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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References and Further Reading
Gray D (1997) Nature 385:795
Mayor M, Queloz D (1995) Nature 378:355
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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
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Latest
51 Pegasi B- Published:
- 29 July 2022
DOI: https://doi.org/10.1007/978-3-642-27833-4_1840-3
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51 Pegasi B- Published:
- 24 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_1840-2