Abiotic Nitrous Oxide Production From Sediments and Brine of Don Juan Pond, Wright Valley Antarctica, at Mars Analog Temperatures (−40°C)
The presence of biogenic gases such as oxygen, methane, and nitrous oxide (N2O) in the atmospheres of extraterrestrial bodies has been postulated as a biosignature of life. Abiotic N2O production was documented recently in Don Juan Pond (DJP), Antarctica, a cold, hypersaline Mars analog environment....
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Veröffentlicht in: | Geophysical research letters 2022-02, Vol.49 (3), p.n/a |
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creator | Schutte, Charles A. Samarkin, Vladimir A. Bowles, Marshall W. Peters, Brian Casciotti, Karen L. Madigan, Michael T. Joye, Samantha B. |
description | The presence of biogenic gases such as oxygen, methane, and nitrous oxide (N2O) in the atmospheres of extraterrestrial bodies has been postulated as a biosignature of life. Abiotic N2O production was documented recently in Don Juan Pond (DJP), Antarctica, a cold, hypersaline Mars analog environment. Here we quantify the temperature‐driven kinetics of abiotic N2O production and combine this with stable isotope labeling to demonstrate that N2O is produced from DJP sediment and brine at Mars‐analog temperatures down to at least −40°C. Further, we show that at any given temperature, N2O production is controlled by the availability of reduced Fe‐bearing minerals rather than nitrate. We conclude that abiotic N2O production is possible on Mars and on other extraterrestrial bodies and exoplanets. Thus, the presence of atmospheric N2O on these bodies should not be taken by itself as an indicator of microbial life.
Plain Language Summary
The search for extraterrestrial life has long captured our collective imagination, but it is hindered by the difficulty of actually visiting extraterrestrial planets, moons, asteroids, etc. to search for life. An alternative strategy is to remotely analyze the atmospheres of these planets to look for trace gases that exist in Earth's atmosphere because they are produced by living organisms across the biosphere. One such gas is nitrous oxide. We visited a remote, extremely cold, and salty desert pond in the Dry Valleys of Antarctica, an environment that is considered to be among the most similar to Mars that can be found on Earth. There, we studied the production of nitrous oxide in the absence of microbial life. We show that this gas is produced through the interaction between rock and chemical precursors in water at extremely cold temperatures (−40°C) that are similar to those observed on Mars. Because nitrous oxide can be produced in the absence of life, we conclude that its presence in the atmosphere of another planet or planetary moon does not necessarily indicate the presence of life on that object.
Key Points
Abiotic nitrous oxide production occurs at temperatures down to −40°C in Mars‐analog environment (DJP), Antarctica
Across temperatures, abiotic nitrous oxide production is controlled by the availability of reduced iron rather than nitrate availability
The presence of atmospheric nitrous oxide on an extraterrestrial body should not by itself be considered evidence of life |
doi_str_mv | 10.1029/2021GL094635 |
format | Article |
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Plain Language Summary
The search for extraterrestrial life has long captured our collective imagination, but it is hindered by the difficulty of actually visiting extraterrestrial planets, moons, asteroids, etc. to search for life. An alternative strategy is to remotely analyze the atmospheres of these planets to look for trace gases that exist in Earth's atmosphere because they are produced by living organisms across the biosphere. One such gas is nitrous oxide. We visited a remote, extremely cold, and salty desert pond in the Dry Valleys of Antarctica, an environment that is considered to be among the most similar to Mars that can be found on Earth. There, we studied the production of nitrous oxide in the absence of microbial life. We show that this gas is produced through the interaction between rock and chemical precursors in water at extremely cold temperatures (−40°C) that are similar to those observed on Mars. Because nitrous oxide can be produced in the absence of life, we conclude that its presence in the atmosphere of another planet or planetary moon does not necessarily indicate the presence of life on that object.
Key Points
Abiotic nitrous oxide production occurs at temperatures down to −40°C in Mars‐analog environment (DJP), Antarctica
Across temperatures, abiotic nitrous oxide production is controlled by the availability of reduced iron rather than nitrate availability
The presence of atmospheric nitrous oxide on an extraterrestrial body should not by itself be considered evidence of life</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2021GL094635</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Abiotic factors ; Analogs ; Antarctica ; Asteroids ; Atmosphere ; biosignatures ; Biosphere ; Brines ; Cold ; Earth ; exobiology ; Extrasolar planets ; Extraterrestrial environments ; Extraterrestrial life ; Extraterrestrial materials ; extreme environment ; Gases ; Kinetics ; Mars ; Mars environment ; Mars surface sediments ; Microorganisms ; Minerals ; Moon ; Nitrous oxide ; Oxygen ; Planetary atmospheres ; Planets ; Ponds ; Sediments ; Stable isotopes ; Temperature ; Trace gases</subject><ispartof>Geophysical research letters, 2022-02, Vol.49 (3), p.n/a</ispartof><rights>2022. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-a3677-1d7bade6a7080d0d292a40b9d5ce19a6c9cc8e5273c5683f9ed3dbf381adb5803</citedby><cites>FETCH-LOGICAL-a3677-1d7bade6a7080d0d292a40b9d5ce19a6c9cc8e5273c5683f9ed3dbf381adb5803</cites><orcidid>0000-0002-0464-5880 ; 0000-0003-3312-6972 ; 0000-0002-5286-7795 ; 0000-0003-1610-451X ; 0000-0002-3907-7828 ; 0000-0002-7785-4026</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2021GL094635$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2021GL094635$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,780,784,1417,1433,11514,27924,27925,45574,45575,46409,46468,46833,46892</link.rule.ids></links><search><creatorcontrib>Schutte, Charles A.</creatorcontrib><creatorcontrib>Samarkin, Vladimir A.</creatorcontrib><creatorcontrib>Bowles, Marshall W.</creatorcontrib><creatorcontrib>Peters, Brian</creatorcontrib><creatorcontrib>Casciotti, Karen L.</creatorcontrib><creatorcontrib>Madigan, Michael T.</creatorcontrib><creatorcontrib>Joye, Samantha B.</creatorcontrib><title>Abiotic Nitrous Oxide Production From Sediments and Brine of Don Juan Pond, Wright Valley Antarctica, at Mars Analog Temperatures (−40°C)</title><title>Geophysical research letters</title><description>The presence of biogenic gases such as oxygen, methane, and nitrous oxide (N2O) in the atmospheres of extraterrestrial bodies has been postulated as a biosignature of life. Abiotic N2O production was documented recently in Don Juan Pond (DJP), Antarctica, a cold, hypersaline Mars analog environment. Here we quantify the temperature‐driven kinetics of abiotic N2O production and combine this with stable isotope labeling to demonstrate that N2O is produced from DJP sediment and brine at Mars‐analog temperatures down to at least −40°C. Further, we show that at any given temperature, N2O production is controlled by the availability of reduced Fe‐bearing minerals rather than nitrate. We conclude that abiotic N2O production is possible on Mars and on other extraterrestrial bodies and exoplanets. Thus, the presence of atmospheric N2O on these bodies should not be taken by itself as an indicator of microbial life.
Plain Language Summary
The search for extraterrestrial life has long captured our collective imagination, but it is hindered by the difficulty of actually visiting extraterrestrial planets, moons, asteroids, etc. to search for life. An alternative strategy is to remotely analyze the atmospheres of these planets to look for trace gases that exist in Earth's atmosphere because they are produced by living organisms across the biosphere. One such gas is nitrous oxide. We visited a remote, extremely cold, and salty desert pond in the Dry Valleys of Antarctica, an environment that is considered to be among the most similar to Mars that can be found on Earth. There, we studied the production of nitrous oxide in the absence of microbial life. We show that this gas is produced through the interaction between rock and chemical precursors in water at extremely cold temperatures (−40°C) that are similar to those observed on Mars. Because nitrous oxide can be produced in the absence of life, we conclude that its presence in the atmosphere of another planet or planetary moon does not necessarily indicate the presence of life on that object.
Key Points
Abiotic nitrous oxide production occurs at temperatures down to −40°C in Mars‐analog environment (DJP), Antarctica
Across temperatures, abiotic nitrous oxide production is controlled by the availability of reduced iron rather than nitrate availability
The presence of atmospheric nitrous oxide on an extraterrestrial body should not by itself be considered evidence of life</description><subject>Abiotic factors</subject><subject>Analogs</subject><subject>Antarctica</subject><subject>Asteroids</subject><subject>Atmosphere</subject><subject>biosignatures</subject><subject>Biosphere</subject><subject>Brines</subject><subject>Cold</subject><subject>Earth</subject><subject>exobiology</subject><subject>Extrasolar planets</subject><subject>Extraterrestrial environments</subject><subject>Extraterrestrial life</subject><subject>Extraterrestrial materials</subject><subject>extreme environment</subject><subject>Gases</subject><subject>Kinetics</subject><subject>Mars</subject><subject>Mars environment</subject><subject>Mars surface sediments</subject><subject>Microorganisms</subject><subject>Minerals</subject><subject>Moon</subject><subject>Nitrous oxide</subject><subject>Oxygen</subject><subject>Planetary atmospheres</subject><subject>Planets</subject><subject>Ponds</subject><subject>Sediments</subject><subject>Stable isotopes</subject><subject>Temperature</subject><subject>Trace gases</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp9kE1uFDEQRi1EJIbAjgOUxAak6aRsd9vdy2EgQ6LJj0KAZcttu4OjmfbEdgtygyxY5SScIUfhJHE0LFhlVdJXT5-qHiFvKO5RZM0-Q0YXS2xKwatnZEKbsixqRPmcTDCnRc2keEFexniFiBw5nZDfs8755DScuBT8GOH0lzMWzoI3o07OD3AQ_Bq-WOPWdkgR1GDgQ3CDBd_Dx7w_GtUAZ34wU_ge3OWPBN_UamVvYDYkFXKHVlNQCY5ViDlTK38JF3a9sUGlMdgI7_7e3pV4_2f-_hXZ6dUq2tf_5i75evDpYv65WJ4uDuezZaG4kLKgRnbKWKEk1mjQsIapErvGVNrSRgndaF3bikmuK1HzvrGGm67nNVWmq2rku-TttncT_PVoY2qv_BjyabFlgkkqMJvM1HRL6eBjDLZvN8GtVbhpKbaPvtv_fWecbfGfLn__JNsuzpeCCyr5A0Edgm8</recordid><startdate>20220216</startdate><enddate>20220216</enddate><creator>Schutte, Charles A.</creator><creator>Samarkin, Vladimir A.</creator><creator>Bowles, Marshall W.</creator><creator>Peters, Brian</creator><creator>Casciotti, Karen L.</creator><creator>Madigan, Michael T.</creator><creator>Joye, Samantha B.</creator><general>John Wiley & Sons, Inc</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>7TN</scope><scope>8FD</scope><scope>F1W</scope><scope>FR3</scope><scope>H8D</scope><scope>H96</scope><scope>KL.</scope><scope>KR7</scope><scope>L.G</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0002-0464-5880</orcidid><orcidid>https://orcid.org/0000-0003-3312-6972</orcidid><orcidid>https://orcid.org/0000-0002-5286-7795</orcidid><orcidid>https://orcid.org/0000-0003-1610-451X</orcidid><orcidid>https://orcid.org/0000-0002-3907-7828</orcidid><orcidid>https://orcid.org/0000-0002-7785-4026</orcidid></search><sort><creationdate>20220216</creationdate><title>Abiotic Nitrous Oxide Production From Sediments and Brine of Don Juan Pond, Wright Valley Antarctica, at Mars Analog Temperatures (−40°C)</title><author>Schutte, Charles A. ; Samarkin, Vladimir A. ; Bowles, Marshall W. ; Peters, Brian ; Casciotti, Karen L. ; Madigan, Michael T. ; Joye, Samantha B.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a3677-1d7bade6a7080d0d292a40b9d5ce19a6c9cc8e5273c5683f9ed3dbf381adb5803</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Abiotic factors</topic><topic>Analogs</topic><topic>Antarctica</topic><topic>Asteroids</topic><topic>Atmosphere</topic><topic>biosignatures</topic><topic>Biosphere</topic><topic>Brines</topic><topic>Cold</topic><topic>Earth</topic><topic>exobiology</topic><topic>Extrasolar planets</topic><topic>Extraterrestrial environments</topic><topic>Extraterrestrial life</topic><topic>Extraterrestrial materials</topic><topic>extreme environment</topic><topic>Gases</topic><topic>Kinetics</topic><topic>Mars</topic><topic>Mars environment</topic><topic>Mars surface sediments</topic><topic>Microorganisms</topic><topic>Minerals</topic><topic>Moon</topic><topic>Nitrous oxide</topic><topic>Oxygen</topic><topic>Planetary atmospheres</topic><topic>Planets</topic><topic>Ponds</topic><topic>Sediments</topic><topic>Stable isotopes</topic><topic>Temperature</topic><topic>Trace gases</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Schutte, Charles A.</creatorcontrib><creatorcontrib>Samarkin, Vladimir A.</creatorcontrib><creatorcontrib>Bowles, Marshall W.</creatorcontrib><creatorcontrib>Peters, Brian</creatorcontrib><creatorcontrib>Casciotti, Karen L.</creatorcontrib><creatorcontrib>Madigan, Michael T.</creatorcontrib><creatorcontrib>Joye, Samantha B.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Oceanic Abstracts</collection><collection>Technology Research Database</collection><collection>ASFA: Aquatic Sciences and Fisheries Abstracts</collection><collection>Engineering Research Database</collection><collection>Aerospace Database</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) 2: Ocean Technology, Policy & Non-Living Resources</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Civil Engineering Abstracts</collection><collection>Aquatic Science & Fisheries Abstracts (ASFA) Professional</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Geophysical research letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Schutte, Charles A.</au><au>Samarkin, Vladimir A.</au><au>Bowles, Marshall W.</au><au>Peters, Brian</au><au>Casciotti, Karen L.</au><au>Madigan, Michael T.</au><au>Joye, Samantha B.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Abiotic Nitrous Oxide Production From Sediments and Brine of Don Juan Pond, Wright Valley Antarctica, at Mars Analog Temperatures (−40°C)</atitle><jtitle>Geophysical research letters</jtitle><date>2022-02-16</date><risdate>2022</risdate><volume>49</volume><issue>3</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>The presence of biogenic gases such as oxygen, methane, and nitrous oxide (N2O) in the atmospheres of extraterrestrial bodies has been postulated as a biosignature of life. Abiotic N2O production was documented recently in Don Juan Pond (DJP), Antarctica, a cold, hypersaline Mars analog environment. Here we quantify the temperature‐driven kinetics of abiotic N2O production and combine this with stable isotope labeling to demonstrate that N2O is produced from DJP sediment and brine at Mars‐analog temperatures down to at least −40°C. Further, we show that at any given temperature, N2O production is controlled by the availability of reduced Fe‐bearing minerals rather than nitrate. We conclude that abiotic N2O production is possible on Mars and on other extraterrestrial bodies and exoplanets. Thus, the presence of atmospheric N2O on these bodies should not be taken by itself as an indicator of microbial life.
Plain Language Summary
The search for extraterrestrial life has long captured our collective imagination, but it is hindered by the difficulty of actually visiting extraterrestrial planets, moons, asteroids, etc. to search for life. An alternative strategy is to remotely analyze the atmospheres of these planets to look for trace gases that exist in Earth's atmosphere because they are produced by living organisms across the biosphere. One such gas is nitrous oxide. We visited a remote, extremely cold, and salty desert pond in the Dry Valleys of Antarctica, an environment that is considered to be among the most similar to Mars that can be found on Earth. There, we studied the production of nitrous oxide in the absence of microbial life. We show that this gas is produced through the interaction between rock and chemical precursors in water at extremely cold temperatures (−40°C) that are similar to those observed on Mars. Because nitrous oxide can be produced in the absence of life, we conclude that its presence in the atmosphere of another planet or planetary moon does not necessarily indicate the presence of life on that object.
Key Points
Abiotic nitrous oxide production occurs at temperatures down to −40°C in Mars‐analog environment (DJP), Antarctica
Across temperatures, abiotic nitrous oxide production is controlled by the availability of reduced iron rather than nitrate availability
The presence of atmospheric nitrous oxide on an extraterrestrial body should not by itself be considered evidence of life</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2021GL094635</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-0464-5880</orcidid><orcidid>https://orcid.org/0000-0003-3312-6972</orcidid><orcidid>https://orcid.org/0000-0002-5286-7795</orcidid><orcidid>https://orcid.org/0000-0003-1610-451X</orcidid><orcidid>https://orcid.org/0000-0002-3907-7828</orcidid><orcidid>https://orcid.org/0000-0002-7785-4026</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Abiotic factors Analogs Antarctica Asteroids Atmosphere biosignatures Biosphere Brines Cold Earth exobiology Extrasolar planets Extraterrestrial environments Extraterrestrial life Extraterrestrial materials extreme environment Gases Kinetics Mars Mars environment Mars surface sediments Microorganisms Minerals Moon Nitrous oxide Oxygen Planetary atmospheres Planets Ponds Sediments Stable isotopes Temperature Trace gases |
title | Abiotic Nitrous Oxide Production From Sediments and Brine of Don Juan Pond, Wright Valley Antarctica, at Mars Analog Temperatures (−40°C) |
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