42058 17 011A 4353 F 20170303014242250 17 75 1926552+586250 56 42058 17 011A 4353 F 20170303014257250 17 75 1939252+564870 56 42058 17 011A 4353 F 20170303014317250 17 75 1952461+538200 56 42058 17 011A 4353 F 20170303014332250 17 75 2001031+519470 56 42058 17 011A 4353 F 20170303014347250 17 75 2008250+500970 56 42058 17 011A 4353 F 20170303033142250 17 75 0525154+732600 56 42058 17 011A 4353 F 20170303033147250 17 75 0510024+738320 56 42058 17 011A 4353 F 20170303033157250 17 75 0436283+747410 56 42058 17 011A 4353 F 20170303033207250 17 75 0359370+752850 56 42059 17 011B 4353 F 20170303014242250 17 75 1931466+577740 56 42059 17 011B 4353 F 20170303014257250 17 75 1943276+556700 56 42059 17 011B 4353 F 20170303014317250 17 75 1956043+530300 56 42059 17 011B 4353 F 20170303014332250 17 75 2003540+511850 56 42059 17 011B 4353 F 20170303014347250 17 75 2010487+494040 56 42059 17 011B 4353 F 20170303033142250 17 75 0505444+739890 56 42059 17 011B 4353 F 20170303033147250 17 75 0449110+744610 56 42059 17 011B 4353 F 20170303033157250 17 75 0413214+751470 56 42059 17 011B 4353 F 20170303033207250 17 75 0335283+754390 56 ------------------------------------------------------------------------- Canon EOS 60D + SamYang 1.4/85 mm, 800 ISO + ASTRORECORD astrometric software. What these numbers mean: http://www.satobs.org/position/IODformat.html ------------------------------------------------------------------------- In the table above, the A object is the brighter trailing object, B the fainter leading object. Both objects were well separated using a 2.5 second exposure and the SamYang 1.4/85 mm lens. The sky cleared in the afternoon, and stayed reasonably clear during the night, although there was some thin haze, especially during the second pass, which suffered from a field of cirrus. Two passes were imaged. During the first pass both objects were of about similar brightness. During the second pass, the leading object (B) was fainter and the trailing object (A) brighter. The A object was some 3.6 seconds early on my previous elset, the B object about 9.5 seconds early. During both passes, the NOSS 3-3 duo also passed through the FOV. I will measure these later. - Marco ----- Dr Marco Langbroek - SatTrackCam Leiden, the Netherlands. e-mail: sattrackcam_at_langbroek.org Cospar 4353 (Leiden): 52.15412 N, 4.49081 E (WGS84), +0 m ASL Cospar 4355 (Cronesteyn): 52.13878 N, 4.49937 E (WGS84), -2 m ASL Station (b)log: http://sattrackcam.blogspot.com Twitter: _at_Marco_Langbroek ----- _______________________________________________ Seesat-l mailing list http://mailman.satobs.org/mailman/listinfo/seesat-lReceived on Thu Mar 02 2017 - 23:10:52 UTC
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