Remaining classfd last night. If I get time, I'll double check star field of last point for OFEQ 10 Ted had to kick. It would really help if all UNIDs would pass between bright, well known pairs and asterisms in future. At least the fast retrograde motion made it obvious. Incidentally Ted, I modified your elset (per my understanding of your correction parameters) to this for finding OFEQ 10: 1 70002U 14999A 14099.92856667 .00000000 00000-0 00000-0 0 01 2 70002 141.7700 213.2941 0179000 47.0000 314.6161 15.33000000 01 28888 05 042A 8336 F 20140412014238260 17 25 1349410+304607 28 S 28888 05 042A 8336 F 20140412014316130 17 25 1415655+390901 38 S 28888 05 042A 8336 F 20140412014318110 17 25 1417346+393566 48 S 28096 03 054B 8336 F 20140412020116870 17 25 1230013+583521 18 R 28096 03 054B 8336 F 20140412020131350 17 25 1253549+593668 18 R 28096 03 054B 8336 F 20140412020148030 17 25 1320267+602237 57 R 25746 99 028C 8336 F 20140412023034620 17 25 2227890+804843 38 R 25746 99 028C 8336 F 20140412023316580 17 25 1856879+753090 38 R Brad Young Bright:20 x 80 Garrett binoculars fluid pan head tripod Dim:22" f/4.2 UC Obsession @ 100x. Numbers above and methods explained at: http://satobs.org/seesat/Aug-2013/0140.html COSPAR 8336 = TULSA1 +36.139208,-95.983429 660ft, 201m COSPAR 8335 = TULSA2 +35.8311 -96.1411 1083ft, 330m _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-lReceived on Sat Apr 12 2014 - 12:56:16 UTC
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