|
m1 |
m2 |
ρ |
θ |
Year |
|
Coordinates (J2000) |
|
|
STF3056 |
|
AB |
7m7 |
8m1 |
0.7'' |
143° |
2018 |
And |
00h04m40.09s |
+34°15'54.70" |
|
|
|
|
AB-C |
7m1 |
10m1 |
26.3'' |
4° |
2017 |
|
|
|
|
|
|
|
AB-D |
7m1 |
10m6 |
95.3'' |
238° |
2012 |
|
|
|
|
|
|
|
CD |
10m1 |
10m6 |
113.1'' |
227° |
2015 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
76mm (29x) |
AB-C: bei 29x ist nach Norden eine ganz schwache Komponente erkennbar, gut getrennt - AB wirkt leicht gelblich, C eher kupfergrau |
|
Sarah Gebauer
Germany |
100mm (73x) |
die Komponenten AB erscheinen als ein Stern, C liegt nördlich davon und ist wesentlich schwächer und Komponente D, die ähnlich hell wie C erscheint, liegt westlich von AB gesehen |
|
|
|
|
STT547 |
|
AB |
9m0 |
9m2 |
6.0'' |
190° |
2018 |
And |
00h05m41.03s |
+45°48'43.30" |
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 64x klare Trennung - ein relativ schwaches Pärchen - zurück auf 32x stehen beide dichter zusammen und können knapp getrennt werden |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
Der nahe gelegene ß997 konnte nicht getrennt werden |
|
|
|
|
STF3060 |
|
AB |
9m3 |
9m7 |
3.4'' |
136° |
2016 |
Peg |
00h05m55.56s |
+18°04'34.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close, ~3", equal brightness, pretty faint. |
|
|
|
|
STF3062, V640 Cas |
|
|
6m4 |
7m3 |
1.5'' |
3° |
2018 |
Cas |
00h06m15.81s |
+58°26'12.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Nice view, clearly split, but tight with visible difference in brightness. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (460x) |
leicht |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Light yellow and a more orange yellow B, 3-4", 1 delta mag. PC (70.07 L.Y.) |
|
René Merting
Drachhausen (Germany) |
320mm (320x) |
erst bei 320x ist Komponente B knapp getrennt nördlich von A zu erkennen - beide Sterne sind relativ hell und haben relativ große Beugungsscheibchen, so dass die Trennung nur knapp zu sehen ist - nicht wirklich schön, wenn man in den Nächten vorher mit einem Refraktor Doppelsterne beobachtet hat |
|
|
|
★
|
STF2 |
|
|
6m7 |
6m9 |
0.9'' |
17° |
2018 |
Cep |
00h09m20.18s |
+79°42'52.40" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (198x) |
Schneemann-Figur. Abstand 0“91 |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
|
★
|
AC1 |
|
|
7m3 |
8m3 |
1.9'' |
290° |
2018 |
And |
00h20m54.10s |
+32°58'40.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
Very attractive, relatively close with a clearly visible difference in brightness. In the immediate vicinity a brighter star shines in a lovely orange. Very nice contrast! |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
orange. Leuchtend gelber Stern in 5' Abstand |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tight yellow-white pair, near equal magnitudes. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (205x) |
Orange star, slightly out of round. |
|
|
|
★
|
BU394 |
|
AB |
8m5 |
8m8 |
0.8'' |
278° |
2017 |
Cas |
00h30m45.56s |
+47°31'47.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very fine, pop split with seeing, near equal. |
|
|
|
|
STT12, lam Cas |
|
|
5m3 |
5m6 |
0.2'' |
210° |
2010 |
Cas |
00h31m46.32s |
+54°31'20.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Lambda Cas: Maybe out of round? Marginal |
|
|
|
★★★
|
eta Cas, 24 Cas |
STF60 |
AB |
3m5 |
7m4 |
13.4'' |
326° |
2019 |
Cas |
00h49m06.29s |
+57°48'54.70" |
|
|
|
STF60 |
AC |
3m5 |
11m4 |
225.0'' |
260° |
2000 |
|
|
|
|
|
|
STF60 |
AD |
3m5 |
12m8 |
189.4'' |
354° |
2011 |
|
|
|
|
|
|
STF60 |
AE |
3m5 |
10m2 |
75.6'' |
126° |
2015 |
|
|
|
|
|
|
STF60 |
AF |
3m5 |
11m5 |
378.3'' |
276° |
2000 |
|
|
|
|
|
|
STF60 |
AG |
3m5 |
9m5 |
419.7'' |
259° |
2012 |
|
|
|
|
|
|
STF60 |
AH |
3m5 |
8m4 |
701.1'' |
355° |
2012 |
|
|
|
|
|
|
SMR2 |
AI |
3m5 |
11m6 |
90.3'' |
73° |
2012 |
|
|
|
|
|
|
SMR2 |
AJ |
3m5 |
12m3 |
237.1'' |
262° |
2012 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
AB: Easy to split with big difference in brightness. Fainter component appeared deep orange to slightly red colored, brighter component tends to be more slightly yellowish. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
AB: bei 32x ist Komponente A so hell, dass B trotz des augenscheinlich großen Abstandes von 13,4" nur knapp getrennt zu sehen ist - Komponente A ist gleißend hell-gelb, B dürfte mindestens 3 Größenklassen schwächer sein und wirkt dadurch dumpfer |
|
Uwe Pilz
Leipzig (Germany) |
105mm (53x) |
AB: leicht |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
kein Sternentstehungsgebiet! |
|
Sarah Gebauer
Germany |
150mm (54x) |
AB: bei 54x erst nur einen Stern gesehen, doch da, ganz schwach darunter doch die wesentlich schwächere, zweite Komponente entdeckt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Nice yellow pair. A is a red tainted yellow, B is cleaner. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
AB: bei 72x ein echt fetter Farbkontrast, Komponente A ist gleißend hell und zitronengelb, B zeigt sich knallig orange - beide Sterne sind gut getrennt voneinander zu beobachten - sehenswert |
|
|
|
★
|
BU232 |
|
AB |
8m5 |
8m8 |
0.9'' |
256° |
2018 |
Cas |
00h50m25.10s |
+50°37'49.60" |
|
|
|
|
AB-C |
8m5 |
10m1 |
24.5'' |
300° |
2018 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
AB: Nice, well split, near equal. Part of a triple, the next one much wider in same PA and two delta mag. [AB-C is 10.06 24.5"] |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Neat near equal orange and yellow. Split with seeing, 1". |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB-C: C 2 delta mag fainter than B, about 25" separated, is the +1 star with BU232AB |
|
|
|
|
HLD4 |
|
|
9m0 |
9m5 |
0.3'' |
38° |
2007 |
Cas |
00h57m35.79s |
+54°23'44.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Yellowish stars, nicely split, a near equal. [this pair is widening, will get a little easier, was 1" at discovery in 1881 -- Holden, Lick director.] |
|
|
|
★
|
A2901 |
|
|
7m1 |
7m8 |
0.4'' |
64° |
2018 |
Cas |
01h01m30.15s |
+69°21'30.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Elongated to notched with seeing |
|
|
|
|
STT21 |
|
|
6m8 |
8m1 |
1.3'' |
175° |
2018 |
And |
01h03m01.54s |
+47°22'34.10" |
|
|
Uwe Pilz
Leipzig (Germany) |
120mm (180x) |
weiß |
|
|
|
|
STT515, phi And |
|
AB |
4m6 |
5m6 |
0.6'' |
115° |
2016 |
And |
01h09m30.12s |
+47°14'30.60" |
|
|
Uwe Pilz
Leipzig (Germany) |
120mm (180x) |
|
|
|
|
|
BU235 |
|
Aa-Ab |
7m5 |
7m8 |
0.8'' |
143° |
2018 |
Cas |
01h10m34.31s |
+51°00'47.80" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
Mehrfachsystem |
|
|
|
|
STF113, 42 Cet |
|
A-BC |
6m5 |
7m0 |
1.6'' |
22° |
2018 |
Cet |
01h19m48.30s |
-00°30'32.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pale orange and slight blue, PA to NW, ~1 delta mag. 2". Pretty. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Gold and blue, pretty. 2" PA to north. |
|
|
|
★
|
STF115 |
|
AB |
7m1 |
7m3 |
0.5'' |
160° |
2018 |
Cas |
01h23m21.27s |
+58°08'35.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Peanut, near equal. in nearly the same FOV with Detla Cas, V 465 pretty orange star, and NGC 457, a loose moderately rich open cluster |
|
|
|
|
STF158 |
|
AB |
9m0 |
9m4 |
2.2'' |
272° |
2018 |
Tri |
01h46m44.07s |
+33°09'45.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Nice split, pretty wide considering low magnification. Orange-yellow stars about half delta mag |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern noch gut zu trennen. Der Helligkeitsunterschied beträgt knapp eine Magnitude und der etwas hellere Stern leuchtet gelblich und der schwächere orange gelb. |
|
|
|
|
HO311 |
|
|
8m2 |
7m8 |
0.4'' |
178° |
2018 |
Ari |
01h51m13.34s |
+24°39'08.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Nice clear split with seeing, more near equal but there is a noticeable magnitude difference, white stars |
|
|
|
|
BU260 |
|
|
8m8 |
9m0 |
1.1'' |
261° |
2018 |
Ari |
01h53m14.21s |
+15°26'00.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Fine pair, well split, half delta mag |
|
|
|
|
BU513, 48 Cas |
|
AB |
4m7 |
6m7 |
0.6'' |
320° |
2013 |
Cas |
02h01m57.55s |
+70°54'25.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Searched around the swollen, shimmering bright A star disk and felt there was a faint close B trying to resolve in the first diffraction at 553x. Apodizing mask cleaned up the image but no B resolved |
|
|
|
|
alpha Psc, 113 Psc, Alrischa, Kaitain, Okda |
STF202 |
AB |
4m1 |
5m2 |
1.8'' |
262° |
2017 |
Psc |
02h02m02.80s |
+02°45'49.40" |
|
|
|
PWL1 |
AC |
4m1 |
8m2 |
404.9'' |
63° |
2006 |
|
|
|
|
|
|
PWL1 |
AD |
4m1 |
8m6 |
434.5'' |
335° |
2006 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
AB: der hellere Stern ist weiß |
|
|
|
★
|
STF208, 10 Ari |
|
AB |
5m8 |
7m9 |
1.3'' |
349° |
2018 |
Ari |
02h03m39.26s |
+25°56'07.60" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
helle Stelle im ersten Ring |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
10 Ari Pretty white and slightly off-white or blue-white B, 2.5 delta mag, ~1.5" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
~2 delta mag, ~1" very nice. ~1 disk split. Nice! |
|
|
|
★
|
STF234 |
|
AB |
8m7 |
9m4 |
0.6'' |
222° |
2012 |
Cas |
02h17m23.00s |
+61°21'06.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (885x) |
Light orange star, definitely elongated, maybe notched, but no convincing split. Tough little Struve. |
|
|
|
|
A2329 |
|
|
9m4 |
9m6 |
0.5'' |
101° |
2018 |
Cet |
02h27m45.86s |
+04°25'55.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Split at 533x but used barlow to confirm the PA accurately since this is a short period pair. Nicely split orange stars, half delta mag. Seeing it now at nearly the furthest extent of its orbit, it will become more difficult with time. The pair is a "mere" 55.91 lightyears away |
|
|
|
★★
|
STF262, iota Cas |
|
AB |
4m6 |
6m9 |
2.9'' |
230° |
2017 |
Cas |
02h29m03.96s |
+67°24'08.70" |
|
|
|
|
AC |
4m6 |
9m1 |
6.7'' |
117° |
2015 |
|
|
|
|
|
|
|
AD |
4m6 |
8m5 |
210.9'' |
60° |
2016 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
Only the D component was well visible. The components B & C were not visible even at magnifications up to 167x. The sky was clearly brightened (Bortle 7). |
|
Robert Zebahl
Leipzig (Germany) |
70mm (120x) |
Components A, B and C pretty close together, D far apart. Component B appeared slightly elongated on the first diffraction ring of the primary component. Rewarding! |
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
AB: bei 142x zeigt sich Komponente B im SW mit gut einem Drittel das Abstandes AC, Helligkeitsunterschied 1.5 bis 2 Größenklassen
AC: bei 64x getrennt, schöner Farbkontrast, Komponente A ist weiß mit einem Stich ins Gelbe, C leicht bräunlich
AD: bei 32x extrem weiter Abstand zwischen A und D, Helligkeitsunterschied mehr als 2 Größenklassen (laut Stelle Doppie sogar 3.85 mag) |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
Dreifachstern lohnend |
|
Sarah Gebauer
Germany |
150mm (160x) |
bei 160x sind die Komponenten AC getrennt, B leider nicht, die schwache Komponente C versinkt fast im Strahlen der hellen Komponente A, ein sehr reizvoller Anblick! Von Komponente D wusste ich während der Beobachtung noch nichts, sie taucht unter den Feldsternen der Zeichnung auch auf |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Component D easy to see even at lowest magnification. Component C is also easily visible at 49x. At 69x the component B is indicated, at 100x clearly visible. C appears slightly grey-bluish and obviously fainter than B. Grand sight at 129x! |
|
|
|
|
STF295, 84 Cet |
|
|
5m8 |
9m7 |
3.6'' |
301° |
2012 |
Cet |
02h41m14.00s |
-00°41'44.40" |
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
Quite easy at a moderate distance, whereby the companion appeared rather faint and was best visible with averted vision. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
trotz diesigem Himmel bei 144x indirekt erkennbar. Schwieriger bei 200x |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Easy. The quite dim companion is immediately visible in moderate distance clearly outside of the first diffraction ring despite few, high clouds. The primary component appeared white-yellowish. |
|
|
|
★
|
A2906 & STF314 |
A2906 |
AB |
7m3 |
8m8 |
0.3'' |
115° |
2018 |
Per |
02h52m52.03s |
+52°59'50.60" |
|
|
|
STF314 |
AB-C |
7m0 |
7m3 |
1.6'' |
316° |
2018 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
STF314 (AB-C): Beautifully separated, quite close together. Difference in brightness visible, but rather small. Easy to find and bright. Very nice. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (460x) |
STF314 (AB-C): ähnlich hell |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
A2906 (AB): This is the brighter of the STF 314 pair. I have a feeling it is slightly elongated but nothing certain. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF314 (AB-C): a nice half delta mag pair ~2" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF314 (AB-C): near equal brightness, AB more yellow yellow-white of the two, ~2 disk separation |
|
|
|
|
BU525 |
|
|
7m5 |
7m5 |
0.5'' |
276° |
2018 |
Ari |
02h58m53.11s |
+21°37'03.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Star is decidedly not round but does not show shape other than a stretching. |
|
|
|
|
STF333, eps Ari |
|
AB |
5m2 |
5m6 |
1.4'' |
211° |
2018 |
Ari |
02h59m12.73s |
+21°20'25.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Equal bright white just split with seeing. |
|
|
|
|
STF360 |
|
|
8m0 |
8m3 |
2.7'' |
126° |
2015 |
Per |
03h12m09.59s |
+37°13'03.30" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (67x) |
Pretty faint double star. At 57x barely separable with almost touching diffraction disks. The components seemed similarly bright. At 67x still very close together, at 100x easy to separate. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (69x) |
Split, but close together, similarly bright. The double star appears overall slightly orange compared to the surrounding stars. |
|
|
|
★★
|
STT51 |
|
|
8m5 |
8m7 |
0.6'' |
346° |
2018 |
Per |
03h12m57.08s |
+44°17'14.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very fine clean split at the finest moments, which is once every 10 seconds. 0.5", equal mag. |
|
|
|
|
HU544 |
|
|
6m7 |
8m2 |
1.7'' |
103° |
2018 |
Per |
03h15m48.70s |
+50°57'21.20" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
Clearly seen as figure '8' with noticeable difference in brightness. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (196x) |
klebt am ersten Ring |
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
im ersten Ring |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Wonderfully separated in equally beautiful star surroundings! Clear difference in brightness visible. To the east there is a brighter star, which shines yellowish-orange. HU544 itself seems rather cool in color. |
|
|
|
|
STF412, 7 Tau |
|
AB |
6m6 |
6m9 |
0.8'' |
349° |
2018 |
Tau |
03h34m26.62s |
+24°27'52.10" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
A-B länglich |
|
|
|
★
|
BU533 |
|
AB |
7m5 |
7m7 |
1.0'' |
222° |
2018 |
Per |
03h35m37.81s |
+31°40'48.70" |
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (225x) |
At 129x clearly elongated, notched. At 225x just so separable with similarly bright components. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
Overlapping yellow-orange disks, equal mag |
|
|
|
|
STF425 |
|
AB |
7m5 |
7m6 |
1.9'' |
59° |
2018 |
Per |
03h40m07.24s |
+34°06'59.30" |
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Beautifully separated, relatively close together, very little difference in brightness. |
|
|
|
★★
|
BU536 & S437, SAO76169 |
S437 |
AB-C |
8m1 |
7m7 |
38.8'' |
308° |
2017 |
Tau |
03h46m16.00s |
+24°11'23.50" |
|
|
|
BU536 |
AB |
8m1 |
9m4 |
1.1'' |
178° |
2016 |
|
|
|
|
|
|
BU536 |
CD |
7m7 |
12m9 |
18.3'' |
5° |
2015 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
in den Plejaden |
|
|
|
|
STT66 |
|
|
8m1 |
8m5 |
1.0'' |
146° |
2018 |
Per |
03h52m04.69s |
+40°47'50.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
light orange equal magnitude, split with seeing, close ~1" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Wide separation orange stars of similar brightness |
|
|
|
|
STF483 |
|
|
7m4 |
9m3 |
1.6'' |
53° |
2018 |
Per |
04h04m07.10s |
+39°30'35.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
Yellow-orange star, very close, 1", 2 delta mag. |
|
|
|
|
STT531, 50 Per |
|
AB |
7m3 |
9m7 |
2.7'' |
353° |
2018 |
Per |
04h07m34.35s |
+38°04'28.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
AC is a finder split. The fainter of these has another star split 4", 2-3 delta mag., this is the AB pair. |
|
|
|
★
|
omicron 2 Eri, 40 Eri, STF518 |
|
A-BC |
4m4 |
9m3 |
83.7'' |
102° |
2016 |
Eri |
04h15m16.32s |
-07°39'10.30" |
|
|
|
|
BC |
9m5 |
11m2 |
8.3'' |
331° |
2017 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (244x) |
A ist gelblich. B fiel sofort ins Auge, auch bei 144x. C war extrem schwierig. A musste außerhalb des Gesichtsfeldes stehen, aber auch dann war er nur indirekt sichtbar. Dann aber überraschte der verhältnismäßig große Abstand B-C. ~ A ist ein Hauptreihenstern ähnlich der Sonne. B ist ein weißer Zwerg, einer der hellsten am Himmel. C ist ein Roter Zwerg, davon gibt es nicht viele in der Reichweite kleiner Instrumente. Insgesamt hat man drei Zwergsterne auf einen Blick: Einen gewöhnlichen (=Hauptreihen-) Zwerg, einen weißen und einen roten. |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
A-BC: Triplesystem with a white Dwarf |
|
|
|
|
HO328 |
|
|
7m4 |
9m1 |
0.4'' |
358° |
2016 |
Tau |
04h17m01.22s |
+19°40'32.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Olive shape. Light yellow-orange star, no clean split but clearly elongated. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very faint, very close ~0.8", emerges with seeing, hair split. Marginal |
|
|
|
★
|
STF520 |
|
|
8m3 |
8m4 |
0.7'' |
81° |
2018 |
Tau |
04h18m14.55s |
+22°48'24.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Faint elongated to overlapping disks. |
|
|
|
|
STT82 |
|
AB |
7m3 |
8m6 |
1.2'' |
327° |
2018 |
Tau |
04h22m44.10s |
+15°03'22.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close, 0.8" 1.5 delta mag, PA to N/NW. |
|
|
|
|
STT81, 56 Per |
|
AB |
5m8 |
9m2 |
4.2'' |
13° |
2017 |
Per |
04h24m37.46s |
+33°57'34.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
56 Per. Pretty yellow and slight red pair, 2 delta mag. |
|
|
|
|
STF554, 80 Tau |
|
|
5m7 |
8m1 |
1.5'' |
16° |
2015 |
Tau |
04h30m08.60s |
+15°38'16.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
1" 2 delta mag, PA N. Nice! |
|
|
|
|
STF572 |
|
AB |
7m4 |
7m2 |
4.4'' |
189° |
2018 |
Tau |
04h38m29.58s |
+26°56'25.60" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Clearly separated, easy with beautiful color contrast: A slightly orange, B white. |
|
|
|
|
STT92, 5 Aur |
|
AB |
6m0 |
9m5 |
4.1'' |
285° |
2017 |
Aur |
05h00m18.35s |
+39°23'40.90" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (160x) |
schwierig |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
Nur bei sehr hoher Vergrößerung überhaupt zu trennen, schwierig |
|
|
|
|
STF648 |
|
AB |
8m1 |
8m9 |
4.7'' |
62° |
2019 |
Aur |
05h10m59.19s |
+32°02'19.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (40x) |
At 40x tight with obviously fainter component. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (33x) |
Separated, but tight with noticeable difference in brightness. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
beide Komponenten gelb |
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
Light orange, half delta mag, wide. |
|
|
|
|
STT517 |
|
AB |
6m8 |
7m0 |
0.7'' |
241° |
2018 |
Ori |
05h13m31.55s |
+01°58'03.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Consistently split but images are bloated by poor seeing, yellowish white stars, <1", near equal |
|
|
|
★★★
|
WNC2 |
|
A-BC |
6m9 |
7m0 |
3.3'' |
158° |
2018 |
Ori |
05h23m51.32s |
-00°51'59.80" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
Double star appeared elongated. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ein extrem eng stehendes wunderschönes Pärchen zweier gleich heller gelber Sterne - keine 8 mehr, beide sind schon getrennt - bei 107x kommt etwas mehr Luft zwischen beide, aber sie scheinen auch ein wenig Farbe zu verlieren |
|
Robert Zebahl
Leipzig (Germany) |
120mm (150x) |
Clearly split with nearly equally bright components. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice near equal, light yellow-white stars, well split. nice pair [BC is A 847 7.67/7.84 0.3" and could have been gotten on a better night!] |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Easy and obvious pair, bright 7th mag stars ~3". [This was a first try at the short period list but I missed the object, which is A 847 BC, 7.67/7.84 0.3" -- need to try again.] |
|
|
|
|
A848 |
|
|
6m9 |
7m9 |
0.3'' |
179° |
2016 |
Ori |
05h25m31.08s |
-00°32'38.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Suspect elongation at 333x, at 533x I get a snowman, very definite with seeing. White stars, noticeable mag difference |
|
|
|
|
STF728, 32 Ori |
|
|
4m4 |
5m8 |
1.3'' |
44° |
2017 |
Ori |
05h30m47.06s |
+05°56'53.30" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
sauber getrennt, Beugungsscheiben berühren sich gerade |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
32 Ori White and off white pair, 1.5 delta mag, ~1.5". Nice and very clean with seeing |
|
|
|
★
|
STF742 |
|
|
7m1 |
7m5 |
4.2'' |
275° |
2019 |
Tau |
05h36m26.38s |
+21°59'35.10" |
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (62x) |
Beautifully separated, relatively tight with well visible difference in brightness. Points directly toward Messier 1 and can be observed with it in one field of view. Very nice! |
|
Robert Zebahl
Leipzig (Germany) |
120mm (48x) |
Nice, evident double near Messier 1. Easy to split with almost equally bright components. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (69x) |
At 49x just so, at 69x easily separable. The fainter component appeared a little warmer in terms of color. Great view together with Messier 1 in the field of view. |
|
Robert Zebahl
Leipzig (Germany) |
200mm (80x) |
Nice double star with nearly equally bright components. |
|
|
|
|
STF749 |
|
AB |
6m5 |
6m5 |
1.1'' |
319° |
2017 |
Tau |
05h37m08.84s |
+26°55'28.30" |
|
|
|
|
AC |
6m5 |
10m5 |
181.6'' |
299° |
2011 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB: I had the impression that in the correct position angle, without knowing that angle during observation, a minimal elongation could be detected. But observation is borderline and too doubtful. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Hair-split, equal brightness white stars. Nice. |
|
|
|
|
STF774, zeta Ori, 50 Ori, Alnitak |
|
AB |
1m9 |
3m7 |
2.4'' |
167° |
2017 |
Ori |
05h40m45.52s |
-01°56'33.30" |
|
|
|
|
AC |
1m9 |
9m6 |
58.5'' |
10° |
2017 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (128x) |
AB: Big difference in brightness. I could see the fainter component near the first ring of the Airy pattern of the brighter component. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
AB: sauber getrennt, Beugungsscheiben berühren sich gerade |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Alnitak. Easy, 2 delta mag,~2", white |
|
Mark McCarthy
Fremont (California/USA) |
317mm (207x) |
AC: Alnitak:AC is a very faint star widely separated outside of the main star's glare. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (207x) |
AB: about 2" and 1.5 delta mag. |
|
|
|
|
BU560 |
|
|
7m8 |
8m2 |
1.7'' |
124° |
2019 |
Aur |
05h47m24.87s |
+29°39'26.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
Clearly visible as a double star with overlapping diffraction disks (figure '8') and small difference in brightness. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
Separated with very little difference in brightness, relatively tight. Overall easy. |
|
|
|
|
STT119 |
|
|
8m1 |
8m9 |
0.7'' |
355° |
2009 |
Ori |
05h47m54.88s |
+07°57'37.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Suspect elongations with 8" 533x & 20" 533x, but image not good enough. But I got a nice clean split with apodizing mask, nearly perfrect disks. Orange stars well split, <1", about 1 delta mag |
|
|
|
|
STF795, 52 Ori |
|
|
6m0 |
6m0 |
1.0'' |
220° |
2017 |
Ori |
05h48m00.21s |
+06°27'14.50" |
|
|
Sarah Gebauer
Germany |
150mm (125x) |
bei 125x und 250x nicht getrennt im April 2020 |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright white, near equal magnitude, near touching disks hairline split |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
52 Ori. Close but well split, near equal, ivory white. with apodising mask |
|
|
|
|
STF3115 |
|
|
6m5 |
7m5 |
0.9'' |
337° |
2017 |
Cam |
05h49m04.64s |
+62°48'29.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gerade eben trennbar mit schwarzem Zwischenraum |
|
|
|
★★
|
BU1053 |
|
|
6m9 |
8m8 |
1.9'' |
0° |
2019 |
Aur |
05h53m28.64s |
+37°20'20.70" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
Border observation! Companion is temporarily visible in the correct position angle as an extremely dim brightening of the first diffraction ring of the primary component. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
Nice!! Blazing white and close but nicely split light blue B, 2 delta mag. |
|
|
|
|
STT124 |
|
|
6m1 |
7m4 |
0.6'' |
299° |
2018 |
Ori |
05h58m53.23s |
+12°48'29.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (170x) |
Seeing not good. Bloated yellow star with bluish B just attached to the edge, like a wart. B is very faint, small. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Briefly split in the best moments, 1 second out of 10. A star yellow-white and small, hard blue B. |
|
|
|
|
STT545, 37 Aur, theta Aur |
|
AB |
2m6 |
7m2 |
4.1'' |
303° |
2018 |
Aur |
05h59m43.24s |
+37°12'45.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
At 57x nothing seen at first sight. At 133x the much fainter component was visible after a short time as a tiny star in the correct position angle. With this knowledge, the observation at 57x was also successful, even if one has to look very closely. The challenge here is not so much the angular distance as the large difference in brightness. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
blauweiß. Wegen der etwas unruhigen Luft und des Helligkeitsunterschiedes nicht einfach. |
|
|
|
|
J335 |
|
|
8m4 |
9m5 |
1.3'' |
271° |
2015 |
Ori |
06h04m08.29s |
+11°00'57.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
White A, B resolves with seeing, hairline split and two delta mag. Tough at this aperture |
|
|
|
|
STT132 |
|
|
7m2 |
9m6 |
1.8'' |
332° |
2012 |
Aur |
06h08m11.68s |
+37°58'57.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (270x) |
White A and slightly red B. Fine pair. 2 delta mag. |
|
|
|
|
BU1008, eta Gem, 7 Gem, Propus |
|
|
3m5 |
6m2 |
1.8'' |
258° |
2017 |
Gem |
06h14m52.69s |
+22°30'24.60" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
Aufhellung im ersten Ring |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
sehr schwierig |
|
Robert Zebahl
Leipzig (Germany) |
152mm (225x) |
Already comparatively easy at 180x. The faint companion can be seen well as a quite distinct, slightly elongated, partly round brightening. At 225x and above it becomes easy and immediately apparent, even if the diffraction rings of the primary component are not permanently visible due to the seeing. The primary component was shining in a bright orange. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Propus. Yellow A and blue-yellow B, 2 delta mag, 1.5" very nice |
|
|
|
|
STF881, 4 Lyn |
|
AB |
6m1 |
7m7 |
0.6'' |
149° |
2016 |
Lyn |
06h22m03.57s |
+59°22'19.50" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig wegen Helligkeitsunterschied |
|
|
|
|
STF932 |
|
|
8m3 |
8m5 |
1.6'' |
305° |
2017 |
Gem |
06h34m21.57s |
+14°45'08.30" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (150x) |
Unfortunately a nearby lamp bothered me. I could see the double star at least elongated. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Very neat near equal white stars, well split |
|
|
|
★
|
AGC1, 9 CMa, alpha CMa, Sirius |
|
AB |
-1m5 |
8m4 |
10.7'' |
75° |
2016 |
CMa |
06h45m08.92s |
-16°42'58.00" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (198x) |
mit ADV, ohne nicht trennbar. Eindeutig |
|
Mark McCarthy
Fremont (California/USA) |
203mm (368x) |
Small disk formed on diffraction spike at correct separation and PA (Feb. 2016) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
A faint yellow-orange disk, to the edge of Sirius A’s diffraction and just below my spider’s diffraction spike. I let Sirius pass beyond the field stop, and for an instant there was Sirius B, clearly separated, before it too passed beyond the field stop. |
|
|
|
★★★
|
STF948, 12 Lyn |
|
AB |
5m4 |
6m0 |
1.9'' |
64° |
2019 |
Lyn |
06h46m14.15s |
+59°26'30.10" |
|
|
|
|
AC |
5m4 |
7m0 |
8.8'' |
310° |
2018 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
AC: Components A/B and C well separated, but tight. Significant difference in brightness. The fainter C companion appeared slightly orange, the brighter one white-bluish. |
|
Robert Zebahl
Leipzig (Germany) |
55mm (167x) |
AB: Components A and B separated, whereby the Airy disks slightly overlap. The difference in brightness was well visible. |
|
Robert Zebahl
Leipzig (Germany) |
63mm (140x) |
AB: Components A and B split with almost no space in between. The difference in brightness was visible. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
AC: Well split, relatively close together with significant difference in brightness. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB: Both components A + B clearly split, whereby the diffraction rings where merged together. A very nice view together with component C. I sketched this triplet, which reflects my impression well. Unfortunately, the distance and position angle are not particularly well observed. Also the difference in brightness I didn't noticed during my observation. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (129x) |
At 28x the pair AC is nicely separated without any problems. The close pair AB is already recognizable at 86x as a clear figure '8', at 125x wonderfully separated. The components A & B appear yellowish. Very nice view together with STF 946 in one field of view! |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
im selben Feld mit STF 946 |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
At 49x the pair AC is beautifully separated with a significant difference in brightness. At 100x, the close pair AB is also separated, although still very close together. A slight difference in brightness is noticeable. At 129x, the view is magnificent. The two bright components A & B present themselves yellowish, the fainter component C rather greyish. STF 948 can be well observed in a field of view with the neighbouring double star STF 946. Both show a nice overall scenery. |
|
|
|
|
STT157 |
|
|
7m2 |
9m2 |
0.6'' |
161° |
2018 |
Mon |
06h47m47.56s |
+00°20'24.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Yellow A, widely separated from blue B. 2 magnitude difference. Did not notice 0.8" separation in A |
|
|
|
★
|
STF958 |
|
AB |
6m3 |
6m3 |
4.5'' |
77° |
2019 |
Lyn |
06h48m12.29s |
+55°42'15.10" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (33x) |
Clearly split, equally bright, close together. Nice view. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (62x) |
Very nicely split. Both components appear similarly bright and white-yellowish. |
|
|
|
★
|
STF982, 38 Gem |
|
AB |
4m8 |
7m8 |
7.4'' |
143° |
2018 |
Gem |
06h54m38.63s |
+13°10'40.10" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
At 27x pretty tight with much fainter component. At 71x clearly separated with clear difference in brightness. Brighter component appeared slightly yellowish, the weaker one slightly bluish. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (33x) |
Easy to separated with noticeable difference in brightness. The fainter component appeared slightly orange, the brighter one rather white. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (130x) |
recht attraktiv |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
38 Gem. Light yellow A and blue B, quite wide, very pretty. AC much wider separation much fainter not noticed |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Pretty yellow and orange, 2 delta mag, wide separation |
|
Mark McCarthy
Fremont (California/USA) |
371mm (553x) |
Bright orange and slightly red star, 2-3 delta mag. |
|
|
|
|
STF981 |
|
|
8m7 |
9m0 |
0.9'' |
119° |
2016 |
Gem |
06h55m28.54s |
+30°09'42.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close orange pair, equal magnitude. Clean split, ~1". |
|
|
|
|
STT159, 15 Lyn |
|
AB |
4m5 |
5m5 |
0.7'' |
236° |
2017 |
Lyn |
06h57m16.60s |
+58°25'23.00" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
nicht getrennt im April 2020 |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
relativ einfach |
|
|
|
|
STT163 |
|
AB |
7m2 |
8m2 |
0.2'' |
99° |
1997 |
Mon |
07h01m09.85s |
+11°46'28.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Not perfectly round AB, a faint bluish haze in the diffraction to the south. Marginal. |
|
|
|
|
BU573 |
|
|
7m2 |
7m8 |
0.8'' |
311° |
2018 |
Mon |
07h01m49.89s |
-10°52'56.30" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (247x) |
schwach gekerbt |
|
|
|
★
|
A2462 |
|
AB |
9m2 |
9m0 |
0.2'' |
259° |
2018 |
Gem |
07h02m37.42s |
+15°58'26.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Short period list. Notched, noticeable magnitude difference, B star pointed in direction of apex of right triangle it forms with two other eighth magnitude stars. Light orange stars |
|
|
|
|
STF1037 |
|
AB |
7m2 |
7m3 |
0.8'' |
304° |
2018 |
Gem |
07h12m49.08s |
+27°13'30.20" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
eingekerbt |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
leichter, gleich hell |
|
|
|
|
STT170 |
|
AB |
7m4 |
7m7 |
0.6'' |
288° |
2018 |
CMi |
07h17m38.51s |
+09°17'31.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Notched, near equal at 333x. At 667x, hairline split very easy to see, near equal white stars |
|
|
|
|
STF1066, delta Gem, 55 Gem |
|
|
3m5 |
8m2 |
5.4'' |
234° |
2017 |
Gem |
07h20m07.39s |
+21°58'56.40" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (71x) |
Large difference in brightness. The fainter component was well separated, but just a very tiny star. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
Easy to separate with relatively large distance. The companion appeared as a tiny, faint star. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
erster Ring in SSW heller, zweiter nur an dieser Stelle sichtbar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wasat = Delta Geminorum: Pretty white-yellow and red-orange pair, PA to west, ~4". |
|
|
|
★★★
|
STF1110, alpha Gem, 66 Gem, Castor |
|
AB |
1m9 |
3m0 |
5.4'' |
53° |
2019 |
Gem |
07h34m35.86s |
+31°53'17.80" |
|
|
|
|
AC |
1m9 |
9m8 |
69.8'' |
163° |
2017 |
|
|
|
|
|
|
|
AD |
1m9 |
10m1 |
179.8'' |
221° |
2017 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
AB: At 27x slight difference in brightness visible. Double star appeared as '8'. At 38x clearly split, but tight. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
AB: At 44x the double star appeared as an '8'. At 100x clearly split with noticeable difference in brightness. Both components appeared white. |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 32x wirkt der Stern leicht länglich - bei 107x stehen die beiden Sterne schön eng mit überlagernden Beugungsscheibchen, die Komponenten sind dennoch getrennt erkennbar - Komponente B im Osten ist eine halbe Magnitude schwächer - ganz schwacher Farbkontrast |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
AB: blauweiß-weiß |
|
Winfried Kräling
Marburg (Germany) |
127mm (250x) |
AB: 13.03.2017: Beide Komponenten gelblich mit geringem Helligkeitsunterschied, bereits bei V=60x getrennt. |
|
|
|
★★
|
STF1126 |
|
AB |
6m5 |
7m0 |
0.9'' |
176° |
2017 |
CMi |
07h40m06.99s |
+05°13'51.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
A bit more delta mag than listed, split, white, rather bright pair |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wow, very close <1" hair-split, near equal brightness |
|
|
|
|
HO247 |
|
|
7m7 |
9m2 |
0.4'' |
259° |
2010 |
Gem |
07h46m07.95s |
+21°07'19.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Clean split with seeing, 1 delta mag, fairly bright pair. I found the apodizing mask worked better than the 8-inch mask, gave more resolving power. The 8-inch was only snowman |
|
|
|
★
|
BU101, 9 Pup |
|
|
5m6 |
6m5 |
0.4'' |
304° |
2018 |
Pup |
07h51m46.31s |
-13°53'52.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
9 Pup. Elongated to notched, orientation correct, light orange. Very tough. [B is coming off it's furthest orbit and will be exceptionally difficult in 10 years, but easier in 15 years] |
|
|
|
|
STT182 |
|
|
7m8 |
7m9 |
0.9'' |
9° |
2017 |
CMi |
07h52m42.12s |
+03°23'02.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Compact white pair, more near equal than Sky Tools says, white, easy split |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Moderately bright A with 4 much fainter wide and close stars, forms a right triangle. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close, ~1", near equal brightness white. |
|
|
|
★
|
STT185 |
|
|
7m1 |
7m3 |
0.4'' |
22° |
2018 |
CMi |
07h57m16.39s |
+01°07'37.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Without the apodizing mask I get a clean split with seeing but constant split with the mask. Light orange stars, noticeable mag difference |
|
|
|
★
|
BU581 |
|
AB |
8m5 |
8m8 |
0.4'' |
226° |
2018 |
Cnc |
08h04m23.10s |
+12°17'23.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Light orange near equal, very small, elongated to notched. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange A is not quite round. Marginal |
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
With apodizing mask. Beautiful clean split, almost wide, light orange stars, slight mag difference. There is a third 2x fainter star further out, might be plus one. Wow. [3rd is AB-C, 8.46/11.78 5.5"] |
|
|
|
|
STF1187 |
|
AB |
7m2 |
8m0 |
3.1'' |
20° |
2019 |
Cnc |
08h09m30.45s |
+32°13'18.80" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Split. Components very tight with noticeable difference in brightness. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow and orange, 1 delta mag, 5" |
|
|
|
★★★
|
STF1196 & HUT1, zeta Cnc, 16 Cnc |
STF1196 |
AC |
5m3 |
5m8 |
6.3'' |
51° |
2019 |
Cnc |
08h12m12.79s |
+17°38'51.20" |
|
|
|
STF1196 |
AB-C |
4m9 |
5m8 |
6.0'' |
64° |
2018 |
|
|
|
|
|
|
STF1196 |
AB |
5m3 |
6m2 |
1.1'' |
9° |
2018 |
|
|
|
|
|
|
HUT1 |
Ca-Cb |
6m2 |
7m1 |
0.3'' |
233° |
2018 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
The wide pair AB-C is already separable at 22x. The pair AB shows at 133x two clearly overlapping diffraction disks with small difference in brightness, but without any notch. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (86x) |
AB-C: Easy to separate. A: light grey, B: pale orange. |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (164x) |
AB-C clearly split, AB obviously elongated but not split |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
weißblau-gelb-gelb |
|
Robert Zebahl
Leipzig (Germany) |
120mm (67x) |
AB-C: Evident difference in brightness, easy to split. Both components of similar color. |
|
Robert Zebahl
Leipzig (Germany) |
120mm (200x) |
AB: Very tight. The Airy disks were still touching. Slight difference in brightness. Extremely beautiful triple star! |
|
Winfried Kräling
Marburg (Germany) |
127mm (250x) |
08.04.2018: Sehr schön, 3-fach Stern, A = weißgelb, B = weißgelb, C = weißgelb |
|
Sarah Gebauer
Germany |
150mm (83x) |
AB-C: bei 83x sind AB-C sauber getrennt, laut Atlas 2020 6,1'' Abstand, die Komponenten A und B mit 1,1'' lassen sich nicht trennen, viele schöne Feldsterne dabei |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (200x) |
AB-C: AB (1,1") nicht bemerkt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 2+1 system, the +1 star is HUT 1. STF 1196AB make a nice tight pair. They are all nearly the same magnitude, white & brilliant |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Ca-Cb: not quite round, oval/olive shaped. It is the AB-C of STF 1196. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Triple, all near equal magnitude, yellow-white. AB ~0.8", hair split. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: Triple, all near equal magnitude, yellow-white. AC ~6", wide split. |
|
|
|
★
|
A551, LO Hya |
|
AB |
7m0 |
7m1 |
0.4'' |
63° |
2018 |
Hya |
08h28m29.16s |
-02°31'01.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
LO Hya. With apodizing mask. Easy split, noticeable half delta mag. Another fainter star further out likely +1 [The +1 is STF 1233 AB-C, 6.42/10.49 18.3". AB at furthest extent of orbit, will tighten considerably the next 20 years] |
|
|
|
|
AG154 |
|
|
9m6 |
9m8 |
2.7'' |
1° |
2019 |
Cnc |
08h36m55.78s |
+23°14'49.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
HO Cnc. Near equal well separated, light orange stars |
|
|
|
★★★
|
11 Hya, epsilon Hya |
SP1 |
AB |
3m5 |
5m0 |
0.2'' |
241° |
2018 |
Hya |
08h46m46.51s |
+06°25'07.70" |
|
|
|
STF1273 |
AB-C |
3m5 |
6m7 |
2.9'' |
309° |
2017 |
|
|
|
|
|
|
STF1273 |
AB-D |
3m5 |
12m5 |
18.1'' |
201° |
2017 |
|
|
|
|
|
|
STF1273 |
AB-E |
3m5 |
10m8 |
340.5'' |
2° |
2015 |
|
|
|
|
|
|
STF1273 |
AB-F |
3m5 |
10m4 |
406.5'' |
265° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB-C: Not split. Although a slight brightening was visible in the first diffraction ring, it could also have come from slight coma of the refractor. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
AB-C: 2020-03-27: The much fainter companion is well visible as an almost round knot directly at the diffraction ring of the primary component. Very nice sight. The seeing was mediocre (3/5). |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
AB-C: bei 144x schwierig |
|
Robert Zebahl
Leipzig (Germany) |
152mm (150x) |
AB-C: 2020-03-27: The companion is immediately visible as a tiny star close to the primary component. Due to the chromatic aberration of the achromat, there is a slight tendency to outshine. Nevertheless a nice view. The seeing was mediocre (3/5). |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
AB-C: Epsilon Hya A is bright orange-yellow, B is much fainter and a little blue, ~3". [SP 1 AB is 3.49/5.00 0.2" not seen] |
|
|
|
★
|
A2552 |
|
|
9m1 |
8m5 |
0.3'' |
208° |
2018 |
Hya |
08h48m40.30s |
+00°56'31.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Wow fine split. Pale yellow A and blue B, about one delta mag. Nice split, amazing [82.4 year period] |
|
|
|
★
|
STF1291, 57 Cnc |
|
AB |
6m1 |
6m4 |
1.6'' |
309° |
2019 |
Cnc |
08h54m14.65s |
+30°34'45.80" |
|
|
|
|
AB-C |
5m5 |
9m2 |
54.6'' |
204° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB: Immediately apparent as a double star. Diffraction disks overlapping slightly ('8'). Difference in brightness visible. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
gelb |
|
Sarah Gebauer
Germany |
150mm (125x) |
AB: sowohl bei 83x als auch bei 125x knapp vorm Trennen |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: 57 Cnc. Very nice pair, strong orange yellow colors, ~1 delta mag, bright, nice close split |
|
|
|
|
STF1280 |
|
AB |
8m8 |
9m1 |
3.4'' |
358° |
2018 |
UMa |
08h55m24.82s |
+70°47'39.20" |
|
|
René Merting
Drachhausen (Germany) |
100mm (72x) |
ein knapp getrenntes Sternpaar - beide Sterne sind annähernd gleich hell und strahlen rein weiß - bei 144x eine ordentlichere Trennung, Komponente A im Süden strahlt in einem wärmeren Weiß |
|
|
|
|
HJ2477 & HU628, iota UMa, 9 UMa, Talitha |
HJ2477 |
A-BC |
3m1 |
9m2 |
2.4'' |
90° |
2017 |
UMa |
08h59m12.45s |
+48°02'30.60" |
|
|
|
HU628 |
BC |
9m9 |
10m1 |
0.9'' |
206° |
2017 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (300x) |
A-BC: 2020-04-24: The seeing (3/5) was not good enough for a split. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (213x) |
A-BC: Iota UMa = Talitha. Using 25mm occulting bars with barlow, no mask, putting the bright star's diffraction spikes under the bars, I can see the hard point of the B star, brighter & closer than Procyon B outside of A's glare. One other field star. [HJ 2477's period is 2735 years. The short period is BC is HU 628 9.90/10.10 0.9" 39 year period -- how in the world did he see that?] |
|
|
|
★★
|
STF1306, sigma 2 UMa, 13 UMa |
|
AB |
4m9 |
8m8 |
4.3'' |
348° |
2016 |
UMa |
09h10m23.53s |
+67°08'03.30" |
|
|
|
|
AC |
4m9 |
10m3 |
197.8'' |
148° |
2003 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
AB: Companion almost permanently visible as elongated, non-condensed brightening of the first diffraction ring of the primary component at the correct position angle. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
AB: sehr schwierig bei 88x |
|
|
|
|
STF1321 |
|
AB |
7m8 |
7m9 |
17.0'' |
98° |
2018 |
UMa |
09h14m22.79s |
+52°41'11.80" |
|
|
|
|
AC |
7m8 |
14m5 |
145.7'' |
64° |
2010 |
|
|
|
|
|
|
|
AD |
7m8 |
11m9 |
136.4'' |
129° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
16x70 |
AB: 2020-07-05: Very nice view, striking, easily separable. A slight difference in brightness is visible. At first glance the double star appeared noticeably orange compared to the surrounding stars, on closer look a color difference of the two components was visible: orange & rather white. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
AB: 2020-04-11: At 22x pretty wide pair with equally bright components. Striking colors: slightly orange & white-bluish, but it was a bit difficult to assign the colors to the components. At 44x slightly better color perception. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (31x) |
AB: 2020-04-19: Together with STF1312 in one field of view. At 22x very nice sight, easy to separate, attractive separation. Immediately apparent. A color difference is visible: dark yellow, orange. Also beautiful to see at 44x. Best view at 31x. |
|
|
|
|
STF1332 |
|
|
7m9 |
8m1 |
5.9'' |
29° |
2015 |
Cnc |
09h17m19.21s |
+23°39'09.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Near equal wide pair, ~5", maybe half delta mag |
|
|
|
★
|
STF3121 |
|
AB |
7m9 |
8m0 |
0.5'' |
205° |
2017 |
Cnc |
09h17m53.45s |
+28°33'37.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
IP Cnc Split at 533x, used 1067x to recheck orientation. With apodizing mask. Light yellow-orange stars, nice and clean split, very slight mag difference. Real nice |
|
|
|
|
STF1334, 38 Lyn |
|
AB |
3m9 |
6m1 |
2.5'' |
229° |
2017 |
Lyn |
09h18m50.64s |
+36°48'09.30" |
|
|
Uwe Pilz
Leipzig (Germany) |
60mm (198x) |
Aufhellung im ersten Ring |
|
Robert Zebahl
Leipzig (Germany) |
63mm (140x) |
Fainter companion only seen as permanent brightening on the first diffraction ring. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
gelb, trennbar bei 66x |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
38 Lyn: Very bright A with 3x fainter dull white B, 3-4" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
38 Lyn. A is a bright light yellow and B is a ~2 delta mag orange-yellow, well split and bright |
|
|
|
|
STF1338 |
|
AB |
6m7 |
7m1 |
1.1'' |
314° |
2017 |
Lyn |
09h20m59.40s |
+38°11'17.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Wonderful light yellow stars, near equal, ~1" separation |
|
|
|
|
STT201 |
|
AB |
8m5 |
9m5 |
1.4'' |
206° |
2017 |
Leo |
09h23m54.50s |
+27°54'00.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Extremely fine split, with seeing only, finest of the night, significant mag difference, just above 1" separation |
|
|
|
★★
|
STF1355 |
|
|
7m7 |
7m8 |
1.8'' |
357° |
2018 |
Hya |
09h27m16.69s |
+06°13'59.00" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
2020-04-10: At 67x clearly elongated, equally bright. At 80x detectable notch. At 100x and 133x clearly visible as figure '8'. Near the double star STF 1348. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
Im selben Aufsuchfeld wie stf1348, ähnliche Erscheinung |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Light yellow pair, near equal, very nice, ~2" |
|
|
|
|
HU1128, 11 LMi |
|
|
4m8 |
12m5 |
6.7'' |
61° |
2012 |
LMi |
09h35m39.50s |
+35°48'36.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
11 LMi: Very faint A & extremely faint B, wide separation. From the orbital chart this is approaching maximum elongation now (May 2017), by 2143 it will be 1". Only 39 light years away. |
|
|
|
★
|
STF1362 |
|
|
7m0 |
7m2 |
4.9'' |
125° |
2017 |
Dra |
09h37m56.18s |
+73°04'49.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (31x) |
2020-04-21: At 22x extremely tight, but separable. At 31x very fine separation. Both components appeared white. Very nice sight! At 57x well separated, similarly bright. One component appeared white-yellowish with a hint of orange, the other more white. |
|
|
|
|
STF1374 |
|
AB |
7m3 |
8m7 |
2.8'' |
311° |
2017 |
LMi |
09h41m21.88s |
+38°57'01.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
2020-04-01: Separable at 67x, but difficult due to the bright primary component. Clearly separable at 80x and higher magnifications with a significant difference in brightness. The companion stands close to the primary component and appears as a tiny star. Nice view. |
|
Robert Zebahl
Leipzig (Germany) |
120mm (168x) |
At 50x elongated, at 75x seen as '8'. At 168x clearly split with obviously fainter component. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Pretty orange-yellow stars, ~2 delta mag, ~3 separation |
|
|
|
|
HO369 |
|
AB |
8m0 |
9m8 |
0.4'' |
99° |
2011 |
LMi |
09h51m09.34s |
+36°29'20.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
With 533x I can tell this is not single, but the elongation is too tentative. At 1067x the best I can manage is elongated notched, with seeing. Seeing and transparency are not good enough |
|
|
|
|
STT208, phi UMa |
|
|
5m3 |
5m4 |
0.5'' |
304° |
2017 |
UMa |
09h52m06.36s |
+54°03'51.40" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
länglich, schwierig |
|
|
|
|
AC5, gam Sex |
|
AB |
5m4 |
6m4 |
0.5'' |
41° |
2016 |
Sex |
09h52m30.47s |
-08°06'17.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Gamma Sex: I get a split with seeing of nearly equal orange yellow stars, only momentarily |
|
|
|
|
STT213 |
|
AB |
8m6 |
9m8 |
1.1'' |
121° |
2017 |
Leo |
10h13m08.88s |
+27°25'10.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Bright yellow A, ~2 magnitudes fainter B, very wide separation. |
|
|
|
|
STT215 |
|
|
7m2 |
7m5 |
1.5'' |
176° |
2019 |
Leo |
10h16m16.05s |
+17°44'24.60" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
Appeared partly separated, partly as '8'. Brightness seemed to be equal. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
trennbar bei 120x |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
very close split (1.7" separation) near equal bright white stars |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Near equal light yellow stars, ~1.5" |
|
|
|
★
|
STF1423 |
|
|
9m4 |
10m1 |
0.7'' |
308° |
2018 |
Leo |
10h19m10.64s |
+20°33'48.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tough! Elongated to hairline split. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Split with seeing, light orange A and very faint, ~3 delta mag B, very close, within diffraction ring <1" |
|
|
|
★★
|
STF1424, gamma Leo, 41 Leo, Algieba |
|
AB |
2m4 |
3m6 |
4.9'' |
126° |
2019 |
Leo |
10h19m58.35s |
+19°50'29.40" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (38x) |
At 38x split, but very tight with noticeable difference in brightness. At 56x and higher beautiful view of both components, which seemed to have similar colors. |
|
Robert Zebahl
Leipzig (Germany) |
55mm (59x) |
Very nice unequal double. A appeared yellow-orange, B rather white-bluish. |
|
Christopher Hay
Seeheim (Germany) |
60mm (58x) |
At 25x Algieba is already very elongated. At 58x a sliver of dark between the components, with clear brightness difference. At 70x split becomes more stable, but view not so pleasing as at 58x. Both components display vivid orange. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
At 67x still a relatively close pair, but well separated with quite a clear difference in brightness. At 100x easy to separate and visible color difference: A yellowish to slightly orange, B white-yellowish. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
Very nicely separated with wonderful contrast in brightness and color. Primary component slightly orange, companion yellowish. |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (164x) |
very bright double star, slight colour contrast |
|
Uwe Pilz
Leipzig (Germany) |
105mm (120x) |
schon bei 37x sehenswert; trennbar bei 55x; orange-blauweiß |
|
Robert Zebahl
Leipzig (Germany) |
120mm (66x) |
At 48x easily seen as double star. It appeared as '8'. At 66x pretty tight with visible difference in brightness. |
|
Winfried Kräling
Marburg (Germany) |
127mm (250x) |
08.04.2018: merklicher Helligkeitsunterschied, A = gelb-orange, B = gelb-orange |
|
Sarah Gebauer
Germany |
150mm (83x) |
bei 83x sauber getrennt, ein leichter Farbunterschied (Weiß und helles Gelb) sichtbar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Algieba: Bright yellow and yellow-orange pair, 1 delta mag, 4-6" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright yellow and yellow-white, 1 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very bright yellow, 1 delta mag wide. |
|
René Merting
Drachhausen (Germany) |
320mm (240x) |
bei 240x sehe ich zwei ordentlich getrennte Sterne (naja, nicht wirklich Sterne, sondern wild zappelnde Glitzerbällchen) - Komponente A strahlt in einem zarten Gelb, B ist weiß - zurück auf 144x sehe ich nur ein Stäbchen mit leichter Einschnürung, so wild tanzen die Sterne |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Algieba. Very bright, A is yellow-orange and B is a blazing white orange, like a fire |
|
|
|
★
|
STF1426 |
|
AB-C |
7m3 |
9m4 |
7.6'' |
9° |
2018 |
Leo |
10h20m32.32s |
+06°25'47.60" |
|
|
|
|
AB |
8m0 |
8m3 |
0.9'' |
313° |
2018 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 213x in guten Momenten als Stäbchen erkennbar
AB-C: bei 107x ist nördlich vom Hauptstern AB eine gut 2 Größenklassen schwächere Komponente erkennbar - AB ist weiß, C ist grau |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
AB-C: Quite large angular distance and therefor easy to separate. The C component was pretty faint. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
AB: At first glance elongated, on closer look visible as '8'. |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (164x) |
AB-C easily split, A-B not detectable as double |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
A-B länglich, C weit |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Split with seeing, white, very close, near equal. Part of plus one, a two delta mag not far away |
|
|
|
★★
|
STT216 |
|
|
7m4 |
10m3 |
2.3'' |
231° |
2016 |
Leo |
10h22m43.81s |
+15°20'39.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
A white and bright (7.3), B red & much fainter (10.3), a close split (2"). |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Yellow and very much fainter orange B, 1 delta mag, ~4" separated |
|
|
|
★
|
STF1429 |
|
|
9m1 |
9m3 |
0.8'' |
155° |
2017 |
Leo |
10h25m01.79s |
+24°36'44.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very tough. Faint, need averted vision to brighten and sharpen. Elongated to clean split in the best moments with seeing, near equal magnitude |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Elongated to hairline at 333x, split at 533x. Light orange stars, near equal |
|
|
|
★
|
STT217 |
|
|
7m8 |
8m6 |
0.8'' |
149° |
2017 |
Leo |
10h26m53.01s |
+17°13'09.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Just split cleanly, ~1 delta mag, yellow-tinged white stars. Nice close pair |
|
|
|
★
|
HU879, bet LMi |
|
|
4m6 |
6m0 |
0.5'' |
228° |
2017 |
LMi |
10h27m53.09s |
+36°42'26.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Beta LMi. With apodizing mask I see an out of roundness / olive shape, too much glare to tell orientation, no other field stars |
|
|
|
★
|
STF1439 |
|
|
8m3 |
8m9 |
1.4'' |
73° |
2019 |
Leo |
10h30m06.42s |
+20°48'04.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Very clean images, light yellow-orange stars, ~1 delta mag, well split, very pretty |
|
|
|
★
|
STF1454 |
|
|
9m0 |
11m0 |
1.3'' |
358° |
2016 |
LMi |
10h38m11.10s |
+26°36'24.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Quite tough: averted vision only, very tight, similar magnitude, when seeing stills. |
|
|
|
|
STF1457 |
|
|
7m7 |
8m2 |
1.9'' |
334° |
2019 |
Sex |
10h38m43.14s |
+05°44'02.90" |
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
bei 107x sehe ich in guten Momenten eine Stäbchen, manchmal auch schon leichte Einschnürungen - bei 142x zeigt sich das Sternpaar deutlich als 8 und mit etwas Geduld auch getrennt - B steht im NO und ist eine halbe Größenklasse schwächer - bei 213x dann eindeutige Trennung |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Attractive bright sunny yellow pair, more than 2" separation, slight mag difference |
|
|
|
|
A2768 |
|
|
6m9 |
8m4 |
0.6'' |
240° |
2018 |
Sex |
10h42m37.53s |
+03°34'58.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Feels like a not round disk, but uncertain. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
34 Sex. Surprisingly difficult. Light orange A and a very small 2 delta mag pin prick appears within the first diffraction ring, so about 0.5" separation. Very tough. With seeing only |
|
|
|
|
A2771 |
|
|
9m2 |
9m7 |
0.6'' |
112° |
2018 |
Sex |
10h44m38.71s |
+05°29'55.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Elongated with 333x but a good clean split with 533x. Stars settle to fine points with seeing , ~1 delta mag, ~0.5" separation |
|
|
|
|
STT228 |
|
|
8m2 |
8m9 |
1.7'' |
170° |
2017 |
Leo |
10h47m16.93s |
+22°34'32.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
With fine focus, split with seeing, ~1 delta mag, ~1" separation. Pretty tough needed 533x to split, elongated at 333x |
|
|
|
★★
|
STT229 |
|
|
7m6 |
7m9 |
0.7'' |
256° |
2017 |
UMa |
10h48m02.55s |
+41°06'35.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Just wider than a thin hair split of equal white stars, ~8th mag. 0.63"! in 40 years it will be 0.2" |
|
|
|
★
|
UC2059 & HDS1574 & COU1422 |
UC2059 |
AB |
7m5 |
10m7 |
46.9'' |
46° |
2015 |
UMa |
11h01m45.73s |
+36°40'41.60" |
|
|
|
HDS1574 |
Aa-Ab |
7m6 |
11m1 |
0.2'' |
26° |
2019 |
|
|
|
|
|
|
COU1422 |
Ba-Bb |
11m2 |
11m5 |
0.6'' |
38° |
2008 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
UC2059 (AB): Pretty well separated, 1.5 delta mag, not remarkable as I hoped given the odd designation. |
|
Mark McCarthy
Fremont (California/USA) |
762mm (1219x) |
COU1422 (Ba-Bb): Cou 1422 is a pair of 11th magnitude stars very close to UC 2059 -- best I could get of Cou 1422 was an elongation with the seeing. Tried 1219x without improving the elongation. |
|
|
|
|
BU1077, alpha UMa, 50 UMa, Dubhe |
|
AB |
2m0 |
5m0 |
0.8'' |
342° |
2017 |
UMa |
11h03m43.84s |
+61°45'04.00" |
|
|
|
|
AC |
2m0 |
7m2 |
370.0'' |
205° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
AC: 2020-04-07: Very wide, uneven & inconspicuous pair. A appeared white-yellowish, for B I could not detect any color. |
|
|
|
★★
|
HO378 |
|
AB |
8m2 |
9m1 |
1.1'' |
237° |
2017 |
UMa |
11h04m57.29s |
+38°24'38.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
In a pretty cluster in the finder (~ 12 stars loose and poor, wide magnitude range, triangle shape). Pair is a fine split 1 delta mag 1", ice blue A and slightly yellow B. |
|
|
|
|
STF1510 |
|
|
7m7 |
9m0 |
5.7'' |
328° |
2019 |
UMa |
11h08m00.06s |
+52°49'17.90" |
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x wirkt der Stern leicht länglich - bei 64x dann gelingt die Trennung - Komponente B hängt nordwestlich über A und ist mehr als eine Größenklasse schwächer - ein schönes enges Paar bei dieser Vergrößerung - B wirkt trotz des Größenunterschiedes nicht so schmutzig grau, wie es sonst immer ist |
|
|
|
★
|
STF1517 & BU1431 |
STF1517 |
AB |
7m5 |
8m0 |
0.7'' |
314° |
2017 |
Leo |
11h13m40.99s |
+20°07'43.30" |
|
|
|
BU1431 |
AB-C |
7m5 |
10m8 |
246.1'' |
97° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (187x) |
STF1517 (AB): 2020-03-28: At 187x the double star immediately appears elongated, but without notching. On closer observation, the slight difference in brightness could be detected. Not better at higher magnifications. Observation at quite good seeing (4/5). |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
STF1517 (AB): länglich |
|
Robert Zebahl
Leipzig (Germany) |
152mm (225x) |
STF1517 (AB): 2020-03-27: Clearly elongated. In some moments the double star appeared notched with a small difference in brightness. Observation at moderate seeing (3/5). |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
STF1517 (AB): Very tight, hair split small orange stars of equal magnitude. Wow! |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
STF1517 (AB): Touching disks with 333x, clean slit with 533x, ~0.5" separation, Yellow-orange stars, near equal |
|
|
|
★★
|
STF1523, xi UMa, 53 UMa, Alula Australis |
|
AB |
4m3 |
4m8 |
2.1'' |
155° |
2019 |
UMa |
11h18m10.90s |
+31°31'45.00" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (83x) |
2019-02-09: Already seen as '8' at 83x. At 125x the overlapping of both Airy disks was visible, but also a slight difference in brightness. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
2018-02-18: Very close together with similar brightness. At first glance seen as an '8', looking closer I partly split both components. Similar view also at 128x. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
2020-03-15: Splendid sight! Beautifully separated with almost touching diffraction disks. The rather small difference in brightness was well visible. The diffraction rings of both components coalesced. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
2020-03-16: Awesome! Bright with lovely, subtle diffraction rings. The distance between both components is a smaller than the diameter of the diffraction disk of the fainter component. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
Gemessen: 162° |
|
Robert Zebahl
Leipzig (Germany) |
120mm (168x) |
2018-02-14: Well split with slight difference in brightness. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (129x) |
2019-02-06: Well split with visible difference in brightness. The colors of both components appeared equal. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Alula Australis. Short period. Pretty orange-yellow stars, ~half delta mag, ~2" separation |
|
|
|
|
STF1527 |
|
|
7m0 |
8m0 |
0.4'' |
279° |
2017 |
Leo |
11h18m59.91s |
+14°16'06.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
At 205x I know something is up with this star. At 333x it is overlapping disks and notched. At 533x it is still only notched but a bit larger and hazier |
|
|
|
|
STF1534 |
|
|
8m1 |
11m1 |
5.1'' |
315° |
2017 |
Leo |
11h21m49.34s |
+18°11'24.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Orange-yellow A, very faint B brightens with averted vision, but can hold direct. Wide, ~3 delta mag |
|
|
|
★
|
STF1536, iota Leo, 78 Leo |
|
AB |
4m1 |
6m7 |
2.2'' |
96° |
2018 |
Leo |
11h23m55.37s |
+10°31'46.90" |
|
|
|
|
AB-C |
4m1 |
11m1 |
332.1'' |
346° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB: 2020-03-28: The companion was well visible as brightening on the diffraction ring of the primary component. Sketch see observation with my 102mm refractor. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
AB: 2020-03-28: At 125x clearly separated. A very beautiful sight! The companion was visible as almost round brightening close to the first diffraction ring of the primary component. The diffraction ring itself appeared very fine. At 224x also a very nice sight with a clear diffraction ring and the companion, which now appeared roundish. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
AB: Quite close, very bright yellow white A and brownish B, split in A's diffraction ring. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB: Iota Leo. Light orange A and a richer orange B, ~2 delta mag, ~2" separation |
|
|
|
★★
|
STF1540, 83 Leo |
|
AB |
6m5 |
7m5 |
28.4'' |
150° |
2018 |
Leo |
11h26m45.32s |
+03°00'47.20" |
Stefan Loibl
Rosenheim (Germany) |
10x50 |
clearly split, little difference in magnitude |
|
René Merting
Drachhausen (Germany) |
18x70 |
ein ordentlich getrenntes und dennoch schön eng stehendes Pärchen - Komponente A ist leicht gelblich, Komponente B im SO ist eine dreiviertel Magnitude schwächer und grauweiß |
|
Robert Zebahl
Leipzig (Germany) |
55mm (16x) |
Wonderful double with slight color contrast in a very nice field. Together with tau Leo stunning view. Slightly unequal. A appeared white-yellowish, B rather grey-bluish. |
|
Mark McCarthy
Fremont (California/USA) |
80mm (13x) |
Finder split, in same field as Tau. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
Yellow A and reddish B wide separation. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
bei 72x steht das Paar zwar weit auseinander, es wirkt aber trotzdem gut zusammengehörend - Komponente B im SO ist eine dreiviertel Magnitude schwächer |
|
|
|
|
STT234 |
|
|
7m5 |
8m1 |
0.4'' |
181° |
2017 |
UMa |
11h30m49.91s |
+41°17'12.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Surprisingly tough. Had indications of elongation at powers starting from 533x, but needed 1067x to get the clear bump, but even then it wasn't cleanly split |
|
|
|
★
|
STF1547, 88 Leo |
|
AB |
6m3 |
9m1 |
15.5'' |
332° |
2018 |
Leo |
11h31m44.94s |
+14°21'52.20" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (42x) |
Well split with moderate distance. Primary component appeared white-yellowish. Pretty unequal pair. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x erscheint Komponente B nordwestlich von A etwas mehr als knapp getrennt ganz schwach, bestimmt 3 Größenklassen Helligkeitsunterschied - Komponente A warmweiß, B ist grau |
|
Gerd Kohler
Langenzenn (Germany) |
254mm (76x) |
Der Doppelstern ist getrennt.Bläulich-weiß - orange-leicht rötlich. Etwas schwächerer Begleiter. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
Bright yellow A, 3x fainter red B. Wide separation. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
88 Leonis: A favorite! Yellow and blue pair, wide |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ein schönes enges Sternpaar, ordentlich getrennt - Komponente A strahlt hellgelb, B ist deutlich schwächer und empfiehlt sich mit einem Kupferton - ein schöner Farbkontrast |
|
|
|
★★
|
STT235 |
|
AB |
5m7 |
7m5 |
0.9'' |
43° |
2017 |
UMa |
11h32m20.76s |
+61°04'57.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Nice! Yellow and orange, 1.5 delta mag, split when seeing shows perfect disks. The stars both show albedo effects, look like suns / globes with shadowing. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Short period. Pretty yellow A, orange B, ~1" ~2 delta mag |
|
|
|
★
|
STF1555 & HJ503 |
STF1555 |
AB |
6m4 |
6m8 |
0.8'' |
149° |
2016 |
Leo |
11h36m17.94s |
+27°46'52.70" |
|
|
|
HJ503 |
AB-C |
5m8 |
11m2 |
22.5'' |
156° |
2016 |
|
|
|
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
STF1555 (AB): blickweise gerade eben trennbar |
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
STF1555 (AB): Nice! AB tight hair-split white pair, with fainter & wide separated AB-C in a row to the east. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
HJ503 (AB-C): Nice! STF 1555AB tight hair-split white pair, with fainter & wide separated C in a row to the east. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (553x) |
STF1555 (AB): Hairline split at 333x, clear split with 533x, very close ~0.5", bright. Part of plus one |
|
|
|
|
STF1553 |
|
|
7m7 |
8m2 |
6.2'' |
165° |
2018 |
UMa |
11h36m35.69s |
+56°08'07.30" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (31x) |
2020-04-19: At 22x medium bright double star with apparently similar bright components. At first sight visible as '8', on closer look separated. At 31x very fine split of the components with small difference in brightness. The two components appeared yellowish and slightly orange. |
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x sehe ich zwei fast gleich helle Sterne ganz eng beieinander stehen, da passt sprichwörtlich kein Blatt Papier dazwischen - bei 72x Helligkeitsunterschied eine knappe halbe Magnitude - ein ganz feiner Farbunterschied, Komponente A leicht weißgelblich, B im Osten wirkt ein bisschen grau |
|
|
|
|
STF1561 |
|
AB |
6m5 |
8m2 |
8.9'' |
247° |
2017 |
UMa |
11h38m44.90s |
+45°06'30.30" |
|
|
|
|
AC |
6m5 |
9m5 |
176.8'' |
90° |
2015 |
|
|
|
|
|
|
|
AD |
6m5 |
7m6 |
718.2'' |
76° |
2015 |
|
|
|
|
|
|
|
AE |
6m5 |
12m1 |
60.7'' |
338° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (31x) |
AB: 2020-04-19: At 22x separated, but relatively tight together with significant difference in brightness. The pair stands close to 2 medium bright stars. Both components appear white. At 31x beautiful sight, the color of the components looks slightly different: white-yellowish with darker ( slightly orange?) companion. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
AB: 2020-04-07: At 22x separated. The fainter companion is still very close to the primary component. At 44x beautiful sight with a clear difference in brightness. A: slightly yellowish, B: pale bluish. |
|
|
|
★
|
BU603 |
|
AB |
6m0 |
8m5 |
1.0'' |
329° |
2018 |
Leo |
11h48m38.71s |
+14°17'03.20" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
nicht getrennt |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Suspected at 205x and 333x but needed higher magnification to see it. B is a very small point, with seeing, in the first diffraction ring. ~1" and ~3 delta mag |
|
|
|
|
STF1608 |
|
AB |
8m1 |
8m3 |
13.6'' |
221° |
2017 |
UMa |
12h11m27.76s |
+53°25'17.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
2020-04-19: Easy to find, medium bright. At 22x quite conspicuous with rather small difference in brightness. A difference in color is clearly visible: slightly orange, white-bluish. At 31x nice color contrast with a little more intensive colors: light orange & light blue. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
bei 72x ein schönes helles Pärchen, beide Komponenten sind gleich hell und zahncremeweiß |
|
|
|
|
STF1639 |
|
AB |
6m7 |
7m8 |
1.8'' |
323° |
2018 |
Com |
12h24m26.81s |
+25°34'56.70" |
|
|
|
|
AC |
6m7 |
11m4 |
91.4'' |
159° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (133x) |
AB: 2020-04-04: The double star is clearly elongated, with the fainter companion attached to the primary component. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: White and slightly blue pair, close, around 3" |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: White and slightly blue pair, close, around 3"? |
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
AB: Close but well split, 1.5 delta mag, ~2.5" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB: Pretty yellow stars, ~2" separation, ~2 delta mag |
|
|
|
|
STF1643 |
|
AB |
9m0 |
9m4 |
2.7'' |
4° |
2018 |
Com |
12h27m13.72s |
+27°01'29.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Equal orange pair, ~3", PA to north. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
Yellow-white stars, ~3" separation, ~2 delta mag |
|
|
|
|
STT251 |
|
|
8m3 |
9m3 |
0.7'' |
55° |
2018 |
CVn |
12h29m07.72s |
+31°23'25.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Decidedly not round disk -- there's also a brightening in the diffraction. Marginal. |
|
|
|
★★
|
WRH12, 23 Com |
|
|
5m0 |
6m9 |
0.3'' |
12° |
2016 |
Com |
12h34m51.12s |
+22°37'45.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
23 Com. I get a definite snowman and can tell the larger from the smaller star, pointed in a certain direction in relation to a faint field star. Short Period double |
|
|
|
|
STF1663 |
|
|
8m0 |
9m2 |
0.5'' |
65° |
2017 |
Com |
12h37m10.81s |
+21°11'52.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Hairline split, ~1 delta mag, tough. Light yellow-orange A |
|
|
|
★★★
|
STF1670, gamma Vir, 29 Vir, Porrima |
|
AB |
3m5 |
3m5 |
2.7'' |
0° |
2018 |
Vir |
12h41m39.60s |
-01°26'57.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (56x) |
2019-05-18: At 38x slightly elongated. At 56x touching diffraction disks. At 71x clearly separated with very small gap. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (104x) |
2019-05-04: At 47x clearly visible as '8', at 73x split with almost touching diffraction disks. At 104x clearly separated, equally bright and pretty close together. The gap was smaller than the diameter of the diffraction disk. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
2019-05-01: Extremely nice double star! Equally bright and relatively close together. Both components appeared yellowish-white. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
weiß-weiß, die nördliche Komponente ist eine Winzigkeit heller |
|
Winfried Kräling
Marburg (Germany) |
127mm (146x) |
21.04.2018: Bei V=100x erscheint dieser orangefarbene Doppelstern bereits als „8“. Bei V=146x ist Porrima voll getrennt. |
|
Sarah Gebauer
Germany |
150mm (166x) |
die 2,8'' entfernten Komponenten A und B konnten haarscharf bei 83x und 166x getrennt werden, beide strahlen gleich hell als ganz dichte Glanzpünktchen; Komponenten E und F wurden gesehen, C und D allerdings nicht; bei 83x waren AB ganz knapp nicht mehr voneinander getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (170x) |
Porrima. Very pretty yellow-white, near equal, close split at 170x. Star disks improved with apodizing mask. |
|
|
|
|
STF1687, 35 Com |
|
AB |
5m2 |
7m1 |
1.2'' |
199° |
2018 |
Com |
12h53m17.77s |
+21°14'42.10" |
|
|
|
|
AC |
5m2 |
9m8 |
28.5'' |
127° |
2016 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AC: Rich light yellow and much fainter wide blue B. Near M64. [Need to re-observe. I saw the wide AC, but not the AB which is 5.15/7.08 1.2" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (205x) |
AC: Rich light yellow and much fainter wide blue B. Near M64. (Need to re-observe. I saw the wide AC, but not the AB which is 5.15/7.08 1.2") |
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
AC: Orange and blue, 3 delta mag, very wide separation to the east. Did not notice AB |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: 35 Com: Bright orange & fainter B, showpiece, ~1.5" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
AB: 35 Com. Can see the 7th magnitude B at 333x, but it's easier to resolve with 533x. Part of plus one. Bright orange A and deeper orange B |
|
|
|
|
STT256 |
|
|
7m3 |
7m6 |
1.1'' |
101° |
2017 |
Vir |
12h56m26.59s |
-00°57'16.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wide separation equal brightness white stars |
|
|
|
|
78 UMa, BU1082 |
|
|
5m0 |
7m9 |
0.8'' |
127° |
2017 |
UMa |
13h00m43.59s |
+56°21'58.80" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (260x) |
nicht getrennt |
|
|
|
|
STT261 |
|
|
7m4 |
7m6 |
2.6'' |
339° |
2017 |
CVn |
13h12m02.02s |
+32°05'07.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
2020-04-20: At 44x immediately visible as figure '8', even separable on closer look. The components appeared similarly bright. Overall rather dim. At 57x clearly split, but still very close together with a small difference in brightness. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Light yellow-white equal pair, ~1.5" |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Light yellow-white equal pair, ~1.5". |
|
|
|
|
RST3829 & SHJ162 |
RST3829 |
Aa-Ab |
7m3 |
9m1 |
0.5'' |
166° |
2018 |
Vir |
13h14m55.72s |
-11°22'09.90" |
|
|
|
SHJ162 |
AB |
7m1 |
8m2 |
113.2'' |
45° |
2017 |
|
|
|
|
|
|
SHJ162 |
BC |
8m2 |
13m3 |
66.2'' |
136° |
2015 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
SHJ162 (AB): bei 32x weit auseinander stehend - ein eigentümlicher Farbkontrast, A strahlt weiß, B kupfern |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
SHJ162 (AB): a widely separated yellow A and orange B, 1 magnitude difference. |
|
|
|
★
|
BU800 |
|
AB |
6m7 |
9m5 |
7.6'' |
104° |
2018 |
Com |
13h16m51.05s |
+17°01'01.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Lovely yellow and orange, very pretty. Wide separation, 2.5 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Lovely yellow and orange, very pretty, wide separation, 2.5 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice pair, A is a light but rich yellow, B is blue-white. Wide, ~2 delta mag |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Not difficult, orange-yellow A with bluish B, 3 delta mag. pretty wide to east. |
|
|
|
★★
|
HU644 |
|
AB |
9m1 |
9m9 |
0.1'' |
354° |
2019 |
CVn |
13h19m45.58s |
+47°46'41.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (443x) |
Orange-red pair, near equal mag, split with seeing at 443x |
|
|
|
|
STF1734 |
|
|
6m8 |
7m3 |
1.1'' |
173° |
2017 |
Vir |
13h20m41.57s |
+02°56'31.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (104x) |
Double star appeared slightly elongated without noticeable notching. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Blue-white A, light orange B, half delta mag, close ~1.5". Nice! |
|
|
|
|
STT266 |
|
|
8m0 |
8m4 |
2.0'' |
358° |
2018 |
Com |
13h28m26.68s |
+15°42'30.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
~0.5 delta mag, ~2 separation, nice looking pair |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Close 2" near equal white. Period of 1954.11 years. Near its closest separation now (May 2017), will be ~4" by the year 2822. |
|
|
|
|
STF1752 |
|
AB |
8m2 |
9m9 |
1.0'' |
107° |
2017 |
UMa |
13h28m49.82s |
+59°55'41.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange star perhaps a little elongated, tough. |
|
|
|
|
VYS6, VW Com |
|
|
11m4 |
11m3 |
2.6'' |
55° |
2018 |
Com |
13h32m44.59s |
+16°48'39.00" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
VW Com. Seen best with averted vision and when seeing stills. Close but pretty well split, ~2-3". Extremely faint reddish pair, PA NE. |
|
|
|
|
STF1757 |
|
AB |
7m8 |
8m8 |
1.7'' |
143° |
2018 |
Vir |
13h34m16.38s |
-00°18'49.80" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
schwierig |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Close, ~2", a dull orange, ~1.5 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange-yellow, half a delta mag, pretty, ~1.5" |
|
|
|
|
BU932 |
|
AB |
6m3 |
7m3 |
0.4'' |
67° |
2018 |
Vir |
13h34m40.48s |
-13°12'51.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (170x) |
Out of round with apodizing mask |
|
|
|
★
|
25 CVn |
STF1768 |
AB |
5m0 |
7m0 |
1.7'' |
99° |
2018 |
CVn |
13h37m27.70s |
+36°17'41.40" |
|
|
|
STF1768 |
AC |
5m0 |
11m6 |
214.3'' |
321° |
2015 |
|
|
|
|
|
|
KZA73 |
AD |
5m0 |
13m0 |
335.6'' |
92° |
2015 |
|
|
|
|
|
|
KZA73 |
AE |
5m0 |
12m7 |
369.5'' |
139° |
2015 |
|
|
|
|
|
|
KZA73 |
AF |
5m0 |
9m4 |
437.3'' |
118° |
2015 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
60mm (160x) |
AB: 2020-03-16: 102/1122mm ED refractor stopped down to 60mm. The diffraction ring of the primary component is virtually invisible. The companion appears only in few moments as an extremely faint, elongated brightening in the diffraction ring. Very difficult. Telescope should be in very good optical condition! |
|
Robert Zebahl
Leipzig (Germany) |
70mm (160x) |
AB: 2020-03-16: 102/1122mm ED refractor stopped down to 70mm. Companion only visible as a subtle, elongated, not permanently visible brightening. The diffraction ring of the primary component is only visible occasionally. Difficult. Telescope should be in good optical condition! |
|
Robert Zebahl
Leipzig (Germany) |
80mm (160x) |
AB: 2020-03-16: 102/1122mm ED refractor stopped down to 80mm. Companion permanently visible as elongated brightening in the diffraction ring. But the diffraction ring itself appears rather faint. Moderately difficult. |
|
Robert Zebahl
Leipzig (Germany) |
90mm (160x) |
AB: 2020-03-16: 102/1122mm ED refractor stopped down to 90mm. Companion quite clearly recognizable as elongated brightening in diffraction ring. Relatively simple. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (160x) |
AB: 2020-03-16: The faint companion is immediately recognizable as a distinct, slightly elongated brightening in the diffraction ring. Easy. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (150x) |
AB: 2020-03-19: At 150x the clearly fainter companion is visible as a roundish brightening. Due to the chromatic aberration of the achromat (152mm f/5.9) the companion is almost outshined. At 180x the companion is then well, at 225x and 300x very well visible as a tiny separated star. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Very tight pair, a little more than hairline split, ~2 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Very tight pair, a little more than hairline split, ~2 delta mag. 8" 333x: white and dull blue, ~1", Nice! |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: White and dull blue, ~1" Nice! |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: schwierig wegen Helligkeitsunterschied |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Very pretty pale yellow and orange, 2-3 delta mag, ~2" |
|
|
|
|
STF1781, HT Vir |
|
AB |
7m9 |
8m1 |
1.0'' |
195° |
2017 |
Vir |
13h46m06.75s |
+05°06'56.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
White A and slightly yellow B, ~2", half delta mag |
|
|
|
|
STF1785 |
|
|
7m4 |
8m2 |
2.8'' |
190° |
2019 |
Boo |
13h49m04.00s |
+26°58'47.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Slightly orange-tinged white stars, near equal, well separated |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Im CLT bei 180 x Vergrößerung gut zu trennen. Leichter Helligkeitsunterschied und beider Sterne erscheinen gelborange. |
|
|
|
★
|
STF1788 |
|
AB |
6m7 |
7m3 |
3.7'' |
101° |
2018 |
Vir |
13h54m58.20s |
-08°03'31.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (47x) |
Very nice view! Pretty tight together with a moderate difference in brightness. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 107x zeigt sich ein schönes, knapp getrenntes Pärchen - B im Osten ist nur knapp schwächer als A - Komponente A ist weiß, B ist grau, wirkt aber auch leicht gelb gefärbt - zurück auf 64x kann ich die beiden Sterne auch schon knapp getrennt erkennen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (340x) |
bright pair of near equal magnitude, both yellow-while color. |
|
|
|
|
A1097 & STF1800 |
A1097 |
AB |
9m1 |
8m2 |
0.4'' |
259° |
2016 |
UMa |
14h02m00.60s |
+57°13'28.60" |
|
|
|
STF1800 |
AB-C |
7m8 |
10m4 |
28.4'' |
20° |
2015 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
A1097 (AB): Hair-split at best moments, half delta mag, <0.8". A fainter star likely in the system about 30" distant -- this is STF 1800 AB-C. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF1800 (AB-C): Faint star ~30" from A1097 |
|
|
|
|
STF1820 |
|
|
9m1 |
9m4 |
2.8'' |
123° |
2019 |
UMa |
14h13m00.76s |
+55°19'31.10" |
|
|
René Merting
Drachhausen (Germany) |
320mm (144x) |
bei 72x ist ein Stäbchen mit einer angedeuteten Einschnürung erkennen - bei 144x sind beide Komponenten getrennt voneinander sichtbar - beide sind gleich hell |
|
|
|
★
|
BU224 |
|
|
8m9 |
9m3 |
0.6'' |
101° |
2016 |
Boo |
14h13m26.94s |
+12°34'26.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Hairline split with seeing, light yellow-white stars, noticeable mag difference. Snowman when seeing is not stable |
|
|
|
|
STF1821, kappa Boo, 17 Boo, Asellus Tertius |
|
AB |
4m5 |
6m6 |
13.7'' |
236° |
2017 |
Boo |
14h13m29.00s |
+51°47'23.80" |
|
|
René Merting
Drachhausen (Germany) |
18x70 |
Komponente A strahlt so hell, dass B deutlich schwächer ganz knapp im SW von A abgesetzt sichtbar ist - Helligkeitsunterschied schätzungsweise 3 Magnituden (nur 2.09 mag laut Stelle Doppie) |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
2020-04-24: Clearly separated with significant difference in brightness. The primary component showed a pale yellowish-orange color with a greyish companion. To the southeast there is the double star STFA 26. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (144x) |
weiß-grau, trennbar bei 22x |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Im CLT leicht zu trennen. Beider Sterne erscheinen weißlich. |
|
|
|
★
|
STF1816 |
|
|
7m4 |
7m8 |
0.4'' |
99° |
2016 |
Boo |
14h13m54.63s |
+29°06'19.50" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
gelb |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Rod-shaped equal white. July 2017 |
|
|
|
★★
|
A1101 |
|
AB |
9m7 |
10m3 |
0.3'' |
224° |
2018 |
Boo |
14h15m50.57s |
+10°17'59.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
I stared for a long time and had brief instants of an elongation or bump, and even a tentative split of a star. Sketched the orientation will check the PA later [I think I have it. My orientation on the sketch is in the correct position as in relation to the AB-C & AB-D pairs.] |
|
|
|
★
|
STF1825 |
|
|
6m5 |
8m4 |
4.2'' |
154° |
2019 |
Boo |
14h16m32.84s |
+20°07'18.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Cream white A and light blue B, wide ~5", ~2 delta mag |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
White and orange, 3 delta mag, well split. |
|
|
|
|
STF1834 |
|
|
8m1 |
8m3 |
1.6'' |
104° |
2018 |
Boo |
14h20m17.60s |
+48°30'25.10" |
|
|
Robert Zebahl
Leipzig (Germany) |
120mm (150x) |
At 108x elongated, at 150x barely split with similarly bright components. |
|
|
|
★★
|
STF1835 & BU1111 |
STF1835 |
A-BC |
5m0 |
6m8 |
6.2'' |
196° |
2018 |
Boo |
14h23m22.74s |
+08°26'47.90" |
|
|
|
BU1111 |
BC |
7m4 |
7m7 |
0.3'' |
16° |
2018 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
STF1835 (A-BC): bei 32x erscheint der Stern leicht unrund, verschmiert - bei 107x präsentiert sich BC gut getrennt im Süden von A - Helligkeitsunterschied eine Größenklasse (1.75 mag laut Stelle Doppie) - bei 64x sind beide Sterne auch getrennt erkennbar, BC strahlt warmweiß |
|
Robert Zebahl
Leipzig (Germany) |
102mm (62x) |
STF1835 (A-BC): At 28x barely split with visible difference in brightness. At 62x easy to separate. The colors seemed similar. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
STF1835 (A-BC): Yellow A and slightly yellow B, wide. Did not notice BU1111 BC, 0.3" 7.4/7.7 |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF1835 (A-BC): In a line of three stars, white and slightly red B. Wide, ~6", 2 delta mag. Did not detect BC 0.3" |
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
BU1111 (BC): Short period pair, it is a component of STF 1835. I get a nothed near equal elongation with a clear direction in relation to the A star. Very cool |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
STF1835 (A-BC): Doppelstern konnte im CLT gut getrennt werden. Helligkeitsunterschied ist merklich, aber nicht extrem. Der hellere erscheint eher weißlich und der kleinere eher bläulich. Der Farbunterschied ist aber minimal. |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
STF1835 (A-BC): close DS |
|
|
|
|
STF1858 |
|
AB |
8m1 |
9m0 |
3.0'' |
38° |
2019 |
Boo |
14h33m36.45s |
+35°35'08.00" |
|
|
|
|
AC |
8m1 |
14m3 |
19.7'' |
335° |
2013 |
|
|
|
|
|
|
|
AD |
8m1 |
14m7 |
36.6'' |
322° |
2013 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
AB: bei 64x ein extrem dicht stehendes Pärchen, Trennung fast greifbar - bei 142x stehen die Sterne noch immer sehr eng, die Trennung ist nun aber eindeutig - Komponente B im NO ist etwas schwächer - beide Sterne leicht gelblich, hin und wieder mit Farbkontrast in Richtung orange |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
AB: nicht getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Near equal orange 3-4" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: 13th magnitude, a wide pair? Seen with averted vision, comes and goes with seeing |
|
|
|
|
STF1863 |
|
|
7m7 |
7m8 |
0.6'' |
63° |
2018 |
Boo |
14h38m00.71s |
+51°34'42.10" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gerade trennbar |
|
|
|
|
STF1867 |
|
|
8m4 |
8m8 |
0.7'' |
355° |
2017 |
Boo |
14h40m44.21s |
+31°17'23.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
0.5 delta mag, hair to figure 8 split, white. |
|
|
|
|
STF1872 |
|
AB |
7m5 |
8m3 |
7.4'' |
50° |
2019 |
Dra |
14h41m00.84s |
+57°57'28.10" |
|
|
René Merting
Drachhausen (Germany) |
320mm (45x) |
bei 45x ist die B-Komponente nordöstlich über A erkennbar, ein Blatt Papier passt zwischen die beiden - leichter Farbunterschied - bei 72x zeigt sich ein gut getrenntes Pärchen, B ist eine dreiviertel Magnitude schwächer und blauweiß, A ist gelbweiß |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern ist gut zu trennen. Helligkeitsunterschied ist erkennbar, aber nicht besonders auffällig. Der hellere Stern erscheint weißgelblich und der schwächere gelblich. |
|
|
|
★★
|
zeta Boo |
STF1865 |
AB |
4m5 |
4m5 |
0.3'' |
283° |
2018 |
Boo |
14h41m08.92s |
+13°43'42.00" |
|
|
|
H6 104 |
AB-C |
4m5 |
11m0 |
104.3'' |
260° |
2015 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
AB-C |
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
AB: Zeta Boo. Short period. First impression was moderately well notched overlapping disks (eg. not barely notched, but not strongly notched either). With more time observing & getting used to the image, and in moments of better seeing, the notch became more distinct. It would not separate in spite of moments of better seeing. I could also see the elongation, but only subtly notched due to the smaller scale, at 667x |
|
|
|
|
STF1878, DL Dra |
|
|
6m3 |
9m2 |
4.2'' |
314° |
2015 |
Dra |
14h42m03.25s |
+61°15'42.90" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (198x) |
starke Aufhellung im ersten Ring |
|
|
|
★★
|
HU575 |
|
AB |
9m8 |
10m1 |
0.5'' |
152° |
2011 |
Boo |
14h42m33.63s |
+19°28'46.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Short period. Small, faint, but definite split of these orange-red near equal stars. I sketched a clear orientation to field stars. Awesome |
|
|
|
★
|
A1109 |
|
AB |
7m4 |
9m4 |
1.9'' |
88° |
2017 |
Vir |
14h42m47.60s |
+06°35'26.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Both stars light yellow, big magnitude difference, ~3-4 delta mag, about 2". Not difficult |
|
|
|
|
STF1879 |
|
AB |
7m8 |
8m4 |
1.7'' |
82° |
2018 |
Boo |
14h46m15.58s |
+09°38'48.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Fairly close yellow and orange-yellow, ~1 delta mag, ~3" |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern konnte gerade so getrennt werden. Beide erscheinen weißlich. |
|
|
|
★
|
STF1884 |
|
|
6m6 |
7m5 |
2.1'' |
58° |
2019 |
Boo |
14h48m23.37s |
+24°22'01.00" |
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ist der Doppelstern als 8 erkennbar, 107x reicht dann für die knappe Trennung - die B-Komponente im NO ist nur unwesentlich schwächer - ein sehenswertes Pärchen |
|
Robert Zebahl
Leipzig (Germany) |
102mm (86x) |
At 86x pretty tight and unequal. At 160x clearly split. A: white, B: slightly orange. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
White, fairly close ~3", half delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
White, fairly close ~3", half delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Prototypical pair, >1 delta mag, ~3" separation, white to off white color |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
einfach |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Orange-white, 3 delta mag, ~5" |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern konnte gerade so getrennt werden. Beide Sternen leuchten weißlich. |
|
|
|
|
BU346 |
|
|
7m5 |
7m9 |
2.7'' |
277° |
2017 |
Lib |
14h48m31.71s |
-17°20'24.40" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Easy, well split, yellow-orange stars, half delta mag. |
|
|
|
|
STF1883 |
|
|
7m0 |
8m9 |
1.0'' |
278° |
2015 |
Vir |
14h48m53.22s |
+05°57'15.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Strongly suspect a split / elongation in 80mm finder. In the scope it is a tight 2 delta mag orangish-white pair, ~1" |
|
|
|
|
BU106, mu Lib, 7 Lib |
|
AB |
5m6 |
6m6 |
2.0'' |
4° |
2016 |
Lib |
14h49m19.09s |
-14°08'56.30" |
|
|
|
|
AC |
5m6 |
14m7 |
12.9'' |
294° |
2000 |
|
|
|
|
|
|
|
AD |
5m6 |
14m1 |
25.7'' |
168° |
2000 |
|
|
|
|
|
|
|
AE |
5m6 |
12m6 |
26.6'' |
232° |
2015 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Close, 1.5-2", half to one delta mag, off-white stars |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
AB: Close, 1.5-2", half to one delta mag, off-white stars. |
|
Gerd Kohler
Langenzenn (Germany) |
254mm (346x) |
AB: Bläulich-weiß - bläulich-weiß. A und B haben nur einen geringen Helligkeitsunterschied. |
|
Gerd Kohler
Langenzenn (Germany) |
254mm (346x) |
AE: Bläulich-weiß - weiß. Stern E ist sehr schwach. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: getrennt, schwierig wegen Südlage |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Mu Lib: Easy, white & off white, 1 delta mag, ~3" |
|
|
|
★
|
STF1890, 39 Boo |
|
|
6m3 |
6m7 |
2.5'' |
46° |
2019 |
Boo |
14h49m41.37s |
+48°43'15.60" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (67x) |
2020-04-01: At 44x elongated, partly notched. At 67x split, but very tight. A difference in brightness was not seen. At 133x clearly separated with little difference in brightness. A appeared pale yellow, B rather warm-white. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
2020-04-18: At 57x very finely separated with extremely tightly spaced components that appeared equally bright. At 100x a very nice pair with little difference in brightness. Fantastic sight! The color of the components was slightly different: creamy-white & a touch of yellow-orange. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gleich hell |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright white pair, well split |
|
|
|
★
|
STF1888 & ARN11, xi Boo, 37 Boo |
STF1888 |
AB |
4m8 |
7m0 |
5.3'' |
300° |
2018 |
Boo |
14h51m23.38s |
+19°06'01.70" |
|
|
|
STF1888 |
AC |
4m8 |
13m8 |
71.3'' |
340° |
2015 |
|
|
|
|
|
|
STF1888 |
AD |
4m8 |
11m7 |
160.8'' |
286° |
2015 |
|
|
|
|
|
|
ARN11 |
AE |
4m8 |
8m7 |
271.5'' |
98° |
2015 |
|
|
|
|
|
|
ARN11 |
AF |
4m8 |
9m2 |
337.5'' |
37° |
2015 |
|
|
|
|
|
|
STF1888 |
BC |
7m0 |
13m8 |
63.9'' |
340° |
2001 |
|
|
|
|
|
|
STF1888 |
BE |
7m0 |
8m7 |
273.5'' |
102° |
2009 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
AB: 2020-04-24: Beautifully separated with quite a large difference in brightness in a lovely star field. The primary component shines yellowish with a faint companion. |
|
Sarah Gebauer
Germany |
150mm (83x) |
AB: die 6'' entfernten Komponenten A und B konnten mühelos bei 83x getrennt werden, Komponente E war zu sehen, C, D und F waren nicht sichtbar |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: A star a very pretty light yellow with 2 delta mag. light orange B star, ~5" separation |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: A star a very pretty light yellow with 2 delta mag. light orange B, ~5". |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
AB: Xi Boo Pretty yellow & orange pair, 2 delta mag, ~8". |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Pretty. Yellow and orange pair, ~6", 3 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB: Xi Boo. Short period. Richly colored yellow and orange stars, ~1 delta mag, ~5" separation, with several other stars in view. Very pretty |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
AB: Ein recht schöner Doppelstern, wobei neben dem Helligkeitsunterschied von 2,2 mag auch die Sternfarben ein schönes Gesamtbild geben. Der hellere Stern erstrahlt gelblich weiß und der schwächere orangegelb.
Hier handelt es sich auch um ein recht nahes System mit 21,9 Lichtjahren Entfernung. |
|
|
|
★
|
STT287 |
|
|
8m4 |
8m6 |
0.5'' |
6° |
2018 |
Boo |
14h51m27.53s |
+44°55'42.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Wow! Hair-split, ~0.7", near equal to half a delta mag. |
|
|
|
★
|
BU31 |
|
AB |
8m5 |
10m3 |
2.0'' |
222° |
2017 |
Boo |
14h52m30.05s |
+18°44'19.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
White A and light yellow B, finely split, ~2 delta mag |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern konnte gerade so getrennt werden. Die Distanz von 2,0 Bogensekunden und die Helligkeit beider Sterne, macht die Sichtung nicht leicht. |
|
|
|
|
STT288 |
|
|
6m9 |
7m5 |
1.0'' |
157° |
2018 |
Boo |
14h53m23.35s |
+15°42'18.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Consistent split, better with seeing, ~1 delta mag, ~1" separation, blue-white stars |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
rel. einfach |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Notched / figure 8 with 277x, split with 553x. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Needed 553x to separate, resolved with the seeing. Near equal yellow-white, ~1" or less. |
|
|
|
★
|
STF1909, 44 Boo |
|
|
5m2 |
6m1 |
0.4'' |
91° |
2018 |
Boo |
15h03m47.30s |
+47°39'14.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
2015 getrennt zu sehen (1") |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
I Boo. Figure 8 to hair split, ~0.9". This pair shrinking separation fast, will be <0.5" in a couple of years. Only 40 LY away. (July 2017) |
|
|
|
★
|
BU119 |
|
AB |
8m1 |
8m8 |
2.3'' |
275° |
2017 |
Lib |
15h05m31.91s |
-07°00'48.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Tried 667x at first but it was too much power, too dim and seeing too choppy. 333x was perfect, clean and well split ~2" near equal, slightly orange |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
8" 667x Too much power, too dim and seeing too choppy. 8" 333x perfect, clean and well split ~2" near equal, slightly orange. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very like BU 346. well split near half delta mag yellow stars, 2.5” |
|
|
|
|
STFA27, delta Boo, 49 Boo |
|
AB |
3m6 |
7m9 |
105.0'' |
78° |
2017 |
Boo |
15h15m30.16s |
+33°18'53.40" |
René Merting
Drachhausen (Germany) |
18x70 |
ein sehr ungleiches, weit auseinander stehendes Sternpaar - Komponente A im Westen strahlt gleißend cremegelb, die wesentlich schwächere Komponente B im Osten ist weißgrau bis bräunlich |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
2020-04-24: Widely separated pair with large difference in brightness. Less striking. The bright primary component shines in a bright yellow. |
|
Mark McCarthy
Fremont (California/USA) |
80mm (13x) |
Split in 80mm finder. Very wide pair, very bright A, 3 delta mag B. Orange-yellow and blue-white B |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
Bright star with many nearby faint stars. Didn't bother trying to figure out which are which. |
|
|
|
★
|
STF1932 |
|
AB |
7m3 |
7m4 |
1.4'' |
268° |
2019 |
CrB |
15h18m20.19s |
+26°50'24.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Near equal, yellowish white, ~2" |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Near equal, yellowish white, ~2" |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Very beautiful near equal white stars, ~1.5" |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gleich hell, getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal yellow-white, very close but clean split, ~1.5". Nice! |
|
|
|
★★
|
mu Boo, 51 Boo, Alkalurops |
CHR181, mu 1 Boo |
Aa-Ab |
4m3 |
|
0.1'' |
188° |
2012 |
Boo |
15h24m29.54s |
+37°22'37.10" |
|
|
|
STFA28, mu 1 Boo |
AB |
4m3 |
7m1 |
109.0'' |
172° |
2018 |
|
|
|
|
|
|
STF1938, mu 2 Boo |
Ba-Bb |
7m1 |
7m6 |
2.3'' |
3° |
2019 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
8x40 |
STFA28 (AB): Easily split with obvious difference in brightness. |
|
René Merting
Drachhausen (Germany) |
16x70 |
STFA28 (AB): weit getrenntes Pärchen, aufgrund der großen Helligkeitsunterschiedes schöner Farbkontrast - Komponente A im Norden gelblich, B im Süden mehr grau-braun |
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
STFA28 (AB): Evident, very wide apart and unequal. A: white-yellowish, B: grey. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
STF1938 (Ba-Bb): Beautiful view! This triple system includes STFA 28 and STF 1938. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
ein heller 4m und zwei nahe dunkle 7m, lohnend. |
|
Robert Zebahl
Leipzig (Germany) |
120mm (23x) |
STFA28 (AB): Easy to split with large angular distance and noticeable difference in brightness. |
|
Sarah Gebauer
Germany |
150mm (125x) |
A-BC mit 109'' sind bei 125x sehr weit getrennt, es ist der Ansatz eines engen Doppelsterns zu erkennen, der sich mit 2,2'' Abstand auch bis 250x nicht auftrennen ließ |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
STFA28 (AB): Bright A star does not seem round. The B star is a tight equal pair, pretty set. [Aa,Ab is CHR 181 0.1", and I'd be shocked if I actually detected it. STFA 28 is technically the bright star and the tight pair, the tight pair is Ba,Bb = STF 1938, 7.09/7.63, 2.2"] |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
STFA28 (AB): Bright A star does not seem round (CHR181). B star is a tight equal pair (STF1938 Ba-Bb). Pretty set. STFA 28 is technically the bright star and the tight pair |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
CHR181 (Aa-Ab): Bright A star does not seem round (CHR181). B star is a tight equal pair (STF1938 Ba-Bb). Pretty set. STFA 28 is technically the bright star and the tight pair |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
STF1938 (Ba-Bb): Bright A star does not seem round (CHR181). B star is a tight equal pair (STF1938 Ba-Bb). Pretty set. STFA 28 is technically the bright star and the tight pair |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
STF1938 (Ba-Bb): 3er System, schön |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF1938 (Ba-Bb): Tight 3 detla mag pair, fainter than the bright white A star Mu Boo. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STFA28 (AB): Bright white star with tight yellow pair STF 1938 as its companion. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STFA28 (AB): Striking. Bright star with near equal double STF 1938 paired with it. A star is a spectroscopic binary |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF1938 (Ba-Bb): Near equal close but well split double also paired with STFA28 |
|
Karsten Kopp
Köln (Germany) |
600mm (257x) |
Hier handelt es sich um ein Dreifachsternsystem, welches jetzt aber nicht durch eine besondere Färbung der Sterne auffällt. Die A - B/C Komponenten stehen noch sehr weit auseinander, wobei auch die A-Komponente um einiges heller erscheint. Die beiden Komponenten B/C sind wesentlich näher beieinander und unterscheiden sich auch kaum in ihrer Helligkeit. |
|
|
|
|
HU149 |
|
|
7m5 |
7m6 |
0.7'' |
272° |
2017 |
Dra |
15h24m35.30s |
+54°12'46.10" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
mit Zwischenraum zu sehen |
|
|
|
★★
|
STT296 |
|
AB |
7m8 |
9m1 |
2.1'' |
274° |
2019 |
Boo |
15h26m26.56s |
+44°00'13.20" |
|
|
|
|
AC |
7m8 |
12m7 |
80.7'' |
313° |
2016 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Very fine but well split, ~2", yellow-white A, reddish B, 2 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: Very fine but well split, ~2", yellow-white A, reddish B, 2 delta mag. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Very beautiful, 2", 2 delta mag, with very faint third (AC) seen with averted vision widely separated. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AC: Very beautiful, 2", 2 delta mag, with very faint third (AC) seen with averted vision widely separated. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Close near equal, 1 delta mag, white. |
|
|
|
|
STF1954, delta Ser, 13 Ser |
|
AB |
4m2 |
5m2 |
4.0'' |
171° |
2019 |
Ser |
15h34m48.14s |
+10°32'20.00" |
|
|
|
|
AC |
4m2 |
13m9 |
66.6'' |
18° |
2014 |
|
|
|
|
|
|
|
CD |
13m9 |
14m6 |
4.0'' |
341° |
2018 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
AB: Easy to separate with relatively close components and a clear difference in brightness. A appeared rather white, B slightly orange. |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 142x zwei gut getrennte reinweiße Komponenten - B wirkt eine halbe Größenklasse schwächer - zurück auf 107x ist die Trennung ebenfalls einfach - zurück auf 64x ist es eine 8 mit tiefen Einschnürungen, kurz vor der Trennung |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
AB: sparse field |
|
Sarah Gebauer
Germany |
150mm (85x) |
AB: Mit 85x schon schön getrennt, ein leichter Größenunterschied der Sterne zu erkennen, einige schwache Feldsterne im Okular bei 0,95° Gf. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: getrennt, Del Ser |
|
|
|
★
|
STT298 |
|
AB |
7m2 |
8m4 |
1.3'' |
187° |
2017 |
Boo |
15h36m02.22s |
+39°48'08.90" |
|
|
|
|
AB-C |
6m9 |
7m8 |
120.4'' |
328° |
2017 |
|
|
|
|
|
|
|
AB-D |
6m9 |
13m9 |
167.4'' |
224° |
2002 |
|
|
|
|
|
|
|
AB-E |
6m9 |
12m1 |
456.0'' |
335° |
2002 |
|
|
|
|
|
Robert Zebahl
Leipzig (Germany) |
102mm (28x) |
AB-C: Wide, moderately unequal pair. Little difference in color: Primary components appeared a bit more orange colored. |
|
Robert Zebahl
Leipzig (Germany) |
120mm (23x) |
AB-C: Easy to split with large angular distance and noticeable difference in brightness. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: At zenith, but worth the effort to slew to. Another great 2+1. The tight pair [AB] is near equal and split a little more than a hairline |
|
Mark McCarthy
Fremont (California/USA) |
203mm (205x) |
AB: At zenith, but worth the effort to slew to. Another great 2+1. The tight pair (AB) is near equal and split a little more than a hairline split. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: One component of compicated 6 star system, some of which is split in 80mm finter. This is a close equal pair, ~2". |
|
|
|
★★
|
STF1964 & HU1167 |
HU1167 |
AB |
8m1 |
9m9 |
1.4'' |
80° |
2016 |
CrB |
15h38m12.91s |
+36°14'48.60" |
|
|
|
STF1964 |
AC |
8m1 |
8m1 |
14.5'' |
90° |
2017 |
|
|
|
|
|
|
STF1964 |
AD |
8m1 |
9m0 |
15.1'' |
84° |
2018 |
|
|
|
|
|
|
STF1964 |
CD |
8m1 |
9m0 |
1.5'' |
21° |
2019 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
18x70 |
STF1964 (AC): zu erkennen sind zwei gleich helle, sehr dicht stehende Sterne - Trennung ein wenig mehr als knapp |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
STF1964 (AC): bei 20x ein gut getrenntes Pärchen gleich heller Sterne, auffallend im Sternumfeld |
|
Robert Zebahl
Leipzig (Germany) |
102mm (62x) |
STF1964 (AC): Rather wide pair, equal without visible difference in color. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (16x) |
Dreifachstern nicht trennbar |
|
Robert Zebahl
Leipzig (Germany) |
120mm (23x) |
STF1964 (AC): Nice double star, well split with equally bright components. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
STF1964 (AC): Well split equal pair. I suspect B is pair as it is an elongated orange smear at 277x -- it is STF 1964CD. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF1964 (CD): Split, light orange 1 delta mag pair |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
STF1964 (CD): Faint near equal pair about 3" separation. In the same field with HU 1167. Magnificent |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
HU1167 (AB): Bright star with much fainter pair, about 1" separation, 3-4 delta mag. In same field with STF 1964. Magnificent |
|
|
|
|
STF1989, pi UMi |
|
|
7m3 |
8m2 |
0.7'' |
23° |
2013 |
UMi |
15h39m38.61s |
+79°58'59.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
blickweise als 8 zu sehen, schwierig |
|
|
|
★
|
STF1967, gam CrB |
|
|
4m0 |
5m6 |
0.6'' |
111° |
2012 |
CrB |
15h42m44.57s |
+26°17'44.30" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Definite mis-shape, oval to egg, observation made June 2019 |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Gamma CrB. Definite mis-shape, oval to egg. |
|
|
|
|
STT303 |
|
AB |
7m7 |
8m1 |
1.6'' |
175° |
2019 |
Ser |
16h00m54.16s |
+13°16'18.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal white, ~1.5". Nice! |
|
|
|
|
S676, rho CrB |
|
|
5m5 |
10m5 |
141.7'' |
47° |
2012 |
CrB |
16h01m02.65s |
+33°18'12.60" |
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Rho CrB. bright orange star with very obvious wide B, 3 delta mag |
|
|
|
★
|
STF2021, 49 Ser |
|
AB |
7m4 |
7m5 |
4.0'' |
358° |
2019 |
Her |
16h13m18.45s |
+13°31'37.20" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Lovely split. Almost equal pair with relatively close components. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x zeigen sich zwei gleich helle weiße Sterne, die sich gerade noch berühren - bei 64x dann knappe Trennung, B ist nur minimal schwächer |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Equal yellow-white stars, ~4". |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern ist gut zu trennen, bei fast identischer Helligkeit. Ein weißliches Augenpaar schaut mich an. |
|
|
|
|
sigma CrB, 17 CrB, STF2032 |
|
AB |
5m6 |
6m5 |
7.2'' |
239° |
2019 |
CrB |
16h14m40.85s |
+33°51'31.00" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (22x) |
At 22x clearly separated, but very close with a clear difference in brightness. At 57x easy without any noticeable difference in color. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 20x zwei knapp zusammenstehende Sterne mit tiefer Einschnürung - bei 32x dann ein knapp getrenntes Pärchen - B-Komponente südwestlich gut eine halbe Größenklasse schwächer - beide Sterne mit weißem Brautkleid |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (26x) |
Already split at 26x. Component A orange, B yellow. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Nice wide white, ~1 delta mag. |
|
René Merting
Drachhausen (Germany) |
320mm (72x) |
bei 72x ein schick anzusehendes, knapp getrenntes Pärchen - A im Osten ist hellgelb - B ist vielleicht eine halbe Größenklasse schwächer und auch gelblich, aber nicht so stark wie A |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Sigma CrB. AB nice bright half delta mag wide. two more stars in system, one (AC) closer fainter, other (AD) further away. |
|
Karsten Kopp
Köln (Germany) |
600mm (135x) |
Sehr einfaches, auffälliges Objekt im Okular, ansonsten keine weiteren Auffälligkeiten. |
|
|
|
|
STF2026 |
|
AB |
9m5 |
9m9 |
3.5'' |
16° |
2019 |
Her |
16h15m57.07s |
+07°21'24.80" |
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x sind die Sterne so schwach, dass ich hellere Sterne im Umfeld zum Fokussieren nutzen muss - beide Komponenten sind als 8 erkennbar, die Einschnürung ist aber nur in guten Momenten da - bei 107x dann gelingt die Trennung, B wirkt deutlich schwächer (in Wirklichkeit ist B nur 0m4 schwächer), aber vielleicht liegt es daran, dass die beiden Sterne ohnehin nur sehr schwach beobachtbar sind - das hat wenig Freude bereitet |
|
|
|
|
KUI72 |
|
|
5m5 |
10m0 |
2.1'' |
127° |
1997 |
Her |
16h19m55.24s |
+39°42'30.90" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Distinct faint point appears with perfect seeing ~2-3". Much smaller and fainter than A. |
|
|
|
★★★
|
rho Oph, 5 Oph |
H2 19 |
AB |
5m1 |
5m7 |
3.0'' |
334° |
2017 |
Oph |
16h25m35.03s |
-23°26'47.00" |
|
|
|
H2 19 |
AC |
5m1 |
7m3 |
149.2'' |
0° |
2000 |
|
|
|
|
|
|
H2 19 |
AD |
5m1 |
6m8 |
156.4'' |
252° |
2000 |
|
|
|
|
|
|
KOU63 |
CF |
5m8 |
11m7 |
4.8'' |
206° |
2000 |
|
|
|
|
|
|
BU1115 |
DE |
6m8 |
8m4 |
0.3'' |
196° |
2018 |
|
|
|
|
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
AB: possible components (DE) and (CF) already visible at 27x magnification with ca. 2 arcmin distance |
|
|
|
★
|
STF2052 |
|
AB |
7m7 |
7m9 |
2.5'' |
118° |
2018 |
Her |
16h28m52.67s |
+18°24'50.60" |
|
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x zwei gleichhelle Sterne, die sich gerade so berühren - bei 107x ein knapp getrenntes Pärchen, Komponente B im SO ist nur marginal schwächer |
|
Stefan Loibl
Rosenheim (Germany) |
102mm (102x) |
Does not appear as a multiple star at 28x, elongated at 68x, splith with 102x. Component A blueish, B reddish. Observation of component C questionable. Occasional observation of a star at the presumably correct position. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Pretty pale yellow-orange pair of equal magnitude, about 2" separation. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Near equal orange, ~3" |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern war noch gut zu trennen, bei fast identischer Helligkeit. Komponente A wirkt weißlich, während die etwas schwächere Komponente B gelblich orange strahlt. |
|
|
|
★
|
lambda Oph, 10 Oph, STF2055, Marfic |
|
AB |
4m2 |
5m2 |
1.6'' |
45° |
2018 |
Oph |
16h30m54.84s |
+01°59'02.80" |
|
|
Stefan Loibl
Rosenheim (Germany) |
102mm (205x) |
components cannot be split at 205x |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
schöner Farbkontrast, lohnend. |
|
Sarah Gebauer
Germany |
150mm (160x) |
habe den Doppelstern zwar gefunden und konnte auch erkennen, dass es zwei Sterne sind, eine Trennung war aber heute Abend nicht möglich |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
|
★
|
STF2059 |
|
|
8m8 |
8m8 |
0.3'' |
179° |
2016 |
Her |
16h30m55.71s |
+38°03'52.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Overlapping disks, notched. Need perfect seeing. This was 1.2" at Struve's discovery, so easier for him to see -- I doubt he would have found it now, near its closest separation. August 2017 |
|
|
|
★
|
STF2084, zeta Her, 40 Her |
|
|
3m0 |
5m4 |
1.6'' |
115° |
2018 |
Her |
16h41m17.16s |
+31°36'09.80" |
|
|
Sarah Gebauer
Germany |
100mm (136x) |
auf Anhieb ganz haarscharf getrennt, aber leider nur wenige Sekunden haltbar; dennoch erfolgreiche Trennung! |
|
Robert Zebahl
Leipzig (Germany) |
102mm (224x) |
Faint companion as distinct brightening on the first diffraction ring visible. In steadier moments visible as small, round condensation. |
|
Robert Zebahl
Leipzig (Germany) |
102mm (280x) |
After a longer, concentrated observation, a permanent brightening of the first diffraction ring of the primary component could be seen at the correct position angle. The brightening appeared only arch-shaped without any noticeable condensation. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
äußerst schwierig |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
Bei sehr ruhiger Luft ohne Probleme sichtbar, trotz der störenden Restkoma meines Refraktors |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
René Merting
Drachhausen (Germany) |
320mm (320x) |
in der Nacht konnte ich nur bis 320x gewinnbringend vergrößern - Komponente A zeigt schöne Beugungsscheibchen, B offenbarte sich mir nicht |
|
|
|
|
STF2091 |
|
|
8m4 |
9m3 |
0.4'' |
324° |
2010 |
Her |
16h42m09.74s |
+41°11'42.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
I "see" rod shape once I know it is 0.4" separation. Marginal. (This one 1.3" at Struve's discovery, so easy for him! August 2017) |
|
|
|
|
D15 |
|
|
9m0 |
9m3 |
0.6'' |
335° |
2016 |
Her |
16h43m56.29s |
+43°28'31.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Light orange elongated, with notch, near equal. (0.9" at discovery). |
|
|
|
★★
|
52 Her |
A1866 |
BC |
9m5 |
9m6 |
0.3'' |
266° |
2012 |
Her |
16h49m14.20s |
+45°59'00.40" |
|
|
|
BU627 |
A-BC |
4m8 |
8m4 |
2.2'' |
44° |
2018 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
100mm (142x) |
BU627 (A-BC): bis 142x probiert, hat nicht funktioniert - der Helligkeitsunterschied ist vermutlich zu groß und das Beugungsscheibchen von A so hell wie BC selbst |
|
Robert Zebahl
Leipzig (Germany) |
102mm (280x) |
BU627 (A-BC): At 160x the faint component is already beginning to be visible as brightening in the first diffraction ring. At 280x the brightening is quite clearly visible and appears partly clear as a small knot in the first diffraction ring. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
BU627 (A-BC) |
|
Uwe Pilz
Leipzig (Germany) |
120mm (180x) |
BU627 (A-BC) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
BU627 (A-BC): 52 Her. Very bright white star with a companion disk 2", 4-5 delta mag. Wow! B appears as if it is illuminated by A's light. Did not detect BC, 0.3" |
|
|
|
★★
|
STF2107 |
|
AB |
6m9 |
8m5 |
1.5'' |
109° |
2018 |
Her |
16h51m50.10s |
+28°39'58.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Yellow and orange pair, very close ~1.5", 1 delta mag. Very pretty. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Nice pair yellow and slightly blue two delta mag, about 1.5" (AC is 11.5 and much further separated) |
|
Karsten Kopp
Köln (Germany) |
600mm (385x) |
Doppelstern ist bei 180-facher Vergrößerung gerade so als 8 zu erkennen. Bei 385-facher Vergrößerung in den seltenen Augenblicken des ruhigen Seeings gerade so eben zu trennen. Sehr schwierig auch wegen des Helligkeitsunterschied von 1,6 mag. |
|
|
|
|
STF2118, 20 Dra |
|
AB |
7m1 |
7m3 |
0.9'' |
65° |
2018 |
Dra |
16h56m25.32s |
+65°02'20.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
sehr einfach |
|
|
|
★★
|
mu Dra, 21 Dra, Alrakis, Arrakis |
STF2130 |
AB |
5m7 |
5m7 |
2.5'' |
2° |
2018 |
Dra |
17h05m20.20s |
+54°28'14.30" |
|
|
|
BU1088 |
AC |
5m7 |
13m7 |
12.2'' |
174° |
2015 |
|
|
|
|
|
Christopher Hay
Seeheim (Germany) |
80mm (100x) |
In May 2019 neatly split, no colours seen. A physical system with a period of 812 years. Periastron was in 1946, since then the distance is widening to reach 2.7“ in 2025 and 2.8“ in 2030 |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
AB: bei 107x zeigen sich zwei knapp getrennte Perlchen, beide gleichhell und weiß schimmernd - ein schickes Paar |
|
Robert Zebahl
Leipzig (Germany) |
102mm (125x) |
AB: Easy to separate. Beautiful sight. Components equally bright with no discernible color difference. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (460x) |
AB: gleich hell |
|
|
|
|
A1145 |
|
|
6m3 |
7m8 |
0.7'' |
340° |
2018 |
Oph |
17h08m13.65s |
-01°04'46.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Marginal observation of a very faint, very close-in star which briefly resolves as a point and not a flare. |
|
|
|
|
eta Oph, 35 Oph |
BU1118 |
AB |
3m0 |
3m3 |
0.5'' |
229° |
2018 |
Oph |
17h10m22.66s |
-15°43'30.50" |
|
|
|
BU1118 |
AB-C |
2m4 |
12m3 |
99.8'' |
148° |
2012 |
|
|
|
|
|
|
BU1118 |
AD |
2m4 |
11m2 |
101.2'' |
281° |
2012 |
|
|
|
|
|
|
DAL52 |
AE |
2m4 |
11m1 |
62.7'' |
317° |
2012 |
|
|
|
|
|
Stefan Loibl
Rosenheim (Germany) |
102mm (205x) |
B component recognizable in the airy disk, E component not visible |
|
|
|
|
STF2135 |
|
AB |
7m6 |
8m9 |
8.7'' |
195° |
2018 |
Her |
17h12m06.06s |
+21°13'44.40" |
|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 64x ein locker getrenntes Pärchen - Komponente B im Süden halb so hell wie A - zurück auf 32x sind beide Sterne als enges Pärchen erkennbar, nicht zu knapp getrennt - noch weiter zurück auf 20x sehe ich ein längliches Sternchen, Trennung bei dieser Vergrößerung noch nicht möglich |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Pretty yellow star with widely separated 2 delta mag bluish B. (Not physical) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Dull orange and almost green B, wide, 2 delta mag. |
|
|
|
★★
|
STF2140, alpha Her, 64 Her, Ras Algethi |
|
AB |
3m5 |
5m4 |
4.8'' |
105° |
2018 |
Her |
17h14m38.86s |
+14°23'24.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (41x) |
Well split with noticeable difference in brightness. |
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 32x ist noch nichts erkennbar - bei 64x wird östlich von Rasalgethi der schwache Begleiter B knapp getrennt sichtbar - A ist strahlend gelb, B mit einer Tendenz zum gelb, eher ein warmes weiß |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
himmelblau und hellgelb, getrennt bei 53x |
|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
gelb-lachsfarben |
|
Robert Zebahl
Leipzig (Germany) |
120mm (100x) |
Easily split with noticeable difference in brightness. A: intensively orange colored, B: slightly orange. |
|
Karsten Kopp
Köln (Germany) |
140mm (94x) |
Konnte erst mit 94-facher Vergrößerung gut getrennt wahrgenommen werden. |
|
Sarah Gebauer
Germany |
150mm (85x) |
bei Halbmond auf der Schwäbischen Alb: sehr eng, aber sauber getrennt, eine Komponente ist viel heller und größer, mein Farbeindruck ist allerdings unerwartet eher gelb |
|
Sarah Gebauer
Germany |
150mm (160x) |
richtig gold, es strahlt mich richtiggehend an, auch sehr schön getrennt, ein toller Doppelstern! |
|
Mark McCarthy
Fremont (California/USA) |
203mm (667x) |
Rasalgethi. 8" inch mask due to seeing. AB orange and blue 4 delta mag. Faint AD seen very wide separation. pretty star. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
gelblich und bläulicher Stern |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Rasalgethi, Bright orange A & pale green much fainter B. Very nice! |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Bright orange and blue-green-grey B. |
|
Karsten Kopp
Köln (Germany) |
600mm (135x) |
Leicht zu trennen. Komponente A erscheint orange, Komponente B gelblich. |
|
Karsten Kopp
Köln (Germany) |
600mm (180x) |
Doppelstern ist gut zu trennen. Komponente A erstrahlt orange und Komponente B gelblich. |
|
|
Jens Leich
Germany |
130mm |
|
|
|
|
|
SHJ243, 36 Oph |
|
AB |
5m1 |
5m1 |
5.1'' |
140° |
2017 |
Oph |
17h15m20.78s |
-26°36'06.10" |
|
|
|
|
AC |
5m1 |
6m5 |
731.6'' |
74° |
2000 |
|
|
|
|
|
|
|
AD |
5m1 |
7m8 |
276.9'' |
338° |
2000 |
|
|
|
|
|
|
|
AE |
5m1 |
12m3 |
38.2'' |
313° |
2000 |
|
|
|
|
|
Stefan Loibl
Rosenheim (Germany) |
102mm (68x) |
Komponente AB separated at 68x magnification, componente C at greater distance of 12.2 arcmin |
|
|
|
★★★
|
BU628 |
|
|
9m5 |
9m6 |
0.6'' |
262° |
2016 |
Her |
17h18m22.22s |
+32°39'38.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Wow split clean, amazing. No resolution at 667x but at 1067x two airy disks, sep by half disk, half delta mag. Remarkable |
|
|
|
|
DON832, xi Oph |
|
AB |
4m4 |
8m9 |
4.1'' |
27° |
2015 |
Oph |
17h21m00.37s |
-21°06'46.50" |
|
|
Stefan Loibl
Rosenheim (Germany) |
102mm (205x) |
fainter 9 mag component not visible |
|
|
|
★★
|
STF2241, psi 1 Dra, 31 Dra |
|
AB |
4m6 |
5m6 |
30.1'' |
17° |
2018 |
Dra |
17h41m56.36s |
+72°08'55.80" |
Christopher Hay
Seeheim (Germany) |
15x45 |
Stabilised binoculars, handheld. Easily split. A appears pearl white, B brick red. A very fine pair for 15x. Resolved in stabilised 10x42 but not so pleasantly. Psi1 Dra is a physical double with a period of roughly 10,000 years. |
|
René Merting
Drachhausen (Germany) |
16x70 |
ein auffälliges Pärchen in einem wilden Sterngewimmel vieler heller Sterne, beide Komponenten sind knapp getrennt zu erkennen - Komponente B ist mindestens eine Größenklasse schwächer und strahlt nicht so schön reinweiß wie A |
|
Christopher Hay
Seeheim (Germany) |
80mm (30x) |
Widely split. A light yellow, B light blue. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (55x) |
weiß-orange |
|
|
|
|
HU1285 |
|
|
8m9 |
9m2 |
0.5'' |
211° |
2016 |
Her |
17h43m38.76s |
+22°36'43.20" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
unsicher, sehr schwierig |
|
|
|
|
STF2205 |
|
|
9m4 |
9m6 |
0.9'' |
11° |
2016 |
Her |
17h45m41.03s |
+17°43'00.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Half delta mag light orange star about 1" separated (in this scope it is quite wide) |
|
|
|
★★★
|
HU1288 |
|
|
8m3 |
9m4 |
0.4'' |
163° |
2016 |
Her |
17h47m09.16s |
+15°02'13.80" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Awesome! clean split, very clean star images. Split by half disk, half delta mag. very cool great catch! suspected at 667x, ramped up power to 1067x to split. |
|
|
|
★
|
STT338 |
|
AB |
7m2 |
7m4 |
0.9'' |
168° |
2018 |
Her |
17h51m58.46s |
+15°19'34.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Just split, a pair of bright near equal orange stars. |
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Yellow-white very clean split stars seem more equal than what the data says |
|
|
|
★★
|
STF2308 |
40/41 Dra |
AB |
5m7 |
6m0 |
18.7'' |
232° |
2018 |
Dra |
18h00m09.07s |
+80°00'13.70" |
|
|
|
|
AC |
5m7 |
8m3 |
224.7'' |
129° |
2015 |
|
|
|
|
|
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. |
|
|
|
|
STF2267 |
|
|
8m4 |
8m8 |
0.4'' |
281° |
2018 |
Her |
18h01m41.17s |
+40°10'41.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
|
|
STF2262, tau Oph |
|
AB |
5m3 |
5m9 |
1.5'' |
289° |
2018 |
Oph |
18h03m04.91s |
-08°10'48.90" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (240x) |
getrennt |
|
|
|
|
70 Oph, P Oph, STF2272 |
|
AB |
4m2 |
6m2 |
6.8'' |
121° |
2018 |
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 |
|
|
|
★
|
STT341 |
|
AB |
7m4 |
8m8 |
0.0'' |
79° |
2018 |
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 |
|
|
|
★
|
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) |
Extremely faint B, just on diffraction ring, with seeing, both 553x & 885x. ~1" |
|
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" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
99 Her. Faint point seen in the diffraction of brighter star disk. |
|
|
|
|
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 |
|
|
|
|
STF2281, 73 Oph |
|
AB |
6m0 |
7m5 |
0.8'' |
283° |
2018 |
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'' |
219° |
2018 |
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 |
|
|
|
|
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 |
|
|
|
★
|
STF2323, 39 Dra |
|
AC |
5m1 |
8m0 |
89.1'' |
19° |
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. |
|
|
|
★
|
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) |
317mm (553x) |
Near contact / overlapping disks, 0.5 delta mag. September 2017 |
|
|
|
|
HU66 |
|
BC |
8m4 |
8m2 |
0.8'' |
27° |
2018 |
Dra |
18h25m18.20s |
+48°45'42.50" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very fine near equal pair, yellowish A and blue-white B. ~1" or less. |
|
|
|
★★
|
STT359 |
|
|
6m3 |
6m6 |
0.9'' |
7° |
2018 |
Her |
18h35m30.40s |
+23°36'19.90" |
|
|
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 |
|
|
|
★★
|
STT358 |
|
AB |
6m9 |
7m1 |
1.7'' |
149° |
2018 |
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. |
|
|
|
|
STT363 |
|
|
7m5 |
8m1 |
0.6'' |
336° |
2018 |
Dra |
18h37m23.92s |
+77°41'12.40" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
als 8 zu sehen |
|
|
|
|
STF2367 |
|
AB |
7m7 |
8m0 |
0.4'' |
75° |
2018 |
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 |
|
|
|
★★★
|
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'' |
346° |
2018 |
|
|
|
|
|
|
STF2383, 5 Lyr, epsilon 2 Lyr |
CD |
5m2 |
5m4 |
2.4'' |
75° |
2018 |
|
|
|
|
|
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 |
|
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 |
|
|
|
|
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 |
|
|
|
★
|
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") |
|
|
|
|
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. |
|
|
|
|
BU648 |
|
AB |
5m3 |
8m0 |
1.3'' |
243° |
2015 |
Lyr |
18h57m01.61s |
+32°54'04.60" |
|
|
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 (277x) |
In diffraction but steady disk of B within it, 2" 3 delta mag. |
|
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. |
|
|
|
|
STF2438 |
|
|
7m0 |
7m4 |
0.9'' |
358° |
2018 |
Dra |
18h57m28.47s |
+58°13'30.00" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
leicht; beide gleich hell |
|
|
|
★
|
STF2437 |
|
|
8m4 |
8m8 |
0.5'' |
8° |
2017 |
Sge |
19h01m53.16s |
+19°10'11.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Small faint, notched peanut when seeing stills. Orange. |
|
|
|
|
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 |
|
|
|
|
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") |
|
|
|
|
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 |
|
|
|
★
|
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. |
|
|
|
★
|
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. |
|
|
|
|
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. |
|
|
|
|
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. |
|
|
|
|
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. |
|
|
|
★★
|
STFA46, 16 Cyg |
|
AB |
6m0 |
6m2 |
39.9'' |
134° |
2018 |
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. |
|
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 |
|
|
|
|
STT383 |
|
AB |
7m0 |
8m3 |
0.8'' |
15° |
2014 |
Cyg |
19h42m56.26s |
+40°43'18.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
|
★
|
STF2579, delta Cyg, 18 Cyg |
|
AB |
2m9 |
6m3 |
2.8'' |
218° |
2016 |
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! |
|
|
|
|
STF2580, 17 Cyg |
|
AB |
5m1 |
9m2 |
26.1'' |
68° |
2015 |
Cyg |
19h46m25.60s |
+33°43'39.30" |
|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 20x locker getrennt - Komponente A satt gelb, B wegen des großen Helligkeitsunterschiedes gräulich-bräunlich |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
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?) |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
17 Cyg: Yellow and blue, wide separation. 11 stars in the system, it should just be called an open cluster |
|
|
|
★
|
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. |
|
|
|
|
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 |
|
|
|
|
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. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Definite clear split, 2 airy disk widths. |
|
|
|
★★
|
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. |
|
|
|
|
STF2613 |
|
AB |
7m5 |
8m0 |
3.5'' |
354° |
2018 |
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) |
203mm (533x) |
Easy pair, wide, 1 delta mag light orange color, 4". |
|
|
|
|
STT395, 16 Vul |
|
|
5m8 |
6m2 |
0.7'' |
129° |
2018 |
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 |
|
|
|
|
STF2658 |
|
AB |
7m2 |
9m4 |
5.4'' |
106° |
2015 |
Cyg |
20h13m40.70s |
+53°07'00.00" |
|
|
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 |
|
|
|
★
|
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] |
|
|
|
|
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 |
|
|
|
|
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 |
|
|
|
|
STF2723 |
|
AB |
7m0 |
8m3 |
1.0'' |
140° |
2018 |
Del |
20h44m54.58s |
+12°18'45.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
bright, very close near equal magnitude peanut shape |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
very bright A and a very faint C widely separated. |
|
|
|
★★
|
STF2725 |
|
AB |
7m5 |
8m2 |
6.1'' |
12° |
2018 |
Del |
20h46m13.31s |
+15°54'26.40" |
|
|
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) |
317mm (277x) |
Near equal yellow-white stars, wide separation. |
|
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) |
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. |
|
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 STF2525 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) |
317mm (277x) |
Gamma Delphinus. Rich gold-yellow A, blue-white B, ~6" separation estimated by eye. Very pretty pair. |
|
|
|
★
|
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. |
|
|
|
|
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 |
|
|
|
|
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. |
|
|
|
★
|
STF2737, epsilon Equ, 1 Equ |
|
AB |
6m0 |
6m3 |
0.2'' |
281° |
2018 |
Equ |
20h59m04.54s |
+04°17'37.80" |
|
|
|
|
AD |
6m0 |
13m1 |
69.3'' |
293° |
2013 |
|
|
|
|
|
|
|
AB-C |
5m3 |
7m0 |
10.6'' |
67° |
2018 |
|
|
|
|
|
René Merting
Drachhausen (Germany) |
12x50 |
AB-C: in ruhigen Momenten präsentieren sich beide Sterne präsentieren sich 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 |
|
|
|
|
59 Cyg, STF2743 |
MCA65 |
Aa-Ab |
4m8 |
7m6 |
0.2'' |
2° |
2008 |
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 |
|
|
|
★
|
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. |
|
|
|
|
STF2744 |
|
AB |
6m8 |
7m3 |
1.2'' |
110° |
2018 |
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 |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Close, equal magnitude, bright yellow-white. |
|
|
|
★★
|
STF2758, 61 Cyg |
|
AB |
5m2 |
6m0 |
31.6'' |
154° |
2018 |
Cyg |
21h06m53.95s |
+38°44'57.90" |
|
|
Christopher Hay
Seeheim (Germany) |
15x45 |
Clear to wide separation. Both components of orange hue. Brighter northern component seemed to go slightly into yellow. In 10x42 also clearly split, northern component of orange hue, southern component of indeterminate colour (sky not quite dark enough at the time to see 61 Cyg naked-eye). Piazzi’s Flying Star, flying more than 5” per year to the northeast, and a true physical double with a period of 678 years. |
|
Sarah Gebauer
Germany |
50mm (7x) |
Zufallsfund im Fernglas aufgrund des deutlichen Farbunterschiedes (orange und blau) |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x sind beide Sterne gut getrennt, Komponente A strahlt in einem schmutzig dunklem gelb, schwächere Komponente B leicht orange |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
gelb und orange. Der weitere Stern im Bild ist TYC 3168-6781 |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
TYC 3168-5901 kann dazu dienen, den sich ändernden Positionswinkel abzuschätzen. |
|
Jörg S. Schlimmer
Germany |
127mm (203x) |
Intensive Farbe |
|
Sarah Gebauer
Germany |
150mm (125x) |
auch hoch vergrößert noch die zwei Farben orange und blau zu sehen, aber schwächer als im Fernglas |
|
Robert Zebahl
Leipzig (Germany) |
152mm (22x) |
2020-06-24: Beautifully separated, bright, striking, especially the colors: bright orange and orange. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (121x) |
61 Cyg. Nice near equal wide orange pair, bright [18 stars in system -- if so should be an OC] |
|
|
Berthold Fuchs
Wiesbaden (Germany) |
130mm |
easy DS |
|
|
|
|
H1 48 |
|
|
7m2 |
7m3 |
0.7'' |
244° |
2018 |
Cep |
21h13m42.46s |
+64°24'15.10" |
|
|
Robert Zebahl
Leipzig (Germany) |
152mm (270x) |
Clearly elongated, of equal brightness with partly visible, slight notching. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
getrennt |
|
|
|
|
STF2783 |
|
|
7m7 |
8m1 |
0.7'' |
352° |
2017 |
Cep |
21h14m04.90s |
+58°17'49.80" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht leicht trennbar wegen Luftunruhe |
|
|
|
|
AGC13, tau Cyg |
|
AB |
3m8 |
6m6 |
1.1'' |
190° |
2017 |
Cyg |
21h14m47.49s |
+38°02'43.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Tau Cygni: Near equal orange with fainter nearby, could be triple. (There are 13 stars in the system. They ought to just call it an open cluster) |
|
|
|
|
STF2807 |
|
|
8m7 |
8m8 |
1.9'' |
309° |
2016 |
Cep |
21h17m33.47s |
+82°31'03.70" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (128x) |
Barely split without any noticeable difference in brightness. |
|
|
|
|
BU163 |
|
AB |
7m3 |
8m9 |
0.9'' |
257° |
2018 |
Equ |
21h18m34.85s |
+11°34'08.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Can resolve in 20" and once know where B is, can split with 8", but B is much fainter and is more a brightening in the first diffraction than at star [Several other fainter pairs] |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Very close but clean split momentarily with seeing, both yellow-orange, 3 delta mag, <1" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Close but definite split when seeing stills |
|
|
|
★★
|
STF2789 |
|
AB |
7m7 |
7m9 |
6.8'' |
115° |
2018 |
Cyg |
21h19m58.84s |
+52°58'44.10" |
Robert Zebahl
Leipzig (Germany) |
70mm (44x) |
At 22x almost separated. The double star appeared strikingly orange and forms a conspicuous, nearly isosceles triangle with neighbouring stars. At 44x clearly separated, relatively close together with a small difference in brightness. |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
bei 32x zwei gleichhelle ganz dicht beieinander stehende weiße Lichtpünktchen, ganz knapp getrennt - wunderschön mit dieser Teleskopöffnung |
|
|
|
|
STT437 |
|
AB |
7m2 |
7m4 |
2.4'' |
19° |
2018 |
Cyg |
21h20m50.12s |
+32°27'10.20" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
At 57x separated, but close together. Near, slightly brighter star in nice contrast. The double star shows a distinct orange coloration. At 100x small difference in brightness visible. |
|
René Merting
Drachhausen (Germany) |
100mm (107x) |
bei 64x eine schöne 8, die beiden etwa gleich hellen Sterne berühren sich noch ganz leicht und scheinen fast getrennt zu sein - bei 107x ist die Trennung dann knapp aber deutlich |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
orange und orangegelb, schön auch bei 88x |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
einfach |
|
|
|
|
STT435 |
|
|
8m3 |
8m2 |
0.7'' |
239° |
2018 |
Equ |
21h21m23.70s |
+02°53'14.60" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
|
★
|
STFB11, 1 Peg |
|
AB |
4m2 |
9m3 |
36.3'' |
312° |
2019 |
Peg |
21h22m05.13s |
+19°48'15.70" |
|
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
der helle Stern ist weiß. |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
1 Peg: Easy yellow-orange & wide separated B |
|
|
|
|
STF2799 |
|
AB |
7m4 |
7m4 |
1.8'' |
259° |
2018 |
Peg |
21h28m52.79s |
+11°05'05.20" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
At 100x, barely, at 128x clearly split with equally bright components. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (200x) |
beide Komponenten gelb |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Very nice pair, only slightly unequal, ~3" |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Equal yellow-orange |
|
|
|
★★
|
B1008 |
|
AB |
8m9 |
8m1 |
0.1'' |
226° |
2018 |
PsA |
21h30m57.70s |
-36°32'49.70" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Propus (means "forefoot") = Eta Geminorum: So cool! Bright orange star with B very close, ~1.5", just preceding, ~3 delta mag. B is in diffraction but is well separated & has its own airy disk, bluish white. |
|
|
|
★
|
STF2804 |
|
AB |
7m7 |
8m0 |
3.7'' |
1° |
2018 |
Peg |
21h32m58.30s |
+20°42'44.50" |
|
|
Robert Zebahl
Leipzig (Germany) |
70mm (57x) |
Clearly split, pretty close, moderately uneven. The primary components looked slightly orange. Very nice pair. |
|
Uwe Pilz
Leipzig (Germany) |
105mm (88x) |
der südliche Stern ist einen Hauch heller. Gelb und orange. |
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
Nice light orange and light blue, sharp, 1 delta mag 3". pretty. |
|
|
|
|
BU688 |
|
AB |
8m1 |
8m6 |
0.5'' |
198° |
2016 |
Cyg |
21h42m33.41s |
+41°02'51.00" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
länglich, unsicher |
|
|
|
★
|
mu Cyg, 78 Cyg, STF2822 |
|
AB |
4m8 |
6m2 |
1.6'' |
321° |
2018 |
Cyg |
21h44m08.57s |
+28°44'33.40" |
|
|
|
|
AD |
4m8 |
6m9 |
196.9'' |
44° |
2014 |
|
|
|
|
|
Uwe Pilz
Leipzig (Germany) |
60mm (198x) |
AB: Aufhellung innerhalb des ersten Rings |
|
Robert Zebahl
Leipzig (Germany) |
70mm (128x) |
AB: At 128x I was able to see this double at least elongated. |
|
Sarah Gebauer
Germany |
150mm (160x) |
AD: bei der Sichtung noch eher unsicher, welche der hellen Sterne die Komponenten AB enthalten, denn diese habe ich nicht getrennt, AD mit einem Abstand von 196'' stehen mit drei weiteren Feldsternen in einer mehr oder minder interessanten Konstellation |
|
Robert Zebahl
Leipzig (Germany) |
200mm (171x) |
AB: Quite well split with noticeable fainter component. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
AB: getrennt |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Yellow and light orange pair, ~1", 1 delta mag. Very pretty, subtle colors |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
AB: Yellow, 1 delta mag, 2-3” |
|
|
|
|
BU75 |
|
AB |
8m4 |
8m6 |
1.1'' |
26° |
2018 |
Peg |
21h55m31.42s |
+10°52'49.50" |
|
|
|
|
AB-C |
7m7 |
12m5 |
35.3'' |
211° |
2012 |
|
|
|
|
|
Mark McCarthy
Fremont (California/USA) |
203mm (533x) |
AB: With patience for poor conditions and some critical focus I get a good clean split, slightly unequal |
|
Mark McCarthy
Fremont (California/USA) |
508mm (333x) |
AB-C: Yellow white and faint blue, well split. Did not see AB 1.1" |
|
|
|
|
STF2873 |
|
AB |
7m0 |
7m5 |
13.8'' |
66° |
2017 |
Cep |
21h58m13.53s |
+82°52'10.80" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (25x) |
Easy to split with visible difference in brightness. Stands out immediately. |
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
bei 32x ein gut getrenntes Pärchen, B ist eine halbe Magnitude schwächer und strahlt ein wenig kühler als A - eine richtig schöne Vergrößerung ist 20x, dann stehen beide Sterne sehr dicht und zeigen schön ihren leichten Farbkontrast |
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|
STF2863, xi Cep, 17 Cep |
|
AB |
4m5 |
6m4 |
8.2'' |
274° |
2019 |
Cep |
22h03m47.45s |
+64°37'40.70" |
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|
Robert Zebahl
Leipzig (Germany) |
55mm (27x) |
At 27x well separable, but quite close together with a clear difference in brightness. At 71x very nice view. |
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|
|
|
STF2872 |
|
A-BC |
7m1 |
8m0 |
21.7'' |
316° |
2018 |
Cep |
22h08m36.04s |
+59°17'22.20" |
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|
|
AD |
7m1 |
11m8 |
117.3'' |
153° |
2014 |
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|
BC |
8m0 |
8m0 |
0.8'' |
297° |
2018 |
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|
|
René Merting
Drachhausen (Germany) |
100mm (20x) |
A-BC: bei 32x einfach zu trennen, die B-Komponente im NW ist nur knapp schwächer - dezenter Farbunterschied, A leuchtet weiß-bläulich und BC weiß-gelblich - zurück auf 20x zeigt sich der Doppelstern weiter gut getrennt |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
BC: BC in ruhigen Momenten trennbar |
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|
|
★
|
COU136 |
|
|
9m2 |
7m6 |
0.4'' |
19° |
2015 |
Peg |
22h10m02.22s |
+23°07'33.00" |
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|
Mark McCarthy
Fremont (California/USA) |
508mm (1067x) |
Awesome hairline at 533x, nice clean split at 1067x. The stars are split the diffraction patters merge at the boarders, perfect images. Appears more near equal than SkyTools data suggests |
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|
|
STF2881 |
|
|
7m7 |
8m2 |
1.3'' |
76° |
2017 |
Peg |
22h14m34.67s |
+29°34'20.60" |
|
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Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Light orange stars, ~1 delta mag, 2-3" |
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|
|
SHJ345, 53 Aqr |
|
AB |
6m3 |
6m4 |
1.4'' |
86° |
2018 |
Aqr |
22h26m34.30s |
-16°44'31.90" |
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|
Frederik Wanink
Itterbeck (Germany) |
254mm (240x) |
länglich, horizontnah |
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|
|
|
KR60, DO Cep, Kruger 60 |
|
AB |
9m9 |
11m4 |
1.5'' |
266° |
2016 |
Cep |
22h27m59.20s |
+57°41'43.80" |
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|
Uwe Pilz
Leipzig (Germany) |
105mm (288x) |
Unsicher – nur des Positionswinkel wurde zwar blickweise erkannt, aber die Komponenten verwechselt. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (150x) |
Observed at magnifications between 129x and 300x. The seeing and transparency (Bortle 6-) were only average. The rather faint B component seemed to appear in few moments. |
|
Robert Zebahl
Leipzig (Germany) |
152mm (150x) |
The seeing was more average (3/5). Observation under suburban conditions (Bortle 6, SQM-L 19.1). Initially observed at 270x, later at 300x. The extremely faint companion was always visible at the same position if the air was steady enough. Difficult because of the low magnitude! |
|
Uwe Pilz
Leipzig (Germany) |
320mm (387x) |
äußerst schwierig, nur blickweise sichtbar |
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|
|
BU701 |
|
AB |
7m3 |
9m6 |
1.1'' |
179° |
2017 |
Peg |
22h28m07.24s |
+12°14'55.50" |
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|
|
AC |
7m3 |
12m0 |
126.7'' |
133° |
2015 |
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|
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Mark McCarthy
Fremont (California/USA) |
317mm (513x) |
AB: Orange star with a slightly mis-shaped disk |
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Mark McCarthy
Fremont (California/USA) |
317mm (513x) |
AC: very wide separated bluish star 2-3 delta mag. |
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★★
|
STF2909, zet 2 Aqr |
|
AB |
4m3 |
4m5 |
2.5'' |
161° |
2018 |
Aqr |
22h28m49.81s |
-00°01'12.20" |
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|
Christopher Hay
Seeheim (Germany) |
180mm (120x) |
Neatly split, whereby the first difraction rings of each component touch the Airy discs of the other. Component A in the north seems marginally more yellowish than component B in the south.
Zeta Aqr is called Sadaltager, meaning „Merchant’s Luck“. It is framed nicely by Pi, Gamma and Eta Aquarii, with which it forms a striking triangular asterism known as „The Tent“. Moreover, Zeta Aqr is a true physical double. This constellation and the beautiful telescopic appearance warrant a two-star rating. |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (240x) |
einfach |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Very bright white, equal magnitude, fairly close ~2". |
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|
|
★
|
8 Lac |
CHR112 |
Aa-Ab |
5m7 |
|
0.0'' |
131° |
2018 |
Lac |
22h35m52.28s |
+39°38'03.60" |
|
|
|
STF2922 |
AB |
5m7 |
6m3 |
22.3'' |
186° |
2018 |
|
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|
|
A1469 |
AC |
5m7 |
10m4 |
48.8'' |
168° |
2016 |
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|
A1469 |
CD |
10m4 |
9m1 |
42.4'' |
116° |
2016 |
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|
A1469 |
AD |
5m7 |
9m1 |
81.6'' |
145° |
2017 |
|
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|
A1469 |
AE |
5m7 |
7m2 |
335.2'' |
239° |
2016 |
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|
|
DAL28 |
AG |
5m7 |
14m1 |
77.6'' |
193° |
2015 |
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|
COM8 |
BF |
6m3 |
11m0 |
127.6'' |
175° |
2012 |
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|
|
A1469 |
DI |
9m1 |
13m3 |
10.0'' |
227° |
2015 |
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|
DAL28 |
GJ |
14m1 |
13m0 |
6.5'' |
78° |
2016 |
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|
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
A1469 (CD): das Paar gehört zum interessanten Mehrfachsystem STF2922 - während bei 32x Komponente C nur knapp sichtbar ist, zeigt sich D wieder deutlicher - Abstand CD ist doppelt so groß wie BC (STF2922) |
|
René Merting
Drachhausen (Germany) |
100mm (32x) |
STF2922 (AB): AB: bei 32x sind beide Komponenten gut getrennt sichtbar - B im Süden ist eine halbe Größenklasse schwächer
BC: bei 32x schimmert südöstlich von der Komponente B ein ganz schwacher Lichtpunkt, die Komponente C, durch - Komponenten BC mit gleichem Abstand wie AB
nachrichtlich zu D: interessant ist das Mehrfachsystem allemal, denn in doppelter Entfernung weiter südöstlich steht eine vierte Komponente D (eigene Bezeichnung: A1469, D mit Helligkeit 9.08 mag), so dass 4 Sterne problemlos mit dieser Öffnung zu erfassen sind |
|
|
|
★
|
BU1092 |
|
AB |
8m3 |
8m3 |
0.4'' |
223° |
2016 |
Cep |
22h36m08.65s |
+72°52'51.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Notched! Near equal. With seeing. |
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|
|
|
STF2934 |
|
|
8m6 |
9m6 |
1.4'' |
57° |
2016 |
Peg |
22h41m51.68s |
+21°25'53.00" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwieriger wegen schwacher Sterne |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
1.5 delta mag, well split, ~1.5", bluish white stars |
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|
|
|
STF2944 |
|
AB |
7m3 |
7m7 |
1.8'' |
307° |
2018 |
Aqr |
22h47m50.05s |
-04°13'43.60" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Pretty close equal white pair, ~2.0", split. |
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|
|
★
|
HU985 |
|
|
9m6 |
9m9 |
0.7'' |
134° |
2016 |
Peg |
22h47m54.00s |
+12°58'36.20" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Wow I got it! Light orange star and a very faint star just outside first diffraction, very subtle and tough |
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|
|
|
STF2950 |
|
AB |
6m0 |
7m1 |
1.1'' |
274° |
2018 |
Cep |
22h51m22.51s |
+61°41'47.90" |
|
|
Sarah Gebauer
Germany |
100mm (136x) |
bei 136x ist neben der Hauptkomponente etwas ganz Schwaches zu sehen, aber eher unsicher und nicht sauber getrennt, höhere Vergrößerung ist an diesem Abend nicht möglich |
|
Mark McCarthy
Fremont (California/USA) |
203mm (333x) |
Nice pair indeed. Bright yellow-white A and 2 delta mag B, clean split, ~2". May be third fainter much wider split (AC, 39.2" 11.05) |
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|
|
|
HO482 |
|
AB |
7m3 |
8m3 |
0.6'' |
13° |
2017 |
Peg |
22h51m26.66s |
+26°23'27.90" |
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|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
A star does not seem round, but seeing is poor. Marginal. |
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|
|
|
BU382 |
|
AB |
6m0 |
7m8 |
0.7'' |
244° |
2016 |
Lac |
22h53m40.16s |
+44°44'57.10" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
schwierig, Helligkeitsunterschied stark |
|
|
|
|
HU987 |
|
|
9m2 |
9m7 |
1.2'' |
75° |
2016 |
Peg |
22h55m43.52s |
+15°46'45.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Well separated one delta mag pair, nice |
|
|
|
★
|
BU180 |
|
AB |
8m0 |
9m2 |
0.5'' |
134° |
2016 |
Cep |
23h07m09.99s |
+60°49'57.10" |
|
|
Mark McCarthy
Fremont (California/USA) |
508mm (667x) |
Exceedingly fine split at best moments, hairline, 1 delta mag. |
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|
|
|
STT489, pi Cep |
|
AB |
4m6 |
6m8 |
1.1'' |
4° |
2016 |
Cep |
23h07m53.84s |
+75°23'15.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
nicht als DS gesehen |
|
|
|
|
BU385 |
|
AB |
7m4 |
8m2 |
0.7'' |
84° |
2018 |
Peg |
23h10m17.15s |
+32°29'13.40" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
in ruhigen Momenten getrennt |
|
|
|
|
STF3007 |
|
AB |
6m7 |
9m8 |
5.5'' |
92° |
2017 |
Peg |
23h22m48.67s |
+20°33'32.20" |
|
|
René Merting
Drachhausen (Germany) |
100mm (64x) |
bei 64x ist Komponente B ganz schwach östlich von A knapp getrennt zu erkennen - ein riesiger Helligkeitsunterschied von 3.5 Größenklassen |
|
Mark McCarthy
Fremont (California/USA) |
508mm (533x) |
Yellow-white A and a bit orange B, ~6" and three delta mag, nice pair [Ba,Bb is TOK 704, 8.4 and 0.8", should have been noticeable! try again!] |
|
|
|
★
|
72 Peg, BU720 |
|
|
5m7 |
6m1 |
0.6'' |
107° |
2018 |
Peg |
23h33m57.19s |
+31°19'31.00" |
|
|
Uwe Pilz
Leipzig (Germany) |
120mm (250x) |
gelb und orange |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
als 8 zu sehen |
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
72 Peg. Small, hard, faint point very tight to A, but split. Stays with seeing. |
|
|
|
|
STT500 |
|
AB |
6m1 |
7m4 |
0.5'' |
21° |
2018 |
And |
23h37m32.03s |
+44°25'44.50" |
|
|
Mark McCarthy
Fremont (California/USA) |
317mm (553x) |
Disk seems not round, but unsure |
|
|
|
|
STT507 |
|
AB |
6m8 |
7m8 |
0.7'' |
323° |
2018 |
Cas |
23h48m39.03s |
+64°52'35.30" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
eindeutig zu trennen, 3er System |
|
|
|
|
STT510 |
|
AB |
7m9 |
8m4 |
0.6'' |
120° |
2018 |
And |
23h51m33.03s |
+42°04'57.70" |
|
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
3er System, gerade getrennt zu sehen |
|
|
|
★
|
STF3050 |
|
AB |
6m5 |
6m7 |
2.5'' |
342° |
2018 |
And |
23h59m29.33s |
+33°43'26.90" |
|
|
Robert Zebahl
Leipzig (Germany) |
55mm (83x) |
At 83x seen as '8'. From 100x to 166x seen as '8', temporarily visible with space between. |
|
Robert Zebahl
Leipzig (Germany) |
70mm (100x) |
Wonderful double star. Easy to split with slight difference in brightness. |
|
René Merting
Drachhausen (Germany) |
76mm (95x) |
bei 57x deutet sich an, dass es sich um einen Doppelstern handeln könnte - bei 95x zeigt sich dann ein extrem knapp getrenntes Pärchen - beide Sterne sind gleich hell |
|
Sarah Gebauer
Germany |
100mm (136x) |
ui, schön! Ein sehr enges Pärchen, bei 136x ganz knapp getrennt, zwei winzig kleine, gleich helle Äuglein nebeneinander |
|
Frederik Wanink
Itterbeck (Germany) |
254mm (640x) |
einfaches Paar, gleich hell |
|
Mark McCarthy
Fremont (California/USA) |
317mm (277x) |
Nice near equal yellow-white, ~3" |
|
|
