Transformation from proper time on Earth to coordinate time in solar system barycentric space-time frame of reference

DOI10.1007/BF01228544zbMath0454.70010OpenAlexW2992297713MaRDI QIDQ5904649

Theodore D. Moyer

Publication date: 1981

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

Full work available at URL: https://doi.org/10.1007/bf01228544

zbMATH Keywords

relativistic effectsDoppler observablesn-body metric tensor of Eddington and Clark

Mathematics Subject Classification ID

Astronomy and astrophysics (85A99) Celestial mechanics (70F15) Orbital mechanics (70M20) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) General models, approaches, and methods in mechanics of particles and systems (70G99)

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Cites Work

• A note on velocity-related series expansions in the two-body problem
• Transformation from proper time on Earth to coordinate time in solar system barycentric space-time frame of reference
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