Sensitivity of Biomarkers to Changes in Chemical Emissions in the Earth's Proterozoic Atmosphere
John Lee Grenfell, Stefanie Gebauer, Philip von Paris, Mareike Godolt,, Pascal Hedelt, Beate Patzer, Barbara Stracke, Heike Rauer

TL;DR
This study investigates how biomarkers like ozone and nitrous oxide in Earth's Proterozoic atmosphere respond to changes in microbial emissions, revealing potential for these gases to serve as detectable signs of past life on exoplanets.
Contribution
It provides new insights into the stability of ozone and the significance of nitrous oxide as biomarkers in early Earth's atmosphere under varying microbial emission scenarios.
Findings
Ozone persists in Proterozoic atmospheres despite increased nitrous oxide emissions.
Nitrous oxide can become a prominent spectral biomarker under certain early Earth conditions.
Enhanced microbial emissions of nitrous oxide can lead to surface warming of 3.5K.
Abstract
The search for life beyond the Solar System is a major activity in exoplanet science. However, even if an Earth-like planet were to be found, it is unlikely to be at a similar stage of evolution as the modern Earth. It is therefore of interest to investigate the sensitivity of biomarker signals for life as we know it for an Earth-like planet but at earlier stages of evolution. Here, we assess biomarkers i.e. species almost exclusively associated with life, in present-day and in 10% present atmospheric level oxygen atmospheres corresponding to the Earth's Proterozoic period. We investigate the impact of proposed enhanced microbial emissions of the biomarker nitrous oxide, which photolyses to form nitrogen oxides which can destroy the biomarker ozone. A major result of our work is regardless of the microbial activity producing nitrous oxide in the early anoxic ocean, a certain minimum…
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