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- W1993174911 abstract "Asymmetric comas and repetitive appearances of structures in the heads and tails of comets are used to infer nuclei rotation periods. However, periodic behaviour of optically-thick expanding comas or of ion plasma production may contribute spurious results. The spin periods of comets are longer than those of asteroids, ranging generally over 10-100 h and above probable limits for gravitational escape. The periods show a flatter distribution, which may reflect an accretional rather than collisional fragmentation history. Arguments for spin-up with age due to sublimating gases are weak; the converse is possible and spin-down due to preferential escape of particles from equatorial regions appears likely." @default.
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- W1993174911 date "1984-11-27" @default.
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- W1993174911 title "Rotation of cometary muclei" @default.
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- W1993174911 doi "https://doi.org/10.1098/rsta.1984.0092" @default.
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