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dc.contributor.authorBeard, S. P.
dc.contributor.authorSwindle, T. D.
dc.date.accessioned2018-06-27T15:57:15Z
dc.date.available2018-06-27T15:57:15Z
dc.date.issued2017-11
dc.identifier.citationBeard, S. P. and Swindle, T. D. (2017), Search for evidence of source event grouping among ureilites. Meteorit Planet Sci, 52: 2343-2352. doi:10.1111/maps.12939en_US
dc.identifier.issn10869379
dc.identifier.doi10.1111/maps.12939
dc.identifier.urihttp://hdl.handle.net/10150/628151
dc.description.abstractWe use cosmic-ray exposure (CRE) ages of ureilites, combined with magnesium numbers of olivine, and oxygen isotopes, to search for evidence of specific source events initiating exposure for groups of ureilites. This technique can also be used to investigate the heterogeneity of the body from which the samples were derived. There are a total of 39 ureilites included in our work, which represents the largest collection of ureilite CRE age data used to date. Although we find some evidence of possible clusters, it is clear that most ureilites did not originate in one or two events on a homogeneous parent body.en_US
dc.description.sponsorshipNASA [NNX13AF57G]en_US
dc.language.isoenen_US
dc.publisherWILEYen_US
dc.relation.urlhttp://doi.wiley.com/10.1111/maps.12939en_US
dc.rights© The Meteoritical Society, 2017.en_US
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.titleSearch for evidence of source event grouping among ureilitesen_US
dc.typeArticleen_US
dc.contributor.departmentUniv Arizona, Lunar & Planetary Laben_US
dc.identifier.journalMETEORITICS & PLANETARY SCIENCEen_US
dc.description.note12 month embargo; published online: 24 August 2017en_US
dc.description.collectioninformationThis item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.en_US
dc.eprint.versionFinal accepted manuscripten_US
dc.source.journaltitleMeteoritics & Planetary Science


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