Tony Beresford, Scott Campbell, Pierre Neirinck, Jim Nix, Alberto Rango, Greg Roberts, and I, contributed observations used to determine one or more of the following element sets. SDS 3-4 r 297 X 16075 km 1 32379U 07060B 10278.02414855 .00004978 00000-0 92633-3 0 01 2 32379 60.7674 127.9154 5416464 32.1733 351.7558 4.93899365 04 Arc 20100911.16-1005.08 WRMS resid 0.012 totl 0.009 xtrk X-37B OTV 1-1 433 X 444 km 1 36514U 10015A 10278.73792454 .00000561 00000-0 12188-4 0 04 2 36514 39.9880 62.1228 0007830 334.9144 25.1283 15.43395766 05 Arc 20101001.77-1005.78 WRMS resid 0.025 totl 0.004 xtrk FIA Radar 1 1065 X 1083 km 1 37162U 10046A 10278.73465053 .00000000 00000-0 00000-0 0 04 2 37162 122.9959 142.8185 0011800 88.6611 271.5705 13.49456815 00 Arc 20101001.09-1005.78 WRMS resid 0.027 totl 0.018 xtrk 06829A 218 X 11606 km 1 90070U 06829A 10278.79781480 .00047270 00000-0 11401-2 0 05 2 90070 27.4948 325.6714 4632771 250.2694 55.2045 6.37461515 07 Arc 20100925.74-1005.8 WRMS resid 0.013 totl 0.006 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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