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2020
DOI: 10.48550/arxiv.2012.07337
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Lava Worlds: From Early Earth to Exoplanets

Keng-Hsien Chao,
Rebecca deGraffenried,
Mackenzie Lach
et al.

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 understandi… Show more

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Cited by 3 publications
(4 citation statements)
references
References 370 publications
(486 reference statements)
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“…WASP-47 e, Kepler-78 b, Kepler-10 b, CoRot-7 b, and Kepler-36 b: These planets have been the focus of several theoretical studies that conjecture -in agreement with our analysisthat they should either have secondary atmospheres (and magma oceans) or/and low density interiors (e.g. Schaefer & Fegley 2009;Ito et al 2015;Dorn et al 2017b;Dai et al 2019;Chao et al 2020). Unfortunately, their host stars are much dimmer than 55 Cnc with V ∼ 11 to 12 mag (Léger et al 2009;Queloz et al 2009;Howard et al 2013;Becker et al 2015;Batalha et al 2011).…”
Section: Planet Candidates That Are Best Modeled With Secondary Atmos...supporting
confidence: 81%
“…WASP-47 e, Kepler-78 b, Kepler-10 b, CoRot-7 b, and Kepler-36 b: These planets have been the focus of several theoretical studies that conjecture -in agreement with our analysisthat they should either have secondary atmospheres (and magma oceans) or/and low density interiors (e.g. Schaefer & Fegley 2009;Ito et al 2015;Dorn et al 2017b;Dai et al 2019;Chao et al 2020). Unfortunately, their host stars are much dimmer than 55 Cnc with V ∼ 11 to 12 mag (Léger et al 2009;Queloz et al 2009;Howard et al 2013;Becker et al 2015;Batalha et al 2011).…”
Section: Planet Candidates That Are Best Modeled With Secondary Atmos...supporting
confidence: 81%
“…Thus, a mixture of these gases should be considered to study the thermal structure of planets with secondary atmospheres. Planets b and c in the TRAPPIST-1 system could present magma oceans due to their high surface temperatures (T ≥ 1300 K) (Barr et al 2018;Chao et al 2020), and the maximum surface pressure we have obtained here can be used to assess the current outgassing rate in magma ocean studies (Noack et al (2017), Baumeister et al submitted) and better constrain the WMF for the interior magma ocean models (e.g Katyal et al (2020)) in the future.…”
Section: Discussionmentioning
confidence: 75%
“…The integrated model should also include a description escape processes, such as hydrodynamic or Jeans escapes, which is particularly interesting to explore the lifetime of secondary atmospheres. Close-in, low-mass planets are likely to outgas atmospheric species, such as CO 2 , and form O 2 via photodissociation of outgased H 2 O, during their magma ocean stage or due to plate tectonics (Chao et al 2020). Thus, a mixture of these gases should be considered to study the thermal structure of planets with secondary atmospheres.…”
Section: Discussionmentioning
confidence: 99%
“…The youth of TOI-1807 b makes it an even more compelling target for secondary eclipse spectroscopy, as the luminosity of the planet's cooling core may be an order of magnitude higher than it would be at older (> 1 Gyr) ages (Linder et al 2019). Finally, as a candidate "lava world" (Chao et al 2020), TOI-1807 b presents an opportunity to study the early evolution of these poorly-understood objects.…”
Section: Discussionmentioning
confidence: 99%