Gravitational field of a rotating planet with a polytropic exponent equal to unity

Details Gravitational field of a rotating planet with a polytropic exponent equal to unity Gravitational field of a rotating planet with a polytropic exponent equal to unity

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974azh....51.1052h&link_type=abstract

Astronomicheskii Zhurnal, vol. 51, Sept.-Oct. 1974, p. 1052-1059. In Russian.

Computer Science

Numerical Analysis

2

Density Distribution, Gravitational Fields, Planetary Gravitation, Planetary Rotation, Poisson Equation, Astronomical Models, Boundary Value Problems, Equations Of State, Jupiter (Planet), Numerical Analysis, Planetary Mass, Polytropic Processes

Scientific paper

An exact solution of the Poisson equation for the density distribution
in a rotating planet, obtained for a polytropic exponent n = 1, is
applied to the calculation of the gravitational moments J2, J4, and J6
of the planet. The results are used to derive the equation of state of a
polytropic model of the planet Jupiter.

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