The relativistic equations of motion for a satellite in orbit about a finite-size, rotating Earth

DOI10.1007/BF01232285zbMath0607.70022OpenAlexW2089727782MaRDI QIDQ3746953

Mark A. Vincent

Publication date: 1986

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

Full work available at URL: https://doi.org/10.1007/bf01232285

zbMATH Keywords

relativistic equationsbary-centric framemean- length satellite orbit determinationself-gravitating, rotating finite bodies

Mathematics Subject Classification ID

Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Orbital mechanics (70M20)

Related Items (1)

Celestial coordinate reference systems in curved space-time

Cites Work

• Equations of motion for rotating finite bodies in the extended PPN formalism

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