Sara Seager
![Arxiv:1901.00443V2 [Astro-Ph.EP] 19 May 2020 Bolometric flare Energies Range from 1031.0 to 1036.9 Erg, with a Median of 1033.1 Erg](http://data.docslib.org/img/264x/56718eec4e3beb0be19c4a3ecfb038bb.webp)
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- OSIRIS-Rex Asteroid Sample Return Mission
- Submitted to Icarus on August 4, 2021 1 Organic Carbon Cycle In
- Sara Seager MIT
- SPITZER TRANSITS of the SUPER-EARTH Gj1214b and IMPLICATIONS for ITS ATMOSPHERE
- Package 'Extraterrestrial'
- Written in the Stars
- From Influence to Inhabitation: the Transformation of Astrobiology in the Early Modern Period
- Toward a List of Molecules As Potential Biosignature Gases for the Search for Life on Exoplanets and Applications to Terrestrial Biochemistry
- The Search for Habitable Planets with Biosignature Gases Framed by a ‘Biosignature Drake Equation’
- A Statistical Approach to Illustrate the Challenge of Astrobiology for Public Outreach
- The UV Environment for Prebiotic Chemistry: Connecting Origin-Of-Life Scenarios to Planetary Environments
- Statement of Professor Sara Seager Massachusetts Institute of Technology Before the Senate Committee on Commerce, Science, and T
- Astrobiology and JWST
- Exoplanetary Atmospheric Characterization Using Polarimetry and Other Radiative Transfer Modeling Problems
- JWST White Paper
- Marcheselli2019.Pdf (2.760Mb)
- Written in the Stars
- Professor Sara Seager Massachusetts Institute of Technology