Eagle Creek Observatory
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Double Stars in Lyra
The Lyre
Here is a listing of the 62 or so best doubles in Lyra.
The star name contains a link so you may click there to see more detailed information about this double star.
Some entries may return multiple stars, click on the one of interest and the information will be displayed.
If more than one entry is listed click on each of them to view the data. Use the Aladin Previewer to see a photograph of the star.
Click HERE for an ETX tour.

Name SAO Sep PA Mag1 Mag2 RA Dec Spect Color Comments
STF 2441   5.5 275 7.5 9.5 18:02.7 +31:20 A3    
BU 134 47479 1.1 134 8.0 10.0 18:25.3 +46:52 A0    
STF 2328 86117 3.6 73 8.0 8.5 18:29.4 +29:55 A2    
STF 2333   6.4 334 7.5 8.0 18:31.1 +32:15 A0    
STF 2351   5.1 340 7.5 7.5 18:36.2 +41:16 A0    
STF 2349   7.3 203 5.5 11.0 18:36.6 +33:28 A0    
VEGA 67174 62.8 173 0.0 10.0 18:36.9 +38:46 A0   optical double
STF 2352   15.8 284 7.5 10.0 18:37.0 +34:51 K0    
STF 2356 86271 1.0 61 8.0 9.0 18:38.4 +28:41 F0    
STF 2362 67198 4.2 184 7.0 8.5 18:38.5 +36:03 A5    
STF 2358 67199 2.5 220 8.5 9.0 18:38.6 +30:43 F8    
STF 2372 67266 25.1 83 6.5 8.0 18:42.1 +34:44 B5   Primary is a spectroscopic double
STF 2371 86337 9.7 56 8.5 8.5 18:42.2 +27:38 A0    
STF 2380 47728 25.6 9 6.5 8.0 18:42.9 +44:55 G0    
STF 2376   22.3 64 7.5 8.5 18:43.7 +30:24 A0    
EPSILON 01 LYRA 67310 1.5 93 5.0 6.0 18:44.3 +39:40 A4   B IS SAO 67309 Famous "Double Double"
EPSILON 02 LYRA 67315 1.9 354 5.5 4.5 18:44:3 +39:37 F1   Famous "Double Double"
ZETA 01/02 LYRA 67321 43.7 150 4.5 5.5 18:44.7 +37:36 A1   A is a spectroscopic Binary b is sao 67324
STF 2393   14.8 24 7.5 10.0 18:45.2 +38:19 K0 *** Optical Double, color contrast
STF 2392   3.2 55 8.0 10.0 18:45.2 +39:13 A2   Third component sep 23.4 pa 175 mag 9.5
STF 2394   7.2 201 8.5 9.0 18:45.5 +42:02 A3    
STF 2390   4.2 158 7.5 8.5 18:45.8 +34:31 A5    
STF 2397 67378 3.8 267 7.0 9.5 18:47.2 +31:24 G5    
HU 936 67413 1.8 104 9.0 9.0 18:48.7 +34:01 F8    
8 LYRA 67441 34.8 73 6.0 11.5 18:49.8 +32:48 B2    
STF 2406   4.8 2 7.0 11.0 18:49.9 +26:25 A2    
HJ 1352   11.9 243 7.0 11.0 18:50.0 +29:48 B8   b is 67452
BETA LYRA 67451 46.6 149 3.5 7.0 18:50.0 +29:48 B8    
BU 137 67544 1.4 150 8.0 8.5 18:53.9 +37:22 G0    
STT 525 67566 1.7 128 6.0 10.0 18:54.8 +33:57 G5    
STF 2419 86588 3.3 174 8.5 9.0 18:55.5 +29:13 A2    
STF 3130 47928 2.7 262 7.5 11.0 18:55.9 +44:13 A2   primary is a spectroscopic binary
STF 2422 86619 0.7 82 7.5 7.5 18:57.1 +26:06 A0    
BU 648 67612 1.0 223 5.5 7.5 18:57.1 +32:54 G0    
STF 2427   51.6 60 8.5 9.0 18:58.1 +38:13 K0   B is a binary sep 7.1 pa 80 mag 10/10
STF 2431   19.1 236 7.0 9.0 18:58.8 +40:41 B5    
STF 2430 86669 1.9 1 8.5 8.5 18:59.4 +29:36 G0    
STF 2448 67752 2.7 191 8.0 8.0 19:03.7 +35:44 A3    
BU 1285   39.8 208 7.0 10.5 19:03.9 +34:09 B5    
SAO 48054 48054 2.0 178 7.5 11.0 19:04.2 +43:52 B9    
STF 2454 67811 1.1 276 8.0 9.0 19:06.1 +30:26 K0    
STF 2458 86825 11.9 227 8.5 9.0 19:07.0 +27:45 A0    
17 LYRA 67835 3.7 308 6.0 10.0 19:07.4 +32:29 A7    
STF 2469 67846 1.6 122 7.5 8.5 19:07.8 +38:55 A3    
STF 2466 86844 2.4 105 8.0 8.5 19:08.0 +29:47 A0    
STF 2467 67850 10.3 264 8.5 9.0 19:08.1 +30:47 F8    
STF 2472 67864 20.9 338 7.5 9.0 19:08.5 +37:54 K0    
STF 2473 67865 6.3 293 10.0 10.0 19:08.5 +37:55 F5    
STF 2470 67867 13.5 271 6.5 8.0 19:08.7 +34:45 B3    
STF 2474 67875 16.7 262 6.5 8.0 19:09.0 +34:35 G1    
STF 2481 67936 4.5 208 8.0 8.0 19:11.2 +38:47 G5    
STF 2480 86917 15.3 234 7.0 10.5 19:11.7 +26:15 A3    
STF 2483   9.7 318 7.0 8.0 19:12.3 +30:21 A0    
ETA LYRA 68010 28.2 83 4.0 8.0 19:13.7 +39:08 B2    
STT 366   21.8 230 7.0 10.0 19:14.2 +34:13 B9    
BU 975   33.4 228 7.0 9.5 19:14.4 +34:33 F5    
STT 371 87005 0.9 161 7.0 7.0 19:15.9 +27:27 B5    
STF 2491 87013 1.2 226 8.0 9.0 19:16.2 +28:16 A2    
THETA LYRA 68065 99.8 71 5.0 10.0 19:16.3 +38:08 K0 *** nice color contrast
HO 102   86.1 345 7.0 10.0 19:16.7 +33:07 B5    
STF 2502 68130 1.7 205 8.0 10.0 19:19.0 +39:15 A2    
STF 2505   10.7 316 8.0 9.0 19:19.9 +35:32 A0    

Image created using TheSky 4.0 Level IV
available from Bisque Software


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Some information gathered from Burgham's Celestial Handbooks and converted to J2000, other from my own observations.
Page 2003 Kevin Muenzler, Eagle Creek Observatory.