Prebiotic reactions in a Mars analog iron mineral system: Effects of nitrate, nitrite, and ammonia on amino acid formation. (1st November 2022)
- Record Type:
- Journal Article
- Title:
- Prebiotic reactions in a Mars analog iron mineral system: Effects of nitrate, nitrite, and ammonia on amino acid formation. (1st November 2022)
- Main Title:
- Prebiotic reactions in a Mars analog iron mineral system: Effects of nitrate, nitrite, and ammonia on amino acid formation
- Authors:
- Barge, Laura M.
Flores, Erika
Weber, Jessica M.
Fraeman, Abigail A.
Yung, Yuk L.
VanderVelde, David
Martinez, Eduardo
Castonguay, Amalia
Billings, Keith
Baum, Marc M. - Abstract:
- Abstract: Iron minerals are highly reactive drivers of abiotic/prebiotic organic chemistry, and in the presence of ammonia (NH3 /NH4 + ) or other reduced nitrogen (N) compounds, have been shown to promote amino acid synthesis from organic precursors. On early Mars, oxidized nitrogen species (NOx − ) such as NO3 − and/or NO2 − may have been present, which could be reduced by Fe(II) to form various species including N2 O and/or NH3 /NH4 + . The production of NH3 /NH4 + from Fe(II)-driven NO3 − or NO2 − reduction may be able to feed into prebiotic organic reactions including amino acid formation. In this study, we tested whether iron mineral-driven reduction of NO3 − or NO2 − could provide a source of NH3 /NH4 + to form amino acids from two prebiotically relevant precursors (pyruvate and glyoxylate); or, whether an exogeneous source of NH3 /NH4 + would be required. We observed that pyruvate and glyoxylate reacted with Fe-oxyhydroxide minerals in NOx − -containing experiments to form reduced hydroxy acid products; and in experiments containing only NH3 /NH4 +, amino acids were also formed. However, significant amino acid formation was not observed in any experiments containing NO3 − or NO2 − unless sufficient NH4 + was also added; furthermore, colorimetric analysis did not show any generation of NH4 + from NO3 − /NO2 − reduction at these conditions. NO2 − was observed to be highly reactive with Fe 2+ and Fe(II)-bearing minerals, resulting in Fe oxidation during mineralAbstract: Iron minerals are highly reactive drivers of abiotic/prebiotic organic chemistry, and in the presence of ammonia (NH3 /NH4 + ) or other reduced nitrogen (N) compounds, have been shown to promote amino acid synthesis from organic precursors. On early Mars, oxidized nitrogen species (NOx − ) such as NO3 − and/or NO2 − may have been present, which could be reduced by Fe(II) to form various species including N2 O and/or NH3 /NH4 + . The production of NH3 /NH4 + from Fe(II)-driven NO3 − or NO2 − reduction may be able to feed into prebiotic organic reactions including amino acid formation. In this study, we tested whether iron mineral-driven reduction of NO3 − or NO2 − could provide a source of NH3 /NH4 + to form amino acids from two prebiotically relevant precursors (pyruvate and glyoxylate); or, whether an exogeneous source of NH3 /NH4 + would be required. We observed that pyruvate and glyoxylate reacted with Fe-oxyhydroxide minerals in NOx − -containing experiments to form reduced hydroxy acid products; and in experiments containing only NH3 /NH4 +, amino acids were also formed. However, significant amino acid formation was not observed in any experiments containing NO3 − or NO2 − unless sufficient NH4 + was also added; furthermore, colorimetric analysis did not show any generation of NH4 + from NO3 − /NO2 − reduction at these conditions. NO2 − was observed to be highly reactive with Fe 2+ and Fe(II)-bearing minerals, resulting in Fe oxidation during mineral precipitation and the formation of oxidized mineral phases (hematite). The Fe(II)/Fe(III) ratio in oxyhydroxide minerals is an important parameter for determining organic product distributions from pyruvate and glyoxylate; therefore, Fe-mediated NOx − reduction does impact organic chemistry. However, amino acid formation, at least under these conditions, would also require an exogenous source of NH3 /NH4 + or other reduced N species. These results have implications for organic-N chemistry on early Mars, as well as for some early Earth origin of life scenarios regarding organic synthesis in mineral-containing systems. … (more)
- Is Part Of:
- Geochimica et cosmochimica acta. Volume 336(2022)
- Journal:
- Geochimica et cosmochimica acta
- Issue:
- Volume 336(2022)
- Issue Display:
- Volume 336, Issue 2022 (2022)
- Year:
- 2022
- Volume:
- 336
- Issue:
- 2022
- Issue Sort Value:
- 2022-0336-2022-0000
- Page Start:
- 469
- Page End:
- 479
- Publication Date:
- 2022-11-01
- Subjects:
- Nitrate -- Iron hydroxides -- Astrobiology -- Prebiotic chemistry
Geochemistry -- Periodicals
Meteorites -- Periodicals
Géochimie -- Périodiques
Météorites -- Périodiques
Geochemie
Astrochemie
Electronic journals
551.905 - Journal URLs:
- http://www.sciencedirect.com/science/journal/00167037 ↗
http://catalog.hathitrust.org/api/volumes/oclc/1570626.html ↗
http://books.google.com/books?id=8IjzAAAAMAAJ ↗
http://books.google.com/books?id=mInzAAAAMAAJ ↗
http://www.elsevier.com/journals ↗ - DOI:
- 10.1016/j.gca.2022.08.038 ↗
- Languages:
- English
- ISSNs:
- 0016-7037
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 4117.000000
British Library DSC - BLDSS-3PM
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- 24120.xml