A simple, accurate, geometrical approximation to the Keplerian motion

DOI10.1016/0315-0860(89)90082-7zbMath0697.01004OpenAlexW2022890789MaRDI QIDQ911569

N. E. Zubov

Publication date: 1989

Published in: Historia Mathematica (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1016/0315-0860(89)90082-7

zbMATH Keywords

celestial mechanicseccentric anomalyclassical one-body-motion

Mathematics Subject Classification ID

Celestial mechanics (70F15) History of mathematics in the 17th century (01A45) History of astronomy and astrophysics (85-03) History of mechanics of particles and systems (70-03)

Cites Work

• The Keplerian and mean motions. A geometrical study
• Kepler's hypothesis vicaria
• The Error in Kepler's Acronychal Data for Mars

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