The Tucson ungrouped iron meteorite and its relationship to chondrites

Autores
Kurat, G.; Varela, Maria Eugenia; Zinner, E.; Brandstäetter, F.
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Tucson is an enigmatic ataxitic iron meteorite, an assemblage of reduced silicates embedded in Fe-Ni metal with dissolved Si and Cr. Both, silicates and metal, contain a record of formation at high temperature (∼1800 K) and fast cooling. The latter resulted in the preservation of abundant glasses, Al-rich pyroxenes, brezinaite, and fine-grained metal. Our chemical and petrographic studies of all phases (minerals and glasses) indicate that they have a nebular rather than an igneous origin and give support to a chondritic connection as suggested by Prinz et al. (1987). All silicate phases in Tucson apparently grew from a liquid that had refractory trace elements at approximately 6–20 × CI abundances with nonfractionated (solar) pattern, except for Sc, which was depleted (∼1 × CI). Metal seems to have precipitated before and throughout silicate aggregate formation, allowing preservation of all evolutionary steps of the silicates by separating them from the environment. In contrast to most chondrites, Tucson documents coprecipitation of metal and silicates from the solar nebula gas and precipitation of metal before silicates—in accordance with theoretical condensation calculations for high-pressure solar nebula gas. We suggest that Tucson is the most metal-rich and volatile-element-poor member of the CR chondrite clan.
Fil: Kurat, G.. Universidad de Viena; Austria. Naturhistorisches Museum; Austria
Fil: Varela, Maria Eugenia. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Zinner, E.. Washington University in St. Louis; Estados Unidos
Fil: Brandstäetter, F.. Naturhistorisches Museum; Austria
Materia
Tucson Meteorite
Genesis
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/12975

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spelling The Tucson ungrouped iron meteorite and its relationship to chondritesKurat, G.Varela, Maria EugeniaZinner, E.Brandstäetter, F.Tucson MeteoriteGenesishttps://purl.org/becyt/ford/1.7https://purl.org/becyt/ford/1Tucson is an enigmatic ataxitic iron meteorite, an assemblage of reduced silicates embedded in Fe-Ni metal with dissolved Si and Cr. Both, silicates and metal, contain a record of formation at high temperature (∼1800 K) and fast cooling. The latter resulted in the preservation of abundant glasses, Al-rich pyroxenes, brezinaite, and fine-grained metal. Our chemical and petrographic studies of all phases (minerals and glasses) indicate that they have a nebular rather than an igneous origin and give support to a chondritic connection as suggested by Prinz et al. (1987). All silicate phases in Tucson apparently grew from a liquid that had refractory trace elements at approximately 6–20 × CI abundances with nonfractionated (solar) pattern, except for Sc, which was depleted (∼1 × CI). Metal seems to have precipitated before and throughout silicate aggregate formation, allowing preservation of all evolutionary steps of the silicates by separating them from the environment. In contrast to most chondrites, Tucson documents coprecipitation of metal and silicates from the solar nebula gas and precipitation of metal before silicates—in accordance with theoretical condensation calculations for high-pressure solar nebula gas. We suggest that Tucson is the most metal-rich and volatile-element-poor member of the CR chondrite clan.Fil: Kurat, G.. Universidad de Viena; Austria. Naturhistorisches Museum; AustriaFil: Varela, Maria Eugenia. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; ArgentinaFil: Zinner, E.. Washington University in St. Louis; Estados UnidosFil: Brandstäetter, F.. Naturhistorisches Museum; AustriaMeteoritical Soc2010-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/12975Kurat, G.; Varela, Maria Eugenia; Zinner, E.; Brandstäetter, F.; The Tucson ungrouped iron meteorite and its relationship to chondrites; Meteoritical Soc; Meteoritics & Planetary Science; 45; 12; 12-2010; 1982-20061086-9379enginfo:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2010.01134.x/abstractinfo:eu-repo/semantics/altIdentifier/doi/10.1111/j.1945-5100.2010.01134.xinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T14:27:56Zoai:ri.conicet.gov.ar:11336/12975instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-10-15 14:27:56.475CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv The Tucson ungrouped iron meteorite and its relationship to chondrites
title The Tucson ungrouped iron meteorite and its relationship to chondrites
spellingShingle The Tucson ungrouped iron meteorite and its relationship to chondrites
Kurat, G.
Tucson Meteorite
Genesis
title_short The Tucson ungrouped iron meteorite and its relationship to chondrites
title_full The Tucson ungrouped iron meteorite and its relationship to chondrites
title_fullStr The Tucson ungrouped iron meteorite and its relationship to chondrites
title_full_unstemmed The Tucson ungrouped iron meteorite and its relationship to chondrites
title_sort The Tucson ungrouped iron meteorite and its relationship to chondrites
dc.creator.none.fl_str_mv Kurat, G.
Varela, Maria Eugenia
Zinner, E.
Brandstäetter, F.
author Kurat, G.
author_facet Kurat, G.
Varela, Maria Eugenia
Zinner, E.
Brandstäetter, F.
author_role author
author2 Varela, Maria Eugenia
Zinner, E.
Brandstäetter, F.
author2_role author
author
author
dc.subject.none.fl_str_mv Tucson Meteorite
Genesis
topic Tucson Meteorite
Genesis
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.7
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Tucson is an enigmatic ataxitic iron meteorite, an assemblage of reduced silicates embedded in Fe-Ni metal with dissolved Si and Cr. Both, silicates and metal, contain a record of formation at high temperature (∼1800 K) and fast cooling. The latter resulted in the preservation of abundant glasses, Al-rich pyroxenes, brezinaite, and fine-grained metal. Our chemical and petrographic studies of all phases (minerals and glasses) indicate that they have a nebular rather than an igneous origin and give support to a chondritic connection as suggested by Prinz et al. (1987). All silicate phases in Tucson apparently grew from a liquid that had refractory trace elements at approximately 6–20 × CI abundances with nonfractionated (solar) pattern, except for Sc, which was depleted (∼1 × CI). Metal seems to have precipitated before and throughout silicate aggregate formation, allowing preservation of all evolutionary steps of the silicates by separating them from the environment. In contrast to most chondrites, Tucson documents coprecipitation of metal and silicates from the solar nebula gas and precipitation of metal before silicates—in accordance with theoretical condensation calculations for high-pressure solar nebula gas. We suggest that Tucson is the most metal-rich and volatile-element-poor member of the CR chondrite clan.
Fil: Kurat, G.. Universidad de Viena; Austria. Naturhistorisches Museum; Austria
Fil: Varela, Maria Eugenia. Consejo Nacional de Investigaciones Cientificas y Tecnicas. Centro Cientifico Tecnologico San Juan. Instituto de Ciencias Astronomicas de la Tierra y del Espacio; Argentina
Fil: Zinner, E.. Washington University in St. Louis; Estados Unidos
Fil: Brandstäetter, F.. Naturhistorisches Museum; Austria
description Tucson is an enigmatic ataxitic iron meteorite, an assemblage of reduced silicates embedded in Fe-Ni metal with dissolved Si and Cr. Both, silicates and metal, contain a record of formation at high temperature (∼1800 K) and fast cooling. The latter resulted in the preservation of abundant glasses, Al-rich pyroxenes, brezinaite, and fine-grained metal. Our chemical and petrographic studies of all phases (minerals and glasses) indicate that they have a nebular rather than an igneous origin and give support to a chondritic connection as suggested by Prinz et al. (1987). All silicate phases in Tucson apparently grew from a liquid that had refractory trace elements at approximately 6–20 × CI abundances with nonfractionated (solar) pattern, except for Sc, which was depleted (∼1 × CI). Metal seems to have precipitated before and throughout silicate aggregate formation, allowing preservation of all evolutionary steps of the silicates by separating them from the environment. In contrast to most chondrites, Tucson documents coprecipitation of metal and silicates from the solar nebula gas and precipitation of metal before silicates—in accordance with theoretical condensation calculations for high-pressure solar nebula gas. We suggest that Tucson is the most metal-rich and volatile-element-poor member of the CR chondrite clan.
publishDate 2010
dc.date.none.fl_str_mv 2010-12
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/12975
Kurat, G.; Varela, Maria Eugenia; Zinner, E.; Brandstäetter, F.; The Tucson ungrouped iron meteorite and its relationship to chondrites; Meteoritical Soc; Meteoritics & Planetary Science; 45; 12; 12-2010; 1982-2006
1086-9379
url http://hdl.handle.net/11336/12975
identifier_str_mv Kurat, G.; Varela, Maria Eugenia; Zinner, E.; Brandstäetter, F.; The Tucson ungrouped iron meteorite and its relationship to chondrites; Meteoritical Soc; Meteoritics & Planetary Science; 45; 12; 12-2010; 1982-2006
1086-9379
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://onlinelibrary.wiley.com/doi/10.1111/j.1945-5100.2010.01134.x/abstract
info:eu-repo/semantics/altIdentifier/doi/10.1111/j.1945-5100.2010.01134.x
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Meteoritical Soc
publisher.none.fl_str_mv Meteoritical Soc
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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