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Warm, Water-depleted Rocky Exoplanets With Surface Ionic Liquids: A Proposed Class For Planetary Habitability
astrobiology.com
The discovery of thousands of exoplanets and the emergence of telescopes capable of exoplanet atmospheric characterization have intensified the search for habitable worlds.
Due to selection biases, many exoplanets under study are planets deemed inhospitable because their surfaces are too warm to support liquid water. We propose that such planets could still support life through ionic liquids: Liquid salts with negligible vapor pressure that can persist on warm planets with thin atmospheres, where liquid water cannot. Ionic liquids have not previously been considered as naturally occurring substances, and thus have not been discussed in planetary science.
Warm, Water-depleted Rocky Exoplanets With Surface Ionic Liquids: A Proposed Class For Planetary Habitability - Astrobiology
The discovery of thousands of exoplanets and the emergence of telescopes capable