Physics
Scientific paper
Jun 1970
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970cemec...2..147c&link_type=abstract
Celestial Mechanics, Volume 2, Issue 2, pp.147-165
Physics
1
Scientific paper
This paper treats analytically the problem of the stability of the attitude motions of a gravity-stabilized gyrostat satellite that is in a circular orbit around a spherical planet. The vehicle considered consists of a body with no special symmetries that has any number of rotors attached to it. The ‘internal angular momentum’ vector due to these rotors is parallel to one of the principal axes of the entire satellite; this axis is aligned with (or close to) the normal to the orbit plane. Both the cases in which each rotor is driven by a motor at a constant spin rate relative to the main body of the vehicle and the one in which each rotor is rotating freely, without any friction, are treated. Stability (both infinitesimal and in the sense of Liapunov) of the attitude motions of the vehicle can be quickly predicted by using the results derived here, which are summarized in the form of a continuous, three-dimensional, stability diagram.
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