Density, porosity and magnetic susceptibility of the Košice meteorite shower and homogeneity of its parent meteoroid

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dc.contributor.author Kohout, Tomas
dc.contributor.author Havrila, Karol
dc.contributor.author Toth, Juraj
dc.contributor.author Husarik, Marek
dc.contributor.author Gritsevich, Maria
dc.contributor.author Britt, Daniel
dc.contributor.author Borovicka, Jiri
dc.contributor.author Spurny, Pavel
dc.contributor.author Igaz, Antal
dc.contributor.author Svoren, Jan
dc.contributor.author Kornos, Leonard
dc.contributor.author Veres, Peter
dc.contributor.author Koza, Julius
dc.contributor.author Zigo, Pavol
dc.contributor.author Gajdos, Stefan
dc.contributor.author Vilagi, Jozef
dc.contributor.author Capek, David
dc.contributor.author Krisandova, Zuzana
dc.contributor.author Tomko, Dusan
dc.contributor.author Silha, Jiri
dc.contributor.author Schunova, Eva
dc.contributor.author Bodnarova, Marcela
dc.contributor.author Buzova, Diana
dc.contributor.author Krejcova, Tereza
dc.date.accessioned 2014-10-17T21:17:45Z
dc.date.available 2014-10-17T21:17:45Z
dc.date.issued 2014
dc.identifier.citation Kohout , T , Havrila , K , Toth , J , Husarik , M , Gritsevich , M , Britt , D , Borovicka , J , Spurny , P , Igaz , A , Svoren , J , Kornos , L , Veres , P , Koza , J , Zigo , P , Gajdos , S , Vilagi , J , Capek , D , Krisandova , Z , Tomko , D , Silha , J , Schunova , E , Bodnarova , M , Buzova , D & Krejcova , T 2014 , ' Density, porosity and magnetic susceptibility of the Košice meteorite shower and homogeneity of its parent meteoroid ' , Planetary and Space Science , vol. 93-94 , pp. 96-100 . https://doi.org/10.1016/j.pss.2014.02.003
dc.identifier.other PURE: 37026503
dc.identifier.other PURE UUID: 061f3218-a280-456a-b753-44fe2d46cf37
dc.identifier.other WOS: 000335278000010
dc.identifier.other Scopus: 84898436735
dc.identifier.other ORCID: /0000-0003-4458-3650/work/29570889
dc.identifier.other ORCID: /0000-0003-4268-6277/work/29574363
dc.identifier.uri http://hdl.handle.net/10138/136208
dc.description.abstract Bulk and grain density, porosity, and magnetic susceptibility of 67 individuals of Košice H chondrite fall were measured. The mean bulk and grain densities were determined to be 3.43 g/cm3 with standard deviation (s.d.) of 0.11 g/cm3 and 3.79 g/cm3 with s.d. 0.07 g/cm3, respectively. Porosity is in the range from 4.2 to 16.1%. The logarithm of the apparent magnetic susceptibility (in 10−9 m3/kg) shows narrow distribution from 5.17 to 5.49 with mean value at 5.35 with s.d. 0.08. These results indicate that all studied Košice meteorites are of the same composition down to ∼g scale without presence of foreign (non-H) clasts and are similar to other H chondrites. Košice is thus a homogeneous meteorite fall derived from a homogenous meteoroid. en
dc.language.iso eng
dc.relation.ispartof Planetary and Space Science
dc.rights.uri info:eu-repo/semantics/openAccess
dc.subject 115 Astronomy, Space science
dc.subject METEORITE
dc.subject H CHONDRITE
dc.subject DENSITY
dc.subject POROSITY
dc.subject KOSICE
dc.title Density, porosity and magnetic susceptibility of the Košice meteorite shower and homogeneity of its parent meteoroid en
dc.type Article
dc.contributor.organization Department of Physics
dc.contributor.organization Planetary-system research
dc.description.reviewstatus Peer reviewed
dc.relation.doi https://doi.org/10.1016/j.pss.2014.02.003
dc.relation.issn 0032-0633
dc.rights.accesslevel openAccess
dc.type.version acceptedVersion
dc.identifier.url http://www.sciencedirect.com/science/article/pii/S0032063314000373

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