Queloz was born in Switzerland, on 23 February 1966.[7][8]
Queloz studied at theUniversity of Geneva where he subsequently obtained aMSc degree in physics in 1990, aDEA in Astronomy and Astrophysics in 1992, and aPhD degree in 1995 with Swiss astrophysicistMichel Mayor as his doctoral advisor.[9]
The Daily Telegraph reports him as saying that, "Science inherited a lot from religions".[10]
Michel Mayor and Didier Queloz (2019) during Nobel week ceremony award
Didier Queloz is at the origin of the "exoplanet revolution" in astrophysics when as part of his PhD at theUniversity of Geneva, with his supervisor, they discovered the firstexoplanet around amain sequence star.[11][12]In 1995 with Michel Mayor announced a giant planet orbiting the star51 Pegasi; the planet was identified as51 Pegasi b and determined to be of aHot Jupiter.[11][12] The planet was detected by the measurement of small periodic changes in stellarradial velocity produced by the orbiting planet. Detecting this small variability by theDoppler effect had been possible thanks to the development of a new type of spectrograph, ELODIE,[13] installed at theHaute-Provence Observatory, combined creative approach to measuring precise stellar radial velocity.For this achievement, they were awarded half of the 2019 Nobel Prize in Physics "for the discovery of an exoplanet orbiting a solar-type star"[5] resulting in "contributions to our understanding of the evolution of the universe and Earth's place in the cosmos."[14]
This seminal discovery has spawned a revolution in astronomy and kickstarted the research field of exoplanets. Over the next 25 years, Didier Queloz's main scientific contributions have essentially been focused to expand our detection and measurement capabilities of these systems to retrieve information on their physical structure. The goal is to better understand their formation and evolution by comparison with theSolar System. In the course of his career, he developed new astronomical equipment, novel observational approaches, and detection algorithms. He participated and conducted programs leading to the detection of hundred planets, including breakthrough results.
Early in his career, he identified stellar activity as a potential limitation for planet detection. He published a reference paper describing how to disentangle stellar activity from a planetary signal using proxies, including new algorithms that have become standard practice in all planet publications based on precise Doppler spectroscopy data. With this work he set the foundation to optimize measurements of stellar radial velocity that is still in use today.
Queloz received the 2011BBVA Foundation Frontiers of Knowledge Award of Basic Sciences (co-winner with Mayor) for developing new astronomical instruments and experimental techniques that led to the first observation of planets outside theSolar System.[15]
Shortly after the start of theELODIE planet survey at OHP, he led the installation of an improved version (CORALIE), on theSwiss 1.2-metre Leonhard Euler Telescope. Very quickly this new facility started to detect exoplanets on stars visible in the southern hemisphere. In 2000, he took the responsibility, as a project scientist, in the development of HARPS, a new type of spectrograph for the ESO 3.6m telescope. This instrument commissioned in 2003 was about to become a reference in the business of precise Doppler spectroscopy. HARPS performances, allied with the development of a new analysis software inherited from all past experiences gathered with ELODIE and CORALIE, would considerably improve the precision of the Doppler technique. Eventually, it would deliver spectacular detections of smaller exoplanets in the realm of Neptune, super-Earth systems before Kepler would massively detect them and establish their statistic occurrence.
After the announcement of the detection of the first transiting planet (in 1999), Didier Queloz's research interest got broader with the objective to combine capabilities offered by transiting planets and follow-up Doppler spectroscopy measurements. In 2000 he achieved the first spectroscopic transit detection of an exoplanet using the so-calledRossiter-McLaughlin effect. This type of measurement essentially tells us about the projected angle between the stellar angular momentum vector and the planet orbital angular momentum vector. The pinnacle of this program would be reached 10 years later, after he led a significant upgrade of CORALIE, and established a collaboration with theWide Angle Search for Planets (WASP) consortium in the UK. With his Ph.D. student they demonstrated a significant number of the planets were surprisingly misaligned or in a retrograde orbit, providing a new insight about their formation process. In 2017 he received theWolf Prize in Physics 2017 for that work and all the planet discoveries he had made.
The special geometry of transiting planets combined with precise Doppler spectroscopic observations allow us to measure the mass and radius of planets and to compute their bulk densities to get insights about their physical structure. In 2003 Didier Queloz, recently appointed at a faculty position, with his research team pioneered and established the combination of these techniques by first measuring bulk density ofOGLE transiting planets. They also looked for transit opportunities on known radial velocity planets and they found the first transiting Neptune-size planetGliese 436 b. In the course of this program and a collaboration with his Colleague S. Zucker from Tel-Aviv University, they developed the mathematical foundation to compute residual noise they encountered during the analysis of transit they were trying to model. They established statistical metric to addresspink noise in the data. Today this concept is widely used in the field to estimate systematics in light-curves and transit modelling.
In 2007 Didier Queloz became associate professor. Over the next 5 years following his nomination his research program based on the combination of spectroscopy and transit detection intensified. He took the lead in the spectroscopic follow-up effort of the WASP consortium and theCoRoT space mission.[16] The combination of WASP and Corot data with follow-up observations usingEulerCam (CCD imager ),CORALIE spectrograph,HARPS spectrograph, and other mainESO facilities was amazingly successful. It led to more than 100 publications, some of them breakthroughs providing new insights on the formation and nature of hot Jupiter-type planets. Further, in the same period, the detection ofCOROT-7b combined with an intensive follow-up campaign established the first planet detection with a bulk density similar to a rocky planet.
All follow-up expertise he developed naturally extended to theKepler space telescope era withHARPS-N consortium confirming the Earth-like bulk density ofKepler-10. On the ground-based transit programs, Didier Queloz was deeply involved in the design and installation of a new generation of survey telescope: the NGTS Observatory. His role was decisive during system tests in Europe and to establish the facility at theParanal Observatory in theAtacama Desert in northern Chile.
At the time Didier Queloz moved to theUniversity of Cambridge, he essentially focused his activity to set up a comprehensive research activity directed to the detection of Earth-like planets and life in the Universe, and to further develop the exoplanet community in UK. When he left Switzerland, he was co-directing a major national initiative[17] which eventually got funded. At Cambridge with the help of his colleagues of the IoA and DAMTP he established the Cambridge Exoplanet Research Centre[18] to stimulate joint coordinated efforts and collaborations between departments. In UK he organized the first "Exoplanet community meeting" and installed the idea of a regular yearly "community" workshop. In the European context, he is leading at Geneva (through his joint Professor appointment) the development of the ground segmentCHEOPS[19] space mission and he chairs the science team.[20]
His most recent research highlights are related to the search for transiting Earth-like planets on low mass stars and Universal life. This program, carried out in collaboration with M. Gillon from theUniversity of Liège, is at the origins of the detection ofTRAPPIST-1, a planetary system potentially interesting to further search for atmosphere and life signature. Another successful avenue of research is the characterization of the rocky surface or atmosphere of hot small planets with the work on55 Cancri e. The recent extension of this program towards "Life in the Universe" is carried out in the context of an international research initiative supported by theSimons Foundation. The highlight result of this collaboration is the definition – combining chemistry and astrophysical constraints – of minimum conditions for the origins ofRNA precursors on exoplanets ("abiogenesis zone").
Discoveries of exoplanets attract a lot of attention from the public and media. In parallel to his research and teaching activities, Didier Queloz has participated in numerous documentaries, movies, articles, and TV and radio interviews to share the excitement, and to explain results and promote interest in science in general.
He was also a visiting scientist at theMIT Kavli Institute for Astrophysics and Space Research in 2019.[21]
In October 2019, related to his work in astronomy and exoplanet discoveries, Queloz predicted humans will discover extraterrestrial life in the next 30 years, stating, "I can't believe we are the only living entity in the universe. There are just way [too] many planets, way too many stars, and the chemistry is universal. The chemistry that led to life has to happen elsewhere. So I am a strong believer that there must be life elsewhere."[22]
In December 2019, Queloz took issue with those who are not supportive of helping to limitclimate change, stating, "I think this is just irresponsible, because the stars are so far away I think we should not have any serious hope to escape the Earth [...] Also keep in mind that we are a species that has evolved and developed for this planet. We're not built to survive on any other planet than this one [...] We'd better spend our time and energy trying to fix it."[23]
