Definition
Miranda, discovered by Gerard Kuiper in 1948, is the innermost of Uranus’ five major satellites; it is also the smallest one, with a diameter of 470 km. Its surface mainly consists of water ice. Miranda was explored in 1986 by the Voyager 2 spacecraft whose images revealed a great variety of structures, with heavily cratered terrains but also rift-like canyons, faults, and valleys, showing evidence for an intense tectonic activity in the past history of the satellite. Some features could also result from cryovolcanism driven by tidal heating. In the 1980s it was proposed that these structures could have formed due to an early disruption of the object by a collision, followed by an accretion of the fragments in Uranus’ orbit.
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© 2014 Springer-Verlag Berlin Heidelberg
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Encrenaz, T. (2014). Miranda. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1003-3
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DOI: https://doi.org/10.1007/978-3-642-27833-4_1003-3
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Publisher Name: Springer, Berlin, Heidelberg
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