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...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:Astrophysical journal. Letters 2017-06, Vol.841 (2), p.L31
Hauptverfasser: He, Chao, Hörst, Sarah M., Riemer, Sydney, Sebree, Joshua A., Pauley, Nicholas, Vuitton, Véronique
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext bestellen
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue 2
container_start_page L31
container_title Astrophysical journal. Letters
container_volume 841
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
format Article
fullrecord <record><control><sourceid>proquest_O3W</sourceid><recordid>TN_cdi_proquest_journals_2365616063</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2365616063</sourcerecordid><originalsourceid>FETCH-LOGICAL-c482t-58f126a48bf0319b1620185cd7f4e31e671449a9b24ed7ed7f473a77d6d5a6cb3</originalsourceid><addsrcrecordid>eNp1kE1LxDAYhIMoqKt3jwXBg1g3X03SY1nUFSp60HNI08TN0m1q0hX339tSWS96el-GZ4ZhALhA8JYIyucYUpQKjMhcKU61PgAne-lw_8PsGJzGuIYQQ4bECcgXKlS-TZ58679cbZLCWqN7174nL41qTa_CLin6jY_dygSnk8XKbFzsw-4MHFnVRHP-c2fg7f7udbFMy-eHx0VRppoK3KeZsAgzRUVlIUF5hRiGSGS65pYaggzjiNJc5RWmpuZmlDlRnNeszhTTFZmB6yl3pRrZBbcZGkmvnFwWpXRt3EpIWI4zyD_RAF9OcBf8x9bEXq79NrRDP4kJyxhikJGBghOlg48xGLvPRVCOa8pxLjlOJ6c1B8vVZHG--81U3bqRYkCxLAmSXW0H8OYP8N_cby0vgZ4</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2365616063</pqid></control><display><type>article</type><title>Carbon Monoxide Affecting Planetary Atmospheric Chemistry</title><source>IOP Publishing Free Content</source><creator>He, Chao ; Hörst, Sarah M. ; Riemer, Sydney ; Sebree, Joshua A. ; Pauley, Nicholas ; Vuitton, Véronique</creator><creatorcontrib>He, Chao ; Hörst, Sarah M. ; Riemer, Sydney ; Sebree, Joshua A. ; Pauley, Nicholas ; Vuitton, Véronique</creatorcontrib><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><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 &amp; Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological &amp; 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. The results indicate that CO has an important impact on the chemistry occurring in our experiments and accordingly in planetary atmospheres.</abstract><cop>Austin</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8213/aa74cc</doi><tpages>7</tpages><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><oa>free_for_read</oa></addata></record>
fulltext fulltext_linktorsrc
identifier ISSN: 2041-8205
ispartof Astrophysical journal. Letters, 2017-06, Vol.841 (2), p.L31
issn 2041-8205
2041-8213
language eng
recordid cdi_proquest_journals_2365616063
source IOP Publishing Free Content
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
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-01T22%3A13%3A50IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_O3W&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Carbon%20Monoxide%20Affecting%20Planetary%20Atmospheric%20Chemistry&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=He,%20Chao&rft.date=2017-06-01&rft.volume=841&rft.issue=2&rft.spage=L31&rft.pages=L31-&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8213/aa74cc&rft_dat=%3Cproquest_O3W%3E2365616063%3C/proquest_O3W%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2365616063&rft_id=info:pmid/&rfr_iscdi=true