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51 Pegasi B

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Definition

51 Pegasi b is an extrasolar planet orbiting the solar-type star 51 Pegasi.

History

51 Pegasi b is the first Jupiter-type planet, with a minimum mass slightly smaller than half of that of Jupiter, discovered around a Sunlike star. It was detected by radial-velocity observations obtained with the Elodie spectrometer on the 1.93-m telescope at the Observatoire de Haute Provence in France (Mayor and Queloz 1995). The extraordinarily short period of 4.230785 ± 0.000036 days was completely unexpected for a planet with a mass close to that of Jupiter and led to some initial skepticism that the unseen companion of 51 Pegasi could be a gas giant planet (e.g., Gray 1997). However, the subsequent announcement of several other radial-velocity planet candidates soon convinced most people of the reality of extrasolar planets.

Overview

51 Pegasi is classified as a G dwarf similar to the Sun but slightly cooler, at a distance of 15.6 parsecs (50.9 light years). A periodic variation in the r...

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Correspondence to David W. Latham .

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© 2014 Springer-Verlag Berlin Heidelberg

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Latham, D.W., Haghighipour, N. (2014). 51 Pegasi B. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_1840-2

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  • DOI: https://doi.org/10.1007/978-3-642-27833-4_1840-2

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Online ISBN: 978-3-642-27833-4

  • eBook Packages: Springer Reference Physics and AstronomyReference Module Physical and Materials ScienceReference Module Chemistry, Materials and Physics

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Chapter history

  1. Latest

    51 Pegasi B
    Published:
    29 July 2022

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1840-3

  2. Original

    51 Pegasi B
    Published:
    24 April 2015

    DOI: https://doi.org/10.1007/978-3-642-27833-4_1840-2