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  3. Possible Chemical Composition And Interior Structure Models Of Venus Inferred From Numerical Modelling
 

Possible Chemical Composition And Interior Structure Models Of Venus Inferred From Numerical Modelling

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BORIS DOI
10.48350/177651
Publisher DOI
10.3847/1538-4357/ac410d
Date of Publication
2022
Publication Type
Article
Subject(s)
500 Science > 550 Earth sciences & geology
500 Science > 520 Astronomy
600 Technology > 620 Engineering
500 Science > 530 Physics
Language(s)
en
Contributor(s)
Shah, Oliver Raymond Ferdinand
Physikalisches Institut - Space Research and Planetology Physics
Helled, Ravit
Alibert, Yannorcid-logo
Space Research and Planetology Physics - Planetary Formation
Physikalisches Institut der Universität Bern
Mezger, Klausorcid-logo
Institute of Geological Sciences (GEO) - Isotope Geology Group
Institute of Geological Sciences (GEO)
Additional Credits
Physikalisches Institut - Space Research and Planetology Physics
Space Research and Planetology Physics - Planetary Formation
Institute of Geological Sciences (GEO) - Isotope Geology Group
Series
Astrophysical journal
Publisher
Institute of Physics Publishing IOP
ISSN
0004-637X
Access(Rights)
open.access
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