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dc.contributor.authorCrowther, S. A.
dc.contributor.authorWhitby, J. A.
dc.contributor.authorBusfield, A.
dc.contributor.authorHolland, G.
dc.contributor.authorBusemann, H.
dc.contributor.authorGilmour, J. D.
dc.date.accessioned2021-02-12T22:53:48Z
dc.date.available2021-02-12T22:53:48Z
dc.date.issued2009-01-01
dc.identifier.citationCrowther, S. A., Whitby, J. A., Busfield, A., Holland, G., Busemann, H., & Gilmour, J. D. (2009). Collisional modification of the acapulcoite/lodranite parent body revealed by the iodine‐xenon system in lodranites. Meteoritics & Planetary Science, 44(8), 1151-1159.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2009.tb01214.x
dc.identifier.urihttp://hdl.handle.net/10150/656603
dc.description.abstractThe I-Xe system of three lodranites has been investigated. Samples of Gibson yielded no isochrons, and late model ages are attributed to late addition of iodine. Two metal and one silicate separate from the transitional lodranite Graves Nunataks (GRA) 95209 gave ages that are consistent with each other and with the literature I-Xe age of Acapulco feldspar. These yield a mean closure age 4.19 +/- 0.53 Ma after the Shallowater enstatite reference age (4562.3 +/- 0.4 Ma). Such identical I-Xe ages from distinct phases imply that the parent material underwent a period of rapid cooling, the absolute age of this event being 4558.1 +/- 0.7 Ma. Such rapid cooling indicates an increase in the rate at which heat could be conducted away, requiring a significant modification of the parent body. We suggest the parent body was modified by an impact at or close to the time recorded by the I-Xe system. An age of 10.4 +/- 2.3 Ma after Shallowater has been determined for one whole-rock sample of Lewis Cliff (LEW) 88280. Since the release pattern is similar to that of GRA 95209 this hints that the larger grain size of this sample may reflect slower cooling due to deeper post impact burial.
dc.language.isoen
dc.publisherThe Meteoritical Society
dc.relation.urlhttps://meteoritical.org/
dc.rightsCopyright © The Meteoritical Society
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjectcooling rates
dc.subjectlodranites meteorites
dc.subjectIodine-xenon ages
dc.titleCollisional modification of the acapulcoite/lodranite parent body revealed by the iodine-xenon system in lodranites
dc.typeArticle
dc.typetext
dc.identifier.journalMeteoritics & Planetary Science
dc.description.collectioninformationThe Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information.
dc.eprint.versionFinal published version
dc.description.admin-noteMigrated from OJS platform February 2021
dc.source.volume44
dc.source.issue8
dc.source.beginpage1151
dc.source.endpage1159
refterms.dateFOA2021-02-12T22:53:48Z


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