HEAT MODELS OF ASTEROIDS AND THE YORP EFFECT

Journal Title: Odessa Astronomical Publications - Year 2014, Vol 27, Issue 1

Abstract

The Yarkovsky–O'Keefe–Radzievski–Paddack (YORP) effect is a torque of light pressure recoil forces acting on an asteroid. We show how this torque can be expressed as an integral of a universal function over the surface of an asteroid, and discuss generalizations of this expression for the case of non-Lambert’s scattering laws, non-convex shapes of asteroids, and non-zero heat conductivity. Then we discuss tangential YORP (TYORP), which appears due to uneven heat conductivity in stones lying on the surface of an asteroid. TYORP manifests itself as a drag, which pulls the surface in the tangential direction. Finally, we discuss relation and interplay between the normal YORP and the tangential YORP.

Authors and Affiliations

O. Golubov

Keywords

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  • EP ID EP598911
  • DOI -
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How To Cite

O. Golubov (2014). HEAT MODELS OF ASTEROIDS AND THE YORP EFFECT. Odessa Astronomical Publications, 27(1), 89-90. https://europub.co.uk/articles/-A-598911