Deformation of the gravitational field in ring-type \(N\)-body systems due to the presence of many radiation sources

DOI10.1023/B:MOON.0000034495.99039.6FzbMath1062.85008OpenAlexW2064849966MaRDI QIDQ702162

D. Kazazakis, Telemachus J. Kalvouridis

Publication date: 17 January 2005

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1023/b:moon.0000034495.99039.6f

zbMATH Keywords

equilibrium positions zero-velocity curves \(N\)-body ring-type configurations Radiation pressure

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Equations of motion in general relativity and gravitational theory (83C10) Statistical astronomy (85A35)

Related Items (6)

Periodic motions of a small body in the Newtonian field of a regular polygonal configuration of \(\nu +1\) bodies ⋮ Particle motions in Maxwell's ring dynamical systems ⋮ On some new aspects of the photo-gravitational Copenhagen problem ⋮ BIFURCATIONS IN THE TOPOLOGY OF ZERO-VELOCITY SURFACES IN THE PHOTO-GRAVITATIONAL COPENHAGEN PROBLEM ⋮ Radiation effect on a particle's periodic orbits in a regular polygon configuration of \(N\) bodies ⋮ Impact of the mass parameter on particle dynamics in a ring configuration of \(N\) bodies

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