Secular orbit variation due to solar radiation effects: a detailed model for BYORP

DOI10.1007/S10569-009-9247-9zbMath1375.85004OpenAlexW2052204230MaRDI QIDQ968337

Jay W. McMahon, Daniel J. Scheeres

Publication date: 5 May 2010

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

Full work available at URL: https://doi.org/10.1007/s10569-009-9247-9

zbMATH Keywords

binary asteroidssolar radiation pressurebinary YORPBYORPNEAsorbit perturbations

Mathematics Subject Classification ID

Galactic and stellar dynamics (85A05)

Related Items (3)

Evolution of orbits about comets with arbitrary comae ⋮ Geostationary secular dynamics revisited: application to high area-to-mass ratio objects ⋮ Equilibrium points and associated periodic orbits in the gravity of binary asteroid systems: (66391) 1999 KW4 as an example

Cites Work

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• The non-gravitational perturbations impact on the BepiColombo radio science experiment and the key rôle of the ISA accelerometer: direct solar radiation and albedo effects
• Rotational dynamics of a solar system body under solar radiation torques

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