Prof. Sara Seager

Class of 1941 Professor of Physics and Planetary Science

Primary DLC

Department of Earth, Atmospheric, and Planetary Sciences

MIT Room: 54-1718

Assistant

Kayla Bauer
kbauer@mit.edu

Areas of Interest and Expertise

Astrophysics
Space Travel
Atomospheres and Interiors of Exoplants
Exoplanet Atmospheres and Interiors.
Transiting Planets
Atmospheric Thermal Emission

Research Summary

Professor Seager’s current research interests are focused upon exoplanet atmospheres and interiors. Over 450 exoplanets are known to orbit nearby stars. Now that their existence is firmly established, a new era of exoplanet characterization has begun. A subset of exoplanets, called transiting planets, pass in front of and behind their stars, as seen from Earth. Transiting planets have immeasurably changed the field of exoplanets because their physical properties, including average density and atmospheric thermal emission, can be now be routinely measured. Seager’s group aims to understand the atmospheric composition and the interior structure of exoplanets, with a focus on the new and growing data set of transiting exoplanets.

Recent Work

  • Video

    Sara Seager - RD2017

    November 22, 2017Conference Video Duration: 35:41

    Mapping the Nearest Stars for Habitable Worlds

    Thousands of exoplanets are known to orbit nearby stars and small rocky planets are established to be common. The ambitious goal of identifying a habitable or inhabited world is within reach. But how likely are we to succeed? The race to find habitable exoplanets has accelerated with the realization that “big Earths” transiting small stars can be both discovered and characterized with current technology. While future generations may use very large space-based telescopes to search to find signs of life amidst a yet unknown range of planetary environments, what will it take to identify such habitable worlds with the observations and theoretical tools available to us?

    2017 MIT Research and Development Conference