Asymptotic matching of gravitational fields in the solar system

Details Asymptotic matching of gravitational fields in the solar system Asymptotic matching of gravitational fields in the solar system

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66.1289k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, Nov.-Dec. 1989, p. 1289-1303. In Russian.

Statistics

Computation

5

Asymptotic Methods, Celestial Mechanics, Computational Astrophysics, Gravitational Fields, Solar System, Center Of Gravity, Equations Of Motion, Planetocentric Coordinates, Poincare Problem, Relativistic Effects, Solar Orbits

Scientific paper

The structure of gravitational fields in the solar system is investigated in the framework of general relativity, and relativistic formulas of transformation between nonrotating (in the dynamical sense) harmonic reference systems (i.e., barycentric, planetocentric, and topocentric or satellite) are derived using the asymptotic matching of metric-tensor components. These formulas generalize the linear Poincare transformation to the case of curved space-time. Using the formulas, the relationship between relativistic time scales in the solar system is established.

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