Method for constructing an analytical theory of Pluto's motion

Details Method for constructing an analytical theory of Pluto's motion Method for constructing an analytical theory of Pluto's motion

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pazh....1...39l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal, vol. 1, Oct. 1975, p. 39, 40. In Russian.

Astronomy and Astrophysics

Astronomy

Celestial Mechanics, Orbit Perturbation, Pluto (Planet), Solar Orbits, Neptune (Planet), Perturbation Theory, Secular Variations

Scientific paper

A formula for expanding the perturbation function so that the expansion converges without any limits for every pair of planets in the solar system is presented which allows Pluto's motion to be analyzed in the framework of classical perturbation theory. The first-order secular and long-period perturbations of Pluto by Neptune are determined using this formula.

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