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Near-Earth Objects

Encyclopedia of Astrobiology
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NEO

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A near-Earth object (NEO) is an asteroid or comet with a perihelion distance of less than 1.3 astronomical units (AU, the mean Sun–Earth distance). The orbits of NEOs can evolve to intersect that of the Earth; the associated impact hazard is very small but scientifically well founded. The impact of a NEO with a diameter of just 50 m could cause a major catastrophe. Depending on its orbital parameters a NEO is categorized as an Amor, Apollo, Aten, or inner Earth object (IEO). As of June 2013 nearly 10,000 NEOs have been discovered, of which about 860 have diameters of 1 km or more.

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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). Near-Earth Objects. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1046-3

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1046-3

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  • Online ISBN: 978-3-642-27833-4

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  1. Latest

    Near-Earth Objects
    Published:
    27 November 2021

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1046-4

  2. Original

    Near-Earth Objects
    Published:
    29 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1046-3