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Sara Seager AI simulator
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Sara Seager
Sara Seager OC (born 21 July 1971) is a Canadian-American astronomer and planetary scientist. She is a professor at the Massachusetts Institute of Technology, though she will return to her alma mater the University of Toronto to join the Canadian Institute for Theoretical Astrophysics (CITA) as North Star Distinguished Professor, starting September 1, 2026. Seager 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.
Seager was born in Toronto, Ontario, Canada, and is Jewish. Her father, David Seager, who lost his hair when he was 19 years old, was a pioneer and one of the world's leaders in hair transplantation and the founder of the Seager Hair Transplant Center in Toronto.
She earned her BSc degree in mathematics and physics from the University of Toronto in 1994, assisted by a NSERC University Undergraduate Student Research Award, and a PhD in astronomy from Harvard University in 1999. Her doctoral thesis developed theoretical models of atmospheres on extrasolar planets and was supervised by Dimitar Sasselov.
She held a postdoctoral research fellow position at the Institute for Advanced Study between 1999 and 2002 and a senior research staff member at the Carnegie Institution of Washington until 2006. She joined the Massachusetts Institute of Technology in January 2007 as an associate professor in both physics and planetary science, was granted tenure in July 2007, and was elevated to full professor in July 2010. As of 2013[update] she holds the "Class of 1941" chair.
She was elected a Legacy Fellow of the American Astronomical Society in 2020.
She is married to Charles Darrow and they have two sons from her first marriage. Her first spouse, Michael Wevrick, died of cancer in 2011.
Seager's research has been primarily directed toward the discovery and analysis of exoplanets; in particular her work is centered around ostensibly rare earth analogs, leading NASA to dub her "an astronomical Indiana Jones." Seager used the term "gas dwarf" for a high-mass super-Earth-type planet composed mainly of hydrogen and helium in an animation of one model of the exoplanet Gliese 581c. The term "gas dwarf" has also been used to refer to planets smaller than gas giants, with thick hydrogen and helium atmospheres. Together with Marc Kuchner, Seager had predicted the existence of carbon planets.
Seager has been the chair of the NASA Science and Technology Definition team for a proposed mission, "Starshade", to launch a free-flying occulting disk, used to block the light from a distant star in order for a telescope to be able to resolve the (much dimmer) light from an accompanying exoplanet located in the habitable zone of the star.
Sara Seager
Sara Seager OC (born 21 July 1971) is a Canadian-American astronomer and planetary scientist. She is a professor at the Massachusetts Institute of Technology, though she will return to her alma mater the University of Toronto to join the Canadian Institute for Theoretical Astrophysics (CITA) as North Star Distinguished Professor, starting September 1, 2026. Seager 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.
Seager was born in Toronto, Ontario, Canada, and is Jewish. Her father, David Seager, who lost his hair when he was 19 years old, was a pioneer and one of the world's leaders in hair transplantation and the founder of the Seager Hair Transplant Center in Toronto.
She earned her BSc degree in mathematics and physics from the University of Toronto in 1994, assisted by a NSERC University Undergraduate Student Research Award, and a PhD in astronomy from Harvard University in 1999. Her doctoral thesis developed theoretical models of atmospheres on extrasolar planets and was supervised by Dimitar Sasselov.
She held a postdoctoral research fellow position at the Institute for Advanced Study between 1999 and 2002 and a senior research staff member at the Carnegie Institution of Washington until 2006. She joined the Massachusetts Institute of Technology in January 2007 as an associate professor in both physics and planetary science, was granted tenure in July 2007, and was elevated to full professor in July 2010. As of 2013[update] she holds the "Class of 1941" chair.
She was elected a Legacy Fellow of the American Astronomical Society in 2020.
She is married to Charles Darrow and they have two sons from her first marriage. Her first spouse, Michael Wevrick, died of cancer in 2011.
Seager's research has been primarily directed toward the discovery and analysis of exoplanets; in particular her work is centered around ostensibly rare earth analogs, leading NASA to dub her "an astronomical Indiana Jones." Seager used the term "gas dwarf" for a high-mass super-Earth-type planet composed mainly of hydrogen and helium in an animation of one model of the exoplanet Gliese 581c. The term "gas dwarf" has also been used to refer to planets smaller than gas giants, with thick hydrogen and helium atmospheres. Together with Marc Kuchner, Seager had predicted the existence of carbon planets.
Seager has been the chair of the NASA Science and Technology Definition team for a proposed mission, "Starshade", to launch a free-flying occulting disk, used to block the light from a distant star in order for a telescope to be able to resolve the (much dimmer) light from an accompanying exoplanet located in the habitable zone of the star.