A collaboration of two observers at widely-separated longitudes made CCD photometric observations of the near-Earth asteroid (NEA) 1943 Anteros from 2016 August to October. Analysis of the data led to the possibility that the asteroid is a binary with = 2.86923 ± 0.00006 h, = 0.07 mag and = 23.548 ± 0.002 h, = 0.05-0.10 mag. The estimated effective diameter ratio is ≥ 0.22 ± 0.02.
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| http://www.ncbi.nlm.nih.gov/pmc/articles/PMC7243940 | PMC |
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