title: Exoplanet habitability.
abstract: The search for exoplanets includes the promise to eventually find and identify habitable worlds. The thousands of known exoplanets and planet candidates are extremely diverse in terms of their masses or sizes, orbits, and host star type. The diversity extends to new kinds of planets, which are very common yet have no solar system counterparts. Even with the requirement that a planet's surface temperature must be compatible with liquid water (because all life on Earth requires liquid water), a new emerging view is that planets very different from Earth may have the right conditions for life. The broadened possibilities will increase the future chances of discovering an inhabited world.
authors: Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. seager@mit.edu
authors: Sara
authors: S
authors: Seager
mesh_terms: D002245:Carbon Dioxide; D018534:Earth, Planet; D018559:Exobiology; D005118:Extraterrestrial Environment; D005740:Gases; D017752:Greenhouse Effect; D016083:Planets; D055609:Stars, Celestial; D013696:Temperature; D014867:Water
chemical_list: D005740:Gases; D014867:Water; D002245:Carbon Dioxide