Mathematical Results of the General Planetary Theory in Rectangular Coordinates View Full Text


Ontology type: schema:Chapter     


Chapter Info

DATE

1978

AUTHORS

V. A. Brumberg , L. S. Evdokimova , V. I. Skripnichenko

ABSTRACT

Mathematical construction of the general planetary theory has led to the series of two forms for the coordinates of eight major planets (excluding Pluto). The series of the first form are Poisson series where all orbital elements except the semi-major axes occur in literal, shape. The series of the second form are polynomial-exponential series with respect to the time and serve to calculate the ephemerides. The arbitrary constants of the theory are related to the Keplerian elements. The terms of the zero and first degree in eccentricities and inclinations have been found in the second approximation with, respect to the disturbing masses. Among those of particular interest are the resonant terms caused by the commensurabilities of the mean notations of triplets of planets. More... »

PAGES

33-48

References to SciGraph publications

  • 1973-11. Construction of a general planetary theory of the first order in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • 1975-02. Secular perturbations in general planetary theory in CELESTIAL MECHANICS AND DYNAMICAL ASTRONOMY
  • Book

    TITLE

    Dynamics of Planets and Satellites and Theories of Their Motion

    ISBN

    978-94-009-9811-7
    978-94-009-9809-4

    Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/978-94-009-9809-4_3

    DOI

    http://dx.doi.org/10.1007/978-94-009-9809-4_3

    DIMENSIONS

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