Proposed energy-metabolisms cannot explain the atmospheric chemistry of Venus.
Journal
Nature communications
ISSN: 2041-1723
Titre abrégé: Nat Commun
Pays: England
ID NLM: 101528555
Informations de publication
Date de publication:
14 06 2022
14 06 2022
Historique:
received:
21
12
2021
accepted:
18
05
2022
entrez:
14
6
2022
pubmed:
15
6
2022
medline:
18
6
2022
Statut:
epublish
Résumé
Life in the clouds of Venus, if present in sufficiently high abundance, must be affecting the atmospheric chemistry. It has been proposed that abundant Venusian life could obtain energy from its environment using three possible sulfur energy-metabolisms. These metabolisms raise the possibility of Venus's enigmatic cloud-layer SO
Identifiants
pubmed: 35701394
doi: 10.1038/s41467-022-30804-8
pii: 10.1038/s41467-022-30804-8
pmc: PMC9198073
doi:
Substances chimiques
Sulfur
70FD1KFU70
Types de publication
Journal Article
Research Support, Non-U.S. Gov't
Langues
eng
Sous-ensembles de citation
IM
Pagination
3274Informations de copyright
© 2022. The Author(s).
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