On relativistic equations of motion of an earth satellite

DOI10.1023/B:CELE.0000016821.33627.77zbMath1131.70311OpenAlexW2042851440MaRDI QIDQ1769103

V. A. Brumberg

Publication date: 17 March 2005

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/b:cele.0000016821.33627.77

zbMATH Keywords

general relativityEarth satellite dynamicsgeocentric reference systemrelativistic third-body perturbations

Mathematics Subject Classification ID

Relativistic dynamics for problems in Hamiltonian and Lagrangian mechanics (70H40) Celestial mechanics (70F15) Orbital mechanics (70M20) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)

Related Items (4)

Numerical modeling of motion of near-Earth objects in a parallel computing environment ⋮ Relativistic celestial mechanics on the verge of its 100 year anniversary. (Brouwer Award lecture) ⋮ Numerical integration of relativistic equations of motion for Earth satellites ⋮ An application of symplectic integration for general relativistic planetary orbitography subject to non-gravitational forces

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