Russell Eberst, Pierre Neirinck, Steve Newcomb, Jim Nix, Alberto Rango, Ian Roberts, Peter Wakelin, Brad Young, and I, contributed observations used to determine one or more of the following element sets. USA 129 291 X 908 km 1 24680U 96072A 10220.12304707 .00008837 00000-0 13390-3 0 01 2 24680 97.7695 271.0429 0442178 147.2723 215.6737 14.88422731 03 Arc 20100804.83-0808.13 WRMS resid 0.031 totl 0.011 xtrk USA 186 258 X 1014 km 1 28888U 05042A 10220.15322195 .00006010 00000-0 56604-4 0 03 2 28888 97.9120 282.9294 0538709 245.4484 108.9683 14.76967067 01 Arc 20100805.86-0808.16 WRMS resid 0.024 totl 0.012 xtrk The following is based on the assumption that PAN was synchronous when Ian observed it. PAN 35758 X 35817 km 1 35815U 09047A 10218.79021647 .00000000 00000-0 00000-0 0 03 2 35815 0.0620 264.5764 0007000 19.4190 353.7034 1.00273500 00 Arc 20100807.74-0807.74 WRMS resid 0.001 totl 0.000 xtrk 99750A 2774 X 37437 km 1 90004U 99750A 10219.78266766 .00000000 00000-0 00000-0 0 07 2 90004 64.4548 182.8104 6544205 262.0500 24.5916 2.01426838 02 Arc 20100621.97-0808.19 WRMS resid 0.013 totl 0.012 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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