Stability of nucleic acid bases in concentrated sulfuric acid: Implications for the habitability of Venus' clouds
Sara Seager, Janusz J. Petkowski, Maxwell D. Seager, John H. Grimes, Jr., Zachary Zinsli, Heidi R. Vollmer-Snarr, Mohamed K. Abd El-Rahman, David, S. Wishart, Brian L. Lee, Vasuk Gautam, Lauren Herrington, William Bains,, Charles Darrow

TL;DR
This study demonstrates that nucleic acid bases remain stable in concentrated sulfuric acid under Venus-like conditions, suggesting potential for life-supporting chemistry in Venus' clouds despite harsh surface conditions.
Contribution
It is the first to show nucleic acid bases are stable in concentrated sulfuric acid at Venus-like temperatures, expanding possibilities for extraterrestrial biochemistry.
Findings
Nucleic acid bases are stable in sulfuric acid at Venus cloud conditions.
UV and NMR spectroscopy confirm molecular stability.
Supports potential for life-supporting chemistry in Venus' clouds.
Abstract
What constitutes a habitable planet is a frontier to be explored and requires pushing the boundaries of our terracentric viewpoint for what we deem to be a habitable environment. Despite Venus' 700 K surface temperature being too hot for any plausible solvent and most organic covalent chemistry, Venus' cloud-filled atmosphere layers at 48 to 60 km above the surface hold the main requirements for life: suitable temperatures for covalent bonds; an energy source (sunlight); and a liquid solvent. Yet, the Venus clouds are widely thought to be incapable of supporting life because the droplets are composed of concentrated liquid sulfuric acid-an aggressive solvent that is assumed to rapidly destroy most biochemicals of life on Earth. Recent work, however, demonstrates that a rich organic chemistry can evolve from simple precursor molecules seeded into concentrated sulfuric acid, a result that…
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