Representation of the gravitational field of rotationally symmetrical bodies through the attraction of mass points

Details Representation of the gravitational field of rotationally symmetrical bodies through the attraction of mass points Representation of the gravitational field of rotationally symmetrical bodies through the attraction of mass points

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980velen......103f&link_type=abstract

Leningradskii Universitet, Vestnik, Matematika, Mekhanika, Astronomiia, Jan. 1980, p. 103-106. In Russian.

Astronomy and Astrophysics

Astronomy

Astronomy, Celestial Bodies, Gravitational Fields, Mass, Rotating Bodies, Approximation, Convergence, Ellipsoids

Scientific paper

The paper deals with the problem of approximating the gravitational
potential of celestial bodies, expressed as a series of spherical
functions, through a function representing the potential of a system of
mass points. The necessary and sufficient conditions for the convergence
of this series for this function are obtained.

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