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

DOI10.1007/BF01228543zbMath0454.70009WikidataQ56213770 ScholiaQ56213770MaRDI QIDQ5904648

Theodore D. Moyer

Publication date: 1981

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

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)

Related Items

Celestial coordinate reference systems in curved space-time ⋮ The Pioneer anomaly ⋮ The Fermi coordinate system in the post-Newtonian framework ⋮ Relativistic time scales in the solar system ⋮ On time transfer in X-ray pulsar navigation ⋮ Transformation from proper time on Earth to coordinate time in solar system barycentric space-time frame of reference

Cites Work

• The problem of n bodies in general relativity theory