Two elsets have appeard at OIG as of May 31 12:50 UTC: GRO 480 x 361 1 21225U 91027B 00152.15594577 -.00910124 00000-0 -15414-1 0 8222 2 21225 28.4609 96.2594 0087316 147.1463 213.4605 15.48710815390811 GRO 475 x 362 1 21225U 91027B 00152.09151533 .00000340 00000-0 00000+0 0 8216 2 21225 28.4676 96.6563 0082992 145.7518 214.8470 15.49386774390803 The perigee didn't quite reach 350 km, there are two different MMs given, but (hopefully) no reason to believe the negative drag. I suggest using only Epoch + line2 of elset #822: GRO 480 x 361 1 21225U 91027B 00152.15594577 .00018675 00000-0 25715-3 0 98226 2 21225 28.4609 96.2594 0087316 147.1463 213.4605 15.48710815390811 -- bjorn.gimle@tietotech.se (office) -- -- b_gimle@algonet.se (home) http://www.algonet.se/~b_gimle -- -- COSPAR 5919, MALMA, 59.2576 N, 18.6172 E, 23 m -- -- COSPAR 5918, HAMMARBY, 59.2985 N, 18.1045 E, 44 m -- -- SeeSat-L / Visual Satellite Observer Home Page found at -- -- http://www2.satellite.eu.org/satintro.html -- Sue: > > Culmination at 2000152.11 was about 20 seconds *later* than predicted > by the above elset, 15 seconds earlier than predicted by OIG pre-burn > elset. I'm glad I got to see such a great, high and bright, pass of > GRO before its demise. > ----------------------------------------------------------------- Unsubscribe from SeeSat-L by sending a message with 'unsubscribe' in the SUBJECT to SeeSat-L-request@lists.satellite.eu.org http://www2.satellite.eu.org/seesat/seesatindex.html
This archive was generated by hypermail 2b29 : Wed May 31 2000 - 06:00:01 PDT