Modeling pN2 Through Geological Time: Implications for Planetary Climates and Atmospheric Biosignatures E.E. Stüeken1,2,3,4*, M.A. Kipp1,4, M.C. Koehler1,4, E.W. Schwieterman2,4,5, B. Johnson6, R. Buick1,4 1. Dept. of Earth & Space Sciences and Astrobiology Program, University of Washington, Seattle, WA 98195, USA 2. Dept. of Earth Sciences, University of California, Riverside, CA 92521, USA 3. Department of Earth & Environmental Sciences, University of St Andrews, St Andrews KY16 9AL, Scotland, UK 4. NASA Astrobiology Institute’s Virtual Planetary Laboratory, Seattle, WA 981195, USA 5. Dept. of Astronomy and Astrobiology Program, University of Washington, Seattle, WA 98195, USA 6. School of Earth & Ocean Sciences, University of Victoria, Victoria, BC V8P 5C2, Canada * corresponding author (
[email protected]) Astrobiology, Volume 16, Number 12, doi: 10.1089/ast.2016.1537 Abstract Nitrogen is a major nutrient for all life on Earth and could plausibly play a similar role in extraterrestrial biospheres. The major reservoir of nitrogen at Earth’s surface is atmospheric N2, but recent studies have proposed that the size of this reservoir may have fluctuated significantly over the course of Earth’s history with particularly low levels in the Neoarchean – presumably as a result of biological activity. We used a biogeochemical box model to test which conditions are necessary to cause large swings in atmospheric N2 pressure. Parameters for our model are constrained by observations of the modern Earth and reconstructions of biomass burial and oxidative weathering in deep time. A 1-D climate model was used to model potential effects on atmospheric climate.