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When an orbiting body is affected by tides, its spin axis, spin rate, and orbital plane can reach an equilibrium state in which obliquities (tilts) are nonzero. Cassini states are observed in the Earth-Moon system, Triton-Neptune system, and possibly, Europa-Jupiter system. In these cases, the satellite’s obliquity is locked at a small nonzero value, but in general, with large inclinations, the obliquity could be large.
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© 2014 Springer-Verlag Berlin Heidelberg
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Barnes, R. (2014). Cassini State. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_242-3
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DOI: https://doi.org/10.1007/978-3-642-27833-4_242-3
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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