Scott Campbell, Russell Eberst, Kevin Fetter, Alberto Rango, Greg Roberts, Ian Roberts, Peter Wakelin, and I, contributed observations used to determine one or more of the following element sets. Helios 2B 676 X 680 km 1 36124U 09073A 10241.26013363 .00000000 00000-0 00000-0 0 00 2 36124 98.1220 176.1091 0003000 61.5100 298.6404 14.63859297 08 Arc 20100827.1-0829.28 WRMS resid 0.018 totl 0.011 xtrk Kevin made another video of OTV-1 this morning, from which I extracted the following: 36514 10 015A 1775 G 20100829083452408 36 25 0404390-124284 27 S+033 02 Alberto, Kevin and I, observed the object to be about 1.5 s early relative my day 10240 elset. I have shortened the arc to one day; the mean motion is a little uncertain, but I expect the object to be within a few seconds of prediction, per 24 h since epoch. OTV-1 433 X 444 km 1 36514U 10015A 10241.33912522 .00000000 00000-0 00000-0 0 04 2 36514 39.9880 288.8843 0007599 48.1950 311.9506 15.43371979 00 Arc 20100828.39-0829.36 WRMS resid 0.037 totl 0.010 xtrk AEHF 1 278 X 49989 km 1 36868U 10039A 10240.91700349 .00000109 00000-0 96487-4 0 05 2 36868 22.1043 307.1018 7887796 186.2855 147.6097 1.55238162 09 Arc 20100826.92-0829.27 WRMS resid 0.006 totl 0.005 xtrk AEHF 1 r 230 X 50136 km 1 36869U 10039B 10240.99956524 .00012772 00000-0 43300-2 0 05 2 36869 21.6828 309.2447 7906265 184.2038 158.0189 1.54872774 08 Arc 20100826.96-0829.35 WRMS resid 0.010 totl 0.008 xtrk Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
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