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<ri:Resource created="2021-09-08T08:01:01Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>TEXES spectra of Saturn from February 03 2013</title><shortName>J/A+A/653/A66</shortName><identifier>ivo://CDS.VizieR/J/A+A/653/A66</identifier><altIdentifier>doi:10.26093/cds/vizier.36530066</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Blake J.S.D.</name></creator><creator><name>Fletcher L.N.</name></creator><creator><name>Greathouse T.K.</name></creator><creator><name>Orton G.S.</name></creator><creator><name>Melin H.,Roman M.T.</name></creator><creator><name>Antunano A.</name></creator><creator><name>Donnelly P.T.</name></creator><creator><name>Rowe-Gurney N.</name></creator><creator><name>King O.</name></creator><date role="Updated">2022-01-17T13:05:27Z</date><date role="Created">2021-09-08T08:01:01Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>solar-system</subject><subject>solar-system-planets</subject><subject>spectroscopy</subject><subject>infrared-astronomy</subject><description>The abundance of deuterium in giant planet atmospheres provides constraints on the reservoirs of ices incorporated into these worlds during their formation and evolution. Motivated by discrepancies in the measured deuterium-hydrogen ratio (D/H) on Jupiter and Saturn, we present a new measurement of the D/H ratio in methane for Saturn from ground-based measurements. We analysed a spectral cube (covering 1151-1160cm^-1^ from 6 February 2013) from the Texas Echelon Cross Echelle Spectrograph (TEXES) on NASA's Infrared Telescope Facility (IRTF) where emission lines from both methane and deuterated methane are well resolved. Our estimate of the D/H ratio in stratospheric methane, 1.65(-0.21/+0.27)*10^-5^ is in agreement with results derived from Cassini CIRS and ISO/SWS observations, confirming the unexpectedly low CH3D abundance. Assuming a fractionation factor of 1.34(+/-0.19) we derive a hydrogen D/H of 1.23(-0.23/+0.27)*10^-5^. This value remains lower than previous tropospheric hydrogen D/H measurements of (i) Saturn 2.10(+/-0.13)*10^-5^, (ii) Jupiter 2.6(+/-0.7)*10^-5^ and (iii) the proto-solar hydrogen D/H of 2.1(+/-0.5)*10^-5^, suggesting that the fractionation factor may not be appropriate for stratospheric methane, or that the D/H ratio in Saturn's stratosphere is not representative of the bulk of the planet.</description><source format="bibcode">2021A&amp;A...653A..66B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/653/A66</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/653/A66</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/653/A66</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/653/A66</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/653/A66</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/653/A66</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/653/A66</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability><description>Associated data</description><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://cdsarc.cds.unistra.fr/assocdata/?obs_collection=J/A+A/653/A66</accessURL></interface></capability><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/653/A66/list</name><description>List of fits files</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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