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
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/12975
Ver los metadatos del registro completo
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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 |
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CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
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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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13.22299 |