Carbon Monoxide Affecting Planetary Atmospheric Chemistry
CO is an important component in many atmospheres, including Titan, Triton, and Pluto, and has also been detected in the atmosphere of a number of exoplanets. Numerous experimental simulations have been carried out in the laboratory to understand the chemistry in atmospheres, but very few simulations...
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Veröffentlicht in: | Astrophysical journal. Letters 2017-06, Vol.841 (2), p.L31 |
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creator | He, Chao Hörst, Sarah M. Riemer, Sydney Sebree, Joshua A. Pauley, Nicholas Vuitton, Véronique |
description | CO is an important component in many atmospheres, including Titan, Triton, and Pluto, and has also been detected in the atmosphere of a number of exoplanets. Numerous experimental simulations have been carried out in the laboratory to understand the chemistry in atmospheres, but very few simulations have included CO in the initial gas mixtures. The effect of CO on the chemistry occurring in these atmospheres is still poorly understood. We have investigated the effect of CO on both gas and solid phase chemistry in a series of planetary atmosphere simulation experiments using gas mixtures of CO, , and with a range of CO mixing ratios from 0.05% to 5% at low temperature (∼100 K). We find that CO affects the gas phase chemistry, the density, and the composition of the solids. Specifically, with the increase of CO in the initial gases, there is less but more , HCN, , and produced in the gas phase, while the density, oxygen content, and degree of unsaturation of the solids increase. The results indicate that CO has an important impact on the chemistry occurring in our experiments and accordingly in planetary atmospheres. |
doi_str_mv | 10.3847/2041-8213/aa74cc |
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Numerous experimental simulations have been carried out in the laboratory to understand the chemistry in atmospheres, but very few simulations have included CO in the initial gas mixtures. The effect of CO on the chemistry occurring in these atmospheres is still poorly understood. We have investigated the effect of CO on both gas and solid phase chemistry in a series of planetary atmosphere simulation experiments using gas mixtures of CO, , and with a range of CO mixing ratios from 0.05% to 5% at low temperature (∼100 K). We find that CO affects the gas phase chemistry, the density, and the composition of the solids. Specifically, with the increase of CO in the initial gases, there is less but more , HCN, , and produced in the gas phase, while the density, oxygen content, and degree of unsaturation of the solids increase. The results indicate that CO has an important impact on the chemistry occurring in our experiments and accordingly in planetary atmospheres.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8213/aa74cc</identifier><language>eng</language><publisher>Austin: The American Astronomical Society</publisher><subject>astrobiology ; Atmospheric chemistry ; Carbon monoxide ; Density ; Extrasolar planets ; Gas mixtures ; Gases ; Low temperature ; Mixing ratio ; Organic chemistry ; Oxygen ; Oxygen content ; Planetary atmospheres ; planets and satellites: atmospheres ; planets and satellites: composition ; Pluto ; Pluto (dwarf planet) ; Sciences of the Universe ; Simulation ; Solid phases ; Titan ; Triton ; Vapor phases</subject><ispartof>Astrophysical journal. Letters, 2017-06, Vol.841 (2), p.L31</ispartof><rights>2017. The American Astronomical Society. All rights reserved.</rights><rights>Copyright IOP Publishing Jun 01, 2017</rights><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c482t-58f126a48bf0319b1620185cd7f4e31e671449a9b24ed7ed7f473a77d6d5a6cb3</citedby><cites>FETCH-LOGICAL-c482t-58f126a48bf0319b1620185cd7f4e31e671449a9b24ed7ed7f473a77d6d5a6cb3</cites><orcidid>0000-0001-5142-8689 ; 0000-0003-4596-0702 ; 0000-0001-7273-1898 ; 0000-0002-6694-0965</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/aa74cc/pdf$$EPDF$$P50$$Giop$$H</linktopdf><link.rule.ids>230,314,776,780,881,27901,27902,38845,38867,53815,53842</link.rule.ids><linktorsrc>$$Uhttps://iopscience.iop.org/article/10.3847/2041-8213/aa74cc$$EView_record_in_IOP_Publishing$$FView_record_in_$$GIOP_Publishing</linktorsrc><backlink>$$Uhttps://insu.hal.science/insu-03692507$$DView record in HAL$$Hfree_for_read</backlink></links><search><creatorcontrib>He, Chao</creatorcontrib><creatorcontrib>Hörst, Sarah M.</creatorcontrib><creatorcontrib>Riemer, Sydney</creatorcontrib><creatorcontrib>Sebree, Joshua A.</creatorcontrib><creatorcontrib>Pauley, Nicholas</creatorcontrib><creatorcontrib>Vuitton, Véronique</creatorcontrib><title>Carbon Monoxide Affecting Planetary Atmospheric Chemistry</title><title>Astrophysical journal. Letters</title><addtitle>APJL</addtitle><addtitle>Astrophys. J. Lett</addtitle><description>CO is an important component in many atmospheres, including Titan, Triton, and Pluto, and has also been detected in the atmosphere of a number of exoplanets. Numerous experimental simulations have been carried out in the laboratory to understand the chemistry in atmospheres, but very few simulations have included CO in the initial gas mixtures. The effect of CO on the chemistry occurring in these atmospheres is still poorly understood. We have investigated the effect of CO on both gas and solid phase chemistry in a series of planetary atmosphere simulation experiments using gas mixtures of CO, , and with a range of CO mixing ratios from 0.05% to 5% at low temperature (∼100 K). We find that CO affects the gas phase chemistry, the density, and the composition of the solids. Specifically, with the increase of CO in the initial gases, there is less but more , HCN, , and produced in the gas phase, while the density, oxygen content, and degree of unsaturation of the solids increase. The results indicate that CO has an important impact on the chemistry occurring in our experiments and accordingly in planetary atmospheres.</description><subject>astrobiology</subject><subject>Atmospheric chemistry</subject><subject>Carbon monoxide</subject><subject>Density</subject><subject>Extrasolar planets</subject><subject>Gas mixtures</subject><subject>Gases</subject><subject>Low temperature</subject><subject>Mixing ratio</subject><subject>Organic chemistry</subject><subject>Oxygen</subject><subject>Oxygen content</subject><subject>Planetary atmospheres</subject><subject>planets and satellites: atmospheres</subject><subject>planets and satellites: composition</subject><subject>Pluto</subject><subject>Pluto (dwarf planet)</subject><subject>Sciences of the Universe</subject><subject>Simulation</subject><subject>Solid phases</subject><subject>Titan</subject><subject>Triton</subject><subject>Vapor phases</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2017</creationdate><recordtype>article</recordtype><recordid>eNp1kE1LxDAYhIMoqKt3jwXBg1g3X03SY1nUFSp60HNI08TN0m1q0hX339tSWS96el-GZ4ZhALhA8JYIyucYUpQKjMhcKU61PgAne-lw_8PsGJzGuIYQQ4bECcgXKlS-TZ58679cbZLCWqN7174nL41qTa_CLin6jY_dygSnk8XKbFzsw-4MHFnVRHP-c2fg7f7udbFMy-eHx0VRppoK3KeZsAgzRUVlIUF5hRiGSGS65pYaggzjiNJc5RWmpuZmlDlRnNeszhTTFZmB6yl3pRrZBbcZGkmvnFwWpXRt3EpIWI4zyD_RAF9OcBf8x9bEXq79NrRDP4kJyxhikJGBghOlg48xGLvPRVCOa8pxLjlOJ6c1B8vVZHG--81U3bqRYkCxLAmSXW0H8OYP8N_cby0vgZ4</recordid><startdate>20170601</startdate><enddate>20170601</enddate><creator>He, Chao</creator><creator>Hörst, Sarah M.</creator><creator>Riemer, Sydney</creator><creator>Sebree, Joshua A.</creator><creator>Pauley, Nicholas</creator><creator>Vuitton, Véronique</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><general>Bristol : IOP Publishing</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>1XC</scope><orcidid>https://orcid.org/0000-0001-5142-8689</orcidid><orcidid>https://orcid.org/0000-0003-4596-0702</orcidid><orcidid>https://orcid.org/0000-0001-7273-1898</orcidid><orcidid>https://orcid.org/0000-0002-6694-0965</orcidid></search><sort><creationdate>20170601</creationdate><title>Carbon Monoxide Affecting Planetary Atmospheric Chemistry</title><author>He, Chao ; Hörst, Sarah M. ; Riemer, Sydney ; Sebree, Joshua A. ; Pauley, Nicholas ; Vuitton, Véronique</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c482t-58f126a48bf0319b1620185cd7f4e31e671449a9b24ed7ed7f473a77d6d5a6cb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2017</creationdate><topic>astrobiology</topic><topic>Atmospheric chemistry</topic><topic>Carbon monoxide</topic><topic>Density</topic><topic>Extrasolar planets</topic><topic>Gas mixtures</topic><topic>Gases</topic><topic>Low temperature</topic><topic>Mixing ratio</topic><topic>Organic chemistry</topic><topic>Oxygen</topic><topic>Oxygen content</topic><topic>Planetary atmospheres</topic><topic>planets and satellites: atmospheres</topic><topic>planets and satellites: composition</topic><topic>Pluto</topic><topic>Pluto (dwarf planet)</topic><topic>Sciences of the Universe</topic><topic>Simulation</topic><topic>Solid phases</topic><topic>Titan</topic><topic>Triton</topic><topic>Vapor phases</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>He, Chao</creatorcontrib><creatorcontrib>Hörst, Sarah M.</creatorcontrib><creatorcontrib>Riemer, Sydney</creatorcontrib><creatorcontrib>Sebree, Joshua A.</creatorcontrib><creatorcontrib>Pauley, Nicholas</creatorcontrib><creatorcontrib>Vuitton, Véronique</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>He, Chao</au><au>Hörst, Sarah M.</au><au>Riemer, Sydney</au><au>Sebree, Joshua A.</au><au>Pauley, Nicholas</au><au>Vuitton, Véronique</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Carbon Monoxide Affecting Planetary Atmospheric Chemistry</atitle><jtitle>Astrophysical journal. Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2017-06-01</date><risdate>2017</risdate><volume>841</volume><issue>2</issue><spage>L31</spage><pages>L31-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>CO is an important component in many atmospheres, including Titan, Triton, and Pluto, and has also been detected in the atmosphere of a number of exoplanets. Numerous experimental simulations have been carried out in the laboratory to understand the chemistry in atmospheres, but very few simulations have included CO in the initial gas mixtures. The effect of CO on the chemistry occurring in these atmospheres is still poorly understood. We have investigated the effect of CO on both gas and solid phase chemistry in a series of planetary atmosphere simulation experiments using gas mixtures of CO, , and with a range of CO mixing ratios from 0.05% to 5% at low temperature (∼100 K). We find that CO affects the gas phase chemistry, the density, and the composition of the solids. Specifically, with the increase of CO in the initial gases, there is less but more , HCN, , and produced in the gas phase, while the density, oxygen content, and degree of unsaturation of the solids increase. 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subjects | astrobiology Atmospheric chemistry Carbon monoxide Density Extrasolar planets Gas mixtures Gases Low temperature Mixing ratio Organic chemistry Oxygen Oxygen content Planetary atmospheres planets and satellites: atmospheres planets and satellites: composition Pluto Pluto (dwarf planet) Sciences of the Universe Simulation Solid phases Titan Triton Vapor phases |
title | Carbon Monoxide Affecting Planetary Atmospheric Chemistry |
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