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Trans-Neptunian Object

Encyclopedia of Astrobiology
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Synonyms

Kuiper belt object; TNO

Definition

The name “trans-Neptunian object” (TNO) has been given to the small solar-system bodies that constitute the Kuiper belt, beyond the orbit of Neptune. The existence of this population was first proposed by Kenneth Edgeworth and Gerard Kuiper on the basis of dynamical considerations. Over 1,300 trans-Neptunian objects are presently known. The first discovery of a TNO was made in 1992 by David Jewitt and Jane Luu. Trans-Neptunian objects are classified in different categories: the “classical” objects, at 42–47 AU from the Sun, have a low inclination and a low eccentricity; the “plutinos” are in resonance with Pluto and have the same semimajor axis as Pluto; and the “scattered” objects are more distant and have larger eccentricities.

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Correspondence to Therese Encrenaz .

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© 2014 Springer-Verlag Berlin Heidelberg

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Encrenaz, T. (2014). Trans-Neptunian Object. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1608-2

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1608-2

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  • Online ISBN: 978-3-642-27833-4

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Chapter history

  1. Latest

    Trans-Neptunian Object
    Published:
    06 December 2022

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1608-3

  2. Original

    Trans-Neptunian Object
    Published:
    21 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1608-2