Scott Campbell, Russell Eberst, Kevin Fetter, Pierre Neirinck, Alberto Rango, Greg Roberts, Patrick Schmeer, and I, contributed observations used to determine one or more of the following element sets. XSS-11 375 X 697 km 1 28636U 05011A 10279.15845578 .00005834 00000-0 19303-3 0 06 2 28636 98.5432 86.9630 0233065 199.7263 159.4837 15.09035202 00 Arc 20100930.2-1006.17 WRMS resid 0.029 totl 0.018 xtrk FIA Radar 1 1065 X 1083 km 1 37162U 10046A 10280.06813795 .00000000 00000-0 00000-0 0 03 2 37162 122.9962 147.0156 0011724 90.0034 270.2274 13.49457118 04 Arc 20101001.78-1007.09 WRMS resid 0.026 totl 0.016 xtrk Patrick's reduction of his 10046A obs was relative the wrong star. I believe the following is correct, based on the direct-appulse implicit in his reduction, stated to the same precision: 37162 10 046A 0749 G 20101006025627900 37 25 2048000+803300 18 Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
This archive was generated by hypermail 2b29 : Thu Oct 07 2010 - 19:58:42 UTC