Nitrogen fixation on early Mars by volcanic lightning and other sources

41Citations
Citations of this article
58Readers
Mendeley users who have this article in their library.

This article is free to access.

Abstract

Here, we estimate the amount of reactive nitrogen available for the origin and maintenance of life on early Mars. Lightning formed in explosive volcanic clouds is proposed as a source of nitrogen fixation. Volcanic lightning was simulated in the laboratory using a laser induced plasma. We derived the chemical composition of the gas mixture from an accretion model of Mars and the nitrogen content of Martian meteorites. The mixture contained CH4, H2, H2O and N2 in variable amounts to represent the range of C/N ratio measured in the Martian meteorites. For comparison, other endogenous and exogenous sources of fixed nitrogen in early Mars were calculated. Our experimental simulations indicate that volcanic lightning may be the only endogenous source of hydrogen cyanide (HCN) forming about 107 kg yr-1 of this compound. The total budget of fixed nitrogen for early Mars would be ∼10 kg yr-1 km-2, similar to that calculated for early Earth. Copyright 2005 by the American Geophysical Union.

Cite

CITATION STYLE

APA

Segura, A., & Navarro-González, R. (2005). Nitrogen fixation on early Mars by volcanic lightning and other sources. Geophysical Research Letters, 32(5), 1–4. https://doi.org/10.1029/2004GL021910

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free