Abstract
Tumbling asteroids models
Peter Scheirich








Astronomical Institute, Ondrejov








I present a technique of numerical modeling of non-principal axis rotators (tumblers) that simulates their double-periodic lightcurves. The aim of this work is to derive basic parameters of the tumbling asteroid: the angular momentum (its magnitude and direction), Euler angles describing the orientation of the asteroid at given epoch, and its principal moments of inertia. A shape of the asteroid is approximated with a triaxial ellipsoid. The application of the technique to lightcurve data of the tumbling asteroid 2002 TD60 is presented.
Presenting author:  Peter Scheirich