Russell Eberst, Pierre Neirinck, Alberto Rango, Greg Roberts, Peter Wakelin, and I, contributed observations used to determine one or more of the following element sets. USA 129 291 X 909 km 1 24680U 96072A 10218.10612213 .00015111 00000-0 22878-3 0 04 2 24680 97.7695 269.0580 0442389 153.9477 208.4757 14.88394864 09 Arc 20100802.82-0806.12 WRMS resid 0.019 totl 0.010 xtrk USA 186 256 X 1016 km 1 28888U 05042A 10218.12073054 .00010380 00000-0 93544-4 0 03 2 28888 97.9047 280.9192 0542347 252.3879 101.7416 14.76943095 02 Arc 20100802.81-0806.13 WRMS resid 0.026 totl 0.012 xtrk Peter and I have concluded that the Aug 04 UTC observations of PAN, that he reported, were of another object that was near by; here is the revised elset based on PAN, and the assumption that it was synchronous: PAN 35758 X 35817 km 1 35815U 09047A 10216.76953941 .00000000 00000-0 00000-0 0 09 2 35815 0.0620 259.9997 0007000 19.3648 348.7013 1.00273500 04 Arc 20100804.9-0804.95 WRMS resid 0.007 totl 0.003 xtrk Here is the revised elset based on the assumption that it was drifting: PAN 35752 X 35786 km 1 35815U 09047A 10216.76952112 .00000000 00000-0 00000-0 0 08 2 35815 0.0620 259.9997 0004000 19.3648 348.6806 1.00339479 08 Arc 20100728.75-0804.95 WRMS resid 0.004 totl 0.001 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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