Evolution from Ocean Planet to Land Planet by Water Loss; The Inner Edge of Habitable Zone

Details Evolution from Ocean Planet to Land Planet by Water Loss; The Inner Edge of Habitable Zone Evolution from Ocean Planet to Land Planet by Water Loss; The Inner Edge of Habitable Zone

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2132k&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2132

Physics

Scientific paper

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.

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