A discussion of Hill's method of secular perturbations and its application to the determination of the zero-rank effects in non-singular vectorial elements of a planetary motion

DOI10.1007/BF01230449zbMath0216.24703OpenAlexW2048688654WikidataQ60308792 ScholiaQ60308792MaRDI QIDQ5619662

Peter Musen

Publication date: 1970

Published in: Celestial Mechanics (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf01230449

Mathematics Subject Classification ID

Celestial mechanics (70F15) Perturbation methods for rigid body dynamics (70E20)

Related Items (4)

A second-order Uranus-Neptune theory by Hori's method ⋮ Fast computation of complete elliptic integrals and Jacobian elliptic functions ⋮ A second order Jupiter-Saturn planetary theory ⋮ The construction of a fifth-order Jupiter-Saturn motion: Analytical theory. I: Outline

Cites Work

• Mean motions and zeros of almost periodic functions
• Chebyshev Approximations for the Complete Elliptic Integrals K and E
• Mean Motion

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