The Lightcurve of 2131 Mayall in 2006

Details The Lightcurve of 2131 Mayall in 2006 The Lightcurve of 2131 Mayall in 2006

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007mpbu...34...23w&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

Scientific paper

2131 Mayall was previously observed by Warner as part of an ongoing study at the Palmer Divide Observatory of the Hungaria group and family. Observations were made again in mid-2006 in order to add to the data set for the asteroid, the aim being eventually to derive a spin axis and shape model. The size and previously found rotation period, ~8 km and 2.5 hr, also made the asteroid a potential binary candidate. The data from 2006 did not show any signs of occultation or eclipse events that would indicate the asteroid is binary.

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