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(24465) 2000 SX155: A NEW BINARY HUNGARIA
Robert D Stephens1, Brian D Warner2
1Center for Solar System Studies (CS3) / MoreData!, 11355 Mount Johnson Ct. Rancho Cucamonga, CA 91737 USA.
Abstract:
CCD photometry observations made in 2016 October and November of the Hungaria asteroid (24465) 2000 SX155 showed it to be binary. The primary lightcurve has a period of 2.66087 ± 0.00005 h and an amplitude 0.08 ± 0.02 mag. The orbital period of the satellite is 9.252 ± 0.001 h, the shortest detected so far.
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