Group method of calculating the perturbations of minor planets

Details Group method of calculating the perturbations of minor planets Group method of calculating the perturbations of minor planets

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975cemec..11..265k&link_type=abstract

Celestial Mechanics, vol. 11, Mar. 1975, p. 265-274.

Physics

Asteroids, Disturbing Functions, Orbit Perturbation, Taylor Series, Celestial Mechanics, Convergence, Euler-Lagrange Equation, Kepler Laws, Orbit Calculation, Orbital Mechanics

Scientific paper

An expansion of the distribution function R is proposed for the special
case where the orbits of a group of minor planets have similar
semi-major axes. The characteristics of the Taylor series are discussed.

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