Nitrogen Fixation at Early Mars

Danica Adams; Yangcheng Luo; Michael L Wong; Patrick Dunn; Madeline Christensen; Chuanfei Dong; Renyu Hu; Yuk Yung

doi:10.1089/ast.2020.2273

Nitrogen Fixation at Early Mars

Astrobiology. 2021 Aug;21(8):968-980. doi: 10.1089/ast.2020.2273. Epub 2021 Jul 30.

Authors

Danica Adams¹, Yangcheng Luo¹, Michael L Wong^{2

3}, Patrick Dunn⁴, Madeline Christensen^{1

5}, Chuanfei Dong⁶, Renyu Hu^{1

7}, Yuk Yung^{1

7}

Affiliations

¹ Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California, USA.
² Department of Astronomy and Astrobiology Program, University of Washington, Seattle, Washington, USA.
³ Virtual Planet Laboratory, University of Washington, Seattle, Washington, USA.
⁴ Space Sciences Laboratory, University of California, Berkeley, Berkeley, California, USA.
⁵ Bellarmine Preparatory, Tacoma, Washington, USA.
⁶ Department of Astrophysical Sciences, Princeton University, Princeton, California, USA.
⁷ Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California, USA.

PMID: 34339294
DOI: 10.1089/ast.2020.2273

Abstract

The Mars Science Laboratory (MSL) recently discovered nitrates in Gale Crater (e.g., Stern et al., 2015; Sutter et al., 2017). One possible mechanism for ancient nitrate deposition on Mars is through HNOx formation and rain out in the atmosphere, for which lightning-induced NO is likely the fundamental source. This study investigates nitrogen (N₂) fixation in early Mars' atmosphere, with implications for early Mars' habitability. We consider a 1 bar atmosphere of background CO₂, with abundance of N₂, hydrogen, and methane varied from 1% to 10% to explore a swath of potential early Mars climates. We derive lightning-induced thermochemical equilibrium fluxes of NO and HCN by coupling the lightning-rate parametrization from the study of Romps et al. (2014) with chemical equilibrium with applications, and we use a Geant4 simulation platform to estimate the effect of solar energetic particle events. These fluxes are used as input into KINETICS, the Caltech/JPL coupled photochemistry and transport code, which models the chemistry of 50 species linked by 495 reactions to derive rain-out fluxes of HNOx and HCN. We compute equilibrium concentrations of cyanide and nitrate in a putative northern ocean at early Mars, assuming hydrothermal vent circulation and photoreduction act as the dominant loss mechanisms. We find average oceanic concentrations of ∼0.1-2 nM nitrate and ∼0.01-2 mM cyanide. HCN is critical for protein synthesis at concentrations >0.01 M (e.g., Holm and Neubeck, 2009), and our result is astrobiologically significant if secondary local concentration mechanisms occurred. Nitrates may act as high-potential electron acceptors for early metabolisms, although the minimum concentration required is unknown. Our study derives concentrations that will be useful for future laboratory studies to investigate the habitability at early Mars. The aqueous nitrate concentrations correspond to surface nitrate precipitates of ∼1-8 × 10^-4 wt % that may have formed after the evaporation of surface waters, and these values roughly agree with recent MSL measurements.

Keywords: Astrobiology; Early Mars; Nitrate.; Nitrogen fixation.

Publication types

Research Support, U.S. Gov't, Non-P.H.S.

MeSH terms

Atmosphere
Extraterrestrial Environment
Mars*
Nitrates
Nitrogen Fixation*

Substances

Nitrates