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Exoplanet, Detection and Characterization

Encyclopedia of Astrobiology

Synonyms

Extrasolar planets detection

Definition

An exoplanet, or extrasolar planet, is a planet in orbit around another star. The first of such objects was discovered in 1992 and over 1,800 exoplanets have been identified today (November 2014). Although a few extrasolar plants have been discovered by direct imaging, because an exoplanet’s reflected visible light is (in the case of a system comparable to ours) ∼10−9times weaker than the stellar flux, indirect methods such as Dopple velocitmetry (radial velocity technique), transit photometry, microlensing, etc. have been used to detect these objects. Astrometry was first tried without success, as the available instrumental means were not sensitive enough to detect such small motions. The velocimetry technique was later successfully used, and this has led to the discovery of close to 600 exoplanets. The transit photometry technique has especially been successful in the past few years where CoRoT and Kepler space telescopes provided a...

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References and Further Reading

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Correspondence to Therese Encrenaz .

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Encrenaz, T., Haghighipour, N. (2014). Exoplanet, Detection and Characterization. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_553-5

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_553-5

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  • Online ISBN: 978-3-642-27833-4

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Chapter history

  1. Latest

    Exoplanet, Detection, and Characterization
    Published:
    17 February 2023

    DOI: https://doi.org/10.1007/978-3-642-27833-4_553-6

  2. Original

    Exoplanet, Detection and Characterization
    Published:
    16 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_553-5