IDENTIFYING PLANETARY BIOSIGNATURE IMPOSTORS: SPECTRAL FEATURES OF CO AND O(4) RESULTING FROM ABIOTIC O(2)/O(3) PRODUCTION

O(2) and O(3) have been long considered the most robust individual biosignature gases in a planetary atmosphere, yet multiple mechanisms that may produce them in the absence of life have been described. However, these abiotic planetary mechanisms modify the environment in potentially identifiable wa...

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Gepubliceerd in:Astrophys J Lett
Hoofdauteurs: Schwieterman, Edward W., Meadows, Victoria S., Domagal-Goldman, Shawn D., Deming, Drake, Arney, Giada N., Luger, Rodrigo, Harman, Chester E., Misra, Amit, Barnes, Rory
Formaat: Artigo
Taal:Inglês
Gepubliceerd in: 2016
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Article
Online toegang:https://ncbi.nlm.nih.gov/pmc/articles/PMC6108182/
https://ncbi.nlm.nih.gov/pubmed/30147857
https://ncbi.nlm.nih.govhttp://dx.doi.org/10.3847/2041-8205/819/1/L13
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