Lava Planet - Wikipedia

Terrestrial planet with the surface covered by molten lava

A lava planet is a type of terrestrial planet whose planetary surface is mostly or entirely covered by magma oceans or pools of erupted lava. Situations where such planets could exist include a young terrestrial planet just after its formation, a planet that has recently suffered a large crust-splitting impact event, or a planet orbiting very close to its star causing intense irradiation and tidal forces to melt its surface.[1]

Factors and characteristics

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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 the parent star may possibly have even more volcanic activity than Io, leading some astronomers to use the term super-Io.[2] These "super-Io" exoplanets may resemble Io with extensive sulfur concentrated on their surfaces that is associated with the continuous active volcanism.[3]

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 star-facing surface of a tidally locked planet could be left covered in a lava ocean while the nightside may have lava lakes, or even lava rain caused by the condensation of vaporized rock from the dayside. 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. Also, a Mega Earth may retain so much internal heat from its formation that a solid crust cannot form.

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 the Moon.

A 2020 preprint study finds that lava planets have low geometric albedos of around 0.1 and that molten lava on the surface can cool and harden to form quenched glass.[4]

Candidates

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There are no known lava worlds in the Solar System. But several known exoplanets are likely lava worlds, given their small enough masses, sizes, and orbits. Likely lava exoplanets include CoRoT-7b,[5] Kepler-10b,[6], K2-141b[7] and Kepler-78b.[8]

See also

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• Chthonian planet
• List of planet types
• Magma ocean

References

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1. ^ Henning, Wade G.; O'Connell, Richard J.; Sasselov, Dimitar D. (20 December 2009). "Tidally Heated Terrestrial Exoplanets: Viscoelastic Response Models". The Astrophysical Journal. 707 (2): 1000–1015. arXiv:0912.1907. Bibcode:2009ApJ...707.1000H. doi:10.1088/0004-637X/707/2/1000. S2CID 119286375.
2. ^ Barnes, Rory; Raymond, Sean N.; Greenberg, Richard; Jackson, Brian; Kaib, Nathan A. (1 February 2010). "CoRoT-7b: SUPER-EARTH OR SUPER-Io?". The Astrophysical Journal. 709 (2): L95 – L98. arXiv:0912.1337. Bibcode:2010ApJ...709L..95B. doi:10.1088/2041-8205/709/2/L95. S2CID 19867114.
3. ^ Battaglia, Steven M.; Castillo, Marco E.; Knudson, Christine A. (March 2014). "An investigation of extensive tidally heated super-earths (super-ios) using a sulfur solubility model of Gliese 876 d" (PDF). 45th Lunar and Planetary Science Conference.
4. ^ Essack, Zahra; Seager, Sara; Pajusalu, Mihkel (4 August 2020). "Low-albedo Surfaces of Lava Worlds". The Astrophysical Journal. 898 (2): 160. arXiv:2008.02789. Bibcode:2020ApJ...898..160E. doi:10.3847/1538-4357/ab9cba. S2CID 221006307.
5. ^ Ker Than (October 6, 2009). "Hellish Exoplanet Rains Hot Pebbles, Has Lava Oceans". National Geographic. Archived from the original on October 10, 2009.
6. ^ "Kepler-10b: world of lava oceans". Astronotes. January 11, 2011. Archived from the original on March 19, 2016. Retrieved July 14, 2013.
7. ^ Herath, Mahesh; Boukaré, Charles-Édouard; Cowan, Nicolas B. (October 29, 2024). "Thermal evolution of lava planets". Monthly Notices of the Royal Astronomical Society. 535 (3): 2404–2414. doi:10.1093/mnras/stae2431.
8. ^ Wall, Mike (20 August 2013). "On Strange Lava Planet and Iron World, 'Years' Take Only Hours". Space.com. Retrieved 19 September 2018.

Further reading

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• Lava Worlds: From Early Earth to Exoplanets, Keng-Hsien Chao, Rebecca deGraffenried, Mackenzie Lach, William Nelson, Kelly Truax, Eric Gaidos, 14 Dec 2020

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