Tony Beresford, Russell Eberst, Björn Gimle, Marco Langbroek, Tim Luton, Mike McCants, Pierre Neirinck, Jim Nix, Greg Roberts, Patrick Schmeer, Brad Young, and I, contributed observations used to determine one or more of the following element sets. XSS-11 375 X 696 km 1 28636U 05011A 10292.15421268 .00008640 00000-0 28479-3 0 09 2 28636 98.5432 101.4446 0232282 157.1298 204.0479 15.09266471 07 Arc 20101007.49-1019.16 WRMS resid 0.042 totl 0.016 xtrk AEHF 1 4804 X 49976 km 1 36868U 10039A 10293.35109954 .00000000 00000-0 00000-0 0 08 2 36868 14.9719 296.1754 6688471 203.6247 348.9646 1.39926096 07 Arc 20101017.98-1020.35 WRMS resid 0.006 totl 0.006 xtrk FIA Radar 1 1101 X 1106 km 1 37162U 10046A 10293.17320835 .00000000 00000-0 00000-0 0 07 2 37162 122.9971 187.7707 0003804 89.8704 270.2693 13.41446138 04 Arc 20101012.07-1020.19 WRMS resid 0.037 totl 0.008 xtrk The mean motion and rate of decay of 10792A remain somewhat uncertain, but I expect predictions after 24 h to be accurate to within about 1 min time. 10792A 151 X 3615 km 1 90086U 10792A 10293.39999555 .01166518 00000-0 69902-3 0 01 2 90086 26.3618 16.4800 2096389 273.6213 62.8594 11.57075131 06 Arc 20101019.38-1020.42 WRMS resid 0.013 totl 0.008 xtrk Mike McCants' similar result is here: http://satobs.org/seesat/Oct-2010/0191.html Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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