Derek Breit, Scott Campbell, Kevin Fetter, Alberto Rango, Greg Roberts, Peter Wakelin, Brad Young, and I, contributed observations used to determine one or more of the following element sets. The analytical and observational efforts of several of us to find the AEHF 1 objects have come to fruition, and Scott Campbell and Peter Wakelin have reported observations. I believe the following to be fairly accurate, but the arc is short, and the rate of decay of the Centaur is somewhat uncertain. AEHF 1 285 X 49983 km 1 36868U 10039A 10239.63360755 .00000000 00000-0 00000-0 0 07 2 36868 22.1201 307.4141 7885562 185.7262 150.4454 1.55238993 01 AEHF 1 r 226 X 50151 km 1 36869U 10039B 10239.71344234 .00021320 00000-0 66273-2 0 05 2 36869 21.6894 309.5622 7907799 183.6128 161.0601 1.54833355 00 Standard visual magnitude of both objects is approximately 4 (1000 km, 90 deg phase angle). Kevin made another video of OTV-1 this morning, from which I extracted the following: 36514 10 015A 1775 G 20100828091621335 36 25 0107460-103294 67 S+032 05 OTV-1 434 X 444 km 1 36514U 10015A 10240.36856224 -.00000967 00000-0 -21061-4 0 00 2 36514 39.9880 294.7701 0007591 40.7670 319.3705 15.43341941 07 Arc 20100821.46-0828.39 WRMS resid 0.026 totl 0.011 xtrk I have run out of time this morning, but plan to analyze Peter's other observations later. Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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