| Literature DB >> 32455396 |
Robert D Stephens1, Brian D Warner2.
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.Entities:
Year: 2017 PMID： 32455396 PMCID： PMC7243950
Source DB: PubMed Journal: Minor Planet Bull