TL;DR
This study assesses UV transmission in early Earth's natural waters, revealing that many waters were transparent to UV, but high-salinity and ferrous waters could significantly shield UV, impacting prebiotic chemistry scenarios.
Contribution
It combines laboratory and literature data to constrain UV transmission in early Earth's waters, highlighting the importance of Fe$^{2+}$ speciation and abundance for prebiotic chemistry.
Findings
Freshwaters were largely UV-transparent.
High-salinity waters may lack shortwave UV flux.
Ferrous waters can strongly shield UV, affecting prebiotic pathways.
Abstract
Ultraviolet (UV) light plays a key role in surficial theories of the origin of life, and numerous studies have focused on constraining the atmospheric transmission of UV radiation on early Earth. However, the UV transmission of the natural waters in which origins-of-life chemistry (prebiotic chemistry) is postulated to have occurred is poorly constrained. In this work, we combine laboratory and literature-derived absorption spectra of potential aqueous-phase prebiotic UV absorbers with literature estimates of their concentrations on early Earth to constrain the prebiotic UV environment in marine and terrestrial natural waters, and consider the implications for prebiotic chemistry. We find that prebiotic freshwaters were largely transparent in the UV, contrary to assumptions by some models of prebiotic chemistry. Some waters, e.g., high-salinity waters like carbonate lakes, may be…
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