Scott D. Tremaine Astrophysicist
Scott Tremaine’s research is focused on the dynamics of astrophysical systems, including planet formation and evolution, comets, galaxies, and other stellar systems. He has made seminal contributions to understanding the formation and evolution of planetary systems, comets, black holes, star clusters, galaxies, and galaxy systems. He predicted the Kuiper belt of comets beyond Neptune and, with colleague Peter Goldreich, the existence of shepherd satellites and density waves in Saturn’s ring system, as well as the phenomenon of planetary migration. He interpreted double-nuclei galaxies, such as the nearby Andromeda galaxy, as eccentric stellar disks, and elucidated the role of dynamical friction in galaxy evolution.
Member, U.S. National Academy of Sciences, 2002.
Fellow, Royal Societies of London and Canada, 1994.
Steacie Prize, 1989.
Helen B. Warner Prize, American Astronomical Society, 1983.
Alfred P. Sloan Research Fellow, 1982-1986.
N. Lyskova et al, "Comparison of simple mass estimators for slowly rotating elliptical galaxies," Monthly Notices of the Royal Astronomical Society, vol. 450, no. 4, pp. 3442-3457, 2015.
S. Tremaine, "The Statistical Mechanics of Planet Orbits," The Astrophysical Journal, vol. 807, no. 2, article id. 157, pp. 11, 2015.
B. Kocsis, "A numerical study of vector resonant relaxation," Monthly Notices of the Royal Astronomical Society, Vol. 448, no. 4, pp.3265-3296, 2015
S. Tremaine, "Relativistic Redshifts in Quasar Broad Lines," The Astrophysical Journal, Vol. 794, no, 1, article id. 49, pp. 13, 2014.
J. Lissauer, "Advances in exoplanet science from Kepler," Nature, vol. 513, no. 7518, pp. 336-344, 2014
Advisory Committee Chair Cosmology & Gravity
Institute for Advanced StudySchool of Natural Sciences
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