Alberto Rango did a great job recovering this object, which was about 57 min early relative 28 day old elements. I received his observations in time to produce the preliminary elset I posted earlier, and make these obs: 90019 03 790B 2701 G 20040927090211120 17 25 0347294-233563 28 R 90019 03 790B 2701 G 20040927090249480 17 25 0413004-231602 28 R 90019 03 790B 2701 G 20040927090315370 17 25 0430611-230606 18 R What these numbers mean: http://www.satobs.org/position/IODformat.html Site 2701: 43.68764 N, 79.39243 W, 230 m 03790B 0.0 0.0 0.0 3.5 v 1 90019U 03790B 04271.35980382 .00702348 00000-0 13000-2 0 03 2 90019 27.3085 346.7138 0795000 235.6488 116.6345 14.40951030 08 Arc 2004 Sep 27.10 - 27.38, WRMS residuals = 0.020 deg I set the eccentricity and B* to yield ndot/2 nearly 20 percent greater than its average value during the 28 days since the previous observations. Ted Molczan ------------------------------------------------------------------------- Subscribe/Unsubscribe info, Frequently Asked Questions, SeeSat-L archive: http://www.satobs.org/seesat/seesatindex.html
This archive was generated by hypermail 2b29 : Mon Sep 27 2004 - 07:11:29 EDT