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Updated: Dec 20, 2025

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
Published on: May 10, 2020
LIGHTCURVE OBSERVATIONS OF (348400) 2005 JF21: AN NEA BINARY
Robert D Stephens1, Brian D Warner2
1Center for Solar System Studies (CS3) / MoreData!, 11355 Mount Johnson Ct., Rancho Cucamonga, CA 91737 USA.
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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