Group method of calculating the perturbations of minor planets
Abstract
An expansion of the distribution function R is proposed for the special case where the orbits of a group of minor planets have similar semimajor axes. The characteristics of the Taylor series are discussed.
 Publication:

Celestial Mechanics
 Pub Date:
 March 1975
 Bibcode:
 1975CeMec..11..265K
 Keywords:

 Asteroids;
 Disturbing Functions;
 Orbit Perturbation;
 Taylor Series;
 Celestial Mechanics;
 Convergence;
 EulerLagrange Equation;
 Kepler Laws;
 Orbit Calculation;
 Orbital Mechanics;
 Astronomy