ramses2.jpgI am a research scientist at the Earth-Life Science Institute that studies potentially habitable worlds. I develop climate models that are used to determine which exoplanets are located within the habitable zone, which is the circular region around a star in which water could exist on the surface of a planet. I also study the habitability of worlds within our solar system to better understand extrasolar planet habitability.


The moist greenhouse is sensitive to stratospheric temperature
A warmer and wetter solution for early Mars and the challenges with transient warming
A volcanic hydrogen habitable zone

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