>Return-Path: molczan@neocom.ca >From: Ted Molczan <molczan@neocom.ca> >To: "'Tristan Cools'" <tcools@nic.INbe.net> >Subject: RE: unknown >Date: Sun, 22 Oct 1995 17:55:10 -0400 > >The unknown you saw is ERBS, one of the reddest satellites I have >observed, and readily visible to the unaided eye under favourable >circumstances. In this case, the circumstances were not particularly >favourable, so I am surprised it reached magnitude 3. An ephemeris of >the pass you observed follows the elset. > > >ERBS 4.4 1.5 0.0 6.6 >1 15354U 84108 B 95292.05667138 .00000097 00000-0 88007-5 0 1370 >2 15354 56.9957 265.9358 0008752 126.5912 233.5927 14.94902088600638 > > >21/10/95 17:18 - 05:50 ST J2000.0 EL > 15 Bruges Belgium >ERBS 84108B 15354 Bull = 137 Tristan Cools >SGP4 Age = 2.8 d Unc = 0 s ( 25%) > > TIME %I Mv AZ EL R.A. DEC FE VANG RANGE ALT >-------- -- ---- --- -- ----- ----- -- ---- ----- ----- >19:27:19 13 9.1 272 14 16:12 13.1 7 0.15 1619 586 >19:28:10 16 8.4 279 21 16:12 21.9 7 0.21 1320 586 >19:28:46 20 7.8 285 27 16:11 30.3 8 0.28 1128 586 >19:29:13 24 7.4 292 32 16:09 38.4 8 0.34 1001 586 >19:29:35 28 7.0 300 36 16:05 46.4 8 0.41 913 586 >19:29:53 33 6.7 309 40 15:59 53.9 8 0.47 854 586 >19:30:09 38 6.4 318 43 15:50 61.4 8 0.51 815 586 >19:30:24 ES 43 6.2 329 45 15:33 68.8 9 0.54 790 586 > >Note that the "ES" at the final position means "enters shadow". >The ephemeris generator I use computes this as the approximate >mid-point within the penumbra, so the object would have been >visible for a few seconds later than "ES". > >Incidentally, if you can find a colour photograph of ERBS, you >will see why it so red - it is covered almost completely with >what looks like a gold kapton thermal blanket. It was deployed >on a space shuttle mission, and I have a photograph taken with >the object being held by the remote manipulator, prior to >deployment. Of course, this is also a strong clue as to the >cause of the redness of the Lacrosse satellites. > >Clear skies! > Forwarded from Ted Molczan, I thought it was interesting to put his personal mail to Seesat-L. Thanks to everyone who tried to identify it ! (you all were right on target with identifying it as ERBS !) As Ted Molczan puts it I was surprised to have a very bright transit of ERBS. Although in low orbit a pass from W->N is not so favourable at the time of the observation. Is it still working or is it out of order ? Tristan Cools(tcools@nic.INbe.net)