HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: DEPENDENCE ON PLANETARY MASS
Ravi Kopparapu(Pennsylvania State University), Vincent Eymet(Université de Bordeaux), Ramses M. Ramírez(Pennsylvania State University), Shawn Domagal‐Goldman(National Aeronautics and Space Administration), J. C. Schottelkotte(Pennsylvania State University), James F. Kasting(Pennsylvania State University)
Cited by 663
Related Papers
HABITABLE ZONES AROUND MAIN-SEQUENCE STARS: NEW ESTIMATES
|The Astrophysical Journal|2013|1.6k
A Revised, Hazy Methane Greenhouse for the Archean Earth
|Astrobiology|2008|367
Exoplanet Biosignatures: Understanding Oxygen as a Biosignature in the Context of Its Environment
|Astrobiology|2018|324
A bistable organic-rich atmosphere on the Neoarchaean Earth
|Nature Geoscience|2012|241
Organic haze, glaciations and multiple sulfur isotopes in the Mid-Archean Era
|Earth and Planetary Science Letters|2008|206