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The cosmic-ray exposure history of the Twannberg iron meteorite (IIG)

dc.contributor.authorSmith, T.
dc.contributor.authorHofmann, B.
dc.contributor.authorLeya, I.
dc.contributor.authorMerchel, S.
dc.contributor.authorPavetich, Stefan
dc.contributor.authorRugel, G.
dc.contributor.authorScharf, A.
dc.date.accessioned2020-01-20T05:06:06Z
dc.date.issued2017-07-27
dc.date.updated2022-07-24T08:20:19Z
dc.description.abstractThe Twannberg iron meteorite is one out of only six members of the group IIG. The combined noble gas and radionuclide data obtained in this new systematic study indicate that Twannberg with its ~570 recently recovered specimens was a large object with a preatmospheric radius in the range of ~2 m, which corresponds to ~250 × 103 kg. The cosmic-ray exposure age for Twannberg is 182 ± 45 Ma. The most surprising result is the long terrestrial age of Tterr = math formula ka, which is unexpected considering the humid conditions in Switzerland. However, this age is in accord with glaciation events, indicating that the less shielded samples from Mt. Sujet were found close to the position of the original strewn field, whereas the samples from Gruebmatt and Twannbach, which are from more shielded positions, were glacially transported to the east–northeast during the second last ice age (185–130 ka ago) from an original position west of Mt. Sujet.
dc.description.sponsorshipThis work is supported bythe Swiss National Science Foundation (SNF).en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn1086-9379en_AU
dc.identifier.urihttp://hdl.handle.net/1885/198731
dc.language.isoen_AUen_AU
dc.publisherUniversity of Arkansas
dc.rights© 2017 The Meteoritical Society
dc.sourceMeteoritics and Planetary Science
dc.titleThe cosmic-ray exposure history of the Twannberg iron meteorite (IIG)
dc.typeJournal article
dcterms.dateAccepted2017-05-31
local.bibliographicCitation.lastpage17en_AU
local.bibliographicCitation.startpage1en_AU
local.contributor.affiliationSmith, T., University of Bernen_AU
local.contributor.affiliationHofmann, B., Naturhistorisches Museum der Burgergemeinde Bernen_AU
local.contributor.affiliationLeya, I., University of Bernen_AU
local.contributor.affiliationMerchel, S., Helmholtz Institute Freiberg for Resource Technologyen_AU
local.contributor.affiliationPavetich, Stefan, College of Science, ANUen_AU
local.contributor.affiliationRugel, G., Helmholtz Institute Freiberg for Resource Technologyen_AU
local.contributor.affiliationScharf, A., Helmholtz-Zentrum Dresden-Rossendorfen_AU
local.contributor.authoruidPavetich, Stefan, u1010673en_AU
local.description.embargo2037-12-31
local.description.notesImported from ARIESen_AU
local.identifier.absfor020202 - Nuclear Physicsen_AU
local.identifier.ariespublicationa383154xPUB7541en_AU
local.identifier.citationvolumeOnline Version
local.identifier.doi10.1111/maps.12928en_AU
local.identifier.scopusID2-s2.0-85026299290
local.identifier.thomsonIDWOS:000412173600010
local.publisher.urlhttps://onlinelibrary.wiley.comen_AU
local.type.statusPublished Versionen_AU

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