Large Excess of Heavy Nitrogen in Both Hydrogen Cyanide and Cyanogen from Comet 17P/Holmes

dc.contributor.utaustinauthorCochran, Anita L.en_US
dc.contributor.utaustinauthorCochran, W.en_US
dc.creatorBockelee-Morvan, D.en_US
dc.creatorBiver, N.en_US
dc.creatorJehin, E.en_US
dc.creatorCochran, Anita L.en_US
dc.creatorWiesemeyer, H.en_US
dc.creatorManfroid, J.en_US
dc.creatorHutsemekers, D.en_US
dc.creatorArpigny, C.en_US
dc.creatorBoissier, J.en_US
dc.creatorCochran, W.en_US
dc.creatorColom, P.en_US
dc.creatorCrovisier, J.en_US
dc.creatorMilutinovic, N.en_US
dc.creatorMoreno, R.en_US
dc.creatorProchaska, J. X.en_US
dc.creatorRamirez, I.en_US
dc.creatorSchulz, R.en_US
dc.creatorZucconi, J. M.en_US
dc.date.accessioned2016-10-28T19:34:40Z
dc.date.available2016-10-28T19:34:40Z
dc.date.issued2008-05en_US
dc.description.abstractFrom millimeter and optical observations of the Jupiter-family comet 17P/Holmes performed soon after its huge outburst of 2007 October 24, we derive N-14/N-15 = 139 +/- 26 in HCN and N-14/N-15 = 165 +/- 40 in CN, establishing that HCN has the same nonterrestrial isotopic composition as CN. The same conclusion is obtained for the long-period comet C/1995 O1 (Hale-Bopp) after a reanalysis of previously published measurements. These results are compatible with HCN being the prime parent of CN in cometary atmospheres. The N-15 excess relative to the Earth's atmospheric value indicates that N-bearing volatiles in the solar nebula underwent important N isotopic fractionation at some stage of solar system Formation. HCN molecules never isotopically equilibrated with the main nitrogen reservoir in the solar nebula before being incorporated in Oort Cloud and Kuiper Belt comets. The C-12/C-13 ratios in HCN and CN are measured to be consistent with the terrestrial value.en_US
dc.description.departmentAstronomyen_US
dc.description.sponsorshipINSU/CNRS (France)en_US
dc.description.sponsorshipMPG (Germany)en_US
dc.description.sponsorshipIGN (Spain)en_US
dc.description.sponsorshipFNRS (Belgium)en_US
dc.description.sponsorshipNASA NNG04G162Gen_US
dc.identifierdoi:10.15781/T21G0HX5X
dc.identifier.citationBockelée-Morvan, D., N. Biver, Emmanuel Jehin, A. L. Cochran, H. Wiesemeyer, Jean Manfroid, Damien Hutsemekers et al. "Large excess of heavy nitrogen in both hydrogen cyanide and cyanogen from comet 17P/Holmes." The Astrophysical Journal Letters, Vol. 679, No. 1 (May, 2008): L49.en_US
dc.identifier.doi10.1086/588781en_US
dc.identifier.issnen_US
dc.identifier.urihttp://hdl.handle.net/2152/42936
dc.language.isoEnglishen_US
dc.relation.ispartofen_US
dc.relation.ispartofserialAstrophysical Journal Lettersen_US
dc.rightsAdministrative deposit of works to Texas ScholarWorks: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en_US
dc.rights.restrictionOpenen_US
dc.subjectcomets : generalen_US
dc.subjectcomets : individual (17p/holmes)en_US
dc.subjectradio lines : solaren_US
dc.subjectsystemen_US
dc.subjectbopp c/1995 o1en_US
dc.subjecthale-boppen_US
dc.subjectisotopic fractionationen_US
dc.subjectprimitive meteoritesen_US
dc.subjectb2 hyakutakeen_US
dc.subjectratioen_US
dc.subjectcarbonen_US
dc.subjectabundancesen_US
dc.subjectn-14/n-15en_US
dc.subjectchemistryen_US
dc.subjectastronomy & astrophysicsen_US
dc.titleLarge Excess of Heavy Nitrogen in Both Hydrogen Cyanide and Cyanogen from Comet 17P/Holmesen_US
dc.typeArticleen_US

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