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Lava planet
A lava planet is a hypothetical type of terrestrial planet, with a surface mostly or entirely covered by molten lava. Situations where such planets could exist include a young terrestrial planet just after its formation, a planet that has recently suffered a large collision event, or a planet orbiting very close to its star, causing intense irradiation and tidal forces.〔(Tidally Heated Terrestrial Exoplanets: Viscoelastic Response Models ), Wade G. Henning, Richard J. O'Connell, Dimitar D. Sasselov, (Submitted on 10 Dec 2009)〕
== Factors ==
Lava planets would probably orbit extremely close to their parent star. In planets with eccentric orbits, the gravity from the nearby star would distort the planet periodically, with the resulting friction producing internal heat. This tidal heating could melt rocks into magma, which would then erupt through volcanoes. This would be similar to the solar system moon Io, orbiting close to its parent Jupiter. Io is the most geologically active world in the solar system, with hundreds of volcanic centres and extensive lava flows. Lava worlds orbiting extremely closely to their parent star may possibly have even more volcanic activity than Io, leading some astronomers to use the term ''super-Io''.〔(CoRoT-7 b: Super-Earth or Super-Io? ), Rory Barnes, Sean N. Raymond, Richard Greenberg, Brian Jackson, Nathan A. Kaib, (Submitted on 7 Dec 2009)〕 These "super-Io" exoplanets may resemble Io with extensive sulfur concentrated on their surfaces that is associated with the continuous active volcanism.
However, tidal heating is not the only factor shaping a lava planet. In addition to tidal heating from orbiting close to their parent star, the intense stellar irradiation could melt the surface crust directly into lava. The entire illuminated surface of a tidally locked planet could be left covered in lava oceans while the dark side may have lava lakes, or even rock rain caused by the condensation of vaporized rock from the hotter side. The mass of the planet would also be a factor. The appearance of plate tectonics on terrestrial planets is related to planetary mass, with more massive planets than Earth expected to exhibit plate tectonics and thus more intense volcanic activity.
Protoplanets tend to have intense volcanic activity resulting from large amounts of internal heating just after formation, even relatively small planets that orbit far from their parent stars. Lava planets can also result from giant impacts; Earth was briefly a lava planet after being impacted by a Mars-sized body which formed our Moon.
抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』
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