Searching for Yarkovsky Among the Near-Earth Asteroids

Astronomy and Astrophysics – Astronomy

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Scientific paper

We report the results of a comprehensive search for evidence of the Yarkovsky effect in the orbital fits of near-Earth asteroids. The Yarkovsky effect is a subtle nongravitational acceleration on asteroids related to the anisotropic emission of thermal radiation. It has so far been directly measured in the motions of only two asteroids, 6489 Golevka [2] and 152563 (1992 BF) [1]. In past studies the Yarkovsky effect was modeled by solving the heat diffusion problem either linearly or through finite element methods. Here we take a less cumbersome and more direct approach, modeling the Yarkovsky effect as a purely transverse acceleration that is inversely proportional to the inverse square of the asteroid's heliocentric distance. The best-fitting transverse acceleration leads directly to a mean drift rate in the semimajor axis, which is the chief manifestation of the Yarkovsky acceleration. This study has revealed a number of probable detections of the Yarkovsky effect.
[1] S.R. Chesley et al., Science v. 302, 1739-1742 (2003)
[2] S.R. Chesley et al., BAAS v. 38, 591 (2006)

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