Shape, Rotational Properties and Phase Function of Asteroid 2867 Steins

Details Shape, Rotational Properties and Phase Function of Asteroid 2867 Steins Shape, Rotational Properties and Phase Function of Asteroid 2867 Steins

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009dps....40.2833l&link_type=abstract

American Astronomical Society, DPS meeting #40, #28.33; Bulletin of the American Astronomical Society, Vol. 41, p.558

Astronomy and Astrophysics

Astronomy

Scientific paper

The Optical, Spectroscopic, and Infrared Remote Imaging System OSIRIS observed the E-type asteroid (2867) Steins during the fly-by of ESA's Rosetta spacecraft. Before the flyby, the OSIRIS camera obtained two light curves on 20 August and 4 September 2008. Combined with previously published OSIRIS and ground-based observations, we will present a refined global shape model of the asteroid, the rotational parameters and the phase function (at large phase angles).

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