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A chasma (plural: chasmata) is a broad, deep, elongate trough or depression. Chasmata are bounded by steep scarps that can form a series of terraces. A chasma is preferentially created by extensional tectonic forces. On the terrestrial planets, Venus and Mars have a large number of chasmata. In the outer Solar System, chasmata are major surface features on the icy satellites of Saturn and Uranus.
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© 2011 Springer-Verlag Berlin Heidelberg
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Wagner, R. (2011). Chasma, Chasmata. In: Gargaud, M., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-11274-4_266
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DOI: https://doi.org/10.1007/978-3-642-11274-4_266
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