Nitrogen Oxide Concentrations in Natural Waters on Early Earth

A key challenge in origins-of-life studies is estimating the abundances of species relevant to the chemical pathways proposed to have contributed to the emergence of life on early Earth. Dissolved nitrogen oxide anions (NO-[subscript x]), in particular nitrate (NO-[subscript 3]) and nitrite (NO-[sub...

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Main Authors: Ranjan, Sukrit, Todd, Zoe R., Rimmer, Paul R., Sasselov, Dimitar D., Babbin, Andrew R.
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:English
Published: American Geophysical Union (AGU) 2020
Online Access:https://hdl.handle.net/1721.1/124622
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author Ranjan, Sukrit
Todd, Zoe R.
Rimmer, Paul R.
Sasselov, Dimitar D.
Babbin, Andrew R.
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Ranjan, Sukrit
Todd, Zoe R.
Rimmer, Paul R.
Sasselov, Dimitar D.
Babbin, Andrew R.
author_sort Ranjan, Sukrit
collection MIT
description A key challenge in origins-of-life studies is estimating the abundances of species relevant to the chemical pathways proposed to have contributed to the emergence of life on early Earth. Dissolved nitrogen oxide anions (NO-[subscript x]), in particular nitrate (NO-[subscript 3]) and nitrite (NO-[subscript 2]), have been invoked in diverse origins-of-life chemistry, from the oligomerization of RNA to the emergence of protometabolism. Recent work has calculated the supply of NO-[subscript x] from the prebiotic atmosphere to the ocean and reported steady state [NO-[subscript x] to be high across all plausible parameter space. These findings rest on the assumption that NO-[subscript x] is stable in natural waters unless processed at a hydrothermal vent. Here, we show that NO-[subscript x] is unstable in the reducing environment of early Earth. Sinks due to ultraviolet photolysis and reactions with reduced iron (Fe[superscript 2+]) suppress [NO-[subscript x]] by several orders of magnitude relative to past predictions. For pH = 6.5–8 and T = 0–50 °C, we find that it is most probable that [NO-[subscript x]] <1μM in the prebiotic ocean. On the other hand, prebiotic ponds with favorable drainage characteristics may have sustained [NO-[subscript x]] ≥1μM. As on modern Earth, most NO-[subscript x] on prebiotic Earth should have been present as NO-[subscript 3], due to its much greater stability. These findings inform the kind of prebiotic chemistries that would have been possible on early Earth. We discuss the implications for proposed prebiotic chemistries and highlight the need for further studies of NO-[subscript x] kinetics to reduce the considerable uncertainties in predicting [NO-[subscript x]] on early Earth.
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spelling mit-1721.1/1246222022-09-29T16:35:37Z Nitrogen Oxide Concentrations in Natural Waters on Early Earth Ranjan, Sukrit Todd, Zoe R. Rimmer, Paul R. Sasselov, Dimitar D. Babbin, Andrew R. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences A key challenge in origins-of-life studies is estimating the abundances of species relevant to the chemical pathways proposed to have contributed to the emergence of life on early Earth. Dissolved nitrogen oxide anions (NO-[subscript x]), in particular nitrate (NO-[subscript 3]) and nitrite (NO-[subscript 2]), have been invoked in diverse origins-of-life chemistry, from the oligomerization of RNA to the emergence of protometabolism. Recent work has calculated the supply of NO-[subscript x] from the prebiotic atmosphere to the ocean and reported steady state [NO-[subscript x] to be high across all plausible parameter space. These findings rest on the assumption that NO-[subscript x] is stable in natural waters unless processed at a hydrothermal vent. Here, we show that NO-[subscript x] is unstable in the reducing environment of early Earth. Sinks due to ultraviolet photolysis and reactions with reduced iron (Fe[superscript 2+]) suppress [NO-[subscript x]] by several orders of magnitude relative to past predictions. For pH = 6.5–8 and T = 0–50 °C, we find that it is most probable that [NO-[subscript x]] <1μM in the prebiotic ocean. On the other hand, prebiotic ponds with favorable drainage characteristics may have sustained [NO-[subscript x]] ≥1μM. As on modern Earth, most NO-[subscript x] on prebiotic Earth should have been present as NO-[subscript 3], due to its much greater stability. These findings inform the kind of prebiotic chemistries that would have been possible on early Earth. We discuss the implications for proposed prebiotic chemistries and highlight the need for further studies of NO-[subscript x] kinetics to reduce the considerable uncertainties in predicting [NO-[subscript x]] on early Earth. Simons Foundation (SCOL Grant 495062) 2020-04-14T15:33:15Z 2020-04-14T15:33:15Z 2019-04 2018-11 2020-04-03T18:36:32Z Article http://purl.org/eprint/type/JournalArticle 1525-2027 https://hdl.handle.net/1721.1/124622 Ranjan, Sukrit, et al. “Nitrogen Oxide Concentrations in Natural Waters on Early Earth.” Geochemistry, Geophysics, Geosystems 20, 4 (April 2019): 2021–39. © 2019 The Authors en http://dx.doi.org/10.1029/2018GC008082 Geochemistry, Geophysics, Geosystems Creative Commons Attribution-NonCommercial-NoDerivs License http://creativecommons.org/licenses/by-nc-nd/4.0/ application/pdf American Geophysical Union (AGU) American Geophysical Union (AGU)
spellingShingle Ranjan, Sukrit
Todd, Zoe R.
Rimmer, Paul R.
Sasselov, Dimitar D.
Babbin, Andrew R.
Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title_full Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title_fullStr Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title_full_unstemmed Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title_short Nitrogen Oxide Concentrations in Natural Waters on Early Earth
title_sort nitrogen oxide concentrations in natural waters on early earth
url https://hdl.handle.net/1721.1/124622
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