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In search of the RNA world on Mars

Advances in origins of life research and prebiotic chemistry suggest that life as we know it may have emerged from an earlier RNA World. However, it has been difficult to reconcile the conditions used in laboratory experiments with real‐world geochemical environments that may have existed on the ear...

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Autores principales: Mojarro, Angel, Jin, Lin, Szostak, Jack W., Head, James W., Zuber, Maria T.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: John Wiley and Sons Inc. 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8248371/
https://www.ncbi.nlm.nih.gov/pubmed/33565260
http://dx.doi.org/10.1111/gbi.12433
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author Mojarro, Angel
Jin, Lin
Szostak, Jack W.
Head, James W.
Zuber, Maria T.
author_facet Mojarro, Angel
Jin, Lin
Szostak, Jack W.
Head, James W.
Zuber, Maria T.
author_sort Mojarro, Angel
collection PubMed
description Advances in origins of life research and prebiotic chemistry suggest that life as we know it may have emerged from an earlier RNA World. However, it has been difficult to reconcile the conditions used in laboratory experiments with real‐world geochemical environments that may have existed on the early Earth and hosted the origin(s) of life. This challenge is due to geologic resurfacing and recycling that have erased the overwhelming majority of the Earth's prebiotic history. We therefore propose that Mars, a planet frozen in time, comprised of many surfaces that have remained relatively unchanged since their formation > 4 Gya, is the best alternative to search for environments consistent with geochemical requirements imposed by the RNA world. In this study, we synthesize in situ and orbital observations of Mars and modeling of its early atmosphere into solutions containing a range of pHs and concentrations of prebiotically relevant metals (Fe(2+), Mg(2+), and Mn(2+)) spanning various candidate aqueous environments. We then experimentally determine RNA degradation kinetics due to metal‐catalyzed hydrolysis (cleavage) and evaluate whether early Mars could have been permissive toward the accumulation of long‐lived RNA polymers. Our results indicate that a Mg(2+)‐rich basalt sourcing metals to a slightly acidic (pH 5.4) environment mediates the slowest rates of RNA cleavage, though geologic evidence and basalt weathering models suggest aquifers on Mars would be near neutral (pH ~ 7). Moreover, the early onset of oxidizing conditions on Mars has major consequences regarding the availability of oxygen‐sensitive metals (i.e., Fe(2+) and Mn(2+)) due to increased RNA degradation rates and precipitation. Overall, (a) low pH decreases RNA cleavage at high metal concentrations; (b) acidic to neutral pH environments with Fe(2+) or Mn(2+) cleave more RNA than Mg(2+); and (c) alkaline environments with Mg(2+) dramatically cleaves more RNA while precipitates were observed for Fe(2+) and Mn(2+).
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spelling pubmed-82483712021-07-06 In search of the RNA world on Mars Mojarro, Angel Jin, Lin Szostak, Jack W. Head, James W. Zuber, Maria T. Geobiology Original Articles Advances in origins of life research and prebiotic chemistry suggest that life as we know it may have emerged from an earlier RNA World. However, it has been difficult to reconcile the conditions used in laboratory experiments with real‐world geochemical environments that may have existed on the early Earth and hosted the origin(s) of life. This challenge is due to geologic resurfacing and recycling that have erased the overwhelming majority of the Earth's prebiotic history. We therefore propose that Mars, a planet frozen in time, comprised of many surfaces that have remained relatively unchanged since their formation > 4 Gya, is the best alternative to search for environments consistent with geochemical requirements imposed by the RNA world. In this study, we synthesize in situ and orbital observations of Mars and modeling of its early atmosphere into solutions containing a range of pHs and concentrations of prebiotically relevant metals (Fe(2+), Mg(2+), and Mn(2+)) spanning various candidate aqueous environments. We then experimentally determine RNA degradation kinetics due to metal‐catalyzed hydrolysis (cleavage) and evaluate whether early Mars could have been permissive toward the accumulation of long‐lived RNA polymers. Our results indicate that a Mg(2+)‐rich basalt sourcing metals to a slightly acidic (pH 5.4) environment mediates the slowest rates of RNA cleavage, though geologic evidence and basalt weathering models suggest aquifers on Mars would be near neutral (pH ~ 7). Moreover, the early onset of oxidizing conditions on Mars has major consequences regarding the availability of oxygen‐sensitive metals (i.e., Fe(2+) and Mn(2+)) due to increased RNA degradation rates and precipitation. Overall, (a) low pH decreases RNA cleavage at high metal concentrations; (b) acidic to neutral pH environments with Fe(2+) or Mn(2+) cleave more RNA than Mg(2+); and (c) alkaline environments with Mg(2+) dramatically cleaves more RNA while precipitates were observed for Fe(2+) and Mn(2+). John Wiley and Sons Inc. 2021-02-10 2021-05 /pmc/articles/PMC8248371/ /pubmed/33565260 http://dx.doi.org/10.1111/gbi.12433 Text en © 2021 The Authors. Geobiology published by John Wiley & Sons Ltd. https://creativecommons.org/licenses/by/4.0/This is an open access article under the terms of the http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
spellingShingle Original Articles
Mojarro, Angel
Jin, Lin
Szostak, Jack W.
Head, James W.
Zuber, Maria T.
In search of the RNA world on Mars
title In search of the RNA world on Mars
title_full In search of the RNA world on Mars
title_fullStr In search of the RNA world on Mars
title_full_unstemmed In search of the RNA world on Mars
title_short In search of the RNA world on Mars
title_sort in search of the rna world on mars
topic Original Articles
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8248371/
https://www.ncbi.nlm.nih.gov/pubmed/33565260
http://dx.doi.org/10.1111/gbi.12433
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