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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References
Onset of magma ocean solidification on Mars inferred from Mn-Cr chronometry
TL;DR: In this article, the authors applied the short-lived 53Mn-53Cr system to martian meteorites in order to date the onset of large-scale mantle differentiation on Mars.
28
Formation of the lunar crust - An electrical source of heating
TL;DR: In this article, a model for the formation of the lunar crust based on heating by electrical induction is explored, while adherence is maintained to certain constraints associated with existing models of the solar system.
27
A Rapidly Convecting Lava Lake at Masaya Volcano, Nicaragua
Tom D. Pering,Tehnuka Ilanko,Thomas C. Wilkes,Rebecca Anne England,Siân R. Silcock,Leigh Russell Stanger,Jon R. Willmott,Robert G. Bryant,Andrew J. S. McGonigle,Andrew J. S. McGonigle +9 more
TL;DR: In this paper, the authors report on the dynamics of a rapidly convecting lava lake, which, to the best of their knowledge, manifested the highest lava flow velocities ever reported for a lava lake: 13.7-16.4 m s−1, in addition to unusual fluid dynamic behavior involving alteration in surface flow direction.
Implications for the origins of pure anorthosites found in the feldspathic lunar meteorites, Dhofar 489 group
Hiroshi Nagaoka,Hiroshi Takeda,Yuzuru Karouji,Makiko Ohtake,Akira Yamaguchi,Akira Yamaguchi,Shigekazu Yoneda,Nobuyuki Hasebe +7 more
TL;DR: A comparison with Apollo nearside samples of ferroan anorthosite (FAN) indicated that of the FAN samples returned by the Apollo missions, sample 60015 is the largest anorthosite with the highest plagioclase abundance and homogeneous mafic mineral compositions.
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