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.
Lava planets would likely 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 to use the term super-Io. 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.
Habitability and life Edit
Any lifeforms on such a planet might have to be based on a very different form of biochemistry than life on Earth in order to thrive in extreme heat.
There are no lava worlds in the Solar System and the existence of extrasolar lava planets remains theoretical. Several known exoplanets are likely lava worlds, given their small enough masses, sizes and orbits. Likely lava exoplanets include COROT-7b, Kepler-10b, Alpha Centauri Bb, and Kepler-78b.
See also Edit
- ↑ Tidally Heated Terrestrial Exoplanets: Viscoelastic Response Models, Wade G. Henning, Richard J. O'Connell, Dimitar D. Sasselov, (Submitted on 10 Dec 2009)
- ↑ 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)
- ↑ Ker Than (October 6, 2009). Hellish Exoplanet Rains Hot Pebbles, Has Lava Oceans. National Geographic.
- ↑ Kepler-10b: world of lava oceans. Astronotes (January 11, 2011).
- ↑ New Planet Is Closest Yet: Earth-Size Lava World a Space "Landmark". Daily News. National Geographic (October 17, 2012).
- ↑ Ellie Zolfagharifard (August 20, 2013). The newly discovered lava-filled planet where years are just 8.5 HOURS long. Mail Online.