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- W1609691253 abstract "Harris’ (1979) theory on the collisional evolution of the asteroid spin rates is compared with the observational evidence provided by the statistics of photometric data. The resulting discrepancies can be qualitatively explained as due to different physical processes, occurred in the frame of the asteroid collisional history and connected in particular with the outcomes of catastrophic impact events." @default.
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- W1609691253 date "1982-01-01" @default.
- W1609691253 modified "2023-10-18" @default.
- W1609691253 title "Asteroid Rotation Rates: Comparison between Theory and Observations" @default.
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- W1609691253 doi "https://doi.org/10.1007/978-94-009-7846-1_79" @default.
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