The formalism of the translational-rotational motion of a rigid body in the field of a gravitating and radiating centre

Details The formalism of the translational-rotational motion of a rigid body in the field of a gravitating and radiating centre The formalism of the translational-rotational motion of a rigid body in the field of a gravitating and radiating centre

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.192..257m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 192, no. 2, June 1992, p. 257-262.

Physics

Celestial Mechanics, Gravitational Fields, Rigid Structures, Differential Equations, Field Theory (Physics)

Scientific paper

The problem is addressed of the motion of an arbitrarily shaped rigid body in the field of an attracting center when the body is further acted upon by a force due to the radiation of this center. Assuming that the distance between the body and the source of these two forces is large, the equations of motion are derived on the basis that for an elementary mass both forces act along the line joining their source with this mass.

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