Швейцариялық астрофизик және экзопланеталар ашушысы Мишель Майор

Swiss astrophysicist & Nobel laureate of Physics

Michel Gustave Édouard Mayor (miʃɛl majɔʁ; born 12 January 1942) is a Swiss astrophysicist and professor emeritus at the University of Geneva's Department of Astronomy. 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".

From 1971 to 1984, Mayor worked as a research associate at the Observatory of Geneva, which is home to the astronomy department of the University of Geneva. He became an associate professor at the university in 1984.

Mayor's research interests include extrasolar planets (also known as exoplanets), instrumentation, statistical properties of double stars, globular cluster dynamics, galactic structure and kinematics. Mayor's doctoral thesis at the University of Geneva was devoted to the spiral structure of galaxies. This research led to various fields of interest, including the study of statistical characteristics of solar type binary stars. With fellow researcher Antoine Duquennoy, they examined the radial velocities of several systems believed to be binary stars in 1991. Their results found that a subset of these may in fact be single star systems with substellar secondary objects. Desiring more accurate radial velocity measurements, Mayor, along with Baranne at Marseille, and with graduate student Didier Queloz, developed ELODIE, a new spectrograph based on the work of CORAVEL, which was estimated to have an accuracy of 15 m/s for bright stars, improving upon the 1 km/s from CORAVEL. ELODIE was developed with the specific intent to determine if the substellar secondary objects were brown dwarf stars or potentially giant planets. By 1994, ELODIE was operational at Geneva and Mayor and Queloz began their survey of Sun like systems with suspected substellar secondary objects. In July 1995, the pair's survey of 51 Pegasi affirmed that there was an exoplanet orbiting it, identified as 51 Pegasi b, which was later classified as a hot Jupiter–type planet. This was the first exoplanet to be found orbiting a main sequence star, as opposed to planets that orbited the remains of a star. Mayor's and Queloz's discovery of an exoplanet launched great interest is searching for other exoplanets since. On 21st March 2022, the 5000th exoplanet beyond our solar system was confirmed. Mayor's work focused more on improving instrumentation for radial velocity measurements to improve detecting exoplanets and measuring their properties. Mayor led a team to further improve ELODIE to increase velocity measurement accuracy to 1 m/s via the High Accuracy Radial Velocity Planet Searcher (HARPS) installed on the ESO 3.6 m Telescope at La Silla Observatory in Chile by 2003. Mayor led the team that used HARPS to seek out other exoplanets. In 2007, Mayor was one of 11 European scientists who discovered Gliese 581c, the first extrasolar planet in a star's habitable zone, from the ESO telescope. In 2009, Mayor and his team discovered the lightest exoplanet ever detected around a main sequence star: Gliese 581e. Nonetheless, 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.