The Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect may spin up or spin down 5-km-radius asteroids on a 10 8 -year timescale. Smaller asteroids spin up or down even faster due to the radius-squared dependence of the YORP timescale. The mechanism is the absorption of sunlight and its re-emission
Collisional Spin Up of Nonspherical Asteroids
β Scribed by Masahisa Yanagisawa
- Publisher
- Elsevier Science
- Year
- 2002
- Tongue
- English
- Weight
- 199 KB
- Volume
- 159
- Category
- Article
- ISSN
- 0019-1035
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β¦ Synopsis
We investigate the spin up of nonspherical asteroids by successive random collisions with other smaller asteroids. The spin-up rates are calculated for ellipsoidal and spherical bodies of the same mass. Then, we derive the relative spin-up efficiency, that is, the ratio of the spin-up rate of the ellipsoidal body to that of the spherical body. We suppose a collisional process in our model different from that adopted in the previous works. The results show that ellipsoidal bodies can spin up more rapidly than spherical bodies.
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