New physical models of asteroids derived from sparse and dense photometry

Details New physical models of asteroids derived from sparse and dense photometry New physical models of asteroids derived from sparse and dense photometry

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..396d&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.396

Physics

Scientific paper

We present 78 new physical models of asteroids, namely their spin vectors and rotation periods. The models were derived from the photometric data using the lightcurve inversion method. With the new models, the total number of asteroid models derived from photometry has increased to 300. The new models confirm the clustering of spin vectors of small asteroids towards the ecliptic poles [1].

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