Determination of the rotation parameters of asteroids with large amplitudes of light variation

Details Determination of the rotation parameters of asteroids with large amplitudes of light variation Determination of the rotation parameters of asteroids with large amplitudes of light variation

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...44k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Sept.-Oct. 1986, p. 44-50. In Russian.

Astronomy and Astrophysics

Astronomy

1

Asteroids, Astrometry, Astronomical Photometry, Light Curve, Planetary Rotation, Planet Ephemerides, Polar Coordinates

Scientific paper

A method for determining the pole coordinates and sidereal rotation
period of elongated asteroids is presented which is based on a simple
geometrical model of an asteroid. The method is applied to the asteroids
216 Kleopatra and 433 Eros, which have large amplitudes of light
variation.

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