LIGHTCURVE OBSERVATIONS OF (348400) 2005 JF21: AN NEA BINARY.

The Minor planet bulletin Pub Date : 2016-01-01
Robert D Stephens, Brian D Warner
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Abstract

CCD photometric observations were made of the near-Earth asteroid (348400) 2005 JF21 in 2015 June and August. Initial analysis in June did not find any signs of a satellite. Follow-up analysis in August using both data sets found indications that the asteroid was binary with a primary period of 2.41 h and an orbital period for the satellite of about 14.3 h. In mid-August, analysis of radar observations at Goldstone (Naidu et al., 2015) confirmed that the asteroid is a binary.

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近双星(348400)2005 jf21的光曲线观测。
2015年6月和8月对近地小行星(348400)2005 JF21进行了CCD光度观测。6月份的初步分析没有发现任何卫星的迹象。8月使用两组数据进行的后续分析发现,有迹象表明这颗小行星是双星,其主周期为2.41小时,卫星的轨道周期约为14.3小时。8月中旬,对Goldstone (Naidu et al., 2015)雷达观测的分析证实了这颗小行星是一颗双星。
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