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DOI10.1073/pnas.2006177117
Exoplanet secondary atmosphere loss and revival
Kite E.S.; Barnett M.N.
发表日期2020
ISSN0027-8424
起始页码18264
结束页码18271
卷号117期号:31
英文摘要The next step on the path toward another Earth is to find atmospheres similar to those of Earth and Venus-high-molecularweight (secondary) atmospheres-on rocky exoplanets. Many rocky exoplanets are born with thick (>10 kbar) H2-dominated atmospheres but subsequently lose their H2; this process has no known Solar System analog. We study the consequences of early loss of a thick H2 atmosphere for subsequent occurrence of a high-molecularweight atmosphere using a simple model of atmosphere evolution (including atmosphere loss to space, magma ocean crystallization, and volcanic outgassing). We also calculate atmosphere survival for rocky worlds that start with no H2. Our results imply that most rocky exoplanets orbiting closer to their star than the habitable zone that were formed with thick H2-dominated atmospheres lack high-molecularweight atmospheres today. During early magma ocean crystallization, high-molecular-weight species usually do not form long-lived high-molecular-weight atmospheres; instead, they are lost to space alongside H2. This early volatile depletion also makes it more difficult for later volcanic outgassing to revive the atmosphere. However, atmospheres should persist on worlds that start with abundant volatiles (for example, water worlds). Our results imply that in order to find high-molecular-weight atmospheres on warm exoplanets orbiting M-stars, we should target worlds that formed H2-poor, that have anomalously large radii, or that orbit less active stars. © 2020 National Academy of Sciences. All rights reserved.
英文关键词Atmospheric evolution; Exoplanets; Planetary science
语种英语
scopus关键词Article; astronomy; atmosphere; crystallization; mathematical model; molecular weight; priority journal; volcano
来源期刊Proceedings of the National Academy of Sciences of the United States of America
文献类型期刊论文
条目标识符http://gcip.llas.ac.cn/handle/2XKMVOVA/160858
作者单位Kite, E.S., Department of Geophysical Sciences, University of Chicago, Chicago, IL 60637, United States; Barnett, M.N., Department of Geophysical Sciences, University of Chicago, Chicago, IL 60637, United States
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Kite E.S.,Barnett M.N.. Exoplanet secondary atmosphere loss and revival[J],2020,117(31).
APA Kite E.S.,&Barnett M.N..(2020).Exoplanet secondary atmosphere loss and revival.Proceedings of the National Academy of Sciences of the United States of America,117(31).
MLA Kite E.S.,et al."Exoplanet secondary atmosphere loss and revival".Proceedings of the National Academy of Sciences of the United States of America 117.31(2020).
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