Seager was born in Toronto, Ontario, Canada, and is Jewish.[4][12][13] 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.[4][14]
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.[19][20]
Academic research
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."[21] 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.[22][23] Together with Marc Kuchner, Seager had predicted the existence of carbon planets.[24]
Seager has been the chair of the NASA Science and Technology Definition team for a proposed mission, "Starshade",[25] 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.[26]
In years since 2020, Sara has been focusing on work related to Venus, with the potential discovery of phosphine, a biosignature gas, in the upper atmosphere.[27]
Seager equation
Seager developed a parallel version of the Drake equation to estimate the number of habitable planets in the Galaxy.[28] Instead of aliens with radio technology, Seager has revised the Drake equation to focus on simply the presence of any alien life detectable from Earth. The equation focuses on the search for planets with biosignature gases, gases produced by life that can accumulate in a planet atmosphere to levels that can be detected with remote space telescopes.[28]
where:
N = the number of planets with detectable signs of life
N* = the number of stars observed
FQ = the fraction of stars that are quiet
FHZ = the fraction of stars with rocky planets in the habitable zone
FO = the fraction of stars with observable planets
FL = the fraction of planets that have life
FS = the fraction of life forms that produce planetary atmospheres with one or more detectable signature gases
Asteria Spacecraft
Seager was the principal investigator of the Asteria (Arcsecond Space Telescope Enabling Research in Astrophysics) spacecraft,[29] a 6-U cubesat designed to do precision photometry to search for extrasolar planets, a collaborative project between MIT and NASA's Jet Propulsion Laboratory. ASTERIA was launched into low Earth orbit from the International Space Station on 20 November 2017, and successfully operated until its orbital decay on 24 April 2020.
Venus Life Finder
In 2020, Seager led a team proposing a mission Venus Life Finder,[30] a small spacecraft to investigate the possibility of life in the atmosphere of Venus.[31] The mission will be a privately funded spacecraft to be launched by Rocket Lab on the Electron rocket[32] with a target launch date of January 2025.
She was an honorary graduand at her alma mater, the University of Toronto Spring 2023 Convocation.[42]
In 2024, Seager was awarded the Kavli Prize in Astrophysics.[43]
Publications
Books
Deming, Drake; Seager, Sara (2003). Deming, Drake; Seager, Sara (eds.). Scientific Frontiers in Research on Extrasolar Planets. ASP Conference Proceedings (Volume 294). Vol. 294. San Francisco. Bibcode:2003ASPC..294.....D. ISBN1-58381-141-9.{{cite book}}: CS1 maint: location missing publisher (link)
Seager, Sara (2010). Exoplanet Atmospheres: Physical Processes. Princeton University Press. ISBN9781400835300.
Seager, Sara (2010). Exoplanets. University of Arizona Press. ISBN978-0-8165-2945-2.
Seager, Sara (2020). The Smallest Lights in the Universe: A Memoir. Crown. ISBN978-0-5255-7625-9.
Borucki, William J.; Koch, David G.; Basri, Gibor; Batalha, Natalie; Brown, Timothy M.; Bryson, Stephen T.; Caldwell, Douglas; Christensen-Dalsgaard, Jørgen; Cochran, William D.; Devore, Edna; Dunham, Edward W.; Gautier, Thomas N.; Geary, John C.; Gilliland, Ronald; Gould, Alan; Howell, Steve B.; Jenkins, Jon M.; Latham, David W.; Lissauer, Jack J.; Marcy, Geoffrey W.; Rowe, Jason; Sasselov, Dimitar; Boss, Alan; Charbonneau, David; Ciardi, David; Doyle, Laurance; Dupree, Andrea K.; Ford, Eric B.; Fortney, Jonathan; et al. (2011). "Characteristics of Planetary Candidates Observed by Kepler, II: Analysis of the First Four Months of Data". The Astrophysical Journal. 736 (1): 19. arXiv:1102.0541. Bibcode:2011ApJ...736...19B. doi:10.1088/0004-637X/736/1/19. ISSN0004-637X. S2CID15233153.
^Foss, Kelly (20 September 2018). "Holy Grail". Gazette – Memorial University of Newfoundland. Archived from the original on 7 July 2019. Retrieved 7 July 2019.