Alberto Rango, Greg Roberts and Brad Young, contributed observations used to determine the following element set: OTV-1 432 X 445 km 1 36514U 10015A 10234.09215508 .00000000 00000-0 00000-0 0 09 2 36514 39.9851 332.7784 0009598 358.0505 2.0264 15.43360000 03 Arc 20100819.75-0822.1 WRMS resid 0.040 totl 0.008 xtrk There are now sufficient observations to rule out the more eccentric orbit I discussed in my previous update. Ted Molczan _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-l
This archive was generated by hypermail 2b29 : Sun Aug 22 2010 - 04:52:04 UTC