The Expansion of the Distance Between Two Arbitrary Gravitating Points as Applied to Specific Models of Celestial Bodies

Details The Expansion of the Distance Between Two Arbitrary Gravitating Points as Applied to Specific Models of Celestial Bodies The Expansion of the Distance Between Two Arbitrary Gravitating Points as Applied to Specific Models of Celestial Bodies

Nov 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003cemda..87..241b&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, v. 87, Issue 3, p. 241-256 (2003).

Astronomy and Astrophysics

Astronomy

Scientific paper

For the complete system of biharmonic functions a suitable representation in spheroidal coordinates is found. It is used for expanding the distance between two arbitrary gravitating points and its inverse quantity in appropriate series. Such expansions can be of interest and useful in a number of problems of celestial mechanics and stellar dynamics.

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