Physical models of ten asteroids from an observers' collaboration network

Details Physical models of ten asteroids from an observers' collaboration network Physical models of ten asteroids from an observers' collaboration network

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007a%26a...465..331d&link_type=abstract

Astronomy and Astrophysics, Volume 465, Issue 1, April I 2007, pp.331-337

Astronomy and Astrophysics

Astrophysics

7

Minor Planets, Asteroids

Scientific paper

Aims:We present physical models of ten asteroids obtained by means of lightcurve inversion. A substantial part of the photometric data was observed by amateur astronomers. We emphasize the importance of a coordinated network of observers that will be of extreme importance for future all-sky asteroid photometric surveys. Methods: The lightcurve inversion method was used to derive spin states and shape models of the asteroids. Results: We derived spin states and shape model for ten new asteroids: (110) Lydia, (125) Liberatrix, (130) Elektra, (165) Loreley, (196) Philomela, (218) Bianca, (306) Unitas, (423) Diotima, (776) Berbericia, and (944) Hidalgo. This increases the number of asteroid models up to nearly one hundred.
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