Evolution from Ocean Planet to Land Planet by Water Loss; The Inner Edge of Habitable Zone
Abstract
We discuss the inner edge of Habitable Zone and imaginary planetary evolution from ocean planet to land planet by focus on water loss. When such evolution occur, planets keep habitable. We demonstrate the possibility of the various type of habitable planets.
- Publication:
-
42nd Annual Lunar and Planetary Science Conference
- Pub Date:
- March 2011
- Bibcode:
- 2011LPI....42.2132K