Extreme Exospheric Dynamics at Charon: Implications for the Red Spot
Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi‐annually drives frozen methane off the polar night zones. Charon's pole‐centric red spot has been pro...
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creator | Teolis, Ben Raut, Ujjwal Kammer, Joshua A. Gimar, Caleb J. Howett, Carly J. A. Gladstone, G. Randall Retherford, Kurt D. |
description | Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi‐annually drives frozen methane off the polar night zones. Charon's pole‐centric red spot has been proposed to be the product of Ly‐α photolysis of frozen methane into refractory hydrocarbon “tholins”, but the role of exospheric dynamics in the red material's formation has not been investigated. We show with exospheric modeling that methane “polar‐swap”, in which exospheric CH4 sublimated from the spring polar zone is rapidly re‐frozen onto the autumn hemisphere, deposits ∼30 μm polar frosts too thick for Ly‐α light to penetrate. Ethane, the primary methane photoproduct under these conditions, may unlike methane remain frozen decades after polar sunrise under solar wind exposure. Solar wind radiolysis of polar ethane frost synthesizes higher‐order refractories that may contribute to the coloration of Charon's polar zones.
Plain Language Summary
Charon's thin methane atmosphere undergoes “explosive” pulsations owing to the Pluto‐Charon's systems' near sideways tilt to the Sun, according to new computer simulations that we present here. Spring sunrise may drive polar methane frozen during the centuries long winter night back into Charon's atmosphere, causing the whole atmosphere to briefly and drastically surge in pressure by a factor of almost 1000 every equinox. During these exceedingly brief episodes, taking place just a few years out of the Pluto‐Charon system's 248 year orbit around the Sun, polar caps of methane frost tens of microns thick may be suddenly swapped between north and south, evaporated and then re‐frozen from the spring to the autumnal polar zones. Charon's polar red spot, seen by the New Horizons spacecraft, is suspected to be material synthesized from frozen methane by backscattered solar ultraviolet light. However we find that Charon's polar caps are frozen too fast and thick for synthesis of much material more complex than ethane. Nevertheless ethane, being less volatile than methane, stays frozen to Charon's surface for decades after spring sunrise, and may under exposure to solar wind be converted to permanent red‐colored surface deposits that contribute to the origins of the red spot.
Key Points
Surges in Charon's exosphere, driven by spring‐sunrise sublimation of polar methane, produce “flash frozen” CH4 frost at the autumn pole
Polar frost grows |
doi_str_mv | 10.1029/2021GL097580 |
format | Article |
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Plain Language Summary
Charon's thin methane atmosphere undergoes “explosive” pulsations owing to the Pluto‐Charon's systems' near sideways tilt to the Sun, according to new computer simulations that we present here. Spring sunrise may drive polar methane frozen during the centuries long winter night back into Charon's atmosphere, causing the whole atmosphere to briefly and drastically surge in pressure by a factor of almost 1000 every equinox. During these exceedingly brief episodes, taking place just a few years out of the Pluto‐Charon system's 248 year orbit around the Sun, polar caps of methane frost tens of microns thick may be suddenly swapped between north and south, evaporated and then re‐frozen from the spring to the autumnal polar zones. Charon's polar red spot, seen by the New Horizons spacecraft, is suspected to be material synthesized from frozen methane by backscattered solar ultraviolet light. However we find that Charon's polar caps are frozen too fast and thick for synthesis of much material more complex than ethane. Nevertheless ethane, being less volatile than methane, stays frozen to Charon's surface for decades after spring sunrise, and may under exposure to solar wind be converted to permanent red‐colored surface deposits that contribute to the origins of the red spot.
Key Points
Surges in Charon's exosphere, driven by spring‐sunrise sublimation of polar methane, produce “flash frozen” CH4 frost at the autumn pole
Polar frost grows too thick and fast for efficient Ly‐α CH4 photolysis to hydrocarbons past C2H6 that may contribute to Charon's red spot
Origin of Charon's polar red material may be in part solar wind radiolysis of photolytic ethane remaining surface‐bound past spring sunrise</description><identifier>ISSN: 0094-8276</identifier><identifier>EISSN: 1944-8007</identifier><identifier>DOI: 10.1029/2021GL097580</identifier><language>eng</language><publisher>Washington: John Wiley & Sons, Inc</publisher><subject>Atmosphere ; Atmospheric models ; Backscattering ; Charon ; Coloration ; Colour ; Dynamics ; Equinoxes ; Ethane ; Exosphere ; Frost ; Hydrocarbons ; Mathematical models ; Methane ; New Horizons mission ; Night ; Photolysis ; Pluto ; Pluto (dwarf planet) ; Polar caps ; Polar regions ; Radiolysis ; Refractories ; Seasonal variations ; Solar wind ; Spacecraft ; Spring ; Spring (season) ; Sunrise ; Synthesis ; Ultraviolet radiation</subject><ispartof>Geophysical research letters, 2022-04, Vol.49 (8), 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-c3441-17dd0377ce4e412d57cbb31897c853783684a80b9dfbc9f067c94fb3eabcc4a23</citedby><cites>FETCH-LOGICAL-c3441-17dd0377ce4e412d57cbb31897c853783684a80b9dfbc9f067c94fb3eabcc4a23</cites><orcidid>0000-0002-6036-1575 ; 0000-0003-1869-4947 ; 0000-0001-9470-150X ; 0000-0003-0060-072X ; 0000-0001-8386-6413</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%2F2021GL097580$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2021GL097580$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,777,781,1412,1428,11495,27905,27906,45555,45556,46390,46449,46814,46873</link.rule.ids></links><search><creatorcontrib>Teolis, Ben</creatorcontrib><creatorcontrib>Raut, Ujjwal</creatorcontrib><creatorcontrib>Kammer, Joshua A.</creatorcontrib><creatorcontrib>Gimar, Caleb J.</creatorcontrib><creatorcontrib>Howett, Carly J. A.</creatorcontrib><creatorcontrib>Gladstone, G. Randall</creatorcontrib><creatorcontrib>Retherford, Kurt D.</creatorcontrib><title>Extreme Exospheric Dynamics at Charon: Implications for the Red Spot</title><title>Geophysical research letters</title><description>Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi‐annually drives frozen methane off the polar night zones. Charon's pole‐centric red spot has been proposed to be the product of Ly‐α photolysis of frozen methane into refractory hydrocarbon “tholins”, but the role of exospheric dynamics in the red material's formation has not been investigated. We show with exospheric modeling that methane “polar‐swap”, in which exospheric CH4 sublimated from the spring polar zone is rapidly re‐frozen onto the autumn hemisphere, deposits ∼30 μm polar frosts too thick for Ly‐α light to penetrate. Ethane, the primary methane photoproduct under these conditions, may unlike methane remain frozen decades after polar sunrise under solar wind exposure. Solar wind radiolysis of polar ethane frost synthesizes higher‐order refractories that may contribute to the coloration of Charon's polar zones.
Plain Language Summary
Charon's thin methane atmosphere undergoes “explosive” pulsations owing to the Pluto‐Charon's systems' near sideways tilt to the Sun, according to new computer simulations that we present here. Spring sunrise may drive polar methane frozen during the centuries long winter night back into Charon's atmosphere, causing the whole atmosphere to briefly and drastically surge in pressure by a factor of almost 1000 every equinox. During these exceedingly brief episodes, taking place just a few years out of the Pluto‐Charon system's 248 year orbit around the Sun, polar caps of methane frost tens of microns thick may be suddenly swapped between north and south, evaporated and then re‐frozen from the spring to the autumnal polar zones. Charon's polar red spot, seen by the New Horizons spacecraft, is suspected to be material synthesized from frozen methane by backscattered solar ultraviolet light. However we find that Charon's polar caps are frozen too fast and thick for synthesis of much material more complex than ethane. Nevertheless ethane, being less volatile than methane, stays frozen to Charon's surface for decades after spring sunrise, and may under exposure to solar wind be converted to permanent red‐colored surface deposits that contribute to the origins of the red spot.
Key Points
Surges in Charon's exosphere, driven by spring‐sunrise sublimation of polar methane, produce “flash frozen” CH4 frost at the autumn pole
Polar frost grows too thick and fast for efficient Ly‐α CH4 photolysis to hydrocarbons past C2H6 that may contribute to Charon's red spot
Origin of Charon's polar red material may be in part solar wind radiolysis of photolytic ethane remaining surface‐bound past spring sunrise</description><subject>Atmosphere</subject><subject>Atmospheric models</subject><subject>Backscattering</subject><subject>Charon</subject><subject>Coloration</subject><subject>Colour</subject><subject>Dynamics</subject><subject>Equinoxes</subject><subject>Ethane</subject><subject>Exosphere</subject><subject>Frost</subject><subject>Hydrocarbons</subject><subject>Mathematical models</subject><subject>Methane</subject><subject>New Horizons mission</subject><subject>Night</subject><subject>Photolysis</subject><subject>Pluto</subject><subject>Pluto (dwarf planet)</subject><subject>Polar caps</subject><subject>Polar regions</subject><subject>Radiolysis</subject><subject>Refractories</subject><subject>Seasonal variations</subject><subject>Solar wind</subject><subject>Spacecraft</subject><subject>Spring</subject><subject>Spring (season)</subject><subject>Sunrise</subject><subject>Synthesis</subject><subject>Ultraviolet radiation</subject><issn>0094-8276</issn><issn>1944-8007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><recordid>eNp90E9LwzAYBvAgCs7pzQ8Q8Gr1zZ82iTfZujkoCFPPIU1T1rE2Nelw-_ZW5sGTp-c5_HhfeBC6JfBAgKpHCpQsC1AilXCGJkRxnkgAcY4mAGrsVGSX6CrGLQAwYGSC5vlhCK51OD_42G9caCyeHzvTNjZiM-DZxgTfPeFV2-8aa4bGdxHXPuBh4_DaVfit98M1uqjNLrqb35yij0X-PntJitflavZcJJZxThIiqgqYENZxxwmtUmHLkhGphJUpE5JlkhsJparq0qoaMmEVr0vmTGktN5RN0d3pbh_8597FQW_9PnTjS02zNE2FlJSN6v6kbPAxBlfrPjStCUdNQP_spP_uNHJ64l_Nzh3_tXq5LjIOgrBvVHBn0g</recordid><startdate>20220428</startdate><enddate>20220428</enddate><creator>Teolis, Ben</creator><creator>Raut, Ujjwal</creator><creator>Kammer, Joshua A.</creator><creator>Gimar, Caleb J.</creator><creator>Howett, Carly J. A.</creator><creator>Gladstone, G. Randall</creator><creator>Retherford, Kurt D.</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/0000-0002-6036-1575</orcidid><orcidid>https://orcid.org/0000-0003-1869-4947</orcidid><orcidid>https://orcid.org/0000-0001-9470-150X</orcidid><orcidid>https://orcid.org/0000-0003-0060-072X</orcidid><orcidid>https://orcid.org/0000-0001-8386-6413</orcidid></search><sort><creationdate>20220428</creationdate><title>Extreme Exospheric Dynamics at Charon: Implications for the Red Spot</title><author>Teolis, Ben ; Raut, Ujjwal ; Kammer, Joshua A. ; Gimar, Caleb J. ; Howett, Carly J. A. ; Gladstone, G. Randall ; Retherford, Kurt D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c3441-17dd0377ce4e412d57cbb31897c853783684a80b9dfbc9f067c94fb3eabcc4a23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Atmosphere</topic><topic>Atmospheric models</topic><topic>Backscattering</topic><topic>Charon</topic><topic>Coloration</topic><topic>Colour</topic><topic>Dynamics</topic><topic>Equinoxes</topic><topic>Ethane</topic><topic>Exosphere</topic><topic>Frost</topic><topic>Hydrocarbons</topic><topic>Mathematical models</topic><topic>Methane</topic><topic>New Horizons mission</topic><topic>Night</topic><topic>Photolysis</topic><topic>Pluto</topic><topic>Pluto (dwarf planet)</topic><topic>Polar caps</topic><topic>Polar regions</topic><topic>Radiolysis</topic><topic>Refractories</topic><topic>Seasonal variations</topic><topic>Solar wind</topic><topic>Spacecraft</topic><topic>Spring</topic><topic>Spring (season)</topic><topic>Sunrise</topic><topic>Synthesis</topic><topic>Ultraviolet radiation</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Teolis, Ben</creatorcontrib><creatorcontrib>Raut, Ujjwal</creatorcontrib><creatorcontrib>Kammer, Joshua A.</creatorcontrib><creatorcontrib>Gimar, Caleb J.</creatorcontrib><creatorcontrib>Howett, Carly J. A.</creatorcontrib><creatorcontrib>Gladstone, G. Randall</creatorcontrib><creatorcontrib>Retherford, Kurt D.</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>Teolis, Ben</au><au>Raut, Ujjwal</au><au>Kammer, Joshua A.</au><au>Gimar, Caleb J.</au><au>Howett, Carly J. A.</au><au>Gladstone, G. Randall</au><au>Retherford, Kurt D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Extreme Exospheric Dynamics at Charon: Implications for the Red Spot</atitle><jtitle>Geophysical research letters</jtitle><date>2022-04-28</date><risdate>2022</risdate><volume>49</volume><issue>8</issue><epage>n/a</epage><issn>0094-8276</issn><eissn>1944-8007</eissn><abstract>Charon's exosphere may exhibit extreme seasonal dynamics, with centuries of quiescence punctuated by short lived (∼4 earth years) exospheric surges near the equinoxes, as spring sunrise bi‐annually drives frozen methane off the polar night zones. Charon's pole‐centric red spot has been proposed to be the product of Ly‐α photolysis of frozen methane into refractory hydrocarbon “tholins”, but the role of exospheric dynamics in the red material's formation has not been investigated. We show with exospheric modeling that methane “polar‐swap”, in which exospheric CH4 sublimated from the spring polar zone is rapidly re‐frozen onto the autumn hemisphere, deposits ∼30 μm polar frosts too thick for Ly‐α light to penetrate. Ethane, the primary methane photoproduct under these conditions, may unlike methane remain frozen decades after polar sunrise under solar wind exposure. Solar wind radiolysis of polar ethane frost synthesizes higher‐order refractories that may contribute to the coloration of Charon's polar zones.
Plain Language Summary
Charon's thin methane atmosphere undergoes “explosive” pulsations owing to the Pluto‐Charon's systems' near sideways tilt to the Sun, according to new computer simulations that we present here. Spring sunrise may drive polar methane frozen during the centuries long winter night back into Charon's atmosphere, causing the whole atmosphere to briefly and drastically surge in pressure by a factor of almost 1000 every equinox. During these exceedingly brief episodes, taking place just a few years out of the Pluto‐Charon system's 248 year orbit around the Sun, polar caps of methane frost tens of microns thick may be suddenly swapped between north and south, evaporated and then re‐frozen from the spring to the autumnal polar zones. Charon's polar red spot, seen by the New Horizons spacecraft, is suspected to be material synthesized from frozen methane by backscattered solar ultraviolet light. However we find that Charon's polar caps are frozen too fast and thick for synthesis of much material more complex than ethane. Nevertheless ethane, being less volatile than methane, stays frozen to Charon's surface for decades after spring sunrise, and may under exposure to solar wind be converted to permanent red‐colored surface deposits that contribute to the origins of the red spot.
Key Points
Surges in Charon's exosphere, driven by spring‐sunrise sublimation of polar methane, produce “flash frozen” CH4 frost at the autumn pole
Polar frost grows too thick and fast for efficient Ly‐α CH4 photolysis to hydrocarbons past C2H6 that may contribute to Charon's red spot
Origin of Charon's polar red material may be in part solar wind radiolysis of photolytic ethane remaining surface‐bound past spring sunrise</abstract><cop>Washington</cop><pub>John Wiley & Sons, Inc</pub><doi>10.1029/2021GL097580</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-6036-1575</orcidid><orcidid>https://orcid.org/0000-0003-1869-4947</orcidid><orcidid>https://orcid.org/0000-0001-9470-150X</orcidid><orcidid>https://orcid.org/0000-0003-0060-072X</orcidid><orcidid>https://orcid.org/0000-0001-8386-6413</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Atmosphere Atmospheric models Backscattering Charon Coloration Colour Dynamics Equinoxes Ethane Exosphere Frost Hydrocarbons Mathematical models Methane New Horizons mission Night Photolysis Pluto Pluto (dwarf planet) Polar caps Polar regions Radiolysis Refractories Seasonal variations Solar wind Spacecraft Spring Spring (season) Sunrise Synthesis Ultraviolet radiation |
title | Extreme Exospheric Dynamics at Charon: Implications for the Red Spot |
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