Motion of the orbital plane of a satellite due to a secular change of the obliquity of its mother planet

DOI10.1007/BF00692485zbMath0786.70007OpenAlexW4234479280MaRDI QIDQ1311643

Hiroshi Kinoshita

Publication date: 6 May 1994

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00692485

zbMATH Keywords

equatorial planePlutoUranian satellites

Mathematics Subject Classification ID

Celestial mechanics (70F15) Orbital mechanics (70M20)

Related Items (3)

Long-term evolution of orbits about a precessing oblate planet. II: The case of variable precession ⋮ A resonant-term-based model including a nascent disk, precession, and oblateness: application to GJ 876 ⋮ Long-term evolution of orbits about a precessing oblate planet. I: The case of uniform precession

Cites Work

• Effects of motion of the equatorial plane on the orbital elements of an earth satellite
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