Giovanna Tinetti | |
|---|---|
 Tinetti talks about ARIEL in 2018 | |
| Born | 1 April 1972 Turin |
| Education | University of Turin |
| Employer | University College London |
| Known for | Exoplanets |
Giovanna Tinetti (born 1 April 1972) is an Italian physicist based in London. She is a Professor of Physics and Astronomy at University College London, who researches galactic planetary science, exoplanets and atmospheric science.
Giovanna Tinetti was born in 1972 in Turin, Italy. [1] She earned an MA in Astrophysics in 1997 and an MSc in Fluid Dynamics and Energetics in 1998 at the University of Turin. She completed PhD in Theoretical Physics under Professor Luigi Sertorio in 2003. [2] [1]
Tinetti joined NASA's Jet Propulsion Laboratory in 2003 as a postdoctoral researcher and remained in NASA's Astrobiology Institute until 2005. [3] [4] [5] She joined the Institut d’Astrophysique de Paris as a European Space Agency as an external fellow in 2005, where she was the first to identify water vapour in the atmosphere of a planet beyond our solar system. [6] [7] She went on to secure a STFC Aurora Fellowship to pursue her research at University College London in 2007. [8] [9] [10] [11]
In 2009, Tinetti was made a research fellow of the Royal Society. [12] She coordinated the European Space Agency's EChO Mission (Exoplanet Characterisation Observatory), which was backed by ESA, in 2013. [13] [14] She is the Principal Investigator of ARIEL, Atmospheric Remote-sensing Infrared Exoplanet Large-survey, one of three candidate-missions selected by European Space Agency for the next medium class (M4) science mission and now confirmed to be launched in 2028. [15] [16] [17] She is Principal Investigator for the European Research Council Consolidator program Exo-Lights - Decoding the light from other worlds. [18]
She is on the editorial board of Springer's Experimental Astronomy and of Proceedings of the Royal Society A. [19] [20]
Tinetti regularly shares her enthusiasm for exoplanets and space science with non-expert audiences, contributing to websites, giving public lectures, appearing at science festivals and appearing on the television. [21] [22] [23] [24] [25] [26] [27] [28] Tinetti appears regularly on the BBC's Sky At Night and Stargazing Live. [29] [30] [31] She featured in the 2012 Sky at Night Question and Answer book which accompanied the series. [32] She has discussed the quest for exoplanets on several radio and television programs and podcasts. [33] [34]
In 2012, she was included in the London 2012 Olympics See Britain campaign, where recognised the "UK’s ability to harness the best from the past whilst looking to the future has created the perfect conditions for great scientific innovation". [35] [36]
In 2013 she released a popular science book, "I pianeti extrasolari" (Extrasolar Planets), describing the history of exoplanets, detection techniques and likelihood of finding alien life. [37] In 2016, she was an invited speaker at the Israel Institute for Advanced Studies. [38]
Tinetti is co-director of Blue Skies Space Limited, a commercial enterprise for space science projects. [39] She is the Science Lead for the Citizen Science project Twinkle, a small, low-cost spectroscopy mission that decodes the light from extrasolar planets developed by Surrey Satellite Technology and UCL. [40]
2022 - Sir Arthur Clarke Award, British Interplanetary Society and the Arthur C Clarke Foundation [41]
2011 - Moseley Medal & Prize, Institute of Physics [42]
2009 - NASA Group Achievement Award, with Mark Swain and Gautam Vasisht [43]
2009 - Edward Stone Award, JPL [44]
1999 - SIF Award for best young Italian physicist, Italian Society of Physics [43]
1998 - ENEA Award for best MSc thesis, Italian National Agency for Energy & Environment [1]
Astrobiology is a scientific field within the life and environmental sciences that studies the origins, early evolution, distribution, and future of life in the universe by investigating its deterministic conditions and contingent events. As a discipline, astrobiology is founded on the premise that life may exist beyond Earth.
The NASA Astrobiology Institute (NAI) was established in 1998 by the National Aeronautics and Space Administration (NASA) "to develop the field of astrobiology and provide a scientific framework for flight missions." In December 2019 the institute's activities were suspended.
Sara Seager is a Canadian–American astronomer and planetary scientist. She is a professor at the Massachusetts Institute of Technology and is known for her work on extrasolar planets and their atmospheres. She is the author of two textbooks on these topics, and has been recognized for her research by Popular Science, Discover Magazine, Nature, and TIME Magazine. Seager was awarded a MacArthur Fellowship in 2013 citing her theoretical work on detecting chemical signatures on exoplanet atmospheres and developing low-cost space observatories to observe planetary transits.
Caleb Asa Scharf is a British-American astronomer and popular science author. He is currently the senior scientist for astrobiology at the NASA Ames Research Center in Mountain View, California. He formerly served as the director of the multidisciplinary Columbia Astrobiology Center at Columbia University, New York.
PLAnetary Transits and Oscillations of stars (PLATO) is a space telescope under development by the European Space Agency for launch in 2026. The mission goals are to search for planetary transits across up to one million stars, and to discover and characterize rocky extrasolar planets around yellow dwarf stars, subgiant stars, and red dwarf stars. The emphasis of the mission is on Earth-like planets in the habitable zone around Sun-like stars where water can exist in a liquid state. It is the third medium-class mission in ESA's Cosmic Vision programme and is named after the influential Greek philosopher Plato. A secondary objective of the mission is to study stellar oscillations or seismic activity in stars to measure stellar masses and evolution and enable the precise characterization of the planet host star, including its age.
The Exoplanet Characterisation Observatory (EChO) was a proposed space telescope as part of the Cosmic Vision roadmap of the European Space Agency, and competed with four other missions for the M3 slot in the programme. On 19 February 2014 the PLATO mission was selected in place of the other candidates in the programme, including EChO.
Fast Infrared Exoplanet Spectroscopy Survey Explorer (FINESSE) was a NASA mission proposal for a space observatory operating in the Near-infrared spectrum for the Medium-Class Explorers program. The Principal Investigator was Mark Swain of the Jet Propulsion Laboratory in Pasadena, California.
CHEOPS is a European space telescope. Its objective is to determine the size of known extrasolar planets, which will allow the estimation of their mass, density, composition and their formation. Launched on 18 December 2019, it is the first Small-class mission in ESA's Cosmic Vision science programme.
William J. (Bill) Borucki is a space scientist who worked at the NASA Ames Research Center. Upon joining NASA in 1962, Borucki joined the group conducting research on the heat shield for Apollo program spacecraft. He later turned his attention to the optical efficiency of lightning strikes in the atmospheres of planets, investigating the propensity that these lightning strikes could create molecules that would later become the precursors for life. Subsequently, Borucki's attention turned to extrasolar planets and their detection, particularly through the transit method. In light of this work, Borucki was named the principal investigator for NASA's Kepler mission, launched on March 7, 2009 and dedicated to a transit-based search for habitable planets. In 2013, Borucki was awarded the United States National Academy of Sciences's Henry Draper Medal for his work with Kepler. In 2015 he received the Shaw Prize in Astronomy.
Natalie M. Batalha is professor of Astronomy and Astrophysics at UC Santa Cruz. Previously she was a research astronomer in the Space Sciences Division of NASA Ames Research Center and held the position of Co-Investigator and Kepler Mission Scientist on the Kepler Mission, the first mission capable of finding Earth-size planets around other stars.
The Nexus for Exoplanet System Science (NExSS) initiative is a National Aeronautics and Space Administration (NASA) virtual institute designed to foster interdisciplinary collaboration in the search for life on exoplanets. Led by the Ames Research Center, the NASA Exoplanet Science Institute, and the Goddard Institute for Space Studies, NExSS will help organize the search for life on exoplanets from participating research teams and acquire new knowledge about exoplanets and extrasolar planetary systems.
Stephen Kane is a full professor of astronomy and planetary astrophysics at the University of California, Riverside who specializes in exoplanetary science. His work covers a broad range of exoplanet detection methods, including the microlensing, transit, radial velocity, and imaging techniques. He is a leading expert on the topic of planetary habitability and the habitable zone of planetary systems. He has published hundreds of peer reviewed scientific papers and has discovered/co-discovered several hundred planets orbiting other stars. He is a prolific advocate of interdisciplinarity science and studying Venus as an exoplanet analog.
Jessie Christiansen is an Australian astrophysicist who is the Chief Scientist of the NASA Exoplanet Science Institute at the California Institute of Technology (Caltech). She won the 2018 NASA Exceptional Engineering Achievement Medal for her work on the Kepler planet sample.
The Atmospheric Remote-sensing Infrared Exoplanet Large-survey (ARIEL) is a space telescope and the fourth medium-class mission of the European Space Agency's Cosmic Vision programme. The mission is aimed at observing at least 1000 known exoplanets using the transit method, studying and characterising the planets' chemical composition and thermal structures. Compared to the James Webb Space Telescope, ARIEL will be a much smaller telescope and have more observing time available for planet characterisation. ARIEL is expected to be launched in 2029 aboard an Arianespace Ariane 6 together with the Comet Interceptor.
Suzanne Aigrain is a Professor of Astrophysics at the University of Oxford and a Fellow of All Souls College, Oxford. She studies exoplanets and stellar variability.
Cosmic Vision is the third campaign of space science and space exploration missions in the Science Programme of the European Space Agency (ESA). Formulated in 2005 as Cosmic Vision: Space Science for Europe 2015–2025, the campaign succeeded the Horizon 2000 Plus campaign and envisioned a number of missions in the fields of astronomy and solar system exploration beyond 2015. Ten missions across four funding categories are planned to be launched under Cosmic Vision, with the first being CHEOPS in December 2019. A mission to the Galilean moons (JUICE), the first deep space mission with an opportunistic target, and one of the first gravitational-wave space observatories (LISA), are planned for launch as part of the Cosmic Vision campaign.
Lynnae C. Quick is an American planetary geophysicist and Ocean Worlds Planetary Scientist at NASA Goddard Space Flight Center. Her research centers on theoretical modeling of cryovolcanic processes on the icy moons and dwarf planets in the Solar System as well as modeling volcanic activity on Venus and the Moon. Quick is a member of the Dawn, Europa Clipper, and Dragonfly Mission science teams. She is also a member of the NASA Solar System Exploration Research Virtual Institute (SSERVI) Toolbox for Research and Exploration (TREX) team, and serves as co-chair of the Earth and Planetary Systems Sciences section of the National Society of Black Physicists.
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