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Sökning: onr:"swepub:oai:DiVA.org:uu-487249" > The Long-Term Evolu...

LIBRIS Formathandbok  (Information om MARC21)
FältnamnIndikatorerMetadata
00005118naa a2200529 4500
001oai:DiVA.org:uu-487249
003SwePub
008221103s2022 | |||||||||||000 ||eng|
0247 a https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-4872492 URI
0247 a https://doi.org/10.1007/s11214-022-00924-02 DOI
040 a (SwePub)uu
041 a engb eng
042 9 SwePub
072 7a ref2 swepub-contenttype
072 7a for2 swepub-publicationtype
1001 a Gillmann, Cedricu Rice Univ, Dept Earth Environm & Planetary Sci, Houston, TX 77005 USA.4 aut
2451 0a The Long-Term Evolution of the Atmosphere of Venus :b Processes and Feedback Mechanisms Interior-Exterior Exchanges
264 c 2022-10-07
264 1b Springer,c 2022
338 a electronic2 rdacarrier
520 a This work reviews the long-term evolution of the atmosphere of Venus, and modulation of its composition by interior/exterior cycling. The formation and evolution of Venus's atmosphere, leading to contemporary surface conditions, remain hotly debated topics, and involve questions that tie into many disciplines. We explore these various inter-related mechanisms which shaped the evolution of the atmosphere, starting with the volatile sources and sinks. Going from the deep interior to the top of the atmosphere, we describe volcanic outgassing, surface-atmosphere interactions, and atmosphere escape. Furthermore, we address more complex aspects of the history of Venus, including the role of Late Accretion impacts, how magnetic field generation is tied into long-term evolution, and the implications of geochemical and geodynamical feedback cycles for atmospheric evolution. We highlight plausible end-member evolutionary pathways that Venus could have followed, from accretion to its present-day state, based on modeling and observations. In a first scenario, the planet was desiccated by atmospheric escape during the magma ocean phase. In a second scenario, Venus could have harbored surface liquid water for long periods of time, until its temperate climate was destabilized and it entered a runaway greenhouse phase. In a third scenario, Venus's inefficient outgassing could have kept water inside the planet, where hydrogen was trapped in the core and the mantle was oxidized. We discuss existing evidence and future observations/missions required to refine our understanding of the planet's history and of the complex feedback cycles between the interior, surface, and atmosphere that have been operating in the past, present or future of Venus.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a Venus
653 a Atmosphere
653 a Coupled evolution
653 a Feedback cycles
653 a Volatile exchanges
7001 a Way, Michael J.u Uppsala universitet,Teoretisk astrofysik,NASA, Goddard Inst Space Studies, 2880 Broadway, New York, NY 10025 USA4 aut0 (Swepub:uu)micwa958
7001 a Avice, Guillaumeu Univ Paris Cite, CNRS, Inst Phys Globe Paris, F-75005 Paris, France.4 aut
7001 a Breuer, Dorisu DLR, Inst Planetary Res, D-12489 Berlin, Germany.4 aut
7001 a Golabek, Gregor J.u Univ Bayreuth, Bayer Geoinst, D-95440 Bayreuth, Germany.4 aut
7001 a Hoening, Dennisu Potsdam Inst Climate Impact Res, Potsdam, Germany.;VU, Dept Earth Sci, Amsterdam, Netherlands.4 aut
7001 a Krissansen-Totton, Joshuau Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA.4 aut
7001 a Lammer, Helmutu Austrian Acad Sci, Space Res Inst, Graz, Austria.4 aut
7001 a O'Rourke, Joseph G.u Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA.4 aut
7001 a Persson, Moau Univ Paul Sabatier Toulouse III, CNRS, Inst Rech Astrophys & Planetol, Ctr Natl Etud Spatiales, Toulouse, France.4 aut
7001 a Plesa, Ana-Catalinau DLR, Inst Planetary Res, D-12489 Berlin, Germany.4 aut
7001 a Salvador, Arnaudu No Arizona Univ, Dept Astron & Planetary Sci, Box 6010, Flagstaff, AZ 86011 USA.;Univ Arizona, Habitabil Atmospheres & Biosignatures Lab, Tucson, AZ USA.;Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA.4 aut
7001 a Scherf, Manuelu Austrian Acad Sci, Space Res Inst, Graz, Austria.;Karl Franzens Univ Graz, Inst Phys, Graz, Austria.;Tech Univ, Inst Geodesy, Graz, Austria.4 aut
7001 a Zolotov, Mikhail Y.u Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ USA.4 aut
7102 a Rice Univ, Dept Earth Environm & Planetary Sci, Houston, TX 77005 USA.b Teoretisk astrofysik4 org
7730 t Space Science Reviewsd : Springerg 218:7q 218:7x 0038-6308x 1572-9672
8564 u https://doi.org/10.1007/s11214-022-00924-0y Fulltext
8564 u https://uu.diva-portal.org/smash/get/diva2:1708210/FULLTEXT01.pdfx primaryx Raw objecty fulltext:print
8564 8u https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-487249
8564 8u https://doi.org/10.1007/s11214-022-00924-0

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