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Also known as Michel G. E. Mayor, Michel Gustave Mayor, Michel Gustave E. Mayor, M. G. E. Mayor, M. G. Mayor, M. Mayor
Swiss astrophysicist & Nobel laureate of Physics
Michel Mayor is a Swiss astrophysicist who won the Nobel Prize in Physics for his groundbreaking work in discovering exoplanets—planets that orbit stars outside our solar system. His discoveries fundamentally changed our understanding of planetary systems and opened up the field of exoplanet research, which helps us explore the possibility of life beyond Earth.
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Michel Gustave Édouard Mayor ( French pronunciation: [miʃɛl majɔʁ]; born 12 January 1942) is a Swiss astrophysicist and professor emeritus at the University of Geneva's Department of Astronomy. He formally retired in 2007, but remains active as a researcher at the Observatory of Geneva. He is co-laureate of the 2019 Nobel Prize in Physics along with Jim Peebles and Didier Queloz, and the winner of the 2010 Viktor Ambartsumian International Prize and the 2015 Kyoto Prize.
Together with Didier Queloz in 1995, he discovered 51 Pegasi b, the first extrasolar planet orbiting a sun-like star, 51 Pegasi. For this achievement, they were awarded the 2019 Nobel Prize in Physics "for the discovery of an exoplanet orbiting a solar-type star" resulting in "contributions to our understanding of the evolution of the universe and Earth's place in the cosmos". Related to the discovery, Mayor noted that humans will never migrate to such exoplanets since they are "much, much too far away ... [and would take] hundreds of millions of days using the means we have available today". However, due to discoveries by Mayor, searching for extraterrestrial communications from exoplanets may now be a more practical consideration than thought earlier.
· 1956 · cited 41,857x
· 2009 · cited 22,489x
· 1993 · cited 19,080x
· 2016 · cited 13,788x
· 2021 · cited 11,541x
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Michel Mayor - Associ� �tranger de l'Acad�mie des sciences
academie-sciences.fr →Notice biographique de Michel Mayor, Associé étranger de l’Académie des sciences limited sample. The results show that: 1) stars with planets are significantly metal-rich 2) that the source of metallicity is most probably primordial DUQUENNOY, A., MAYOR, M. Multiplicity among solar-type stars in the solar neighbourhood. II. Distribution of the orbital elements in an unbiased sample. A&A, 248, 485 (1991) One of the 40 most cited papers published by Astronomy and Astrophysics during its first 40 years. A&A, 500 p. 337, (2009) (special issue of A&A) Le 3 mai 2010
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Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).