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Regolith, Terrestrial

Encyclopedia of Astrobiology
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The terrestrial regolith is a layer of unconsolidated material overlying solid rock. It forms as a result of mechanical and chemical weathering, biological processes, deposition of loose material, or brecciation of rock and may consist of soil, alluvium, and other sedimentary deposits, fractured and oxidized rock, and volcanic ash or scoria. Its thickness varies from negligible to several hundred meters. Regolith has been observed on Earth, Moon, some asteroids, and other planets.

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Correspondence to Nicholas Arndt .

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© 2014 Springer-Verlag Berlin Heidelberg

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Arndt, N. (2014). Regolith, Terrestrial. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1365-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1365-3

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  • Online ISBN: 978-3-642-27833-4

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Chapter history

  1. Latest

    Regolith, Terrestrial
    Published:
    19 November 2020

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1365-4

  2. Original

    Regolith, Terrestrial
    Published:
    04 May 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1365-3