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- W3138045009 abstract "The possible detection of the biomarker of phosphine as reported by Greaves et al. in the Venusian atmosphere stirred much excitement in the astrobiology community. While many in the community are adamant that the environmental conditions in the Venusian atmosphere are too extreme for life to exist, others point to the claimed detection of a convincing biomarker, the conjecture that early Venus was doubtlessly habitable, and any Venusian life might have adapted by natural selection to the harsh conditions in the Venusian clouds after the surface became uninhabitable. Here, I first briefly characterize the environmental conditions in the lower Venusian atmosphere and outline what challenges a biosphere would face to thrive there, and how some of these obstacles for life could possibly have been overcome. Then, I discuss the significance of the possible detection of phosphine and what it means (and does not mean) and provide an assessment on whether life may exist in the temperate cloud layer of the Venusian atmosphere or not." @default.
- W3138045009 created "2021-03-29" @default.
- W3138045009 creator A5034285589 @default.
- W3138045009 date "2021-03-20" @default.
- W3138045009 modified "2023-10-01" @default.
- W3138045009 title "The Case (or Not) for Life in the Venusian Clouds" @default.
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- W3138045009 doi "https://doi.org/10.3390/life11030255" @default.
- W3138045009 hasPubMedCentralId "https://www.ncbi.nlm.nih.gov/pmc/articles/8003671" @default.
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