A Shape and Spin Model for 1600 Vyssotsky

Details A Shape and Spin Model for 1600 Vyssotsky A Shape and Spin Model for 1600 Vyssotsky

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008mpbu...35...13w&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

The authors made lightcurve observations of the Hungaria asteroid, 1600 Vyssotsky, during apparitions in 1999, 2004, 2005, and 2007. The synodic rotation rates were determined and previously reported (Warner 1999, 2005; Higgins 2007). In this paper, we used lightcurve inversion on data from those apparitions to determine the spin axis and shape of the asteroid. The results included two possible solutions: l=356°, b=7° and l=219°, b=54°. For both solutions, the sidereal period was 3.201264 hr.

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