A Study of the Trinary NEA 2001 SN263

Details A Study of the Trinary NEA 2001 SN263 A Study of the Trinary NEA 2001 SN263

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mpbu...35..182b&link_type=abstract

The Minor Planet Bulletin (ISSN 1052-8091). Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Obse

Physics

1

Scientific paper

The trinary NEA, 2001 SN263, was observed by the authors in 2008 February in Salvador, Bahia, Brazil. Based on the data obtained, the synodic period of the primary body was estimated to be 3.20 ± 0.01h with a lightcurve amplitude of 0.27 ± 0.07 mag. The orbital period of the smaller satellite (0.4 Km) was estimated to be 46.1 ± 0.3 h. The NIR spectrum suggests the object is of type C according to DeMeo classification. Lance, a CO3 type meteorite, is the best analogous meteorite.

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