DIRECT DETERMINATION OF SATELLITE COORDINATE PERTURBATIONS BY THE VON ZEIPEL METHOD.

Abstract

By utilizing the canonical variables (R, G, H, r, u, h) of Hill, the in-plane variations in a satellite's coordinates are obtained in a simple manner from the conventional generating functions of the von Zeipel procedure. The generating functions are extended and convenient expressions are found for the radius, radial velocity and the central angle, taking into account the first-order periodic influences of any harmonic in the expansion for the Earth's gravitational field. These expressions are non-singular for zero eccentricity orbits but do not apply for zero inclination orbits, orbits at critical inclination nor for orbits in a state or resonance with the tesseral harmonics. (Author)

Document Details

Document Type
Technical Report
Publication Date
Nov 01, 1965
Accession Number
AD0635685

Entities

People

  • Juris Vagners

Organizations

  • Stanford University

Tags

Communities of Interest

  • Space

DTIC Thesaurus Topics

  • Artificial Satellites
  • Eccentricity
  • Gravitational Fields
  • Harmonics
  • Mathematics
  • Motion
  • Perturbations
  • Physical Properties
  • Radial Velocity
  • Resonance

Fields of Study

  • Physics

Readers

  • Calculus or Mathematical Analysis
  • Space Exploration and Orbital Mechanics.

Technology Areas

  • Space
  • Space - Orbital Debris