Russell Eberst, Pierre Neirinck, Greg Roberts, Peter Wakelin, Brad Young, and I, contributed observations used to determine one or more of the following element sets. FIA Radar 1 1064 X 1083 km 1 37162U 10046A 10270.36335477 .00000000 00000-0 00000-0 0 01 2 37162 123.0072 116.4853 0012753 74.0803 286.1566 13.49470918 04 Arc 20100925.08-0927.38 WRMS resid 0.030 totl 0.018 xtrk 10046A's mean motion has been stable over the past couple of days. Excluding a couple faint obs by Brad and myself, its standard visual magnitude appears to be about 4 (1000 km, 90 deg phase angle). 08628A 2325 X 38031 km 1 90081U 08628A 10268.47055706 .00000000 00000-0 00000-0 0 06 2 90081 62.4533 125.6827 6722757 277.5217 16.4699 2.00604163 08 Arc 20100911.93-0925.92 WRMS resid 0.011 totl 0.006 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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