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Asteroid Belt, Main

Encyclopedia of Astrobiology
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Synonym

Main asteroid belt

Definition

The asteroid belt is a region of the Solar System between the orbits of Mars and Jupiter that contains the orbits of most of the known asteroids (over 600,000 to date). The reason for the existence of the asteroid belt is thought to be gravitational perturbations of the orbits of planetesimals and planetary embryos (planetary building blocks) in the region by the massive planet Jupiter that have prevented these objects from combining to form a planet. Collisions between objects in the asteroid belt cause them to be ground down into an ever-increasing number of smaller bodies.

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Correspondence to Alan W. Harris .

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© 2014 Springer-Verlag Berlin Heidelberg

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Harris, A.W. (2014). Asteroid Belt, Main. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_117-2

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_117-2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

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Chapter history

  1. Latest

    Asteroid Belt, Main
    Published:
    26 November 2021

    DOI: https://doi.org/10.1007/978-3-642-27833-4_117-3

  2. Original

    Asteroid Belt, Main
    Published:
    30 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_117-2