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dc.contributor.authorRochette, P.
dc.contributor.authorGattacceca, J.
dc.contributor.authorChevrier, V.
dc.contributor.authorHoffmann, V.
dc.contributor.authorLorand, J. P.
dc.contributor.authorFunaki, M.
dc.contributor.authorHochleitner, R.
dc.date.accessioned2021-02-12T21:17:20Z
dc.date.available2021-02-12T21:17:20Z
dc.date.issued2005-01-01
dc.identifier.citationRochette, P., Gattacceca, J., Chevrier, V., Hoffmann, V., Lorand, J.-P., Funaki, M., & Hochleitner, R. (2005). Matching Martian crustal magnetization and magnetic properties of Martian meteorites. Meteoritics & Planetary Science, 40(4), 529-540.
dc.identifier.issn1945-5100
dc.identifier.doi10.1111/j.1945-5100.2005.tb00961.x
dc.identifier.urihttp://hdl.handle.net/10150/655986
dc.description.abstractMagnetic properties of 26 (of 32) unpaired Martian meteorites (SNCs) are synthesized to further constrain the lithology carrying Martian magnetic crustal sources. Magnetic properties of ultramafic cumulates (i.e., Chassigny, Allan Hills [ALH] 84001) and lherzolitic shergottites (ALH 77005, Lewis Cliff [LEW] 88516) are one or two orders of magnitude too weak to account for the crustal magnetizations, assuming magnetization in an Earth-like field. Nakhlites and some basaltic shergottites, which are the most magnetic SNCs, show the right intensity. Titanomagnetite is the magnetic carrier in the nakhlites (7 meteorites), whereas in most basaltic shergottites (11 meteorites) it is pyrrhotite. Dhofar (Dho) 378, Los Angeles, and NWA 480/1460 and 2046 are anomalous basaltic shergottites, as their magnetism is mainly due to titanomagnetite. Pyrrhotite should be among the candidate minerals for the magnetized Noachian crust.
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.subjectPyrrhotite
dc.subjectMars
dc.subjectMartian meteorites
dc.subjectmagnetite
dc.titleMatching Martian crustal magnetization and magnetic properties of Martian meteorites
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.volume40
dc.source.issue4
dc.source.beginpage529
dc.source.endpage540
refterms.dateFOA2021-02-12T21:17:20Z


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