19h25m03.35s |
+18°38'59.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Detected elongation 8" 333x, but needed 667x to get better a sighting, and 20" to get a wide open split even with indifferent seeing. White stars, about half delta mag. Aperture is king. |
|
|
|
|
STF3111 |
|
|
9m9 |
10m2 |
2.5'' |
116° |
2015 |
Vul |
19h25m06.44s |
+21°50'03.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White stars, very slight magnitude difference, wide >2". Not physical |
|
|
|
|
COU513 |
|
|
9m2 |
9m9 |
0.3'' |
3° |
2009 |
Vul |
19h25m08.84s |
+22°12'56.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Deeply notched overlapping disks -- I think it's hairline split at best moments -- slight mag difference |
|
|
|
|
HJ2871, 4 Vul |
|
AB |
5m2 |
10m0 |
13.5'' |
87° |
2016 |
Vul |
19h25m28.54s |
+19°47'54.70" |
|
|
|
|
AC |
5m2 |
11m7 |
50.9'' |
212° |
2016 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: 4 Vul. Light orange and very faint star near, with another 2x fainter and farther away, noticed with AV only. (AB is first & AC second) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AC: 4 Vul. Light orange and very faint star near, with another 2x fainter and farther away, noticed with AV only. (AB is first & AC second) |
|
|
|
|
BOW7 |
|
|
10m4 |
11m0 |
9.6'' |
251° |
2018 |
Sge |
19h26m25.50s |
+18°38'38.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Unremarkable wide pair, half delta mag. |
|
|
|
|
BOW6 |
|
|
10m8 |
12m5 |
7.2'' |
309° |
2015 |
Sge |
19h26m32.98s |
+18°37'14.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Nothing special, ~1 delta mag wide. Not physical. W.M. Bowyer |
|
|
|
|
STF2525 |
|
AB |
8m2 |
8m4 |
2.1'' |
289° |
2018 |
Vul |
19h26m33.71s |
+27°19'21.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (100x) |
2020-06-24: At 49x slightly elongated, at 69x just separated with visible difference in brightness. At 100x nice view with clear separation and slight difference in brightness, but no visible colors. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal yellow-white stars, wide. An amazingly precise 882.894 year period. I will not notice the change |
|
|
|
|
STF2524 |
|
AB |
9m2 |
9m5 |
5.4'' |
82° |
2018 |
Vul |
19h26m35.78s |
+25°29'48.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal white stars, wide. Not physical |
|
|
|
|
STF2523 |
|
AB |
8m0 |
8m1 |
6.3'' |
148° |
2019 |
Vul |
19h26m48.38s |
+21°09'46.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Near equal white, well separated. Near the Coat Hanger, which I viewed through the finder. |
|
|
|
★★
|
A2786 |
|
|
10m1 |
10m1 |
0.4'' |
108° |
2008 |
Vul |
19h26m57.67s |
+21°09'02.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Wow! Exceptionally fine but clean split, ~1 delta split, best without apodising mask, nearly perfect seeing. In the same FOV as STF 2523. |
|
|
|
|
A159 |
|
AB |
8m5 |
10m4 |
0.8'' |
336° |
2017 |
Vul |
19h27m20.85s |
+20°40'08.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Super difficult. B appears just within A's diffraction ring, extremely faint, with seeing which is 7/10. Coalesces to a point at the correct PA, which I looked up during the observation to make sure I was looking at the correct quadrant of the star. Part of STF 2527 AC. |
|
|
|
|
COU514 |
|
|
9m8 |
9m3 |
0.5'' |
88° |
2007 |
Vul |
19h27m33.15s |
+20°09'17.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Subtle notched elongation, white stars, noticeable magnitude difference. |
|
|
|
|
STF2534 |
|
|
8m2 |
8m4 |
6.9'' |
63° |
2019 |
Cyg |
19h27m40.63s |
+36°31'44.40" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x zwei annähernd gleichhelle Sterne, ganz knapp getrennt - bei 64x passen 2-3 Blatt Papier mehr zwischen die beiden Sterne - Komponente A mit einem etwas kühleren weiß als B |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Near equal white, 7-8" |
|
|
|
|
STF2529 |
|
|
8m6 |
10m2 |
6.7'' |
298° |
2018 |
Sge |
19h28m04.99s |
+17°38'54.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Dull yellow-white A and deeper orange yellow b, two delta, wide. Not physical |
|
|
|
★★
|
STF3132 |
|
AB |
10m1 |
11m8 |
8.0'' |
39° |
2018 |
Vul |
19h28m12.76s |
+20°12'59.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal orange stars with hairline split April 2019 |
|
|
|
|
STF2519 |
|
|
8m3 |
8m5 |
12.0'' |
124° |
2018 |
Aql |
19h28m12.93s |
-09°32'15.90" |
René Merting
Drachhausen (Germany) |
18x70 |
ein genauer Blick ist nötig, aber dann sind beide Komponenten schön voneinander getrennt zu erkennen - beide sind recht schwach und ohne Helligkeitsunterschied |
|
René Merting
Drachhausen (Germany) |
76mm (18x) |
bei 29x ein schön anzusehendes, ordentlich getrenntes Pärchen zweier gleich heller Sterne - 18x reichen ebenfalls noch für eine knappe Trennung |
|
|
|
|
HU340 |
|
|
9m8 |
10m3 |
0.9'' |
120° |
2016 |
Sge |
19h28m21.65s |
+18°29'04.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very finely split even at 205x, noticeable magnitude difference, slightly orange stars |
|
|
|
|
STF2531 |
|
AC |
8m1 |
10m2 |
31.4'' |
28° |
2015 |
Aql |
19h29m30.07s |
+03°05'23.60" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein auffälligeres Pärchen als der unmittelbar südöstlich stehende DS STF2532 - Komponente B ist auch schwach, aber A ist nur 1.5 Größenklassen heller - B steht gut abgesetzt nördlich von A |
|
|
|
|
AG231 |
|
|
9m9 |
10m1 |
4.5'' |
239° |
2018 |
Sge |
19h29m34.45s |
+17°59'46.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Near equal pair, white, wide. Physical |
|
|
|
|
J137 |
|
|
9m7 |
12m0 |
4.5'' |
18° |
2015 |
Sge |
19h30m01.65s |
+18°25'55.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Faint B ~5", ~2 delta. Not physical |
|
|
|
|
STF2533 |
|
|
7m4 |
10m0 |
22.1'' |
212° |
2015 |
Aql |
19h30m04.70s |
-00°26'41.80" |
René Merting
Drachhausen (Germany) |
18x70 |
Komponente B ist ganz schwach knapp abgesetzt südwestlich von A zu erkennen - die Sichtung gelingt nur mit viel Konzentration |
|
|
|
|
STF2532 |
|
AB |
6m3 |
10m5 |
33.0'' |
2° |
2011 |
Aql |
19h30m10.53s |
+02°54'14.70" |
|
|
|
|
AC |
6m3 |
10m9 |
119.4'' |
197° |
2016 |
|
|
|
|
|
|
|
BC |
10m5 |
10m9 |
151.3'' |
194° |
2014 |
|
|
|
|
|
|
|
BD |
10m5 |
13m1 |
33.6'' |
133° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x zeigt sich B gut abgesetzt nördlich von der schönen samtgelben A-Komponente - das Paar fällt nicht als Doppelstern auf, weil B zu schwach ist |
|
|
|
★★★
|
beta Cyg, 6 Cyg, Albireo, STFA43 |
|
AB |
3m2 |
4m7 |
35.2'' |
54° |
2019 |
Cyg |
19h30m43.29s |
+27°57'34.90" |
Robert Zebahl
Leipzig (Germany) |
8x40 |
Well split, but I didn't recognised any color. |
|
René Merting
Drachhausen (Germany) |
10x50 |
Komponente A ist gleißend hell und stroh-gelb, Komponente B ist deutlich schwächer leicht abgesetzt von A erkennbar und strahlt eigenartig mint-grün |
|
Christopher Hay
Seeheim (Germany) |
12x36 |
Well split. A golden-red, B cold blue. Gorgeous! |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-06: Bright orange & white-bluish. |
|
Robert Zebahl
Leipzig (Germany) |
80mm (25x) |
One of the most beautiful double stars in the northern hemisphere. Differences in brightness and color (orange-blue) are brilliant! Even under urban conditions with small aperture an enjoyment! |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x stehen beide Sterne weit getrennt - Komponente A mit einem satten zitronen-gelb, Komponente B mit einem leichten Stich ins Blaue |
|
Jörg S. Schlimmer
Germany |
127mm (203x) |
easy to split |
|
Sarah Gebauer
Germany |
150mm (116x) |
Erstbeobachtung August 2019: deutlicher Farbunterschied zwischen blau und sattem Gelb zu sehen |
|
Jörg S. Schlimmer
Germany |
305mm (170x) |
alle Komponenten einfach zu trennen |
|
|
Werner E. Celnik
Rheinberg (Germany) |
150mm |
|
|
Werner E. Celnik
Rheinberg (Germany) |
150mm |
|
|
|
|
★
|
D20, V822 Aql |
|
AB |
7m2 |
9m6 |
1.3'' |
65° |
1991 |
Aql |
19h31m15.78s |
-02°06'36.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
A has a notched / trailing star in east PA, very close in and very much fainter. With seeing. Tough! |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
tight airy disk of A, and a faint star widely separated, 3 delta mag ~25" Very near to a pretty orange carbon star. |
|
|
|
|
STF2536 |
|
|
8m4 |
11m4 |
1.8'' |
120° |
2018 |
Sge |
19h31m37.80s |
+17°46'58.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A and much fainter ~3 delta B, split close, dull orange color. Very fine. Physical with 672.5 year period |
|
|
|
|
BU650 |
|
AB |
8m2 |
11m7 |
6.5'' |
146° |
2015 |
Aql |
19h32m13.13s |
+06°30'11.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very faint B, wide separation. |
|
|
|
|
HU946 |
|
|
8m2 |
9m9 |
8.7'' |
214° |
2015 |
Cyg |
19h32m22.44s |
+34°17'02.60" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 64x begonnen, Komponente B ist knapp getrennt südwestlich von A sichtbar und deutlich schwächer als A - zurück auf 32x kann man in guten Momenten beide Sterne auch schon getrennt voneinander sehen, wenn man B zu sehen bekommt (B blitzt hin und wieder hervor) |
|
|
|
|
STF2540 |
|
AB |
7m5 |
9m2 |
5.4'' |
145° |
2018 |
Vul |
19h33m17.05s |
+20°24'50.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow and blue, pretty wide 1.5 delta mag. |
|
|
|
|
BU653, 38 Aql |
|
AB |
4m6 |
13m1 |
56.2'' |
289° |
2008 |
Aql |
19h34m05.35s |
+07°22'44.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Orange star and very wide separated B. Other fainter stars nearby, likely part of the 5 other stars in the system |
|
|
|
|
GCB43 |
|
|
9m9 |
11m9 |
7.5'' |
264° |
2015 |
Sge |
19h34m18.03s |
+18°40'19.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very faint pair, ~2 delta B is on the edge of direct vision, wide ~5", probably not physical. M. Giacobini |
|
|
|
|
STT375 |
|
|
7m7 |
8m9 |
0.6'' |
189° |
2017 |
Sge |
19h34m37.45s |
+18°07'41.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Sense an elongation or rod, marginal. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Snowman at 205x, 333x, split with 533x, >1 delta mag, ~0.5". A is orange-yellow and B is blue-white. Physical with 682 year period, just coming apastron now. |
|
|
|
|
HO274 |
|
|
8m3 |
11m1 |
3.9'' |
71° |
2001 |
Sge |
19h34m55.37s |
+16°27'04.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
White A, B is quite faint but resolved, ~4", delicate looking. Not physical |
|
|
|
|
A2787 |
|
|
9m9 |
11m4 |
3.9'' |
111° |
2018 |
Vul |
19h35m47.31s |
+23°33'50.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Seen right away, 1 delta mag and about 4". Nice stars. [not physical] |
|
|
|
|
STF2548 |
|
|
8m5 |
9m8 |
9.4'' |
100° |
2018 |
Vul |
19h36m28.51s |
+25°00'04.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Obvious pair, 1.5 delta mag ~10" |
|
|
|
★★
|
A598 |
|
AB |
9m9 |
10m2 |
1.0'' |
191° |
2016 |
Cyg |
19h36m29.82s |
+41°24'08.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
UV Cyg. Orange-red with very much fainter blue ~1", 1 delta mag. Seeing must still. A a perfect round disk the color of the setting sun. Very special. |
|
|
|
|
STF2541 |
|
|
8m7 |
10m1 |
5.4'' |
327° |
2018 |
Aql |
19h36m45.65s |
-10°26'36.60" |
René Merting
Drachhausen (Germany) |
76mm (95x) |
A ist schon recht schwach, B ist noch schwächer und offenbart sich mir erst bei 95x, B steht nordwestlich von A und zeigt sich gut getrennt - schön ist trotzdem anders |
|
|
|
|
epsilon Sge, 4 Sge, H6 26 |
|
AB |
5m8 |
8m3 |
87.4'' |
82° |
2017 |
Sge |
19h37m17.38s |
+16°27'46.00" |
|
|
|
|
AC |
5m8 |
13m2 |
100.7'' |
278° |
2013 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: ein komfortabel getrenntes, gut sichtbares Pärchen - A im Westen ist weiß, B ist zwei Größenklassen schwächer und grauweiß |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x weit getrennt - Komponente A mit einem satten zitronengelb, B im Osten graubläulich - bei 20x ähnlicher Eindruck, bei B verliert sich der Farbeindruck |
|
|
|
|
STF2551 |
|
AB |
9m7 |
10m5 |
6.8'' |
42° |
2018 |
Vul |
19h37m23.23s |
+22°48'51.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Half delta mag, about 7", may be part of triple with very wide 1 more magnitude fainter C about 60 degrees away from B. |
|
|
|
|
BU144 |
|
|
9m5 |
9m6 |
6.0'' |
356° |
2015 |
Cyg |
19h37m47.09s |
+30°21'18.60" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Clean star images, equal pair, wide, very pretty, in a dense field. Great view |
|
|
|
|
HJ1428 |
|
AB |
6m6 |
10m2 |
35.5'' |
232° |
2015 |
Cyg |
19h37m56.71s |
+49°17'03.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Interesting string of 6 stars, with 7th at right angle from the central bright star in the string, which is orange. |
|
|
|
|
MLB765 |
|
CD |
10m0 |
11m5 |
6.5'' |
237° |
2015 |
Cyg |
19h38m08.56s |
+29°12'40.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice one delta mag pair, wide, very pretty |
|
|
|
|
BU249 |
|
AB |
7m4 |
9m4 |
0.8'' |
109° |
2008 |
Aql |
19h38m21.68s |
+00°20'43.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Some brightening in diffraction, but cannot claim success |
|
|
|
|
BU1471 |
|
AB |
7m5 |
11m9 |
12.5'' |
333° |
2017 |
Sge |
19h38m27.48s |
+17°15'26.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very faint B, needed averted vision to notice it, can just hold it direct. Wide 10-12", 3 delta mag, orange A. |
|
|
|
|
COU1162 |
|
Aa-Ab |
9m8 |
9m9 |
0.8'' |
128° |
2007 |
Cyg |
19h38m37.18s |
+29°52'53.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Fine snowman at 333x but needed 667x to split, very close pair. SLE 654 AB noticed as a very faint star about 15" out and a few degrees difference in PA |
|
|
|
|
STF2545 |
|
AB |
6m8 |
8m5 |
3.9'' |
325° |
2016 |
Aql |
19h38m43.36s |
-10°09'23.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Easy, wide separation yellow and orange. |
|
|
|
|
STF2547 |
|
AB |
8m1 |
9m5 |
20.8'' |
330° |
2015 |
Aql |
19h38m56.50s |
-10°20'20.60" |
|
|
|
|
AC |
8m1 |
11m1 |
49.6'' |
141° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: Komponente A ist schon schwach, B noch schwächer und steht relativ knapp abgesetzt nordwestlich von A - Helligkeitsunterschied schwer abschätzbar, vielleicht eine halbe Magnitude |
|
René Merting
Drachhausen (Germany) |
76mm (57x) |
AB: bei 29x ist B im NW von A leicht abgesetzt erkennbar, B ist auch bei 18x getrennt von A erkennbar und etwas mehr als eine Größenklasse schwächer
AC: erst bei 57x ist C ganz schwach südöstlich von A erkennbar - C ist nochmal deutlich schwächer als B und der Abstand AC dürfte etwas mehr als das Doppelte von AB sein |
|
|
|
★
|
S722 |
|
AB |
7m2 |
7m5 |
10.3'' |
236° |
2016 |
Sgr |
19h39m12.97s |
-16°54'28.30" |
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x wunderschön, zwei gleich helle Sterne ganz dicht aneinander geschmiegt bzw. knapp getrennt - wenn ich mich entscheiden müsste, welcher Stern schwächer ist, dann vermutlich die südwestliche Komponente - zurück auf 18x erscheinen beide Komponenten wie eine 8 kurz vor der Trennung |
|
|
|
|
SEI654 |
|
AB |
9m3 |
10m7 |
14.8'' |
115° |
2015 |
Cyg |
19h39m20.06s |
+31°52'19.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Wide one delta mag. pair |
|
|
|
|
SLE659 |
|
AB |
11m0 |
12m5 |
8.4'' |
107° |
2015 |
Cyg |
19h39m23.17s |
+30°29'09.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Faint and wide pair, B star quite faint at edge of direct vision |
|
|
|
★★★
|
HN 84, V340 Sge |
|
|
6m4 |
9m5 |
28.4'' |
301° |
2013 |
Sge |
19h39m25.33s |
+16°34'16.00" |
René Merting
Drachhausen (Germany) |
12x50 |
verdammt schwer - Komponente B ist ganz schwach nordwestlich von A auszumachen - beide Sterne berühren sich noch |
|
René Merting
Drachhausen (Germany) |
16x70 |
beide Sterne präsentieren sich gut getrennt, nicht zu weit aber auch nicht zu nah - Komponente A meint es gut mit der Farbe gelb, bei Komponente B kann ich keine Farbe erkennen |
|
Christopher Hay
Seeheim (Germany) |
80mm (30x) |
Primary ruddy red, secondary wide apart but too faint for any colour impression. Straw-yellow Epsilon Saggitae half a degree to the west with its ice-blue eastern companion enhances the experience of colour contrast in the FOV and is actually more attractive than HN 84 with this aperture and power. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x sind beide Komponenten weit getrennt - Komponente A auffällig gelb-orange, B dagegen grau-blau, ein schöner Farbkontrast, der sich bei 32x verstärkt |
|
Sarah Gebauer
Germany |
150mm (85x) |
Holden 84, eine sehr goldgelbe Komponente und in 28'' Abstand die zweite, sehr schwache und weiße Komponente mit einem Hauch von Blau, sehr, sehr schön! |
|
Christopher Hay
Seeheim (Germany) |
150mm (96x) |
Main component ruddy tangerine orange, companion wide apart and ice blue. The longer I look the stronger the colour contrast becomes, which is by no means normal in many doubles. Epsilon Saggitae in same 0.8-degree field of view is straw-yellow with a cold blue companion (a field star?) pointing away from Epsilon in the direction of HN 84. I can’t think offhand of a better colour-contrast pair that can be framed in this manner in the same FOV. |
|
Sarah Gebauer
Germany |
150mm (160x) |
die hellere Hauptkomponente ist deutlich und stark goldfarben, die zweite dagegen sehr schwach, silbrig und dumpf |
|
|
|
|
STF2557 |
|
AB |
7m5 |
10m2 |
11.0'' |
103° |
2015 |
Cyg |
19h39m35.20s |
+29°44'55.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
The closest to the 7th mag star, among a constellation of possible pairings visible in the field |
|
|
|
|
BRT198 |
|
|
10m2 |
11m6 |
5.1'' |
154° |
2015 |
Vul |
19h40m06.65s |
+25°15'33.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice picked out if field between two other stars, middle of a string. B can be seen direct but best with some indirect vision. 1.5 delta mag, wide sept about 3" |
|
|
|
|
J776 |
|
AB |
11m1 |
11m6 |
3.5'' |
47° |
2015 |
Cyg |
19h40m08.45s |
+30°35'50.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Faint pair, one is about half a delta mag, the other flashes with averted vision and can hold direct once found. [not physical] |
|
|
|
★
|
A272 |
|
AB |
9m8 |
10m4 |
1.3'' |
193° |
2009 |
Vul |
19h40m09.48s |
+26°11'23.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Wow, I get the split, very close but split, obvious difference in magnitude, about 1 delta mag. Less than 1" sep. Impressed i could get it [CD is 15th mag and 1"!] |
|
|
|
|
A166 |
|
|
9m2 |
9m5 |
0.9'' |
241° |
2016 |
Vul |
19h40m10.51s |
+23°30'43.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Close pair, 1/2 delta mag, elongates and splits with seeing. nice at this magnification. |
|
|
|
|
A2788 |
|
|
9m8 |
10m9 |
1.3'' |
328° |
2015 |
Vul |
19h40m19.26s |
+22°50'11.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Elongated is the best I can get |
|
|
|
|
54 Sgr, HJ599 |
|
AC |
5m4 |
7m7 |
45.5'' |
41° |
2019 |
Sgr |
19h40m43.34s |
-16°17'35.30" |
René Merting
Drachhausen (Germany) |
10x50 |
Komponente C sitzt nordöstlich von A, beide sind einfach zu trennen - großer Helligkeitsunterschied, schwer abschätzbar |
|
René Merting
Drachhausen (Germany) |
76mm (18x) |
bei 29x zeigen sich beide Komponenten in komfortablem Abstand zueinander - C ist gut 2 Größenklassen schwächer - bei 18x sind beide auch gut zu trennen, C hat immernoch ordentlich Abstand zu A - bei 57x habe ich mal nach den Farben geschaut, A stahlt warmweiß bzw. licht gelblich, C ist grau |
|
|
|
|
BLL41, TT Cyg |
|
AB |
7m9 |
12m3 |
70.3'' |
211° |
2015 |
Cyg |
19h40m57.00s |
+32°37'05.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
B very wide, very faint from A. A is orange, B also a little orangish. |
|
|
|
★★
|
STFA46, 16 Cyg |
|
AB |
6m0 |
6m2 |
39.5'' |
132° |
2019 |
Cyg |
19h41m49.09s |
+50°31'31.60" |
Christopher Hay
Seeheim (Germany) |
3x63 |
Self-built binoculars, hence the unusual specification. Made of top-quality teleconverters, apochromatic and sharp to the edge.
With naked eye under good suburban sky 16 Cyg is just seen. In the 3x binoculars the double is split into two finest points of light in good moments despite the low magnification. A physical pair according to Stelledoppie.
Two-star rating awarded because this is a true physical pair that can be split with the smallest binoculars and reveals increasingly more with growing binocular size (brightness disctinction between A and B in 7x50, colour distinction in 15x45). |
|
Christopher Hay
Seeheim (Germany) |
7x50 |
Finely split, A-component appears very slightly brighter than B-component. A very pleasing binocular pair. |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
Wide split, very strong visual presence dominating 4.5° FOV. A-component very pale orange, B-component equally pale blue. |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2021-06-01: Very striking, bright at moderate separation and small difference in brightness. White-yellowish & white. |
|
René Merting
Drachhausen (Germany) |
18x70 |
zwei ordentlich getrennte fast gleich helle Sterne - beide Komponenten sind reinweiß und die hellsten Sterne im unmittelbaren Umfeld - auffällig |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
16 Cyg: Wide equal orange-yellow, also split in 80mm finder |
|
|
|
|
KUI94 |
|
|
6m5 |
7m8 |
0.5'' |
158° |
2014 |
Cyg |
19h41m57.63s |
+40°15'14.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
unsicher, 8förmig |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
STT380, chi Aql |
|
AB |
5m4 |
6m6 |
0.4'' |
76° |
2009 |
Aql |
19h42m34.01s |
+11°49'35.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Diffraction a bit messy but I so see olive shaped "disk" |
|
|
|
|
STF2562 |
|
AB |
7m0 |
8m7 |
27.2'' |
251° |
2019 |
Aql |
19h42m45.86s |
+08°22'57.50" |
|
|
|
|
AC |
7m0 |
12m1 |
82.0'' |
289° |
2015 |
|
|
|
|
|
|
|
AD |
7m0 |
9m9 |
117.2'' |
222° |
2015 |
|
|
|
|
|
|
|
BC |
8m7 |
12m1 |
62.7'' |
305° |
2015 |
|
|
|
|
|
|
|
BD |
8m7 |
9m9 |
94.6'' |
214° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x fällt das Paar sofort auf - Komponente A im Osten ist gut 2 Größenklassen heller als B - schöner Farbkontrast aufgrund des Helligkeitsunterschiedes, Komponente A strahlt weiß mit einem Stich ins orange, B ist grau - bei 20x ist die Trennung auch einfach
AD: bei 32x von A und B ausgehend ist das der nächste erkennbare Stern im Umfeld, er steht etwas weiter südwestlich und ist gut viermal soweit von A entfernt wie B - Komponente D wirkt noch gräulicher und transparenter als B - Komponente B dagegen wirkt schon wieder weiß im Vergleich zu D - bei 20x sind auch alle drei Sterne sichtbar |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
AB: bei 45x weit getrenntes Pärchen - Farbkontrast weiß-gelb/ orange |
|
|
|
|
STTA188 & STU11 |
STTA188 |
AB |
7m7 |
8m0 |
61.1'' |
121° |
2017 |
Cyg |
19h42m48.56s |
+37°41'12.50" |
|
|
|
STU11 |
AC |
7m7 |
8m1 |
146.0'' |
228° |
2013 |
|
|
|
|
|
|
STU11 |
AE |
7m7 |
11m4 |
101.4'' |
196° |
2015 |
|
|
|
|
|
|
STU11 |
AF |
7m7 |
12m3 |
46.2'' |
191° |
2015 |
|
|
|
|
|
|
STTA188 |
AG |
7m7 |
13m5 |
29.8'' |
120° |
2015 |
|
|
|
|
|
|
STU11 |
BD |
8m0 |
9m6 |
60.4'' |
173° |
2015 |
|
|
|
|
|
|
STTA188 |
BG |
8m0 |
13m5 |
30.8'' |
302° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STU11 (BD): bei 20x weit getrennt - Komponente D im Süden deutlich schwächer - viele weitere Sterne im unmittelbaren Umfeld |
|
|
|
|
STT383 |
|
AB |
7m0 |
8m3 |
0.8'' |
15° |
2014 |
Cyg |
19h42m56.26s |
+40°43'18.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
STT384 |
|
AB |
7m6 |
8m2 |
1.0'' |
196° |
2018 |
Cyg |
19h43m47.09s |
+38°19'20.50" |
|
|
|
|
AC |
7m6 |
9m8 |
59.4'' |
297° |
2015 |
|
|
|
|
|
|
|
AD |
7m6 |
10m8 |
116.0'' |
294° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AC: bei 20x weit getrenntes Pärchen - Komponente C ist deutlich schwächer als A |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: deutliches Paar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Nice near equal ~1", rest of field angular with stars (AB seen, AC and AD in the field.) |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
AB |
|
|
|
★★
|
BU658, PS Vul |
|
|
6m7 |
7m9 |
0.3'' |
284° |
1998 |
Vul |
19h43m55.97s |
+27°08'07.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty orange star, subtly out of round / pear shaped. In a large cluster-like group of stars, around 3 degrees angular size, V-shaped, pretty in the finder. If the stars were brighter it would be as famous as the M45. |
|
|
|
|
STF2567 |
|
AB |
7m9 |
10m0 |
17.7'' |
310° |
2015 |
Aql |
19h44m06.10s |
+12°22'21.10" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x braucht es für den schwachen Begleiter etwas Geduld, er ist dann aber gut abgesetzt erkennbar |
|
|
|
|
STF2569 |
|
|
8m4 |
9m1 |
2.2'' |
357° |
2019 |
Sge |
19h44m47.81s |
+16°48'55.10" |
René Merting
Drachhausen (Germany) |
100mm (142x) |
bei 107x ist mit etwas Geduld blickweise eine 8 erkennbar - bei 142x dann sehe ich in guten Momenten beide Komponenten ganz knapp getrennt - beide Sterne mit fast identischer Helligkeit, Komponente A im Süden ist nur ganz knapp heller - Grenzbeobachtung |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
One delta mag, 2", blue-white stars |
|
|
|
|
Winnecke 7, WNC7 |
|
|
10m6 |
11m2 |
95.1'' |
193° |
2015 |
Cyg |
19h44m48.15s |
+50°31'30.30" |
René Merting
Drachhausen (Germany) |
18x70 |
der Zentralstern von NGC 6826 und zugleich Komponente A von WNC 7 ist relativ einfach sichtbar - Komponente B zeigt sich ganz schwach südwestlich von A mit deutlichem Abstand |
|
|
|
|
WRH23, SU Cyg |
|
AE |
7m0 |
10m5 |
24.8'' |
289° |
2015 |
Cyg |
19h44m48.74s |
+29°15'52.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
SU Cyg: Orange in the finder, lighter in the scope. Wide separation, 3 delta mag. |
|
|
|
★
|
AGC10 & STF2570 |
AGC10 |
AB |
8m4 |
8m4 |
0.2'' |
140° |
2000 |
Aql |
19h44m56.78s |
+10°46'30.60" |
|
|
|
STF2570 |
AB-C |
7m6 |
9m8 |
4.3'' |
277° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
STF2570 (AB-C): beide Komponenten erscheinen bei 107x knapp getrennt - der Begleiter ist nur ganz schwach sichtbar, wie ein Geist |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
STF2570 (AB-C): (AB) orange, C red-orange, faint pair, close to gamma Aql |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
STF2570 (AB-C): Easily split, white A and much fainter ruddy B. Did not see AB, which is near equal mag. 0.2", which I could get with the 20-inch on a good night. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
STF2570 (AB-C): bei 72x knapp getrenntes Pärchen, Komponente AB im Osten weiß-gelblich, C deutlich schwächer |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AGC10 (AB): Wide split pair. I was trying for AB 0.2" which only suggested elongation, too marginal to claim success |
|
Mark McCarthy
Fremont (California/USA) |
508mm (410x) |
AGC10 (AB): I can sense olive shape, very tough. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (410x) |
STF2570 (AB-C): White and off white wide separated pair, ~1 delta mag. |
|
|
|
★
|
STF2579, delta Cyg, 18 Cyg |
|
AB |
2m9 |
6m3 |
2.7'' |
215° |
2017 |
Cyg |
19h44m58.44s |
+45°07'50.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (200x) |
At 100x only indicated. At 200x the much fainter companion is visible as a slightly elongated brightening on the first diffraction ring. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
blauweiß |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very bright white with ruddy B, ~4", 4 delta mag. Nice! |
|
|
|
|
STF2577 |
|
AB |
8m4 |
9m6 |
5.9'' |
262° |
2018 |
Vul |
19h45m12.27s |
+20°54'50.30" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x sehe ich nur einen kupferfarbener Stern - bei 64x taucht westlich von ihm ein schwacher Begleiter auf, beide sind gut getrennt - Komponente B passt farblich gut zu Komponente A, auch wenn ich nicht wirklich beschreiben kann, welchen Farbstich ich da sehe |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Wide, one and half delta mag, light orange and blue stars |
|
|
|
|
STF2578 |
|
AB |
6m4 |
7m0 |
14.9'' |
125° |
2019 |
Cyg |
19h45m39.65s |
+36°05'27.60" |
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
At 22x easy with visible brightness and color difference. The slight color difference is even better visible at 44x: A appears white-yellowish, B slightly bluish. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 20x knapp getrennt, bei 32x ein ordentlich getrenntes Pärchen - Komponente B im SO ist nur leicht schwächer und mit leichtem Farbkontrast, aber dieser ist nicht greifbar |
|
|
|
|
STT385 |
|
|
7m8 |
9m6 |
1.2'' |
51° |
2016 |
Cyg |
19h45m48.77s |
+40°33'18.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow disk with fine blue point, with seeing, 1-1.5" |
|
|
|
|
H5 137 |
|
AB |
6m2 |
8m2 |
38.8'' |
25° |
2019 |
Cyg |
19h45m51.35s |
+35°00'45.90" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x weit getrenntes Pärchen - bei 32x Komponente A gelblich, B ohne Färbung |
|
|
|
|
17 Cyg |
STF2580 |
AB |
5m1 |
9m2 |
26.1'' |
68° |
2015 |
Cyg |
19h46m25.60s |
+33°43'39.30" |
|
|
|
STF2580 |
AC |
5m1 |
9m4 |
107.9'' |
126° |
2013 |
|
|
|
|
|
|
WNO56 |
AF |
5m1 |
8m5 |
792.0'' |
235° |
2002 |
|
|
|
|
|
|
STF2580 |
BG |
9m2 |
8m6 |
817.6'' |
236° |
2010 |
|
|
|
|
|
|
STF2576 |
FG |
8m5 |
8m6 |
13.2'' |
155° |
2019 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x locker getrennt - Komponente A satt gelb, B wegen des großen Helligkeitsunterschiedes gräulich-bräunlich |
|
Robert Zebahl
Leipzig (Germany) |
152mm (92x) |
2021-07-24: At 30x the components A, B & C are easily visible, whereby A & B are still quite close together. The bright component A appears in a pale yellow. At 92x also the pair FG is separated easily and looks less belonging to the system because of the wide separation to the other components. All in all it is worth observing. |
|
Winfried Kräling
Marburg (Germany) |
152mm (175x) |
A, B & C |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: 17 Cyg: Yellow and slightly red, well separated, 1 delta mag. (This is an amazingly complex system with 11 stars in all sorts of combinations. Why not just call it an open cluster?) |
|
|
|
|
AG391 |
|
|
7m7 |
9m2 |
52.3'' |
297° |
2015 |
Aql |
19h47m56.98s |
+10°02'23.40" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x easy, ein weit auseinander stehendes Paar - Komponente A im Südosten ist zartgelb, B im Nordwesten wirkt kupfergrau - auffallend im Umfeld |
|
|
|
|
HDS2814 |
|
|
8m5 |
10m6 |
18.3'' |
139° |
2016 |
Sgr |
19h48m01.78s |
-14°34'02.70" |
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ein schickes Sternpaar - gut getrennt und doch eng zusammen stehend - B im Süden ist sehr schwach, bestimmt 2-2.5 Größenklassen schwächer - A strahlt reinweiß, B wirkt grau |
|
|
|
|
STT386 |
|
|
8m5 |
8m6 |
1.0'' |
71° |
2018 |
Cyg |
19h48m16.51s |
+37°09'37.50" |
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
Clearly visible as a double star with touching diffraction disks. Not difficult. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
trotz schwacher Komp. gut zu sehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tight near equal, nice, split with seeing, ~1" |
|
|
|
|
DOO11 |
|
|
10m0 |
10m9 |
2.8'' |
281° |
2015 |
Vul |
19h48m21.40s |
+24°52'56.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Pretty pair of blue stars, one delta mag, 3" sep. Very nice! [not physical] |
|
|
|
|
STF2584 |
|
|
9m1 |
9m2 |
2.0'' |
294° |
2016 |
Vul |
19h48m22.40s |
+22°11'56.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal, well split 2" |
|
|
|
|
STF2586 |
|
AB |
7m6 |
9m3 |
3.3'' |
227° |
2018 |
Vul |
19h48m34.30s |
+24°57'43.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
White and light blue, wide ~5", 1.5 delta mag |
|
|
|
★★
|
STF2583, pi Aql |
|
AB |
6m3 |
6m8 |
1.4'' |
105° |
2019 |
Aql |
19h48m42.05s |
+11°48'57.30" |
Stefan Loibl
Rosenheim (Germany) |
102mm (205x) |
not fully split, seen as constricted '8' |
|
Robert Zebahl
Leipzig (Germany) |
120mm (337x) |
At 100x elongated, at 200x seen as '8'. At 337x split in moments of good seeing, but still very tight. Overall the seeing was not so good. |
|
Sarah Gebauer
Germany |
150mm (160x) |
wieder ganz haarscharf getrennt, bildet ein großes, nettes Dreieck mit Feldsternen, gefällt mir wieder sehr gut! |
|
Sarah Gebauer
Germany |
150mm (170x) |
bei 170x ganz, ganz knapp getrennt, ein haarfeiner, schwarzer Trennstrich ist zu sehen, eine geniale Grenzbeobachtung! |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Pi Aql. Very pretty near equal light blue stars, cleanly separated |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Pi Aql. Pretty yellow-orange A and a little more than 1 delta mag pale blue B, ~1", yet neatly separated |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
Helligkeitsunterschied erkennbar |
|
|
|
|
KU123 |
|
|
9m4 |
11m0 |
21.6'' |
298° |
2015 |
Vul |
19h48m42.71s |
+25°48'28.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Wide pair, one delta mag, bluish color [not physical] |
|
|
|
★
|
STT387 |
|
|
7m1 |
7m9 |
0.4'' |
105° |
2018 |
Cyg |
19h48m43.81s |
+35°18'41.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
zeitweise als 8 zu sehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Red, very close pair? Seeing not supporting higher magnification. Marginal. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Overlapping disks, to a nearly hairline split with seeing. Half delta mag. |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
zeta Sge, 8 Sge |
AGC11 |
AB |
5m6 |
6m0 |
0.2'' |
182° |
2007 |
Sge |
19h48m58.65s |
+19°08'31.10" |
|
|
|
STF2585 |
AB-C |
5m0 |
9m0 |
8.3'' |
311° |
2016 |
|
|
|
|
|
|
STF2585 |
AB-D |
5m0 |
11m0 |
76.0'' |
246° |
2005 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
AB-C: bei 32x noch nichts erkennbar, bei 64x ploppt nordwestlich von Komponente AB ein ganz schwacher Begleiter (Komponente C) auf - gut getrennt die beiden |
|
Christopher Hay
Seeheim (Germany) |
150mm (96x) |
AB-C: Secondary nicely set off as a fine pinprick beside the much brighter primary. Secondary seems ice blue at first sight, but that impression fades the longer I look. Primary essentially colourless. Secondary not seen in 3-inch at 30x. Physical double according to Stelledoppie. |
|
Christopher Hay
Seeheim (Germany) |
150mm (300x) |
AB: Used a moment of unusually good seeing in July 2019 to find out whether anything can be done with the 6-inch on this super-tight pair. No prior PA knowledge. At 200x nothing happening. At 240x a northwest-southeast elongation. At 300x distinctly stretched. According to Stelledoppie a physical pair with a very short period of 23 years. Distance a little over 0.2“ from 2010 to 2020, shrinking to 0.03“ in 2026, reaching 0.2“ again around 2040. This is one of very few double stars whose complete orbit can be observed several times over in a human lifetime, be it only as a periodical elongation/contraction. The observability of the elongation in just 6 inches of aperture is aided greatly by the almost equal brightnesses of the components. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
AB-C: White and blue stars, wide three to four delta mag, clean image with 8" [Did not notice elongation is AB, 6.04 and 0.2"] |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB-C: Bright A and 3x fainter wide B. Did not see AB 0.2" |
|
|
|
|
STF2588 |
|
A-BC |
7m7 |
8m1 |
9.6'' |
159° |
2019 |
Cyg |
19h49m00.90s |
+44°22'45.10" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein schönes enges Paar nicht mehr ganz knapp getrennt - Komponente B ist nur gering schwächer - beide Sterne strahlen weiß um die Wette - zurück auf 20x ist eine 8 zu sehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal white, pretty wide separation. |
|
|
|
|
HJ603, 19 Cyg |
|
AB |
5m4 |
10m5 |
56.8'' |
115° |
2015 |
Cyg |
19h50m33.99s |
+38°43'20.70" |
|
|
|
|
AC |
5m4 |
12m6 |
96.6'' |
318° |
2015 |
|
|
|
|
|
|
|
AD |
5m4 |
11m9 |
163.8'' |
309° |
2014 |
|
|
|
|
|
|
|
BE |
10m5 |
13m5 |
20.8'' |
10° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x fällt A sofort als zartgelber Stern auf, B steht gut abgesetzt im SO, sehr schwach sichtbar - bei 64x wird A sattgelb, B ist grau und farblos |
|
|
|
|
HO275, 51 Aql |
|
|
5m4 |
13m6 |
26.4'' |
121° |
2015 |
Aql |
19h50m46.80s |
-10°45'48.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (410x) |
Seeing poor, A appeared as a fuzz ball, but could see a much fainter fuzz ball B start in A's haze ~20" separated to east. |
|
|
|
|
alpha Aql, 53 Aql, Atair, Altair |
STFB10 |
AB |
0m9 |
9m8 |
195.8'' |
286° |
2015 |
Aql |
19h50m46.99s |
+08°52'05.90" |
|
|
|
STFB10 |
AC |
0m9 |
10m3 |
186.4'' |
110° |
2015 |
|
|
|
|
|
|
DAL27 |
AD |
0m9 |
11m9 |
26.8'' |
105° |
2015 |
|
|
|
|
|
|
SMR5 |
AE |
0m9 |
11m0 |
151.3'' |
354° |
2015 |
|
|
|
|
|
|
SMR5 |
AF |
0m9 |
10m3 |
292.4'' |
48° |
2015 |
|
|
|
|
|
|
GMC5 |
AG |
0m9 |
13m0 |
185.1'' |
121° |
2012 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ist Komponente B sehr schwach westlich vom buttergelbem Stern Altair erkennbar, weit abgesetzt
AC: bei 32x ist C im Osten ebenfalls schwach sichtbar, gleicher Abstand wie AB - alle drei Sterne stehen schön auf einer Linie, aber DS-Feeling eher Fehlanzeige |
|
|
|
|
STF2587 |
|
|
6m7 |
9m4 |
5.0'' |
99° |
2014 |
Aql |
19h51m26.83s |
+04°05'19.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Bright orange A star and faint bluish grey B which appears when seeing stills a fine point, ~4.5" [not physical] |
|
|
|
|
ES357 |
|
AB |
7m1 |
12m4 |
10.1'' |
309° |
2011 |
Cyg |
19h51m41.33s |
+31°08'16.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Moderately bright, 8th mag, with 3 delta mag B well separated. |
|
|
|
|
A1660 |
|
AB-C |
10m2 |
10m3 |
0.7'' |
203° |
2018 |
Aql |
19h52m53.17s |
+14°25'07.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Too tough for this night. Suspect with 205x, @ 333x I have strong sense of elongation but its all a haze, seeing not allow higher magnification. [AB is 0.2"! Very much worth trying with the 20" HD 354044 |
|
|
|
|
STF2593 |
|
AB |
8m8 |
10m3 |
12.1'' |
244° |
2019 |
Aql |
19h53m16.93s |
+11°50'04.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Almost a delicate pair, >1 delta mag, wide, both light orange. I missed BC, 10.1/11.4 3.7" -- transparency not good enough for fainter stars |
|
|
|
|
AG241 |
|
|
10m4 |
10m6 |
8.6'' |
217° |
2017 |
Aql |
19h53m19.36s |
+08°20'24.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Faint pair, one delta, wide. Not physical |
|
|
|
|
STFA48 |
|
AB |
7m1 |
7m3 |
41.7'' |
147° |
2019 |
Vul |
19h53m22.65s |
+20°20'14.10" |
René Merting
Drachhausen (Germany) |
16x70 |
beide etwa gleich helle Sterne sind gut getrennt, kein Farbunterschied, unspektakulär |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x zwei Sterne mit ordentlich Luft dazwischen - Komponente B südlich knapp schwächer - leichter Farbunterschied, aber nicht wirklich definierbar |
|
|
|
|
DJU4, 13 Vul |
|
|
4m6 |
7m4 |
1.4'' |
246° |
2016 |
Vul |
19h53m27.69s |
+24°04'46.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig wegen Helligkeitsunterschied |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
13 Vul: Very bright white A and 3- delta mag B, ~1.5-2", west PA |
|
|
|
|
STF2599 |
|
|
7m5 |
9m9 |
3.8'' |
52° |
2016 |
Vul |
19h53m38.65s |
+22°59'20.30" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x ist nordöstlich vom Hauptstern eine kleine Andeutung erkennbar, ganz schwach und noch nicht getrennt - bei 107x sehe ich den schwachen Begleiter besser, aber zwischen beide Sterne scheint kein Blatt zu passen - nur in guten Momenten sind beide Sterne knapp getrennt zu bewundern |
|
|
|
|
STF2596 |
|
|
7m3 |
8m7 |
2.1'' |
297° |
2016 |
Aql |
19h54m01.95s |
+15°17'31.70" |
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x ist Komponente B knapp abgesetzt nordwestlich von der A-Komponente sichtbar, knappe Trennung - Helligkeitsunterschied gut 1.5 Größenklassen |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Orange pair with 2 delta mag companion, about 2", well split. |
|
|
|
|
STF2594, 57 Aql |
|
AB |
5m7 |
6m3 |
36.3'' |
171° |
2019 |
Aql |
19h54m37.65s |
-08°13'38.30" |
René Merting
Drachhausen (Germany) |
10x50 |
ein einfacher Doppelstern - schön getrennt - Komponente A strahlt etwas weißer (ich weiß, es gibt keine Steigerungsformen von Farben) |
|
René Merting
Drachhausen (Germany) |
16x70 |
ein ansehnliches gut getrenntes Sternpaar - Komponente B im Süden ist gut eine halbe Größenklasse schwächer - das Weiß von Komponente A wirkt etwas kühler, während B eher in einem wärmeren zarten creme-gelb strahlt |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x ein sehr auffälliges, komfortabel getrenntes Sternpaar - Komponente B im Süden ist eine halbe Magnitude schwächer - zurück auf 20x immernoch eine ordentliche Trennung, B wirkt jetzt etwas schmutziger weiß |
|
Uwe Pilz
Leipzig (Germany) |
105mm (22x) |
orange-blau |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
easy DS |
|
|
|
|
HO581 |
|
|
8m0 |
8m7 |
0.3'' |
133° |
2006 |
Cyg |
19h54m58.40s |
+41°52'17.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very subtly notched elongation at best, light orange stars. 25.63 year period, near apastron in a nearly circular orbit, it will widen slightly in the next 5 years and still be a detectable 0.2" in 2035. |
|
|
|
|
STT390 |
|
AB |
6m6 |
9m5 |
9.6'' |
22° |
2015 |
Cyg |
19h55m06.50s |
+30°11'41.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very wide, 2-3 delta mag. |
|
|
|
|
STF2605, psi Cyg, 24 Cyg |
|
AB |
5m0 |
7m5 |
2.9'' |
175° |
2017 |
Cyg |
19h55m37.82s |
+52°26'20.50" |
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
At 80x difficult. At 100x and 133x the fainter component was clearly visible as small, roundish, partly slightly oval brightening. |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x knapp getrennt, A strahlt weiß mit einer schwachen Andeutung von gelb, B im Süden ist deutlich schwächer |
|
Uwe Pilz
Leipzig (Germany) |
105mm (96x) |
nicht schwierig |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow and ruddy, fairly wide, ~4" 2 delta mag. |
|
|
|
|
BU980, eta Cyg |
|
AB |
3m9 |
12m0 |
7.2'' |
206° |
2017 |
Cyg |
19h56m18.40s |
+35°05'00.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Somewhat in glare of A but saw B momentarily with averted vision. Two more faint stars on either side, B closer in. Complicated system, AB AE CE CF. What happened to D? |
|
|
|
|
BLL43 |
|
|
8m6 |
12m1 |
58.4'' |
16° |
2015 |
Cyg |
19h57m12.51s |
+44°15'40.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Intense orange color star, very pretty to look at. Orange in the finder. But no pair noticed -- too faint for urban location |
|
|
|
|
BU425 |
|
AB |
9m2 |
9m2 |
1.4'' |
240° |
2016 |
Sge |
19h57m32.28s |
+20°17'40.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Very fine pair, half delta mag, well split a little over 1". [AC & AD wider and fainter, not seen.] |
|
|
|
|
A1663 |
|
AB |
8m9 |
9m2 |
1.3'' |
237° |
2016 |
Aql |
19h57m34.28s |
+15°24'21.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Clean split, equal, can see disks with seeing. |
|
|
|
|
STT393 |
|
|
8m3 |
9m0 |
16.5'' |
232° |
2015 |
Cyg |
19h57m52.55s |
+44°23'03.10" |
René Merting
Drachhausen (Germany) |
18x70 |
B steht sehr knapp getrennt südwestlich von A, man muss schon sehr genau hinschauen - Helligkeitsunterschied eine Größenklasse |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x gut getrennt - Komponente A ist weiß-gelb und doppelt so hell wie Komponente B, die weiß-blau dagegen hält - runter auf 20x können beide Sterne auch getrennt werden, sie stehen dann schön eng |
|
|
|
|
BU1475 |
|
AB |
7m8 |
9m5 |
10.4'' |
113° |
2015 |
Aql |
19h57m53.70s |
-09°03'30.30" |
|
|
|
|
CD |
8m7 |
11m1 |
4.9'' |
163° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
AB: bereits bei 29x ist B knapp abgesetzt südöstlich von A erkennbar - A ist schön weiß und B ist im Grunde so schwach (gut 1.5 mag schwächer), dass der Stern kupferbraun strahlt |
|
|
|
|
STT392 & STF2607 |
STT392 |
AB |
6m6 |
8m4 |
0.1'' |
184° |
1996 |
Cyg |
19h57m56.12s |
+42°15'38.90" |
|
|
|
STF2607 |
AB-C |
6m6 |
9m1 |
3.0'' |
289° |
2012 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
STF2607 (AB-C): bei 107x ist C knapp westlich von AB zu erkennen, in guten Momenten sind die Komponenten getrennt sichtbar - trotz des großen Helligkeitsunterschiedes von schätzungsweise 1,5 bis 2 Größenklassen wirkt C ggü. AB auch erstaunlich weißlich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF2607 (AB-C): Very close clean split though B is in A's diffraction, somewhat bluish. |
|
|
|
|
BU266 |
|
|
7m6 |
11m5 |
15.8'' |
166° |
2015 |
Aql |
19h57m56.15s |
+11°24'53.00" |
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Pale white star with with a wide, much fainter ~4 delta mag blue companion |
|
|
|
|
BU149 |
|
BC |
10m3 |
12m9 |
8.1'' |
202° |
2015 |
Sge |
19h58m05.54s |
+16°29'55.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
B seen easily, C is noticed with averted vision and then can direct. Not physical |
|
|
|
|
AC12 |
|
|
7m5 |
8m3 |
1.6'' |
298° |
2016 |
Aql |
19h58m22.77s |
-02°13'54.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very nice light yellow-orange and blue-white stars, 1", 1 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Well split, about 1 magnitude difference. |
|
|
|
★★
|
STF2606 |
|
AB |
7m7 |
8m4 |
0.7'' |
146° |
2017 |
Cyg |
19h58m32.66s |
+33°16'38.80" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
sehr schwierig, Luftunruhe |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Hair split to clean split when seeing stills and there is only an airy disk. Near equal, half a delta mag. ~0.8" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Close pair 2 delta mag. |
|
|
|
|
STF2609 |
|
|
6m7 |
7m6 |
1.9'' |
22° |
2019 |
Cyg |
19h58m34.37s |
+38°06'20.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Cleanly split |
|
|
|
|
STF2611 |
|
|
8m5 |
8m5 |
5.3'' |
208° |
2018 |
Cyg |
19h58m51.90s |
+47°21'48.20" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x sind beide Sterne dicht zusammen stehend erkennbar, nur in ruhigen Momenten gelingt die Trennung - bei 64x ist die Trennung dann eindeutig, beide Sterne sind gleich hell und weiß |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Equal yellow, wide. |
|
|
|
★
|
BU1133 |
|
|
6m7 |
9m9 |
1.1'' |
342° |
1991 |
Cyg |
19h59m39.13s |
+31°49'35.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tough find, dense field. Very temporary brightening in diffraction, 20% held. This is a tough one, <1" and large delta mag. |
|
|
|
|
HJ1462 |
|
|
7m5 |
9m9 |
37.2'' |
24° |
2015 |
Vul |
20h00m06.57s |
+25°57'00.00" |
René Merting
Drachhausen (Germany) |
76mm (29x) |
bei 29x zeigt sich die A-Komponente auffällig warmweißgelblich strahlend, B präsentiert sich in gutem Abstand und deutlich schwächer (mind. 2 Größenklassen) - ein schöner Farbkontrast zwischen beiden Sternen |
|
|
|
|
13 Sge |
H4 100 |
AB |
10m0 |
10m1 |
23.9'' |
265° |
2013 |
Sge |
20h00m10.43s |
+17°30'09.10" |
|
|
|
H4 100 |
AC |
10m0 |
5m6 |
112.6'' |
297° |
2013 |
|
|
|
|
|
|
BU1477 |
CD |
5m6 |
13m4 |
27.0'' |
208° |
2013 |
|
|
|
|
|
|
BU1477 |
CE |
5m6 |
13m0 |
43.0'' |
115° |
2001 |
|
|
|
John Raymond
Richmond (Virginia/USA) |
|
|
|
|
|
★
|
STT394 |
|
AB |
7m1 |
10m3 |
11.0'' |
294° |
2015 |
Cyg |
20h00m11.43s |
+36°24'50.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty orange and blue, well separated, 2 delta mag. |
|
|
|
|
BU1289 |
|
AB |
8m2 |
9m2 |
0.7'' |
55° |
2016 |
Cyg |
20h00m59.61s |
+37°41'56.10" |
|
|
|
|
AC |
8m2 |
9m7 |
21.5'' |
90° |
2018 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AC: bei 32x sind zwei Sterne weit getrennt voneinander erkennbar - Komponente C im Osten ist relativ schwach bzw. gut 1.5 Größenklassen schwächer als A |
|
|
|
|
H5 47, 26 Cyg |
|
AB |
5m2 |
8m9 |
41.8'' |
150° |
2018 |
Cyg |
20h01m21.55s |
+50°06'16.80" |
|
|
|
|
BC |
8m9 |
12m9 |
8.8'' |
76° |
2015 |
|
|
|
|
|
|
|
BD |
8m9 |
15m8 |
9.4'' |
258° |
2015 |
|
|
|
|
|
|
|
AE |
5m2 |
11m1 |
168.3'' |
343° |
2012 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x ein weit getrenntes Pärchen mit schönem Farbkontrast - Komponente A im NW ist cremegelb, Komponente B ist mindestens 3 Größenklassen schwächer und zeigt sich weißgrau |
|
|
|
|
STF2612 |
|
AB |
8m3 |
9m9 |
42.5'' |
54° |
2016 |
Aql |
20h01m23.22s |
+06°56'49.70" |
|
|
|
|
BC |
9m9 |
12m3 |
26.9'' |
41° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x weit getrenntes Pärchen - Komponente A im Westen ist schwach und weiß, B ist kupfer-braun bis kupfer-rot und eine halbe Größenklasse schwächer (im Nachgang habe ich festgestellt, dass ich mit meiner Helligkeitseinschätzung deutlich abgewichen bin, der Helligkeitsunterschied beträgt 1.6 mag) - 20x reicht auch völlig für die Trennung, B ist dann nur schwächer und der Farbeindruck schwächer |
|
|
|
|
STF2613 |
|
AB |
7m5 |
8m0 |
3.5'' |
355° |
2019 |
Aql |
20h01m26.66s |
+10°44'54.80" |
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
64x reicht für die Trennung, dann stehen die beiden Sterne aber noch sehr dicht - beide mit gleicher Helligkeit und strahlend weiß - schick |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
White, ~1 delta mag, nice wide split |
|
|
|
|
STTA196 |
|
AB |
7m3 |
9m3 |
53.7'' |
169° |
2015 |
Cyg |
20h01m51.46s |
+40°51'31.70" |
|
|
|
|
AC |
7m3 |
12m3 |
137.0'' |
132° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x stehen beide Sterne weit auseinander - Komponente B im SO ist mindestens 2 Größenklassen schwächer - Farbkontrast durch Helligkeitsunterschied |
|
|
|
|
STT395, 16 Vul |
|
|
5m8 |
6m2 |
0.7'' |
128° |
2019 |
Vul |
20h02m01.45s |
+24°56'16.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
16 Vul. Hairline split at 8" 333x. At 667x I see a more definite split. It appears only half delta mag, rather than the 1 delta mag in Sky Tools. Nice star. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
fast getrennt, eher 8, ähnlich hell |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
STF2616 |
|
|
6m8 |
9m6 |
3.4'' |
268° |
2016 |
Aql |
20h02m46.04s |
+14°34'57.70" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x blitzt B immer westlich von A in dessen Glanz auf, B wirkt mehr wie ein schwacher grauer kompakter Schatten - bei 142x ist mit etwas Geduld B leicht abgesetzt von der gut 3 Magnituden heller geschätzten Komponente A erkennbar |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Pretty orange and blue pair, well separated about 2 delta mag. B very faint in 8", but know is there. With 20" easily seen as a brighter star. Nice pair |
|
|
|
|
STF2615 |
|
|
7m6 |
10m3 |
8.9'' |
301° |
2015 |
Aql |
20h02m54.05s |
+08°23'50.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
White A and much fainter reddish B, wide. Not physical |
|
|
|
|
STF2618 |
|
|
9m4 |
9m8 |
5.6'' |
115° |
2018 |
Aql |
20h03m26.98s |
+15°28'14.40" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Near equal, whiteish blue stars, wide. Nice |
|
|
|
|
STF2624 |
|
AB |
7m1 |
7m7 |
1.9'' |
174° |
2018 |
Cyg |
20h03m29.42s |
+36°01'28.60" |
|
|
|
|
AC |
7m1 |
9m3 |
42.3'' |
327° |
2018 |
|
|
|
|
|
|
|
AD |
7m1 |
12m9 |
29.0'' |
171° |
2018 |
|
|
|
|
|
|
|
BC |
7m7 |
9m3 |
44.7'' |
328° |
2018 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
63mm (120x) |
AB: 2021-08-15: At magnifications from 120x to 168x the double star appears clearly as an '8'. The diffraction disks still overlap slightly. The moderate brightness difference is visible. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
2021-08-15: The pair AB appears separated but very tight with almost touching diffraction disks. A moderate difference in brightness is visible. The fainter component C is clearly more separated. A, B & C form an obtuse triangle. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AC: bei 32x ist Komponente C in weitem Abstand von A erkennbar und bestimmt 2.5 bis 3 Größenklassen schwächer - Komponente B (7.73 mag / Sep. 2"/ P.A. 328°) habe ich wohl übersehen, weil nicht höher vergrößert, schade |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: A with 2x fainter B well separated, plus an arc of 3 stars. (4 stars in system, AB AC AD BC) |
|
|
|
|
HJ1470 |
|
|
7m4 |
9m2 |
29.3'' |
341° |
2016 |
Cyg |
20h03m39.50s |
+38°19'38.30" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x weit getrenntes Pärchen - Komponente B im NW ist nur schwach erkennbar - bei 32x Farbkontrast weiß/grau |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Pretty yellow & blue pair, wide separation. Alberio-like |
|
|
|
|
A1194 |
|
|
9m5 |
9m7 |
1.1'' |
317° |
2015 |
Aql |
20h03m59.56s |
+12°21'23.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Near equal bluish-white (seems nearly all 9th magnitude stars appear bluish white in my 8"). Cleanly split with seeing, 1". |
|
|
|
|
15 Sge |
STT592 |
AB |
5m9 |
9m5 |
163.2'' |
291° |
2015 |
Sge |
20h04m06.22s |
+17°04'12.60" |
|
|
|
STT592 |
AC |
5m9 |
6m9 |
217.0'' |
335° |
2015 |
|
|
|
|
|
|
BUP202 |
AD |
5m9 |
11m3 |
89.1'' |
3° |
2015 |
|
|
|
|
|
|
BUP202 |
AE |
5m9 |
11m8 |
175.0'' |
51° |
2013 |
|
|
|
|
|
|
BUP202 |
AF |
5m9 |
12m3 |
142.4'' |
315° |
2015 |
|
|
|
|
|
|
STTA202 |
BG |
9m5 |
9m0 |
181.4'' |
230° |
2015 |
|
|
|
|
|
|
BUP202 |
CH |
6m9 |
12m3 |
95.6'' |
185° |
2015 |
|
|
|
|
|
|
SMR20 |
AI |
5m9 |
11m1 |
132.1'' |
129° |
2015 |
|
|
|
|
|
|
TNN14 |
AJ |
4m4 |
13m5 |
3.3'' |
283° |
2004 |
|
|
|
|
|
|
TNN14 |
AK |
4m4 |
12m4 |
6.2'' |
162° |
2004 |
|
|
|
|
|
|
TNN14 |
AL |
4m4 |
13m0 |
9.3'' |
140° |
2004 |
|
|
|
John Raymond
Richmond (Virginia/USA) |
|
|
|
|
|
|
STF2622 |
|
AB |
8m7 |
9m5 |
6.0'' |
193° |
2018 |
Sge |
20h04m08.99s |
+17°00'02.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Well separated half delta mag. Part of 2 plus one system [AC 11.7 & 17.1". Ba,Bb is 10th mag & 0.2"] |
|
|
|
|
STF2620, V1470 Aql |
|
AB |
8m2 |
9m2 |
1.9'' |
287° |
2016 |
Aql |
20h04m09.25s |
+11°47'40.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Almost 2 delta mag, ~1.5" easily split pair, nice. [Eclipsing binary] |
|
|
|
|
COU325 |
|
AB |
9m4 |
10m9 |
0.8'' |
227° |
2006 |
Sge |
20h04m22.33s |
+17°14'33.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very finely split with 333x, large delta mag, delicate pair |
|
|
|
|
STF2621 |
|
|
8m4 |
8m6 |
5.7'' |
224° |
2017 |
Aql |
20h04m34.52s |
+09°14'24.20" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x knapp getrennt, da passt maximal eine Lage 80g-Papier dazwischen - bei 64x ein schönes enges Pärchen, etwas besser getrennt - beide Sterne annähernd gleichhell, Komponente B müsste der Stern im NW sein - A reinweiß, B auch mit einem Stich ins grau |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
More equal than SkyTools data shows, one is orange and the other blue. Maybe the orange star is variable. Wide separation, another nice pair |
|
|
|
|
STT397 |
|
|
7m4 |
9m6 |
46.1'' |
179° |
2016 |
Aql |
20h04m46.86s |
+15°54'11.30" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x ein weit getrenntes Pärchen - Komponente B im Süden ist deutlich schwächer und hat kaum Farbe - zurück auf 20x sind beide Sterne noch immer gut getrennt sichtbar, Komponente B ist mit etwas Konzentration knapp sichtbar |
|
|
|
|
BU56 |
|
|
8m0 |
9m1 |
1.3'' |
187° |
2012 |
Aql |
20h05m07.26s |
-04°18'29.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange and blue. <1", 1 delta mag. |
|
|
|
|
BU57 |
|
|
6m6 |
11m0 |
2.6'' |
120° |
2008 |
Aql |
20h05m26.53s |
+15°30'01.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
V1472 Aql. At 8" the B appears as a suspected brightening in the diffraction, whitish to the A star's orange. At 20" the B star is obvious and blue a nice sharp point ~2.5" |
|
|
|
|
SHJ316 |
|
AB |
7m8 |
8m8 |
69.4'' |
323° |
2018 |
Cyg |
20h05m39.80s |
+35°36'28.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ist der kleine Begleiter indirekt zu erkennen, beide sind getrennt sichtbar - schön in Kombination mit dem Mini-W (Asterismus Alessi J0022.7+5417) |
|
|
|
★★
|
SHJ314, V1676 Cyg |
|
AF |
6m8 |
7m3 |
36.3'' |
28° |
2019 |
Cyg |
20h05m57.32s |
+35°47'18.20" |
|
|
|
|
AD |
6m8 |
9m5 |
11.3'' |
300° |
2019 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AD: bei 32x ist westlich von A knapp getrennt ein sehr schwacher Lichtpunkt erkennbar - mindestens 3 Größenklassen Helligkeitsunterschied zwischen A und D - zurück auf 20x sind beide Sterne auch noch ganz knapp getrennt erkennbar
AF: bei 32x sind zwei weit auseinander stehende Sterne erkennbar, Komponente F im NO ist nur unwesentlich schwächer und strahlt nicht ganz so klar wie A |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
liegt gemeinsam mit SHJ 315 im OC NGC 6871. Die Zeichnung des gesamten Haufens enthält nur die hellsten Sterne. |
|
|
|
|
ES25 & SHJ315 & WAL127 & SEI865 |
ES25 |
AB |
7m9 |
12m0 |
8.6'' |
122° |
2015 |
Cyg |
20h06m01.36s |
+35°45'55.90" |
|
|
|
ES25 |
AC |
7m9 |
14m8 |
11.8'' |
297° |
2015 |
|
|
|
|
|
|
SHJ315 |
AD |
7m9 |
8m7 |
20.2'' |
236° |
2018 |
|
|
|
|
|
|
WAL127 |
AE |
7m9 |
11m7 |
33.7'' |
94° |
2015 |
|
|
|
|
|
|
ES25 |
AF |
7m9 |
6m8 |
95.7'' |
329° |
2017 |
|
|
|
|
|
|
SEI865 |
EG |
11m7 |
11m8 |
14.5'' |
196° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
SHJ315 (AD): bei 32x zeigt sich das Sternpaar weit getrennt und insgesamt schwächer als das unmittelbar nordwestlich liegende Dreifachsystem SHJ 314 - Komponente B im SW wirkt graubraun |
|
|
|
|
STTA198 |
|
AB |
7m1 |
7m5 |
64.6'' |
185° |
2018 |
Aql |
20h06m38.76s |
+07°34'34.20" |
René Merting
Drachhausen (Germany) |
12x50 |
ein schöner, einfacher FG-Doppelstern - ein Paar heller Sterne, gut getrennt - das Paar steht gut isoliert - B ist eine halbe Größenklasse schwächer |
|
|
|
|
BU428 |
|
|
7m5 |
9m1 |
0.8'' |
356° |
2008 |
Aql |
20h06m43.37s |
+12°56'12.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Definite hard split with 20", slightly yellow A and yellow-orange B star. With 8" the B is more a round haze snowman-to-hairline split with seeing. |
|
|
|
|
BRT1336 |
|
|
9m9 |
10m8 |
5.5'' |
292° |
2018 |
Aql |
20h07m00.13s |
+12°20'16.80" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Easy wide split about half delta mag, stars appear blue |
|
|
|
|
STF2631 |
|
|
8m1 |
9m1 |
4.6'' |
339° |
2018 |
Sge |
20h07m13.84s |
+21°06'13.40" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x ist Komponente B schon angedeutet nördlich von A erkennbar - bei 64x dann ist B knapp getrennt von A erkennbar - beide Komponenten strahlen weißlich ohne erkennbare Färbung |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Subtle yellow and blue stars, very light. 1.5 delta mag, wide. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very nice orange and blue, a mini Alberio, a little more equal magnitude, though. ~5", 1 delta mag. |
|
|
|
|
STF2629 |
|
|
7m6 |
10m6 |
9.0'' |
188° |
2015 |
Aql |
20h07m20.78s |
+16°04'34.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
White and rather strikingly blue star (and I don't think it's blue because it's faint), wide separation, 2 delta mag. |
|
|
|
|
STT398 |
|
AB |
7m5 |
9m2 |
1.0'' |
82° |
2015 |
Cyg |
20h07m23.69s |
+35°43'05.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
B is very faint, appears as a brightening or pin-prick in A's diffraction. 2-3 delta mag, ~1" |
|
|
|
|
WEB12 |
|
|
8m4 |
8m4 |
40.1'' |
77° |
2019 |
SGE |
20h07m45.66s |
+19°50'14.00" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x weit auseinander stehend - Komponente B im Osten ist nur knapp schwächer als A - Komponente A strahlt gelblich, B wirkt kühler weiß-blau - auch bei 20x sind beide Sterne gut getrennt erkennbar |
|
|
|
|
STF2628 |
|
|
6m6 |
8m7 |
3.0'' |
338° |
2016 |
Aql |
20h07m50.37s |
+09°23'59.40" |
René Merting
Drachhausen (Germany) |
100mm (142x) |
bei 107x ist Komponente A so hell, dass B nur angedeutet nordwestlich von A sichtbar ist und sich noch nicht lösen kann - bei 142x dann knappe Trennung, B erscheint mindestens 3 Magnituden schwächer (lt. WDS/Stelle Doppie nur 2 Magnituden) |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Nice, very pretty white and light orange B star, 3 delta mag, wide separation. Very pretty pair. |
|
|
|
|
STF2633 |
|
AB |
8m0 |
11m0 |
11.6'' |
101° |
2015 |
Cyg |
20h07m57.93s |
+32°35'10.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
3 delta mag, wide, 2 more on the opposite side. (4 stars visible, AC & AC = HJ 1483. CD = SEI 900, not seen) |
|
|
|
|
J1168 |
|
|
10m1 |
10m7 |
0.9'' |
192° |
2015 |
Sge |
20h08m12.46s |
+21°06'11.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very fine split, ~1 delta, <1", nice |
|
|
|
|
HJ606 |
|
|
8m0 |
8m1 |
44.0'' |
229° |
2017 |
Cyg |
20h08m21.92s |
+38°08'20.00" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x zwei gut getrennte gleich helle Sterne, A im NO ist einen kleinen Tick heller - bei 32x Komponente A im NO weiß, B mit einem Stich ins blau-grüne |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Wide separation equal magnitude yellow-white pair. |
|
|
|
★★
|
STF2675, kappa Cep, 1 Cep |
|
AB |
4m4 |
8m3 |
7.3'' |
120° |
2015 |
Cep |
20h08m53.32s |
+77°42'40.90" |
Robert Zebahl
Leipzig (Germany) |
55mm (38x) |
At 27x faint companion not visible. At 38x and higher magnification the companion is quite easily visible as faint, tiny star. Very nice, uneven pair! |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Bright white and 3 delta mag light orange B, well split. |
|
|
|
|
STF2639 |
|
AB |
7m8 |
8m7 |
5.8'' |
302° |
2018 |
Cyg |
20h09m14.32s |
+35°29'01.90" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x ist der Doppelstern als 8 erkennbar, B im NW kann sich noch nicht ganz lösen - bei 64x dann knappe Trennung, Komponente B ist eine Größenklasse schwächer - beide Sterne sind trotzdem ohne Farbunterschied in zart weiß sichtbar |
|
|
|
|
STF2634 |
|
AB |
7m8 |
9m9 |
4.1'' |
14° |
2016 |
Sge |
20h09m34.30s |
+16°48'19.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Blue-white star with 2 delta mag slightly red B, about 4" [AC 13th mag and very wide separation] |
|
|
|
|
HJ1485 |
|
|
8m2 |
8m9 |
4.7'' |
277° |
2018 |
Cyg |
20h09m37.19s |
+33°24'39.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 107x sind beide Sterne ordentlich getrennt erkennbar - beim Helligkeitsunterschied habe ich mich total verschätzt, es sind nur 0.7 mag, ich habe auf 1.5 mag geschätzt - leichter Farbkontrast, Komponente A ist weiß-gelblich, B eher grau - zurück auf 64x sehr knappe Trennung, schönes enges Pärchen |
|
|
|
|
STF2637, theta Sge, 17 Sge |
|
AB |
6m6 |
8m8 |
11.7'' |
331° |
2019 |
Sge |
20h09m56.61s |
+20°54'53.20" |
|
|
|
|
AC |
6m6 |
7m5 |
91.3'' |
222° |
2017 |
|
|
|
|
|
|
|
AD |
6m6 |
11m9 |
172.8'' |
226° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ist nördlich von A ein schwacher Begleiter erkennbar, gut getrennt - Helligkeitsunterschied gut 2 Größenklassen, B wirkt dadurch grau-braun
AC: bei 32x ist südwestlich von Komponente A in einigem Abstand Komponente C (siebenfache Entfernung AB) erkennbar - die Helligkeit von C liegt zwischen A und B |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Theta Sge. White star and slightly red B, wide separation, about 3 delta mag [Several other pairs, not observed] |
|
|
John Raymond
Richmond (Virginia/USA) |
|
|
|
|
|
|
STF2648 |
|
|
8m1 |
9m6 |
6.9'' |
117° |
2018 |
Cyg |
20h10m23.11s |
+49°49'16.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x erscheint Komponente B südöstlich von A ordentlich getrennt - ein schönes schwaches Pärchen, bei dem Komponente B gut eine Größenklasse schwächer scheint - A ist weiß-gelb, B weiß-grau |
|
|
|
|
COU122 |
|
|
7m2 |
9m9 |
0.6'' |
355° |
2007 |
Vul |
20h10m28.04s |
+25°02'56.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Tried 553x & 885x, seems somewhat distorted but no clear shape, so cannot claim success |
|
|
|
|
S738 |
|
AB |
7m8 |
8m4 |
42.6'' |
106° |
2019 |
Cyg |
20h10m35.13s |
+33°38'02.70" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
ein Sternpaar, das sehr dominant im Sternhaufen Roslund 5 steht - bei 32x sind beide Sterne weit getrennt erkennbar - Komponente B im Osten ist eine halbe Größenklasse schwächer als A - beide Sterne weiß, B leicht in gräuliche gehend - zurück auf 20x ist die Trennung nach wie vor leicht |
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|
|
|
STT399 |
|
AB |
7m6 |
9m9 |
4.6'' |
278° |
2015 |
Cyg |
20h10m44.13s |
+37°02'33.50" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x ist Komponente B westlich von A wie ein leichter Hauch erkennbar, knapp getrennt - kein einfacher Doppelstern |
|
|
|
|
S735 |
|
|
7m2 |
8m0 |
56.4'' |
211° |
2019 |
Aql |
20h11m18.86s |
-00°07'35.30" |
René Merting
Drachhausen (Germany) |
10x50 |
ein einfaches zu trennendes Paar - Komponente B im SW ist keine ganze Größenklasse schwächer - leichter Farbkontrast, A weiß, B grau-weiß |
|
René Merting
Drachhausen (Germany) |
12x50 |
leicht zu trennen - B steht im SSW von A und wirkt grau gegen die weißgelb strahlende A-Komponente |
|
|
|
|
BLL46, V1042 Cyg |
|
AB |
8m1 |
10m6 |
53.2'' |
109° |
2015 |
Cyg |
20h11m53.53s |
+36°11'50.60" |
Christopher Hay
Seeheim (Germany) |
23x100 |
Wide split. No colour impression. Reminiscent of view of BLL48 in 15x45 binoculars, see observation.
Not a visually exciting pair, but I visited it intentionally because it is a physical pair which is the source of excitation of the Wolf-Rayet nebula WR 135. Together with WR 137 (aka BLL48, see entry in this listing) and the more well-known WR 134, BLL46 (aka WR 135) is one of the first three objects of its kind to be discovered in 1867.
BLL46 is also listed as the variable star V1042 Cyg, its distance to us is approximately 5000 light years.
All three WR objects can be viewed together in a FOV of just 1.5°. Together they form an arc, concave to the northwest, that is also known as "the Wolf-Rayet Cascade". |
|
|
|
|
STT401 |
|
|
7m3 |
10m6 |
12.8'' |
69° |
2015 |
Cyg |
20h12m13.15s |
+38°26'35.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange and faintly bluish, 1 delta mag, wide 10" |
|
|
|
|
COU123 |
|
|
8m6 |
8m9 |
0.3'' |
233° |
2007 |
Vul |
20h12m17.81s |
+22°48'28.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Nice orange star, but no resolution, do not see any mis-shape -- observation in October 2018 |
|
|
|
|
STF2649 |
|
AB |
7m9 |
9m8 |
21.6'' |
151° |
2018 |
Cyg |
20h12m18.61s |
+32°04'51.80" |
|
|
|
|
AC |
7m9 |
11m4 |
131.0'' |
284° |
2018 |
|
|
|
|
|
|
|
AD |
7m9 |
10m6 |
175.9'' |
36° |
2018 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ist Komponente B weit getrennt von A im SW erkennbar - Helligkeitsunterschied 1.5 bis 2 Magnituden - Komponente weiß, B eher gräulich - kaum weitere Sterne im direkten Umfeld - zurück auf 20x sind beide Sterne auch trennbar, B ist gerade so sichtbar |
|
|
|
★★
|
AC17 |
|
AB |
6m2 |
10m6 |
4.4'' |
82° |
2015 |
Cyg |
20h12m31.73s |
+51°27'49.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wow. Pretty orange-yellow and much fainter 3-4 delta mag B, resolves into view with seeing, just appears then vanishes if seeing quavers. ~4". |
|
|
|
|
STF2644 |
|
|
6m9 |
7m1 |
2.6'' |
206° |
2019 |
Aql |
20h12m35.09s |
+00°52'00.20" |
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Very tight at 57x, but separable without noticeable difference in brightness. At 100x very small difference in brightness visible. The colors of both components appeared to be the same, but not clearly perceptible. |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
both components white at 102x, companion appears slightly reddish at 205x |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Close white stars, near equal, ~2.5" |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gleich hell, leicht |
|
|
|
|
STF2643 |
|
|
7m1 |
9m4 |
3.0'' |
81° |
2015 |
Aql |
20h12m47.31s |
-02°59'45.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
White and reddish stars, wide separation, large magnitude difference. |
|
|
|
|
ES502 |
|
|
8m0 |
10m9 |
13.8'' |
221° |
2015 |
Cyg |
20h13m07.26s |
+49°11'18.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow with pretty faint wide pair, 1 delta mag. |
|
|
|
★★★
|
STFA50, omicron Cyg, 30/31 Cyg |
|
AD |
3m9 |
4m8 |
336.7'' |
322° |
2016 |
Cyg |
20h13m37.90s |
+46°44'28.80" |
|
|
|
|
AC |
3m9 |
7m0 |
108.6'' |
173° |
2016 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
naked eye |
AD: Well split with noticeable difference in brightness. |
|
Christopher Hay
Seeheim (Germany) |
3x63 |
Self-built binoculars, hence the unusual specification.
Widely split, A (31 Cyg) light orange, D (30 Cyg) light blue. |
|
Christopher Hay
Seeheim (Germany) |
7x50 |
A-D: Widely split, A (31 Cyg) luminous orange-red, D (30 Cyg) luminous ice-blue. C set off from A as a fine speck of light. |
|
Robert Zebahl
Leipzig (Germany) |
8x40 |
AD: Wonderful double star for binoculars. Large distance of the components, brighter once (31 Cyg) appeared slightly orange, the fainter (Cyg 30) more bluish. |
|
Robert Zebahl
Leipzig (Germany) |
8x40 |
AC: Observation at full moon. Easily split with big difference in brightness. Brighter component slightly orange. C component rather faint. |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
A-D: Very wide apart but still perceived as belonging together. A (31 Cyg) orange-red, D (30 Cyg) ice-blue. C well set off from A and light ice-blue, like an echo of D. A delightful group of three for binoculars at this power, further accentuated by nearby orange Omicron2 Cygni. Both the brightnesses and colour hues of Omi1A and Omi2 appear practically identical. |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-03: Fantastic sight. A: bright orange, D: white-bluish, C: light blue. Very beautiful field. |
|
René Merting
Drachhausen (Germany) |
18x70 |
wunderschön - Komponente A präsentiert sich buttergelb - die südliche, schwächste Komponente C zeigt sich aquamarinblau - D im Norden ist reinweiß und steht dreimal weitere entfernt wie AC |
|
Robert Zebahl
Leipzig (Germany) |
80mm (25x) |
AC: Similar to the observation with binoculars. C component appeared bluish and gave good contrast to the orange colored 31 Cyg. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x sind alle drei Sterne weit getrennt und doch irgendwie zusammengehörend, Komponente A ist rapsgelb und am auffälligsten, Komponente D strahlt weiß und die schwächste Komponente C schimmert bläulich, schöner Anblick |
|
Robert Zebahl
Leipzig (Germany) |
102mm (28x) |
Bright, wide apart and wonderful contrast in color. A: light yellowish-orange, C: blue, D: light blue. |
|
Sarah Gebauer
Germany |
150mm (30x) |
die drei Komponenten plus Omicron2 bilden ein wunderschönes, sehr langes und spitzes Dreieck und zeigen dabei wundervolle Farben, Komponente A von o1 sowie o2 erscheinen schön gelblich, Komponente D von o1 hat einen deutlichen Blaustich im Weißen, wirklich ein sehr schönes Gesamtbild - auf Komponente C hatte ich nicht geachtet |
|
Sarah Gebauer
Germany |
150mm (85x) |
dieses Mal nur die drei dicht beieinanderstehenden Komponenten A, C und D im Sichtfeld gehabt, Komponente A ist wieder deutlich gelbgold, C wirkt leicht bläulich und Komponente D wirkt dieses Mal eher weiß |
|
|
|
★
|
STF2653 |
|
AB |
6m7 |
9m2 |
2.7'' |
279° |
2016 |
Vul |
20h13m40.56s |
+24°14'20.50" |
René Merting
Drachhausen (Germany) |
76mm (57x) |
bei 57x ist B mit ordentlich Abstand außerhalb des Leuchtens der A-Komponente erkennbar - vorher bei 29x war B nicht auszumachen - ein sehr ungleiches Paar |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Pretty pair, pale white star and blue, very faint and small 3" separated B. Looks like a planet |
|
|
|
|
STF2658 |
|
AB |
7m2 |
9m4 |
5.4'' |
106° |
2015 |
Cyg |
20h13m40.74s |
+53°07'30.30" |
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x ist Komponente B schwach erkennbar östlich von A, es ist schon ordentlich Luft zwischen den beiden - Helligkeitsunterschied 2 Magnituden |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
orangegelb |
|
|
|
|
STF2651 |
|
AB |
8m4 |
8m4 |
0.9'' |
279° |
2018 |
Sge |
20h13m44.90s |
+16°09'28.70" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Clean split, nearer equal than Sky Tools data, about 1", white stars |
|
|
|
|
STF2655 |
|
AB |
7m9 |
8m0 |
6.2'' |
3° |
2019 |
Vul |
20h14m04.52s |
+22°13'21.50" |
|
|
|
|
AC |
7m9 |
10m1 |
60.5'' |
154° |
2016 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (31x) |
AB: 2020-07-29: At 22x clearly visible as '8' and almost separated. At 31x well separated with still very close and almost equally bright components. Color was not visible. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x extrem knapp getrennt das Paar - beide Sterne sind gleichhell, wenn ich schätzen müsste, würde ich die schwächere Komponente B nördlich vermuten
AC: bei 32x ist Komponente C in einigem Abstand südöstlich von dem engen Paar AB erkennbar, sehr schwach |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Pure white stars, half delta mag, wide about 6". [AC 10th mag and very wide] |
|
|
|
|
S740 |
|
AB |
7m8 |
8m1 |
43.9'' |
192° |
2019 |
Aql |
20h14m09.77s |
+06°35'20.30" |
René Merting
Drachhausen (Germany) |
10x50 |
ordentlich getrenntes gut sichtbares Sternpaar - Komponente A im Norden ist nur unwesentlich heller |
|
René Merting
Drachhausen (Germany) |
12x50 |
zwei schwache Sterne, gut getrennt voneinander - B im Süden ist nur knapp schwächer als A |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x zeigen sich beide Sterne weit getrennt und sind gut sichtbar - Helligkeitsunterschied eine halbe Magnitude - Komponente A im Norden ist weiß-gelblich, B leicht blau-grau |
|
|
|
★
|
STT403 & STF2657 |
STT403 |
AB |
7m3 |
7m6 |
0.9'' |
171° |
2019 |
Cyg |
20h14m21.53s |
+42°06'15.60" |
|
|
|
STF2657 |
AC |
7m3 |
9m8 |
11.6'' |
32° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
STF2657 (AC): bei 64x zeigt sich C ganz schwach nordöstlich von A - mindestens 2 Größenklassen Helligkeitsunterschied - A ist reinweiß, bei C bin ich froh, dass ich C überhaupt erkennen kann |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
STT403 (AB): schwierig |
|
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
STT403 (AB): At 129x clearly elongated, notched. At 270x clearly split, but very tight with almost touching diffraction disks. Visible, but very small difference in brightness. Inconspicuous color. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
STT403 (AB): schwaches 3er System, getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STT403 (AB): Dramatic near equal white, just split, ~1", with a third in the system 2x fainter and wide separation (Indeed a triple, as described.) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STT403 (AB): Dramatic near equal white, just split, ~1", with a third in the system 2x fainter and wide separation (Indeed a triple, as described.) |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
STT403 (AB) |
|
|
|
|
CHE227 |
|
|
11m0 |
11m1 |
5.2'' |
46° |
2015 |
Sge |
20h14m25.12s |
+16°11'32.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
By strobing with averted vision can just make out faint near equal stars, pretty wide. Can hold direct once seen. |
|
|
|
|
ES244 |
|
AB |
8m4 |
12m2 |
41.2'' |
130° |
2015 |
Cyg |
20h14m25.83s |
+35°24'25.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
8th & 12th mag, wide separation. B looks like a faint double itself with averted vision. |
|
|
|
|
BLL48 |
|
AB |
8m0 |
10m1 |
113.6'' |
117° |
2015 |
Cyg |
20h14m31.77s |
+36°39'39.60" |
Christopher Hay
Seeheim (Germany) |
15x45 |
Very wide split. B-component just bright enough to hold it steadily in these binoculars under NELM5 sky.
Would not have felt the pair to be double without prior knowledge. But I visited it very intentionally because it is a physical pair whose A-component is the source of excitation of the Wolf-Rayet nebula WR 137. See also observation of BLL46, another Wolf-Rayet double star.
Is also listed as the variable star V1679 Cyg, its distance to us is approximately 7000 light years. |
|
|
|
|
ENG72, 29 Cyg |
|
AB |
5m0 |
6m7 |
215.3'' |
155° |
2016 |
Cyg |
20h14m31.98s |
+36°48'22.10" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-09-20: Widely separated pair in nice star field with moderate difference in brightness and beautiful color contrast: whitish & yellow-orange. |
|
|
|
|
STF2654 |
|
|
7m0 |
8m1 |
14.4'' |
233° |
2019 |
Aql |
20h15m10.63s |
-03°30'12.90" |
René Merting
Drachhausen (Germany) |
12x50 |
lange sehe ich nichts bzw. nur einen Lichtpunkt - mit etwas Geduld ist B ganz schwach und nur knapp abgesetzt südwestlich von A erkennbar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wide, 1 delta mag |
|
|
|
|
HO455 |
|
AB |
7m5 |
12m0 |
35.1'' |
83° |
2015 |
Cyg |
20h15m13.60s |
+54°08'47.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Carbon star with very faint arc of 3 stars and one other star. Interesting! Can see direct vision but averted brightens. |
|
|
|
|
BU983 |
|
AB |
4m8 |
7m5 |
0.4'' |
190° |
2016 |
Vul |
20h15m15.89s |
+25°35'31.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Out of round but not resolved. Bright white. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
QR Vul. Olive shape seen through "rain" of the diffraction. Even with 8-inch mask there is a definite misshape with a faint tail bump to the ball of A's disk. Burnham discovered with 18.5-inch Washburn @ 0.86", so it was easier for him! |
|
|
|
|
ROE101 |
|
AB |
8m4 |
9m6 |
12.7'' |
53° |
2015 |
Sge |
20h15m36.94s |
+19°58'29.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Unremarkable wide ~2 delta. Not physical |
|
|
|
|
STT404 |
|
AB |
7m6 |
9m8 |
28.5'' |
115° |
2015 |
Cyg |
20h15m49.33s |
+52°30'08.20" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein weit getrenntes Pärchen - Komponente B ist schwach als grauer Punkt erkennbar, A nordwestlich davon ist leicht gelblich - zurück auf 20x hat A weiterhin einen Farbstich und B sieht aus wie ein Nadelstich, das Paar ist gut getrennt |
|
|
|
|
A389 |
|
|
9m9 |
10m1 |
1.7'' |
213° |
2017 |
Vul |
20h16m00.80s |
+27°03'10.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Beautiful well split white stars, slight magnitude difference |
|
|
|
|
COU218 |
|
|
9m4 |
9m5 |
0.3'' |
235° |
2011 |
Vul |
20h16m21.85s |
+23°09'03.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Hairline split, equal stars, light yellow-white |
|
|
|
★
|
BU442 & SLV8 & ABH135 & SLE982 |
BU442 |
AB |
9m7 |
8m0 |
18.7'' |
103° |
2015 |
Cyg |
20h16m29.84s |
+37°38'35.40" |
|
|
|
SLV8 |
AC |
9m7 |
8m8 |
31.8'' |
77° |
2015 |
|
|
|
|
|
|
BU442 |
BC |
8m0 |
8m8 |
16.8'' |
49° |
2015 |
|
|
|
|
|
|
ABH135 |
AD |
9m7 |
12m6 |
24.5'' |
50° |
2015 |
|
|
|
|
|
|
ABH135 |
BE |
8m0 |
12m9 |
50.0'' |
88° |
2015 |
|
|
|
|
|
|
ABH135 |
BF |
8m0 |
12m5 |
64.2'' |
140° |
2015 |
|
|
|
|
|
|
SLE982 |
AG |
9m7 |
10m6 |
88.5'' |
10° |
2015 |
|
|
|
|
|
|
SLE982 |
AH |
9m7 |
13m5 |
111.5'' |
20° |
2008 |
|
|
|
|
|
|
SLE982 |
AI |
9m7 |
13m5 |
63.3'' |
44° |
2015 |
|
|
|
|
|
|
SLE982 |
AJ |
9m7 |
13m1 |
96.5'' |
35° |
2012 |
|
|
|
|
|
|
SLE982 |
AK |
9m7 |
11m5 |
114.7'' |
35° |
2012 |
|
|
|
|
|
|
SLE982 |
AL |
9m7 |
9m5 |
177.5'' |
27° |
2015 |
|
|
|
|
|
|
SLE982 |
AM |
9m7 |
13m2 |
89.2'' |
65° |
2015 |
|
|
|
|
|
|
SLE982 |
AN |
9m7 |
12m4 |
156.2'' |
77° |
2012 |
|
|
|
|
|
|
SLE982 |
AO |
9m7 |
12m7 |
59.1'' |
118° |
2015 |
|
|
|
|
|
|
BU442 |
AP |
9m7 |
10m8 |
4.1'' |
156° |
2016 |
|
|
|
|
|
|
BU442 |
AQ |
9m7 |
13m1 |
8.7'' |
157° |
2015 |
|
|
|
|
|
|
BU442 |
AR |
9m7 |
11m1 |
19.2'' |
332° |
2015 |
|
|
|
|
|
|
BU442 |
BS |
8m0 |
14m5 |
3.7'' |
124° |
2016 |
|
|
|
|
|
|
BU442 |
BT |
8m0 |
11m5 |
6.7'' |
164° |
2016 |
|
|
|
|
|
|
BU442 |
BU |
8m0 |
11m5 |
25.4'' |
74° |
2015 |
|
|
|
|
|
|
BU442 |
BV |
8m0 |
12m0 |
31.1'' |
86° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
ein Zehnfachsternsystem mit drei Sternen zwischen 8 und 10 mag und weiteren 7 Sternen zwischen 11 und 15 mag
AB: - bei 32x und genauer Betrachtung zeigt sich im NW von B die Komponente A, die etwa eine halbe Größenklasse schwächer ist als C - bei 107x ist erkennbar, dass A einen kleinen Ticken weiter von B entfernt steht als C
BC: bei 32x sind B und C auffällig und schön anzusehen, C steht weit getrennt nordöstlich von B und ist eine knappe Magnitude schwächer |
|
|
|
|
STF2663 |
|
AB |
8m2 |
8m7 |
5.4'' |
323° |
2018 |
Cyg |
20h16m48.53s |
+39°41'50.40" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x lässt sich der Stern nicht scharf stellen - bei 64x dann ist ein gut getrenntes schwaches Sternpärchen erkennbar - Helligkeitsunterschied zwischen A im SO und B im NW vielleicht eine halbe Größenklasse - der Sternpaar wirkt elegant und filigran im Sternumfeld |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow and blue, near equal, wide 5". |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
~5" equal magnitude white |
|
|
|
★
|
RST4659 |
|
AB |
7m2 |
9m2 |
1.8'' |
7° |
2015 |
Aql |
20h16m50.26s |
-03°29'30.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
White and 2-3 delta mag, ~2" B. |
|
|
|
|
HO588 |
|
AB |
6m9 |
8m9 |
50.8'' |
297° |
2018 |
Cyg |
20h16m54.99s |
+31°30'18.70" |
|
|
|
|
BC |
8m9 |
12m6 |
8.7'' |
30° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ganz einfach, weit auseinander - Komponente A ist weiß, die gut 2 Magnituden schwächere Komponente B im NW strahlt rot-braun-grau-irgendwas - zurück auf 20x ist das Paar auch einfach |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Blue-white with 1 delta mag, very wide twin |
|
|
|
★
|
BU441 |
|
AB |
6m4 |
10m5 |
6.2'' |
64° |
2015 |
Vul |
20h17m31.54s |
+29°08'51.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange star with very faint bluish B seen with averted vision at first then can just hold. Needs fine focus. |
|
|
|
|
COU219 |
|
Aa-Ab |
8m5 |
9m8 |
0.4'' |
109° |
2013 |
Sge |
20h17m44.53s |
+20°25'23.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice split with seeing, ~1 delta mag, ~0.5". A component of J 2308 |
|
|
|
★
|
STFA51, alpha Cap, alpha 1/2 Cap |
|
AE |
3m7 |
4m3 |
381.2'' |
290° |
2012 |
Cap |
20h18m03.22s |
-12°32'41.40" |
Christopher Hay
Seeheim (Germany) |
naked eye |
While waiting for Comet Neowise at 3 in the morning in July 2020 surprised myself with my first naked-eye separation of Alpha1 und Alpha2 Capricornis (observing site at 50° northern latitude, Alpha1/2 passing through meridian). Western, weaker component Alpha 1 Cap well separated from Alpha 2 Cap in good moments. Much more difficult to split naked-eye than Mizar/Alcor (Zeta UMa). Not a physical double. |
|
René Merting
Drachhausen (Germany) |
12x50 |
ein wunderschönes Sternpaar, obwohl beide so weit auseinander stehen - die hellere östliche Komponente strahlt buttergelb, der Begleiter ist weiß |
|
Sarah Gebauer
Germany |
100mm (21x) |
bei 21x sind alpha1 und alpha2 deutlich getrennt voneinander mit ganz leicht orangefarbenem Eindruck, sie stechen wie zwei helle Augen hervor |
|
|
|
★★
|
STF2666 |
|
AB |
6m0 |
8m2 |
2.8'' |
245° |
2018 |
Cyg |
20h18m06.99s |
+40°43'55.60" |
|
|
|
|
AC |
6m0 |
10m7 |
34.0'' |
207° |
2006 |
|
|
|
|
|
|
|
CD |
10m7 |
11m0 |
24.1'' |
143° |
2018 |
|
|
|
Christopher Hay
Seeheim (Germany) |
90mm (145x) |
AB: Cleanly split in moments of stable air column. Companion is just outside the first diffraction ring of the primary.
Observed in the shortest night of the year on 21 June 2018, but in zenith under transparent sky.
Comparison observation nearby: Epsilon Lyrae is substantially easier to split despite its smaller separation. |
|
Christopher Hay
Seeheim (Germany) |
150mm (96x) |
AB: Observed at zenith in late July 2019. Clean split, B a fine speck of light to the south of the much brighter primary. Very charming, the highlight of that night’s double-star observing. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
AB: 2020-06-24: Very nicely separated with clear difference in brightness. The A component appears white-yellowish. The companion was well visible as a tiny star without color. |
|
Christopher Hay
Seeheim (Germany) |
254mm (110x) |
AB: Neatly split with a sliver of black inbetween. A fine double for this aperture and power.
At 65x Struve 2666 is not yet spit, but accompanied by a fine sprinkling of stardust to the south. These are the other members of open cluster Collinder 419, of which Struve 2666 is the lucida. A captivating sight. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: White A, slightly red B, ~2 delta mag, ~4" |
|
|
|
|
HU357 |
|
|
8m0 |
10m9 |
1.8'' |
195° |
1991 |
Sge |
20h18m14.41s |
+18°19'41.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Blue-white A, B is very fine but nicely split, also bluish but much fainter. Physical |
|
|
|
|
HJ1499 |
|
AC |
7m0 |
10m9 |
21.5'' |
355° |
2015 |
Vul |
20h18m17.06s |
+25°38'53.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Pale yellow and bluish secondary star, ~6", well separated. I was trying for BU 985 AB but did not see it. |
|
|
|
|
STF2671 |
|
AB |
6m0 |
7m5 |
3.8'' |
337° |
2016 |
Cyg |
20h18m24.76s |
+55°23'49.80" |
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Pretty tight with a clear difference in brightness. I couldn't see anything conspicuous regarding colors. |
|
|
|
|
HO125 |
|
|
6m6 |
10m6 |
3.5'' |
196° |
2008 |
Cyg |
20h18m57.54s |
+39°00'15.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Nice orange carbon star. I do see some faint stars about, but none close enough to be the pair. |
|
|
|
★★
|
BU1206 |
|
AB |
7m5 |
10m7 |
2.2'' |
355° |
2016 |
Cyg |
20h19m07.08s |
+36°45'07.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very much fainter B, ~2", 3-4 delta mag. Pinpoint when seeing stills. |
|
|
|
|
STF2665 |
|
A-BC |
6m9 |
9m6 |
3.3'' |
12° |
2012 |
Del |
20h19m21.16s |
+14°22'14.60" |
René Merting
Drachhausen (Germany) |
100mm (142x) |
bei 107x kann ich Komponente BC ganz schwach im Norden von A erkennen, beide scheinen sich aber noch nicht voneinander lösen zu wollen - bei 142x ist BC in ruhigen Momenten knapp getrennt von A erkennbar - hart |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Wide, white, near equal, one of these has a close faint blue pair |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Nice! Brighter A, white, very close B ~2", orange-red and much fainter. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Main pair wide and reddish color, B about 3x fainter. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
White and light white, ~2 delta mag, ~3". BC is A 1672, 10.10/10.80, currently 0.1" but at 0.2" at discovery in 1907 -- no orbit given so don't know when this will separate to detectability again |
|
|
|
|
H5 87, sigma Cap, 7 Cap |
|
|
5m4 |
9m4 |
56.0'' |
180° |
2019 |
Cap |
20h19m23.60s |
-19°07'06.70" |
René Merting
Drachhausen (Germany) |
12x50 |
Komponente B zeigt sich südlich ziemlich weit abgesetzt von A ganz schwach - A ist so gleißend, dass man B schnell übersehen könnte |
|
|
|
|
STF2664 |
|
|
8m1 |
8m3 |
27.8'' |
322° |
2019 |
Del |
20h19m38.48s |
+13°00'17.20" |
René Merting
Drachhausen (Germany) |
10x50 |
zwei gleich helle Sterne in Südost-Nordwest-Ausrichtung - Trennung eindeutig, aber sehr knapp |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-08-19: Well separated with a clear, but not too wide separation. Slightly different in color, with the southern component appearing slightly cooler. Beautiful surrounding field. |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2021-09-02: Quite conspicuous as a double star, moderately bright with very little difference in brightness. Slightly orange & white-bluish. |
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x sehr weit getrennt - trotz der großen Trennung auffällig, da kaum weitere Sterne im unmittelbaren Umfeld stehen - Komponente B im NW ist nicht viel schwächer als A - zurück auf 20x ist der Abstand zwischen beiden Sternen immer noch sehr groß |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Wide, white, slight magnitude difference |
|
|
|
|
A1673 |
|
|
9m9 |
10m8 |
1.0'' |
55° |
2007 |
Del |
20h19m40.14s |
+15°21'31.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Finely split, ~1 delta mag, white stars |
|
|
|
★★★
|
BLL49, U Cyg |
|
|
8m0 |
9m0 |
65.4'' |
231° |
2015 |
Cyg |
20h19m41.66s |
+47°54'19.90" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-07-03: Easy split with very good color contrast: white and clear orange. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (28x) |
2019-08-22: While the primary component appears quite unspectacular in a white, the companion U Cygni is much more interesting. It is a carbon star whose brightness varies between 5m9 and 12m1 with a period of about 463 days. It appears in mostly intensely orange, and even deep red in the towards its minimum. Extremely rewarding! |
|
|
|
|
STTA205 |
|
|
7m2 |
8m9 |
45.5'' |
321° |
2018 |
Cyg |
20h19m44.88s |
+41°08'18.70" |
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x ein weit getrenntes Pärchen - Komponente B im NW ist gut 2 Größenklassen schwächer |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wide 1 delta mag white. |
|
|
|
|
HU359 |
|
|
10m1 |
10m1 |
0.2'' |
215° |
1969 |
Sge |
20h20m02.08s |
+18°48'19.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Elongation at 667x & 1067x, need best focus and seeing |
|
|
|
|
A1427 & STF2668 |
A1427 |
AB |
6m6 |
8m2 |
0.3'' |
130° |
2008 |
Cyg |
20h20m15.22s |
+39°24'11.80" |
|
|
|
STF2668 |
AB-C |
6m3 |
8m5 |
3.5'' |
280° |
2016 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
STF2668 (AB-C): bei 64x klebt Komponente C ganz dicht westlich an AB - Helligkeitsunterschied gut 2.5 Größenklassen - bei 107x sind beide Sterne eindeutig knapp getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF2668 (AB-C): White and reddish-brown B, ~3 delta mag., 2" or so. |
|
|
|
|
HEI275 |
|
|
10m6 |
10m4 |
0.3'' |
92° |
1995 |
Del |
20h20m49.74s |
+13°27'13.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (553x) |
Very fine but definite split, near equal, white. Discovered by W.D. Heintz in 1984 with the Swarthmore College 61-cm refractor. Only four observations in WDS so no firm orbit has been determined |
|
|
|
|
STFA52, beta Cap, beta 1/2 Cap, 9 Cap, Dabih |
|
AB |
3m1 |
6m1 |
205.4'' |
267° |
2012 |
Cap |
20h21m00.67s |
-14°46'53.00" |
|
|
|
|
AC |
3m1 |
8m8 |
226.1'' |
133° |
2012 |
|
|
|
|
|
|
|
BC |
6m1 |
8m8 |
396.5'' |
111° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: beide Sterne sind halb so weit getrennt, wie die Komponenten von Alpha Cap (STFA 51), Abstand aber immernoch riesig - B ist deutlich schwächer, schätzungsweise 2.5 Magnituden - B wirkt grau gegen die leicht gelb schimmernde A-Komponente |
|
|
|
★
|
COU327 |
|
AB |
9m1 |
9m1 |
0.2'' |
245° |
2019 |
Del |
20h21m35.69s |
+19°29'40.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
The AB-C pair is easy at 205x, C is a faint star ~4" separated from bright A (8.41/11.97 4.0"). AB is much more difficult. At 1067x it is mostly overlapping disks & I can tell its orientation. But at repeated best moments, I get an instant of the finest hairline split with noticeable magnitude difference & I can estimate an orientation relative to nearby stars. It's PA [246°] is nearly perpendicular to AB-C [131°] -- this is how I confirmed I have it. Cocteau discovered it in 1968 with the Nice 30-inch refractor at 0.2". 42.46 year period, last observation in 2005, with grade 3 orbit (which is certain but not definitive). It is currently coming off apastron with the current orbital solution at 0.167" separation. It will tighten very rapidly the next few years, but even on the opposite side of it's orbit it will not be detectable by me, I need to wait until 2050 to try again -- but since the PA will be similar I won't notice that change. I can only look forward to the tightening and maybe detectability again. If is the 0.167" is correct I have exceeded the Raleigh, Dawes, and Sparrow criteria and it's a new personal best -- and given I did not split some similar pairs later in the night, I was very lucky with the seeing at the time of the observation |
|
|
|
|
COU124 |
|
|
8m7 |
13m0 |
3.8'' |
26° |
2015 |
Vul |
20h22m06.04s |
+22°47'12.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Faint star and maybe see B with averted vision, but not certain, could be too faint for my light polluted location |
|
|
|
★
|
STF2673 |
|
AB |
8m3 |
9m8 |
2.4'' |
326° |
2016 |
Del |
20h22m43.76s |
+13°20'25.40" |
|
|
|
|
AC |
8m3 |
8m6 |
76.5'' |
100° |
2016 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
AB: bei 107x wird Komponente B nordwestlich von A blickweise sichtbar, noch nicht ganz getrennt die beiden - 142x reicht dann aber, um B sauber von A zu trennen - Helligkeitsunterschied eine Größenklasse (1.5 Größenklassen laut Stelle Doppie) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Faint but well-split, ~3 disk separation. B ~2 magnitudes fainter. A is blue-green, B reddish. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB: Bright white stars, ~2 delta mag, ~2" separation |
|
|
|
★
|
STF2681 |
|
AB |
8m0 |
10m6 |
6.8'' |
39° |
2015 |
Cyg |
20h22m49.54s |
+53°25'02.80" |
|
|
|
|
AC |
8m0 |
8m9 |
38.2'' |
199° |
2015 |
|
|
|
|
|
|
|
AD |
8m0 |
11m8 |
42.0'' |
166° |
2015 |
|
|
|
|
|
|
|
CD |
8m9 |
11m8 |
23.3'' |
101° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x gut getrenntes Pärchen, Komponente A nördlich strahlt doppelt so hell wie B im Süden, auf C nicht geachtet |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Nice. 3x fainter B, ~4", another wide pair below. (4 stars in system.) |
|
|
|
|
STF2676 & ARN50 |
STF2676 |
AB |
8m3 |
10m0 |
3.0'' |
170° |
2016 |
Vul |
20h22m51.41s |
+27°07'54.50" |
|
|
|
ARN50 |
AC |
8m3 |
8m8 |
84.8'' |
331° |
2015 |
|
|
|
|
|
|
ARN50 |
AD |
8m3 |
9m1 |
65.2'' |
318° |
2015 |
|
|
|
|
|
|
ARN50 |
CD |
8m8 |
9m1 |
25.9'' |
186° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
STF2676 (AB): Komponente C zeigt sich gut abgesetzt im NW von A - Helligkeitsunterschied enorm, mindestens 3 Größenklassen |
|
|
|
|
STTA206 & SEI1107 |
STTA206 |
AB |
6m7 |
8m6 |
43.7'' |
255° |
2019 |
Cyg |
20h22m57.65s |
+39°12'39.70" |
|
|
|
STTA206 |
AD |
6m7 |
11m0 |
24.5'' |
260° |
2019 |
|
|
|
|
|
|
SEI1107 |
BC |
8m6 |
10m6 |
19.3'' |
69° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
STTA206 (AB): ein auffallendes, gut getrenntes Sternpaar - A ist sehr hell, B erscheint durch den Helligkeitsunterschied graubraun |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STTA206 (AB): bei 32x ein weit getrenntes Pärchen mit schönem Farbkontrast - Komponente A weiß, Komponente B dunkelgrau-orange - die Vergrößerung runter auf 20x zeigen sich beide Protagonisten noch immer weit getrennt, B wirkt jetzt aber nicht mehr farbig, sondern nur noch dunkler |
|
|
|
★
|
A288 |
|
|
8m7 |
9m0 |
0.2'' |
279° |
2006 |
Del |
20h23m08.98s |
+20°51'51.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Hairline split, noticeable mag difference, white. Very fine pair. 163y period, it won't make an appreciable change in my time, though it will widen to the 1901 discovery separation of 0.3" in 2075 |
|
|
|
|
BU443 |
|
AB |
7m3 |
11m0 |
16.7'' |
151° |
2015 |
Vul |
20h24m09.01s |
+29°00'07.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint star, wide. There are two more stars in nearly the same PA, likely a system |
|
|
|
★
|
HO457 |
|
AB |
9m1 |
9m2 |
2.0'' |
61° |
2018 |
Vul |
20h24m21.08s |
+29°22'55.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice! quite a pair. Equal stars, well separated ~2", white stars. [AC 14th mag and wide not seen] |
|
|
|
|
STF2679 |
|
AB |
7m9 |
9m7 |
24.7'' |
77° |
2019 |
Del |
20h24m22.59s |
+19°34'30.00" |
|
|
|
|
AC |
7m9 |
11m6 |
38.6'' |
150° |
2017 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
AB: 2021-09-02: Easy to separate with still moderate separation and rather large difference in brightness. Located in a star rich field. |
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
AB: Sichtung unsicher |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ist Komponente B im Osten von A relativ weit getrennt erkennbar - Komponente B ist sehr schwach und gut 1.5 Magnituden schwächer als A - zurück auf 20x ist B nur noch ganz knapp erkennbar, aber weiterhin mit ordentlichem Abstand zu A |
|
|
|
|
HU1198 |
|
|
8m5 |
10m0 |
0.6'' |
33° |
2016 |
Del |
20h24m23.10s |
+13°00'35.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very finely split at 333x, obvious at 533x, significant magnitude difference |
|
|
|
|
COU125 |
|
|
7m3 |
8m9 |
0.4'' |
117° |
2007 |
Vul |
20h24m25.79s |
+24°16'39.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Orange-yellow star, not exactly round, marginal |
|
|
|
★
|
WOR33 & A1209 |
WOR33 |
Aa-Ab |
8m6 |
9m3 |
0.6'' |
131° |
2016 |
Del |
20h24m26.64s |
+12°12'44.80" |
|
|
|
A1209 |
AB |
9m2 |
10m6 |
1.9'' |
324° |
2016 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
A1209 (AB): Very cool! A is obviously split with a At the opposite side is the wider fainter companion, which is A 1209 AB. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
WOR33 (Aa-Ab): ~1 delta white companion <1" from the A star of A1209 AB. WOR 33 was 0.3" at discovery in 1970 and it has widened very considerably since, so this might be "only" a high proper motion star.* C.E. Worley was a well loved astronomer at the US Naval Observatory |
|
|
|
|
J841 |
|
AB |
10m4 |
11m4 |
0.2'' |
274° |
1949 |
Del |
20h24m56.07s |
+13°08'58.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy wide near equal pair. Unfortunately I did not check the details of this one. There's an AB-C pair 10.4.0/11.40 0.2" which I didn't realize was there to go after -- in any case I didn't notice anything unusual with the disk at 333x |
|
|
|
|
TDS1072 |
|
|
11m5 |
11m6 |
0.9'' |
161° |
2015 |
Del |
20h24m59.46s |
+15°31'52.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very fine split, faint, near equal pair, ~1". Two observations since discovery in 1991 |
|
|
|
|
D22 |
|
AB |
8m2 |
9m5 |
2.9'' |
163° |
2016 |
Cyg |
20h25m31.16s |
+40°05'50.80" |
|
|
|
|
AC |
8m2 |
13m2 |
18.1'' |
114° |
1998 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 64x ist Komponente B südlich von A wahrnehmbar, beide können sich noch nicht voneinander lösen - bei 107x dann ist eine knappe Trennung in ruhigen Momenten möglich - B ist halb so hell wie A, also eine Größenklasse Unterschied |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Yellow and yellow-orange, ~3" 1 delta mag, among a pentagram of stars which may be additional pairings. |
|
|
|
★
|
STF2687 |
|
|
6m4 |
8m3 |
25.1'' |
118° |
2019 |
Cyg |
20h26m23.47s |
+56°38'19.30" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-08-19: Gorgeous sight, separated with distinct brightness difference. Primary component appeared rather white with a greyish companion. With two similarly bright stars to the east and southeast STF 2687 forms a prominent triangle surrounded by several star chains. About 12 arcminutes apart to the southeast of STF 2687 is another pair of stars, which is particularly striking because of its color (bluish & orange). |
|
|
|
|
BU60, pi Cap |
|
AB |
5m1 |
8m5 |
3.6'' |
149° |
2016 |
Cap |
20h27m19.20s |
-18°12'42.10" |
Uwe Pilz
Leipzig (Germany) |
80mm (198x) |
Aufhellung im ersten Ring |
|
|
|
|
S749 |
|
AB |
6m8 |
7m5 |
60.1'' |
189° |
2019 |
Aql |
20h27m27.56s |
-02°06'10.50" |
|
|
|
|
AC |
6m8 |
11m3 |
45.3'' |
329° |
2015 |
|
|
|
|
|
|
|
AD |
6m8 |
12m4 |
90.4'' |
269° |
2015 |
|
|
|
|
|
|
|
CD |
10m8 |
11m0 |
78.1'' |
239° |
2015 |
|
|
|
|
|
|
|
CE |
10m8 |
13m7 |
18.9'' |
198° |
2015 |
|
|
|
|
|
|
|
DF |
11m0 |
13m6 |
5.8'' |
26° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: zwei relativ helle Sterne in Nordsüd-Ausrichtung, komfortabel getrennt - B im Süden ist eine halbe Größenklasse schwächer und blaugrau ggü. der weißen A-Komponente |
|
|
|
|
BRT1343 |
|
|
11m0 |
11m0 |
4.5'' |
335° |
2015 |
Del |
20h27m30.17s |
+14°56'28.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy near equal wide |
|
|
|
|
AG256 |
|
AB |
9m4 |
10m6 |
5.2'' |
351° |
2018 |
Del |
20h27m55.81s |
+09°57'34.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
White A and slightly brown-red B, ~1 delta, wide |
|
|
|
★★
|
HO131 |
|
AB |
7m0 |
10m6 |
3.4'' |
334° |
2015 |
Del |
20h28m18.64s |
+18°46'10.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Seeing needed to be perfectly still so that A's diffraction disappeared. Then B would emerge from the dark as a very faint point to the NW, about 3 disks away. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Bright light yellow A and ~3 delta mag yellow B, ~3" |
|
|
|
|
rho Cap, 11 Cap |
SHJ323 |
AB |
5m0 |
6m9 |
1.7'' |
190° |
2018 |
Cap |
20h28m51.62s |
-17°48'49.20" |
|
|
|
BU61 |
AC |
5m0 |
13m3 |
53.5'' |
149° |
2015 |
|
|
|
|
|
|
SHJ323 |
AD |
5m0 |
6m7 |
258.7'' |
150° |
2011 |
|
|
|
|
|
|
BU61 |
BC |
6m9 |
12m5 |
53.5'' |
149° |
2015 |
|
|
|
|
|
|
DOB13 |
DE |
6m7 |
10m6 |
54.3'' |
96° |
1999 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AD: einfach, ein helles, weit auseinander stehendes Paar - Komponente B im SO ist gut 1.5 Magnituden schwächer und wirkt grau ggü. der weiß strahlenden Komponente A |
|
|
|
|
A610 |
|
|
9m5 |
9m9 |
0.5'' |
93° |
2018 |
Del |
20h29m02.58s |
+07°09'29.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very finely split, white near equal, nice. 170.62y period, will make less than a quarter turn the next couple of decades. |
|
|
|
★★
|
WEI35 |
|
AB |
8m3 |
8m8 |
4.0'' |
214° |
2018 |
Cyg |
20h29m13.54s |
+37°30'45.80" |
|
|
|
|
AC |
8m3 |
9m4 |
87.6'' |
100° |
2015 |
|
|
|
|
|
|
|
CD |
9m4 |
10m6 |
12.1'' |
202° |
2018 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
AB: bei 64x ist ein schön eng stehendes Paar zweier schwacher Sterne erkennbar - Komponente B im SW schwächelt helligkeitstechnisch nur um eine halbe Magnitude gegenüber A - Komponente A wirkt leicht farbig, das aber ist nicht greifbar |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
eine anderer doppelter Doppelstern! Lohnend! Es ist erstaunlich, dass er nicht in den klassischen Katalogen auftaucht |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Double-double! Near equal 3", and closeby a wider pair, 5", 1 delta mag. (AB is first, CD might be second? 4 stars visible in system) |
|
|
|
|
STF2691 |
|
|
8m1 |
8m4 |
16.3'' |
32° |
2019 |
Cyg |
20h29m43.18s |
+38°07'31.50" |
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-08-19: Nicely separated and in one field of view together with 40 Cygni and Messier 29. Moderate distance and brightness difference, relatively conspicuous even though the environment is rather rich in stars. |
|
René Merting
Drachhausen (Germany) |
18x70 |
das Paar ist genau richtig für 18-fache Vergrößerung - ein schön isoliert stehendes, knapp getrenntes Sterndoppel zweier gleichheller Protagonisten - Komponente B im NO ist nur unwesentlich schwächer |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
2020-07-29: At 22x clearly separated with little difference in brightness. Colorwise the components appeared different: yellowish-orange & bluish. The color impression was a bit more intensive at 44x: slightly orange & bluish. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x ein schönes knapp getrenntes Pärchen aus zwei schwächeren Sternen - Komponente A im Süden ist nur unwesentlich heller als B - bei 32x leichter Farbkontrast, weil A warm-weiß strahlt |
|
Uwe Pilz
Leipzig (Germany) |
105mm (53x) |
schon bei 22x auffallend |
|
|
|
★
|
omicron Cap, 12 Cap, SHJ324 |
|
AB |
5m9 |
6m7 |
22.0'' |
239° |
2019 |
Cap |
20h29m53.91s |
-18°34'59.40" |
René Merting
Drachhausen (Germany) |
12x50 |
ein dicht zusammenstehendes, gut getrenntes Paar, beide Komponenten sind schön hell - die Komponente B im SW ist eine halbe Größenklasse schwächer |
|
|
|
|
HJ1525 |
|
AB |
9m1 |
9m6 |
9.2'' |
234° |
2019 |
Cyg |
20h29m54.13s |
+40°22'01.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal wide, 8", white pair. |
|
|
|
|
BU987 & S752 & FOX254 |
BU987 |
AB |
6m8 |
11m1 |
2.5'' |
128° |
2018 |
Del |
20h30m14.44s |
+19°25'15.70" |
|
|
|
S752 |
AC |
6m8 |
7m3 |
106.3'' |
288° |
2015 |
|
|
|
|
|
|
FOX254 |
AE |
6m8 |
13m0 |
21.2'' |
70° |
2013 |
|
|
|
|
|
|
FOX254 |
CD |
7m3 |
15m3 |
35.0'' |
301° |
2015 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
S752 (AC): Widely separated white, near equal brightness. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
BU987 (AB): Bright white A and much fainter B, ~3 delta mag & ~3" separation. Discovered in 1880 with the Dearborn 18.5-inch at 2.32" |
|
|
|
★
|
BU63, 1 Del |
|
AB |
6m2 |
8m0 |
0.9'' |
347° |
2016 |
Del |
20h30m17.95s |
+10°53'45.30" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
1 Delphini: 1 disk split to the NNW when seeing stills. A tough observation. 1 Del is a fascinating star that spins once in 0.9 earth days! See http://stars.astro.illinois.edu/sow/1del.html. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
1 Del. B seen within A's diffraction at 533x and apodising mask, <1", ~2 delta |
|
|
|
|
AG408 |
|
|
9m3 |
10m8 |
5.1'' |
285° |
2018 |
Del |
20h30m36.26s |
+14°04'09.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy wide, ~2 delta. Not physical |
|
|
|
|
STF2688 |
|
|
9m3 |
10m4 |
7.9'' |
175° |
2019 |
Del |
20h30m48.26s |
+13°47'02.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Gold A and blue B, half delta mag. Very like Albireo, and like Albireo it is not physical |
|
|
|
|
S755 |
|
AB |
6m6 |
9m7 |
59.9'' |
278° |
2015 |
Cyg |
20h30m52.72s |
+49°12'47.50" |
René Merting
Drachhausen (Germany) |
18x70 |
ein sehr weit auseinander stehendes Sternpaar und sehr ungleich - viele helle Sterne im Umfeld lenken stark von diesem Paar ab - B im Westen ist so schwach, dass der Größenklassenunterschied nicht abschätzbar ist - ein Doppelstern für Puristen |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x weit getrennt und großer Helligkeitsunterschied, bestimmt 3.5 bis 4 Größenklassen, das macht aber auch ein wenig den Reiz dieses Pärchens aus - A strahlt weiß, B ist mausgrau - zurück auf 20x ist Komponente B noch knapp erkennbar |
|
|
|
★
|
STF2690 & HJ269 & DA1 |
STF2690 |
A-BC |
7m1 |
7m4 |
17.8'' |
255° |
2019 |
Del |
20h31m11.94s |
+11°15'33.70" |
|
|
|
HJ269 |
AD |
7m1 |
12m1 |
23.0'' |
108° |
2016 |
|
|
|
|
|
|
DA1 |
BC |
7m9 |
8m0 |
0.3'' |
184° |
2016 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
10x50 |
STF2690 (A-BC): ein ganz enges Sternpaar mit zwei gleich hellen Sternen - ich würde beide als 8 mit tiefer Einschnürung bezeichnen, also kurz vor der Trennung |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
STF2690 (A-BC): 2020-08-19: Striking, moderately bright with nice separation of the similarly bright components in nice environment. The eastern component seemed slightly brighter and colorwise cooler. |
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
STF2690 (A-BC) |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STF2690 (A-BC): bei 32x ein schön getrenntes Sternpaar mit leichtem Farbkontrast - Komponente A im Osten ist weiß, BC im Westen ist leicht gelblich und dumpfer, aber kaum ein Helligkeitsunterschied zwischen beiden Sternen - zurück auf 20x ist das Paar noch schöner anzusehen, weil beide Sterne dichter zusammen stehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF2690 (A-BC): Widely separated near equal white stars. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
DA1 (BC): This is part of STF 2690 A-BC, which is a white, wide, near equal, pair (7.12/7.39 17.7") observed with 8-inch at 205x. I suspected BC at 8-inch 333x, & had overlapping disks with 8-inch 533x. With 20-inch 533x I see a hairline split, slight magnitude difference. Seeing is not supporting it well, but it's clear. Very nice. Dawes discovered in 1840 at 0.7" -- probably with his 8-inch Cooke refractor -- so at current 0.369" it's not surprising I only had overlapping disks at 8-inch. It's a physical pair, with a 236.52 year period, and will widen another 0.1" in the next 15 years |
|
|
|
|
J3 |
|
|
11m9 |
12m1 |
2.1'' |
130° |
2013 |
Del |
20h31m33.39s |
+11°50'24.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Faint, ~2 separated, noticeable mag difference |
|
|
|
★
|
STF2695 |
|
|
6m6 |
8m8 |
0.4'' |
259° |
2016 |
Vul |
20h31m58.19s |
+25°48'18.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Using 8" mask at 667x, no sign of elongation. With 20" and progressively higher magnifications, I can get to olive shape at 1067x, but extremely marginal. [0.8" at discovery, so easier for Struve] |
|
|
|
|
A1677 |
|
|
8m1 |
10m9 |
1.3'' |
184° |
2016 |
Del |
20h32m07.67s |
+15°11'12.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
B plainly visible, pale yellow to bright white A, ~2 delta mag, ~1" |
|
|
|
|
ROE13 |
|
|
10m0 |
12m0 |
6.4'' |
41° |
2015 |
Vul |
20h32m23.61s |
+22°26'02.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Nice wide pair two delta mag white stars. |
|
|
|
|
J1 |
|
AB |
10m0 |
10m6 |
1.9'' |
58° |
2018 |
Del |
20h32m52.76s |
+11°44'37.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Nice close pair, well split ~2", equal. Physical, at apastron, 528.391 year period (to be exact!) |
|
|
|
|
BU670 |
|
AB |
9m4 |
9m9 |
0.8'' |
5° |
2016 |
Del |
20h32m55.22s |
+13°56'40.00" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Nicely split, noticeable magnitude difference, <1" |
|
|
|
|
STF2698 |
|
|
8m7 |
9m1 |
4.5'' |
304° |
2017 |
Vul |
20h33m45.57s |
+28°07'34.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
One delta mag wide pair. |
|
|
|
|
WRH34, 47 Cyg |
|
AB |
4m8 |
7m3 |
0.3'' |
278° |
1998 |
Cyg |
20h33m54.19s |
+35°15'03.10" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
47 Cyg: Carbon yellow-orange disk, sense it is not round. Marginal. |
|
|
|
★
|
STT408 |
|
|
6m8 |
9m4 |
1.6'' |
193° |
2009 |
Cyg |
20h34m01.96s |
+34°40'44.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very fine dull white A and pinpoint B, split well with seeing, ~2" |
|
|
|
|
BU1208 |
|
|
7m0 |
11m0 |
3.1'' |
332° |
2005 |
Del |
20h34m31.81s |
+06°52'41.10" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
With apodising mask to suppress bright white A's brightness, and with foveal coaxing due to its very faintness, B emerges into view ~3", a very small fine point. Likely tougher than it should have been due to the sky haze -- indeed after seeing it as above, when I went back down to 333x I could see B direct vision, knowing where and what to look for. Discovered with the Lick 36-inch in 1890 at 2.94" |
|
|
|
|
STF2700 |
|
|
7m0 |
8m8 |
24.1'' |
285° |
2019 |
Cyg |
20h34m44.60s |
+32°30'21.10" |
René Merting
Drachhausen (Germany) |
18x70 |
das interessanteste Sternpaar innerhalb der Region um 48 Cyg und Ary 48 - ein getrenntes, aber schönes enges Double - Komponente B im Westen ist gut 2 Größenklassen schwächer |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x steht B in ordentlichem Abstand zu A im Westen und ist gut 1.5 bis 2 Größenklassen schwächer - Komponente A gelblich, B dagegen wirkt weiß-grau - zurück auf 20x ist die Trennung weiterhin leicht, B ist gut erkennbar |
|
|
|
★
|
COU223 |
|
|
11m1 |
11m2 |
0.4'' |
155° |
2008 |
Del |
20h34m46.33s |
+17°25'38.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Elongation with 333x, very finely split with 533x, wider split with 667x. Very faint, more than just a little delta mag., slightly orange stars |
|
|
|
|
TDT2394 |
|
|
9m2 |
9m5 |
0.5'' |
3° |
2011 |
Del |
20h34m54.35s |
+11°20'13.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Hairline split, considerable magnitude difference |
|
|
|
|
STF2702 |
|
|
8m7 |
9m0 |
3.1'' |
208° |
2018 |
Cyg |
20h35m34.94s |
+35°10'10.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fine near equal, well split 4" |
|
|
|
★
|
A2793 |
|
|
9m9 |
10m3 |
0.9'' |
210° |
2016 |
Vul |
20h36m29.63s |
+23°41'43.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Nice! very fine pair, white stars, half delta mag, close, ~1" |
|
|
|
|
AG258 |
|
|
9m3 |
10m0 |
4.2'' |
11° |
2017 |
Del |
20h36m37.44s |
+10°27'03.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
White, wide, half delta mag. |
|
|
|
★★
|
STF2703 |
|
AB |
8m3 |
8m4 |
25.1'' |
290° |
2019 |
Del |
20h36m49.41s |
+14°43'42.40" |
|
|
|
|
AC |
8m3 |
8m8 |
77.8'' |
234° |
2016 |
|
|
|
|
|
|
|
AD |
8m3 |
12m8 |
84.7'' |
347° |
2016 |
|
|
|
|
|
|
|
BC |
8m4 |
8m8 |
67.0'' |
215° |
2016 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2020-08-19: Immediately eye-catching multiple star located between beta and zeta Delphini. Components A, B & C are very easily seen as a triple system forming a striking triangle. A very slight difference in brightness between A & B is perceptible, as well as a color difference, though I cannot name any colors. Very nice. |
|
Uwe Pilz
Leipzig (Germany) |
16x70 |
AB |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 20x einfach - Komponente B im Westen ist nur minimal schwächer
BC: bei 20x ist Komponente C südwestlich von B in mehr als dem doppeltem Abstand von A zu B erkennbar, Helligkeitsunterschied gut eine halbe Größenklasse |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
AB |
|
|
|
|
STF2701 |
|
|
8m3 |
8m6 |
2.1'' |
221° |
2016 |
Del |
20h36m58.85s |
+12°02'55.30" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x ist Komponente B südwestlich von A erkennbar, beide Sterne berühren sich noch, aber die Einschnürung ist schon deutlich - bei 107x dann sind beide Sterne knapp getrennt sichtbar - Komponente B ist eine knappe halbe Magnitude schwächer |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Well split orange-yellow pair, A ~1x brighter. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
White, near equal, well separated |
|
|
|
|
A1680 |
|
|
9m0 |
12m2 |
3.8'' |
295° |
2015 |
Del |
20h37m12.89s |
+12°49'41.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Light yellow A and faint ~3 delta mag blue B, wide ~4". Not physical |
|
|
|
|
HEI7, VW Cep |
|
|
7m7 |
10m5 |
0.7'' |
231° |
2007 |
Cep |
20h37m21.54s |
+75°36'01.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Just glimpsed a speck in the diffraction ring when seeing stills, marginal |
|
|
|
|
HEI586 |
|
|
10m3 |
10m2 |
0.5'' |
222° |
1994 |
Del |
20h37m29.88s |
+10°49'43.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Split, near equal, white |
|
|
|
|
STFA53, 48 Cyg |
|
AB |
6m3 |
6m5 |
182.7'' |
177° |
2012 |
Cyg |
20h37m31.77s |
+31°34'21.10" |
|
|
|
|
AC |
6m3 |
13m5 |
71.3'' |
0° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AB: ein helles, weit auseinanderstehendes Sternpaar, die südliche Komponente ist nur unwesentlich schwächer - die unmittelbar im Umfeld befindlichen Sterne sind alle schwächer, das Sternpaar hat es trotzdem schwer, als solches zu wirken |
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
AB: bei 29x sind zwei weit auseinander stehende helle Sterne zu erkennen, die im Umfeld aber nicht besonders auffallen - trotz der zwei hellen Komponenten, die zudem nicht einmal physikalisch zusammenhängen, eher unspektakulär |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: 48 Cygni: Wide equal pair, easy in 80mm finder |
|
|
|
|
BU151, bet Del |
|
AB |
4m1 |
5m0 |
0.2'' |
218° |
2018 |
Del |
20h37m32.87s |
+14°35'42.70" |
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Rotanev, Beta Delphinus. Best I can get is a slight snowman, with and without apodising mask. 26.68y period. Burnham discovered at 0.7" in his 6-inch in August 1873, and when compiling his catalog in 1899 noted it had made substantially one revolution. This will widen through this decade and should be resolvable in a few years, getting back to ~0.7" in 2030 |
|
|
|
|
STF2705 |
|
AB |
7m5 |
8m5 |
3.1'' |
264° |
2019 |
Cyg |
20h37m44.32s |
+33°21'59.40" |
|
|
|
|
AC |
7m5 |
12m6 |
183.4'' |
341° |
2015 |
|
|
|
|
|
|
|
AD |
7m5 |
12m9 |
54.5'' |
3° |
2015 |
|
|
|
|
|
|
|
AE |
7m5 |
12m4 |
74.2'' |
42° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
AB: bei 64x sind beide Sterne dicht nebeneinander zu sehen, keine 8 mehr, sondern knapp getrennt - Komponente B im Westen ist eine halbe Größenklasse schwächer - bei 107x ist die Trennung dann eindeutig und B zeigt sich doch etwas schwächer, ich denke eine ganze Größenklasse |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Close separation equal reddish. Looks similar to the nearby Ary 48 stars, I wonder if they were formed in the same molecular cloud? |
|
|
|
★★
|
ARY48 |
|
|
8m2 |
8m8 |
53.3'' |
41° |
2016 |
Cyg |
20h37m45.00s |
+32°23'42.90" |
René Merting
Drachhausen (Germany) |
18x70 |
das Paar ist sofort bequem getrennt als solches erkennbar - Komponente B im Osten ist maximal eine halbe Magnitude schwächer |
|
Mark McCarthy
Fremont (California/USA) |
80mm (13x) |
A beautiful split in finder, just equal pair, wide separation, white with red tint. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x zeigt sich B fast gleichhell weit getrennt nordöstlich von A - bei 20x ein kleines schwaches ordentlich getrenntes Pärchen |
|
|
|
|
STF2707 |
|
AB |
7m9 |
9m4 |
21.8'' |
29° |
2015 |
Cyg |
20h37m51.14s |
+47°56'41.90" |
|
|
|
|
AC |
7m9 |
8m6 |
55.3'' |
195° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
AC: ein weit getrenntes Paar mit einem scheinbaren Farbunterschied, C im Süden wirkt leicht grau, A ist weiß - Größenklassenunterschied eine halbe Magnitude - auf B habe ich leider nicht geachtet |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ist Komponente B gut getrennt im NO von A erkennbar - zurück auf 20x stehen beide Sterne richtig schön eng - bei 64x strahlt A rein weiß, B ist grau - noch ein netter Nebeneffekt, nur 37' ost-nordöstlich steht der Veränderliche V Cyg, der schön hell-orange glänzt
AC: bei 32x ist Komponente C weit getrennt im Süden von A erkennbar - Abstand gut 3x so weit wie AB - bei 64x strahlt A reinweiß, C ist braun-grau |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Split in 80mm finder. Ice blue, in a string of five stars (The string of stars comprise other components of the system, AC, AD, BC, which have the same PA of about 195.) |
|
|
|
|
AG260 |
|
|
8m4 |
10m0 |
9.7'' |
219° |
2016 |
Vul |
20h38m09.42s |
+25°10'51.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Yellow and light yellow stars, wide and bright, nice pair |
|
|
|
|
BU1491 |
|
|
8m8 |
11m6 |
3.2'' |
87° |
2002 |
Del |
20h38m15.10s |
+10°43'24.90" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
White A, B appears with foveal coaxing and and then I can hold it direct |
|
|
|
|
BU672, 71 Aql |
|
|
4m4 |
12m0 |
35.8'' |
285° |
2013 |
Aql |
20h38m20.27s |
-01°06'18.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright yellow with very faint, very wide pair. |
|
|
|
★
|
TDT2441 |
|
|
10m6 |
10m6 |
0.6'' |
102° |
1991 |
Vul |
20h38m20.78s |
+21°05'37.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Very difficult and faint B star appears with averted vision, only at the instant seeing settles the A star down to a clean round diffraction. B is a brown hard point on the diffraction ring. very tough. |
|
|
|
|
BU435 |
|
|
8m3 |
10m8 |
3.1'' |
119° |
2010 |
Del |
20h38m50.10s |
+15°00'26.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy white and yellow, wide ~3, ~2 delta mag |
|
|
|
|
SCJ27 |
|
AB |
8m7 |
10m0 |
6.2'' |
263° |
2016 |
Del |
20h39m13.04s |
+10°58'42.00" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
An obvious pair, I wonder why Struve did not note it. Wide, ~6", ~1 delta mag. A is light orange and B a slightly deeper orange. Lies in a dense arrow shaped asterism. Hans Schjellerup was a 19th century Danish astronomer who was something of a polymath, who compiled a list of red stars, and studied Chinese and other languages in order to study old astronomic records |
|
|
|
|
HEI77 |
|
|
10m9 |
10m7 |
1.4'' |
41° |
2015 |
Del |
20h39m15.21s |
+15°31'29.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very fine near equal white pair, really nice |
|
|
|
|
HU362 |
|
|
9m4 |
9m8 |
0.7'' |
312° |
2007 |
Del |
20h39m29.33s |
+18°56'55.30" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Hairline split, white, near equal. Very nice pair |
|
|
|
|
STT410 |
|
AB |
6m7 |
6m8 |
0.9'' |
3° |
2018 |
Cyg |
20h39m33.31s |
+40°34'46.80" |
|
|
|
|
AB-C |
6m8 |
8m7 |
68.6'' |
70° |
2018 |
|
|
|
|
|
|
|
AB-D |
6m8 |
10m0 |
106.6'' |
327° |
2018 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (198x) |
AB: nur mäßig schwierig, Abstand 0“87 |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
AB: nicht getrennt |
|
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
All four components easily visible. The pair AB shows two clear, equally bright, overlapping diffraction disks. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: gleich hell, getrennt |
|
|
|
|
STF2711 |
|
|
8m2 |
9m2 |
2.4'' |
223° |
2016 |
Cyg |
20h39m35.12s |
+30°30'14.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
White, 1 delta mag, 3" |
|
|
|
|
HEI278 |
|
|
11m1 |
11m1 |
3.4'' |
135° |
2015 |
Del |
20h40m31.91s |
+12°40'15.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy wide, near equal |
|
|
|
|
HDS2947 |
|
|
7m3 |
8m1 |
0.2'' |
114° |
2019 |
Del |
20h40m35.25s |
+15°38'35.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
With apodising mask. Not round is best I can say, marginal. Coming off apastron and only getting more difficult. Discovered 1991 by the Hipparcos satellite at 0.2" |
|
|
|
|
HO137 |
|
|
6m1 |
9m3 |
0.7'' |
352° |
2008 |
Cyg |
20h40m36.26s |
+29°48'19.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
At 553x some out of roundness to the disk, but not certain. Used 885x with apodizing mask some lumpiness to dusk but it dances around. Marginal |
|
|
|
|
J191 |
|
|
10m9 |
11m2 |
1.3'' |
167° |
2016 |
Del |
20h40m52.16s |
+17°37'59.20" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Well split, >1", half delta mag, slight color difference of very light blue and orange. Discovered 1895 at 4.5", it has tightened considerably, through binarity is uncertain |
|
|
|
|
STF2713 |
|
|
9m8 |
9m8 |
5.1'' |
63° |
2016 |
Del |
20h40m55.07s |
+10°34'29.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Easy equal white pair, ~5" |
|
|
|
|
STF2716, 49 Cyg |
|
AB |
5m8 |
8m1 |
2.7'' |
44° |
2016 |
Cyg |
20h41m02.54s |
+32°18'26.30" |
|
|
|
|
AC |
5m8 |
12m1 |
67.1'' |
93° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 107x hat die helle leicht gelb-stichige A-Komponente einen schwachen Begleiter im NO, der sich nur in ruhigen Momenten knapp von A befreien kann - Helligkeitsunterschied 2.5 bis 3 Größenklassen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: 49 Cygni: Pretty orange and blue, 1.5-2.0 delta mag, ~2" |
|
|
|
|
STF2715 |
|
|
7m8 |
10m2 |
12.4'' |
2° |
2015 |
Del |
20h41m46.01s |
+12°31'07.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Obvious ~3 delta mag, wide, white. Physical |
|
|
|
★
|
COU226 |
|
AB |
8m0 |
8m3 |
0.4'' |
54° |
2018 |
Del |
20h41m51.24s |
+19°31'13.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Wow really nice 2+1 system. The +1 is a faint wide star (AC, 8.58/11.50, 13.5"). The AB is a very tight double, ~0.5", split, white, near equal |
|
|
|
|
STT411 |
|
AB |
7m7 |
10m6 |
31.8'' |
349° |
2015 |
Cyg |
20h42m20.31s |
+45°49'24.50" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Carbon star with a number of possible pairs. (9 stars in system) |
|
|
|
|
ARG39 |
|
AB |
8m4 |
8m9 |
15.4'' |
184° |
2018 |
Cyg |
20h42m29.79s |
+49°15'59.10" |
René Merting
Drachhausen (Germany) |
18x70 |
ein isoliert stehendes, knapp getrenntes Sternpaar - Komponente B im Süden ist nur unwesentlich schwächer - ein schöner Fernglasprüfer für 15 bis 18-fache Vergrößerung |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x leicht zu trennen - Helligkeitsunterschied zwischen A im Norden und B im Süden eine viertel bis eine halbe Größenklasse - leichter Farbkontrast zwischen beiden Sternen, aber nicht definierbar, beide zusammen haben aber eine andere Farbe als die Sterne im Umfeld - zurück auf 20x zeigt sich ein dicht stehendes getrenntes Pärchen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wide separation, red-yellow pair. (7 visible stars in complex pattern.) |
|
|
|
★
|
STF2718 |
|
AB |
8m3 |
8m4 |
8.6'' |
88° |
2015 |
Del |
20h42m33.47s |
+12°43'41.90" |
|
|
|
|
AC |
8m3 |
9m0 |
167.2'' |
346° |
2015 |
|
|
|
|
|
|
|
BC |
8m4 |
9m0 |
167.3'' |
346° |
2015 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
AB: 2021-09-02: Appears elongated at first glance, on closer observation just separable. A very small difference in brightness is visible. The double star is located in a beautiful surrounding field of stars. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: der Doppelstern steht sehenswert in einem Bogen aus 5 Sternen - bei 32x werden zwei gleich helle knapp getrennte Sterne sichtbar - schwer zu sagen, welches die A-Komponente ist - die westliche Komponente wirkt im Weiß-Farbton etwas kühler |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Easy wide, white, near equal Psychical |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Same brightness white pair. |
|
|
|
|
STF2720 |
|
|
9m2 |
9m6 |
4.0'' |
178° |
2016 |
Del |
20h43m27.91s |
+16°56'41.90" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Fine pair, near equal, wide ~5", white |
|
|
|
|
STF2721 |
|
|
7m8 |
9m9 |
2.6'' |
22° |
2016 |
Del |
20h43m29.80s |
+19°52'52.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Well split ~3", ~2 delta mag |
|
|
|
|
STF2722 |
|
|
8m3 |
8m9 |
7.4'' |
306° |
2016 |
Del |
20h43m38.82s |
+19°43'40.70" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x zeigt sich Komponente B nordwestlich von A knapp getrennt - Helligkeitsunterschied eine halbe Größenklasse |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wide split and nearly equal magnitude. Can squeeze this into same FOV with STF 2721 edge to edge. |
|
|
|
|
STF2724 |
|
|
9m0 |
9m0 |
2.6'' |
150° |
2016 |
Vul |
20h44m28.01s |
+23°56'00.20" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fine, near equal, 2" |
|
|
|
|
STF2723 |
|
AB |
7m0 |
8m3 |
1.0'' |
140° |
2018 |
Del |
20h44m54.58s |
+12°18'45.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Very nice, light blue A and light yellow B, fine split, almost 2 delta mag. Really nice pair |
|
|
|
★★
|
52 Cyg, STF2726 |
|
|
4m3 |
9m5 |
5.9'' |
72° |
2018 |
Cyg |
20h45m39.76s |
+30°43'10.80" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x strahlt A gleißend und hellgelb, Komponente B ist östlich von A schön abgesetzt sehr schwach erkennbar - Helligkeitsunterschied riesig, bestimmt mehr als 4 Größenklassen (5.2 mag laut Stelle Doppie) - zurück auf 64x ist Komponente B nur in ruhigen Momenten zu erhaschen, der Stern klebt förmlich am hellen Strahlenkranz von A |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
52 Cygni: I sight this one by eye to find the Western Veil in the Telrad. Bright orange and 3 delta mag blue B, ~7" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
ES30, RR Cyg |
|
|
9m6 |
12m5 |
17.1'' |
57° |
2015 |
Cyg |
20h46m04.55s |
+44°52'09.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very wide with a very faint B, off to the side. |
|
|
|
★★
|
STF2725 |
|
AB |
7m5 |
8m2 |
6.1'' |
12° |
2018 |
Del |
20h46m13.31s |
+15°54'26.40" |
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2021-09-02: The double star appears clearly elongated at the correct position angle, but nothing more. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein schöner Kontrast zum 15' nördlich stehenden viel helleren Sternpaar STF2727 - hier bei dem wesentlich schwächeren Sternpaar zeigt sich bei 32x die Komponente B knapp getrennt nördlich von A - Helligkeitsunterschied etwas mehr als eine halbe Magnitude, aber Komponente A ist noch deutlich schwächer als die Komponente B von STF2727 |
|
Sarah Gebauer
Germany |
100mm (45x) |
das Doppel lässt sich bei 45x sauber trennen und bildet mit Gamma2 Delphini ein optisches Doppel-Doppel, da beide Doppelsterne sehr gut in ein Gesichtsfeld passen |
|
Uwe Pilz
Leipzig (Germany) |
105mm (66x) |
im selben Feld mit gamma Del |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
OR Del. Light yellow stars, half delta mag, wide. Physical pair with a 2945.18 year period. In same field with bright pair STF 2727 |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Super wide, 1 magnitude difference, both faint yellow-white. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Easy, half delta mag and wide. I was after the super close WSI 110 Aa-Ab 0.1" but had no hope of seeing it. |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
close DS |
|
|
|
★★
|
STF2727, 12 Del, gamma Del |
|
AB |
4m4 |
5m0 |
8.9'' |
265° |
2019 |
Del |
20h46m39.50s |
+16°07'27.40" |
|
|
Christopher Hay
Seeheim (Germany) |
8x42 |
On tripod. Definite elongation, and eastern end of elongation (i.e. component A) is definitely brighter than the other end. PA estimated at 240° without prior knowledge. |
|
Christopher Hay
Seeheim (Germany) |
15x45 |
Stabilised binoculars, handheld. A very elongated figure-8 very close to popping apart. According to Stelledoppie a physical double with a period of 3249 years. Observed in June 2019 when separation was 8,89“. Will be 8.67“ in 2030 according to Stelledoppie. |
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
2021-09-02: Beautiful sight in very nice surrounding. Easy to split, but quite small separation. A rather small difference in brightness is clearly visible. The primary component appears golden in color. |
|
Christopher Hay
Seeheim (Germany) |
18x80 |
Very tight pair but clearly split with black in-between. Observed in July 2019 when separation was 8,89“. An excellent object to test the resolution of large binoculars. Struve 2725 a few arcminutes to the southwest is a further good test object for magnifications >20x. |
|
Christopher Hay
Seeheim (Germany) |
40x80 |
Widely split, visually strong, dominating the field of view. Component A appears yellowish compared to component B. Struve 2725 in same FOV finely split. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x knapp getrennt - Komponente A ist schön gelb, B im Westen ist gut 1.5 Magnituden schwächer (lt. Stelle Doppie Helligkeitsunterschied nur 0.67 mag) - zusammen mit dem wesentlich schwächeren STF2725 gut 15' südlich sehenswert |
|
Sarah Gebauer
Germany |
100mm (45x) |
bei 45x sauber getrennt und zusammen mit dem DS STF 2725 in einem Gesichtsfeld, dadurch wirken sie wie ein optisches Doppel-Doppel, sehr schön! Beide DS bilden auch einen auffälligen Lichthof |
|
Uwe Pilz
Leipzig (Germany) |
105mm (66x) |
im selben Feld mit STF2725 |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
schon trennbar bei 26x. In einem Feld mit STF2725 |
|
Mark McCarthy
Fremont (California/USA) |
152mm (285x) |
Gam 2 Del. ! Most beautiful light orange-yellow A and ~1 delta mag blue-green B |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Gamma Delphinus. Rich gold-yellow A, blue-white B, ~6" separation estimated by eye. Very pretty pair. |
|
|
|
|
ARG93 |
|
|
8m3 |
9m6 |
10.9'' |
87° |
2018 |
Cyg |
20h46m55.48s |
+32°51'50.30" |
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x ein schönes enges Pärchen, nicht mehr ganz knapp getrennt - Helligkeitsunterschied gut 1.5 Magnituden - A ist weiß, B dagegen grau - runter aus 20x ist B nicht mehr detektierbar |
|
|
|
|
HO141 |
|
AB |
9m5 |
11m2 |
1.6'' |
293° |
2013 |
Del |
20h47m05.66s |
+19°17'47.50" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Pretty pair, significant delta mag, wide ~1.5" |
|
|
|
|
BU677, T Cyg |
|
AB |
4m9 |
10m0 |
10.0'' |
120° |
2015 |
Cyg |
20h47m10.72s |
+34°22'26.80" |
|
|
|
|
AC |
4m9 |
11m2 |
16.8'' |
211° |
2015 |
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Needed high magnification in order to see the faint B star, 2 delta mag to A, wide, ~10" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: Needed averted vision to detect the AC pair, but once seen could hold it with direct vision, further separtation than AB pair ~15" |
|
|
|
★
|
STT413, 54 Cyg, lambda Cyg |
|
AB |
4m7 |
6m3 |
0.9'' |
3° |
2018 |
Cyg |
20h47m24.53s |
+36°29'26.70" |
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (280x) |
The diffraction disk of the primary component was slightly elongated towards north. The air here was however a bit too unsteady for an accurate observation. |
|
Uwe Pilz
Leipzig (Germany) |
105mm |
schwierig |
|
Robert Zebahl
Leipzig (Germany) |
152mm (300x) |
Observation with an achromat. The fainter component was visible as a permanent brightening of the first diffraction ring. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (300x) |
2020-08-24: Observation with an ED refractor. At 171x partially, at 200x clearly visible as '8'. At 300x two clear, overlapping diffraction disks of differently bright components. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig aber getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Lambda Cyg: ~1.5 delta mag, blue-white. Bright mess resolves to two disks 0.8-1.0", with seeing. |
|
|
|
|
BU65, 13 Del |
|
|
5m6 |
8m2 |
1.5'' |
199° |
2009 |
Del |
20h47m48.33s |
+06°00'29.50" |
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
13 Del. Suspected at 333x, went up to 533x. The B star seems much fainter about 3 delta mag, and seen only when seeing is still as a blue point just outside first diffraction. ~1.5" |
|
|
|
|
ES93 |
|
|
6m4 |
10m8 |
26.0'' |
321° |
2015 |
Cyg |
20h47m52.97s |
+52°24'25.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow-orange with wide 2 delta mag blue B. |
|
|
|
★★
|
BU66 |
|
|
8m8 |
9m3 |
1.1'' |
169° |
2010 |
Vul |
20h48m06.26s |
+27°27'25.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Exceedingly fine, elongated haze resolved to a clean split, half delta mag, with seeing. 1" Nice! |
|
|
|
|
S763 |
|
AB |
7m2 |
7m8 |
15.8'' |
293° |
2019 |
Cap |
20h48m25.96s |
-18°12'06.10" |
|
|
|
|
AC |
7m2 |
11m7 |
542.3'' |
177° |
2015 |
|
|
|
|
|
|
|
CD |
11m7 |
12m0 |
9.1'' |
333° |
2018 |
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB: ein ganz enges Paar zweier gleich heller Sterne - meist sehe ich eine 8 mit tiefen Einbuchtungen, die Sterne berühren sich gerade so |
|
|
|
|
STF2732 |
|
|
6m4 |
8m6 |
4.3'' |
73° |
2016 |
Cyg |
20h48m42.74s |
+51°54'37.10" |
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 107x Hauptstern mit ganz schwachen Begleiter westlich, knapp getrennt |
|
|
|
|
HJ1581, 55 Cyg |
|
|
4m8 |
11m1 |
22.4'' |
170° |
2012 |
Cyg |
20h48m56.29s |
+46°06'50.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright yellow with 3x fainter blue B, very wide. |
|
|
|
|
STF2731 |
|
AB |
7m7 |
9m6 |
4.1'' |
86° |
2016 |
Cyg |
20h49m00.64s |
+39°47'29.90" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow A and slight blue B, wide ~10", 1-2 delta mag. |
|
|
|
|
BU250 |
|
|
6m3 |
11m5 |
18.3'' |
7° |
2015 |
Cyg |
20h49m54.64s |
+46°39'40.80" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright with 2x fainter, very wide. |
|
|
|
★
|
BU67 |
|
|
6m8 |
9m9 |
1.5'' |
310° |
2015 |
Cyg |
20h50m36.05s |
+30°54'45.70" |
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
Not split. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pale blue A and 3 delta mag B, ~2". In the middle of the Cygnus Loop. |
|
|
|
|
STF2730 |
|
|
8m4 |
8m6 |
3.3'' |
333° |
2019 |
Del |
20h51m03.77s |
+06°23'14.10" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ein schickes sehr eng zusammen stehendes Sternpaar - beide Komponenten haben die gleiche Helligkeit - ich habe B im NW vermutet bei meiner Beobachtung, leider falsch, der Helligkeitsunterschied zwischen beiden beträgt aber auch nur 0.14 mag |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Near equal, fairly wide, white stars ~4" |
|
|
|
|
BU155 |
|
AB |
7m4 |
8m1 |
0.7'' |
41° |
2018 |
Cyg |
20h51m05.41s |
+51°25'01.70" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Clean split, nice disks, 1 delta mag, ~1". Pale yellow and pale easter egg blue. |
|
|
|
|
A613 |
|
|
9m1 |
9m0 |
0.8'' |
327° |
2017 |
Del |
20h51m54.49s |
+05°44'29.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Getting the briefest hairline split, but this one is very marginal seeing is a problem |
|
|
|
|
STT416 |
|
AB |
8m6 |
8m9 |
9.6'' |
118° |
2016 |
Cyg |
20h51m58.64s |
+43°45'28.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange & yellow pair, very wide, 1 delta mag. |
|
|
|
|
STF2733 |
|
|
8m4 |
8m6 |
40.2'' |
145° |
2015 |
Del |
20h52m42.97s |
+07°19'47.60" |
René Merting
Drachhausen (Germany) |
10x50 |
ein Paar schwacher Sterne, Trennung ordentlich - Komponente B im SO ist nur minimal schwächer |
|
René Merting
Drachhausen (Germany) |
12x50 |
zwei flaue, graue Pünktchen, gut getrennt voneinander - SO-NW-Ausrichtung - beide Komponenten sind gleich hell |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x weit getrennt, die A-Komponente nordwestlich ist nur ein wenig heller als B - während mir A warm weiß vorkommt, wirkt B ein wenig kühler, eher weiß-blau - der Farbunterschied ist nicht so groß, wie es klingt - auch bei 20x zeigen sich zwei gut getrennte einfach sichtbare Sterne |
|
|
|
|
STT417 |
|
AB |
8m2 |
8m4 |
0.9'' |
28° |
2018 |
Vul |
20h53m04.23s |
+29°08'43.70" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
einfach |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
|
BAL2548 |
|
|
9m9 |
10m8 |
7.5'' |
258° |
2019 |
Del |
20h53m40.87s |
+03°35'38.50" |
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Easy to pick out ~8" wide, near equal white stars |
|
|
|
★
|
STT420 |
|
|
6m7 |
10m5 |
5.5'' |
2° |
2015 |
Cyg |
20h54m22.25s |
+40°42'10.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Light yellow A and reddish B, very faint, very wide, 3 delta mag. |
|
|
|
★
|
STT419 |
|
|
7m2 |
10m0 |
1.6'' |
23° |
2012 |
Cyg |
20h54m42.00s |
+37°04'25.30" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tough, needed to wait for a while for right seeing. Bright yellowish A with brightening in diffraction which stays put and recedes to a fine point momentarily with the seeing. |
|
|
|
|
STT418 |
|
|
8m2 |
8m3 |
0.9'' |
284° |
2018 |
Cyg |
20h54m49.84s |
+32°42'23.20" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt, gleich hell |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal 1" split, white. |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm |
|
|
|
|
★
|
STF2735 |
|
|
6m5 |
7m5 |
2.0'' |
282° |
2015 |
Del |
20h55m40.64s |
+04°31'57.70" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
Hauptstern leicht gelblich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty orange and blue, Alberio-like, 2 delta mag, well split |
|
|
|
|
STF2736 |
|
|
8m3 |
9m4 |
5.3'' |
219° |
2018 |
Del |
20h56m43.74s |
+12°59'33.80" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x deutet sich an, dass in Richtung SW eine kleine Helligkeitsspitze sichtbar ist - bei 64x kann Komponente B dann knapp getrennt werden - Helligkeitsunterschied eine Größenklasse |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Pretty wide, ~5", 1.5 delta mag, very light orange and blue |
|
|
|
|
BU1034, 7 Aqr |
|
AB |
5m7 |
11m4 |
2.1'' |
165° |
2002 |
Aqr |
20h56m54.02s |
-09°41'51.10" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
A star is orange and bright, the mask is giving a good clean image at moments, with some disturbance (seeing 6/10). B star is faint but a nice hard point outside A's first diffraction, ~2", noticed it right away even though it is on the edge of direct vision, but do not need averted to see it. Dependent on seeing. Tried at full 20" aperture but A was too messy, and did not clean up well enough with apodizing mask. Low in the sky and in fact lost it behind a tree a few minutes after making the observation" |
|
|
|
|
STF2741 |
|
AB |
5m9 |
6m8 |
2.0'' |
25° |
2019 |
Cyg |
20h58m30.03s |
+50°27'42.40" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright A, yellow and blue, ~2" 1 delta mag. |
|
|
|
|
STF2738 |
|
AB |
7m5 |
8m6 |
15.0'' |
254° |
2016 |
Del |
20h58m32.23s |
+16°26'12.20" |
|
|
|
|
AC |
7m5 |
8m1 |
209.4'' |
104° |
2016 |
|
|
|
|
|
|
|
BC |
8m6 |
8m1 |
222.7'' |
102° |
2016 |
|
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
AB: 2021-09-02: Worth seeing in beautiful surroundings. Finely split, clearly uneven pair. |
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
AB: bei 29x gut getrennt und doch schön eng stehend zu erkennen, die B-Komponente im Westen wirkt halb so hell wie A und wirkt dadurch graubraun
AC: in siebenfachem Abstand AB steht C im Osten von A, ohne dass man den Eindruck gewinnen könnte, der Stern muss dort dazu gehören |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
AB: bei 32x ordentlich getrennt - Komponente A im Osten ist deutlich heller (geschätzt 1.5 Größenklassen), B im Westen strahlt dumpfer - Farbkontrast weiß/grau - zurück auf 20x ist der Doppelstern weiterhin nicht zu knapp getrennt sichtbar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: ~1 magnitude difference, widely separated white pair. |
|
|
|
★
|
STF2737, epsilon Equ, 1 Equ |
|
AB |
6m0 |
6m3 |
0.1'' |
280° |
2019 |
Equ |
20h59m04.54s |
+04°17'37.80" |
|
|
|
|
AD |
6m0 |
13m1 |
69.3'' |
293° |
2013 |
|
|
|
|
|
|
|
AB-C |
5m3 |
7m0 |
10.6'' |
67° |
2019 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB-C: in ruhigen Momenten präsentieren sich beide Sterne länglich mit Einschnürung, dann sieht das System aus wie eine kleine Ameise |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
AB-C: At 22x well separated, but still relatively close together with a clear difference in brightness. At 44x AB looked rather white. The color of C was not apparent. |
|
Christopher Hay
Seeheim (Germany) |
80mm (30x) |
AB-C: Well split, C bluish, AB no definite colour, a nice pair at this power. According to Stelledoppie B and C are a physical pair with a period of 5200 years, and A and B are again a physical pair with a period of 104 years. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB-C: bei 32x knapp getrennt - Komponente AB mit einem schönen cremegelb, C steht nordöstlich und ist gut 1.5 Größenklassen schwächer |
|
Sarah Gebauer
Germany |
100mm (45x) |
AB-C: bei 45x ganz eng, aber sauber getrennt, die hellere Komponente AB ist gelbstichig und die nordöstliche, schwächere Komponente C hat phasenweise einen Blaustich, wie ein ganz enger, ganz kleiner und schwächerer Albireo |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB-C: Easy yellow stars, very wide, 1 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 1 Equ / Epsilon Equ / Strongly feel an oval AB pairing, marginal |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
AB-C: close DS |
|
|
|
|
BRT220 |
|
|
9m7 |
9m8 |
4.9'' |
132° |
2016 |
Vul |
20h59m45.13s |
+24°17'28.20" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Near equal stars about 5" sep. |
|
|
|
|
STF2739 |
|
|
9m2 |
9m7 |
3.3'' |
253° |
2016 |
Vul |
20h59m48.38s |
+20°04'09.30" |
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice pair, isolated in field, seems more near equal than SkyTools data. Wide. |
|
|
|
|
59 Cyg, STF2743 |
MCA65 |
Aa-Ab |
4m8 |
7m6 |
0.1'' |
334° |
2015 |
Cyg |
20h59m49.55s |
+47°31'15.40" |
|
|
|
STF2743 |
AB |
4m7 |
9m4 |
21.0'' |
353° |
2012 |
|
|
|
|
|
|
STF2743 |
AC |
4m7 |
11m6 |
26.5'' |
140° |
2012 |
|
|
|
|
|
|
STF2743 |
AD |
4m7 |
11m2 |
39.3'' |
222° |
2012 |
|
|
|
|
|
|
STF2743 |
AE |
4m7 |
12m0 |
70.6'' |
59° |
2003 |
|
|
|
|
|
Christopher Hay
Seeheim (Germany) |
125mm (64x) |
AB: Widely split and striking in field of view, as the pair is a little outside of the star cloud at the swan's tail that adjoins to the south. The A component appears yellowish. The attraction lies in the B component with delta-mag 4m6, which presents as a fine grey-blue pinprick of light. Alias 59 Cygni. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
AB: bei 45x ist Komponente B nördlich von A erkennbar - Komponente A strahlend weiß, bei B ist keine Farbe erkennbar, mindestens 4 Größenklassen Helligkeitsunterschied
AD: bei 72x ist Komponente D südwestlich von A in doppeltem Abstand wie AB erkennbar
AE: bei 72x ist Komponente E nordöstlich von A in doppeltem Abstand wie AD und noch schwächer als D erkennbar |
|
|
|
|
STTA213 |
|
|
6m7 |
9m2 |
70.9'' |
36° |
2015 |
Del |
20h59m50.85s |
+16°49'27.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very wide split, orange-yellow A, white B, 1 delta mag. |
|
|
|
|
STT425 |
|
CD |
10m8 |
12m3 |
4.3'' |
132° |
2016 |
Cyg |
21h00m07.41s |
+48°41'01.70" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
a very faint close pair brightened with averted vision. |
|
|
|
|
BU1329 |
|
AB |
8m9 |
9m1 |
0.3'' |
40° |
2009 |
Cyg |
21h00m26.00s |
+34°10'42.40" |
|
|
|
|
AB-C |
8m8 |
10m5 |
6.8'' |
30° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
AB-C: was für eine schwache Schote - bei 64x ist Komponente B mit großer Konzentration nordöstlich von A erkennbar - einmal erkannt, ist es dann leichter - A ist schon schwach, B bestimmt 2 Magnituden schwächer (1.69 mag laut Stelle Doppie) - bei 107x ist die Trennung ordentlich und B besser sichtbar |
|
|
|
★
|
BU156 |
|
|
7m4 |
9m2 |
0.9'' |
235° |
2012 |
Cyg |
21h00m49.84s |
+46°34'42.80" |
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Using apodising mask. Extraordinarily fine, B is a tiny faint point where light orange A's first diffraction ring would be -- ~1" -- but I need the diffraction ring to disappear, with seeing, to resolve it. 1.2" at discovery at 1873 with his 6-inch! |
|
|
|
|
STT426, 60 Cyg |
|
|
5m4 |
9m5 |
2.9'' |
159° |
2017 |
Cyg |
21h01m10.93s |
+46°09'20.80" |
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Much fainter companion outside of first diffraction ring. Better visible at 270x. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
60 Cyg. Brilliant white A and much fainter ashen B, close ~2" but well split |
|
|
|
|
HO600 |
|
|
6m7 |
10m9 |
2.1'' |
97° |
2004 |
Cyg |
21h01m47.44s |
+44°11'13.60" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Can see moments of steady disk, but no B. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Light yellow orange A star, and very faint greyish B star appears ~2" separated. Suspected with 205x, but needed 333x and apodising mask to reduce A's disk size to clearly resolve it |
|
|
|
|
STF2746 |
|
|
7m9 |
8m7 |
1.2'' |
323° |
2018 |
Cyg |
21h01m50.05s |
+39°15'38.40" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig, schwach, Helligkeitsunterschied, blickweise getrennt |
|
|
|
|
COU2650 |
|
|
10m6 |
11m4 |
1.9'' |
255° |
2009 |
Cyg |
21h01m52.59s |
+48°02'19.40" |
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Very significant delta mag, ~1 delta or more, ~2", white stars, very fine |
|
|
|
★★★
|
STF2742 |
|
|
7m4 |
7m6 |
2.9'' |
215° |
2017 |
Equ |
21h02m12.51s |
+07°10'47.30" |
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
At 44x almost split with slight difference in brightness. At 57x split, but tight. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
ähnlich wie STF2765 und STF2786 weiter nördlich wieder so ein knappes Pärchen bei 64x, das scheint Sternbild-typisch zu sein - beide Sterne sind fast gleich hell, der Stern im NO ist minimal heller |
|
Uwe Pilz
Leipzig (Germany) |
105mm (94x) |
Prachtstück! Weiß-Weißgelb. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
equal light orange, well split, pretty |
|
|
|
|
H4 113 |
|
AB |
6m6 |
9m5 |
18.9'' |
300° |
2018 |
Cyg |
21h02m20.95s |
+39°30'32.50" |
|
|
|
|
AC |
6m6 |
12m5 |
26.7'' |
248° |
2012 |
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x zeigt sich Komponente A weißgelblich, Komponente B ist direkt knapp abgesetzt nordwestlich erkennbar, deutlich schwächer - schönes Kontrastpärchen |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
AB: bei 45x ein schön getrenntes Pärchen - Helligkeitsunterschied 2.5 Größenklassen - schöner Farbkontrast, Komponente A ist butterblumengelb, B dagegen rostigbraun |
|
|
|
★
|
STF2747 |
|
|
8m4 |
8m7 |
4.6'' |
266° |
2019 |
Cyg |
21h02m21.92s |
+37°39'14.00" |
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x ein leicht verformter Stern, nicht ganz rund - bei 64x zwei gleich helle ganz knapp getrennte weiße Lichtpünktchen, schick - bei 107x wird die Trennung deutlicher, der südöstliche Stern strahlt einen kleinen Tick heller |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Light orange near equal, ~5" |
|
|
|
★
|
BU69 |
|
AB |
8m3 |
9m8 |
0.4'' |
6° |
2017 |
Vul |
21h02m36.08s |
+21°41'28.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
I sense overlapping disks at 553x, but marginal. |
|
|
|
★
|
BU1138 |
|
AB |
7m1 |
7m3 |
0.1'' |
172° |
2006 |
Cyg |
21h02m48.62s |
+45°50'56.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Notched elongation with seeing and apodising mask, white, can tell A and B's orientation by difference in magnitude. Current separation 0.155". 314 year period, it will only make modest position angle change in my time. Burnham discovered in 1888 with the Lick 36-inch at 0.3"! It seems Hough also discovered it in 1888 but published his results later, HO 282 |
|
|
|
|
STF2744 |
|
AB |
6m8 |
7m3 |
1.2'' |
108° |
2019 |
Aqr |
21h03m03.09s |
+01°31'55.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Split, ~1.5", near equal yellow-orange stars |
|
|
|
★★
|
BU445 |
|
AB |
7m0 |
11m1 |
4.7'' |
109° |
2015 |
Cyg |
21h03m29.53s |
+29°05'33.00" |
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange-red with exceptionally fainter B, only when seeing stills, else it is lost in the diffraction. Pinpoint. ~2", 4 delta mag. |
|
|
|
|
STTA214 |
|
AB |
6m4 |
8m6 |
57.4'' |
185° |
2018 |
Cyg |
21h03m52.13s |
+41°37'41.40" |
|
|
|
|
BC |
8m6 |
13m2 |
106.3'' |
244° |
2015 |
|
|
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
AB: bei 45x stehen beide Komponenten weit auseinander - großer Helligkeitsunterschied von geschätzt 2.5 Größenklassen - schöner Farbkontrast, Komponente A ist zartgelb, B blau-grau |
|
|
|
|
STF2745, 12 Aqr |
|
AB |
5m8 |
7m5 |
2.5'' |
197° |
2017 |
Aqr |
21h04m04.71s |
-05°49'23.00" |
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
|
|
STF2757 |
|
|
