publication . Article . 2006

THE YARKOVSKY AND YORP EFFECTS: Implications for Asteroid Dynamics

David Parry Rubincam; William F. Bottke;
Open Access
  • Published: 16 Jan 2006 Journal: Annual Review of Earth and Planetary Sciences, volume 34, pages 157-191 (issn: 0084-6597, eissn: 1545-4495, Copyright policy)
  • Publisher: Annual Reviews
The Yarkovsky and YORP (Yarkovsky-O’Keefe-Radzievskii-Paddack) effects are thermal radiation forces and torques that cause small objects to undergo semimajor axis drift and spin vector modifications, respectively, as a function of their spin, orbit, and material properties. These mechanisms help to (a) deliver asteroids (and meteoroids) with diameter D < 40 km from their source locations in the main belt to chaotic resonance zones capable of transporting this material to Earth-crossing orbits; (b) disperse asteroid families, with drifting bodies jumping or becoming trapped in mean-motion and secular resonances within the main belt; (c) modify the rotation rates ...
arXiv: Astrophysics::Earth and Planetary AstrophysicsPhysics::Space Physics
free text keywords: Earth and Planetary Sciences (miscellaneous), Space and Planetary Science, Astronomy and Astrophysics, Perturbation (astronomy), Astronomy, Meteoroid, Orbit, Asteroid family, Yarkovsky effect, Asteroid, Spin-½, Celestial mechanics, Physics
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