Stability of 20 Biogenic Amino Acids in Concentrated Sulfuric Acid: Implications for the Habitability of Venus' Clouds
arXiv:2401.01441 · doi:10.1089/ast.2023.0082
Abstract
Scientists have long speculated about the potential habitability of Venus, not at the 700K surface, but in the cloud layers located at 48-60 km altitudes, where temperatures match those found on Earth's surface. However, the prevailing belief has been that Venus' clouds cannot support life due to the cloud chemical composition of concentrated sulfuric acid-a highly aggressive solvent. In this work, we study 20 biogenic amino acids at the range of Venus' cloud sulfuric acid concentrations (81% and 98% w/w, the rest water) and temperatures. We find 19 of the biogenic amino acids we tested are either unreactive (13 in 98% w/w and 12 in 81% w/w) or chemically modified in the side chain only, after four weeks. Our major finding, therefore, is that the amino acid backbone remains intact in concentrated sulfuric acid. These findings significantly broaden the range of biologically relevant molecules that could be components of a biochemistry based on a concentrated sulfuric acid solvent.
Published in Astrobiology (in press); v2 has corrected Figure 4
References in corpus (6)
- Was Venus the First Habitable World of our Solar System?
- Day-night cloud asymmetry prevents early oceans on Venus but not on Earth
- Production of Ammonia Makes Venusian Clouds Habitable and Explains Observed Cloud-Level Chemical Anomalies
- Rocket Lab Mission to Venus
- Venus Life Finder Missions Motivation and Summary
- Venus' Atmospheric Chemistry and Cloud Characteristics Are Compatible with Venusian Life