Lava Worlds: From Early Earth to Exoplanets
TL;DR: In this paper, the authors provide an overview of evidence for magma oceans throughout the Solar System and consider the factors that control the rocks these oceans leave behind, and summarizes efforts to detect and characterize them, as well as the needs and gaps in our knowledge and points to future opportunities with new planetary missions and space telescopes to identify and better characterize lava worlds around nearby stars.
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Abstract: The magma ocean concept was first conceived to explain the geology of the Moon, but hemispherical or global oceans of silicate melt could be a widespread "lava world" phase of rocky planet accretion, and could persist on planets on short-period orbits around other stars. The formation and crystallization of magma oceans could be a defining stage in the assembly of a core, origin of a crust, initiation of tectonics, and formation of an atmosphere. The last decade has seen significant advances in our understanding of this phenomenon through analysis of terrestrial and extraterrestrial samples, planetary missions, and astronomical observations of exoplanets. This review describes the energetic basis of magma oceans and lava worlds and the lava lake analogs available for study on Earth and Io. It provides an overview of evidence for magma oceans throughout the Solar System and considers the factors that control the rocks these magma oceans leave behind. It describes research on theoretical and observed exoplanets that could host extant magma oceans and summarizes efforts to detect and characterize them. It reviews modeling of the evolution of magma oceans as a result of crystallization and evaporation, the interaction with the underlying solid mantle, and the effects of planetary rotation. The review also considers theoretical investigations on the formation of an atmosphere in concert with the magma ocean and in response to irradiation from the host star, and possible end-states. Finally, it describes needs and gaps in our knowledge and points to future opportunities with new planetary missions and space telescopes to identify and better characterize lava worlds around nearby stars.
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Citations
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Redox hysteresis of super-Earth exoplanets from magma ocean circulation
TL;DR: In this article, scaling analysis indicates that turbulent diffusion in the internal magma oceans of sub-Neptunes can kinetically entrain liquid iron droplets and quench core formation.
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Radioactive Planet Formation
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References
Crystallization and cooling conditions for diogenite formation in the turbulent magma ocean of asteroid 4 Vesta
TL;DR: In this paper, a new differentiation model for crust formation has been developed by taking magma ocean fluid dynamics, chemical equilibrium, the presence of 26Al, and cooling into consideration with a special focus on crystal separation.
6
Venus: A Thick Basal Magma Ocean May Exist Today
Joseph O'Rourke
- 06 Jan 2020
TL;DR: Basal magma oceans develop in Earth and Venus after accretion as their mantles solidify from the middle outwards, and fractional crystallization of the basal mantle is buffered by the core and radiogen as mentioned in this paper.
6
Russian Lunar Landers Luna-25 and Lna-27: goals of the missions and scientific investigations at Moon Polar Regions
Vladislav Tretyakov,Igor Mitrofanov,Lev Zeleniy +2 more
- 09 Mar 2020
TL;DR: In this article, the main and spare landing sites for Russian Landers with Luna-25 and Luna-27 were selected on the base both of engineering suitability (flatness and roughness of surface, radio visibility, solar irradiation and so on) and scientific motivation.
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•Posted Content
Astro2020 Science White Paper: Toward Finding Earth 2.0: Masses and Orbits of Small Planets with Extreme Radial Velocity Precision
David R. Ciardi,Jacob L. Bean,Jennifer Burt,Diana Dragomir,Eric Gaidos,Marshall C. Johnson,Eliza M.-R. Kempton,Quinn Konopacky,Michael Meyer,Johanna Teske,Lauren M. Weiss,George Zhou +11 more
TL;DR: In this paper, the mass and orbit information of the Earth-like planets were determined using the radial velocities of the radii and the masses of the planets, respectively.
Does Io Have a Magma Ocean
TL;DR: In this article, future space missions will further our knowledge of tidal heating and orbital resonances, processes thought to create spectacular volcanism and oceans of magma or water on other worlds.
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