Geochemistry and Cosmochemistry of Calcium Stable Isotopes
Calcium (Ca) is the fifth most abundant element in the rocky planets. As a lithophile, refractory element, Ca does not partition into planetary cores nor is it volatilized during planetary accretion. These characteristics make Ca ideal for investigating the earliest stages of planetary formation and...
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ndltd-ulb.ac.be-oai-dipot.ulb.ac.be-2013-2768662018-10-01T19:14:50Z info:eu-repo/semantics/doctoralThesis info:ulb-repo/semantics/doctoralThesis info:ulb-repo/semantics/openurl/vlink-dissertation Geochemistry and Cosmochemistry of Calcium Stable Isotopes Valdes, Maria Debaille, Vinciane Mattielli, Nadine Bernard, Alain Goderis, Steven Williams, Helen Moynier, Frédéric Universite Libre de Bruxelles Université libre de Bruxelles, Faculté des Sciences – Sciences de la Terre et de l'Environnement, Bruxelles 2018-09-14 en Calcium (Ca) is the fifth most abundant element in the rocky planets. As a lithophile, refractory element, Ca does not partition into planetary cores nor is it volatilized during planetary accretion. These characteristics make Ca ideal for investigating the earliest stages of planetary formation and the subsequent chemical evolution of planetary mantles and crusts. This thesis presents observations of and explores the mechanisms involved in high-temperature mass-dependent Ca isotope fractionation in terrestrial, lunar, and meteoritic material. Chapter 1 reports Ca isotope fractionation among a co-genetic suite of samples from the Guelb el Azib ultramafic-mafic-anorthosite complex, which represents the fractional crystallization sequence of a terrestrial igneous magma chamber. The measurements imply that Ca isotope fractionation in an evolving crystallizing magma is mineralogically controlled and that the degree of fractionation can vary according to the Ca composition of the residual magma. Chapter 2 investigates ureilites, a distinctive group of achondritic meteorites, widely regarded to be mantle remnants of a disrupted asteroidal parent body. To date, it is not clear which of their features were inherited from the original chondritic body and which were created during post-accretionary igneous processes such as partial melting. This chapter presents evidence that partial melting on the ureilite parent body is responsible for two such ambiguous characteristics, Ca isotopic and magnesium number (Mg Géochimie Système solaire Géologie Géologie et minéralogie Minéralogie Pétrologie Géochronologie Geochemistry Cosmochemistry Calcium isotopes Mass spectrometry Layered complex Meteorites Moon Lunar Isotopes Doctorat en Sciences info:eu-repo/semantics/nonPublished http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/276866 No full-text files |
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en |
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Doctoral Thesis |
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Géochimie Système solaire Géologie Géologie et minéralogie Minéralogie Pétrologie Géochronologie Geochemistry Cosmochemistry Calcium isotopes Mass spectrometry Layered complex Meteorites Moon Lunar Isotopes |
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Géochimie Système solaire Géologie Géologie et minéralogie Minéralogie Pétrologie Géochronologie Geochemistry Cosmochemistry Calcium isotopes Mass spectrometry Layered complex Meteorites Moon Lunar Isotopes Valdes, Maria Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
description |
Calcium (Ca) is the fifth most abundant element in the rocky planets. As a lithophile, refractory element, Ca does not partition into planetary cores nor is it volatilized during planetary accretion. These characteristics make Ca ideal for investigating the earliest stages of planetary formation and the subsequent chemical evolution of planetary mantles and crusts. This thesis presents observations of and explores the mechanisms involved in high-temperature mass-dependent Ca isotope fractionation in terrestrial, lunar, and meteoritic material. Chapter 1 reports Ca isotope fractionation among a co-genetic suite of samples from the Guelb el Azib ultramafic-mafic-anorthosite complex, which represents the fractional crystallization sequence of a terrestrial igneous magma chamber. The measurements imply that Ca isotope fractionation in an evolving crystallizing magma is mineralogically controlled and that the degree of fractionation can vary according to the Ca composition of the residual magma. Chapter 2 investigates ureilites, a distinctive group of achondritic meteorites, widely regarded to be mantle remnants of a disrupted asteroidal parent body. To date, it is not clear which of their features were inherited from the original chondritic body and which were created during post-accretionary igneous processes such as partial melting. This chapter presents evidence that partial melting on the ureilite parent body is responsible for two such ambiguous characteristics, Ca isotopic and magnesium number (Mg === Doctorat en Sciences === info:eu-repo/semantics/nonPublished |
author2 |
Debaille, Vinciane |
author_facet |
Debaille, Vinciane Valdes, Maria |
author |
Valdes, Maria |
author_sort |
Valdes, Maria |
title |
Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
title_short |
Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
title_full |
Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
title_fullStr |
Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
title_full_unstemmed |
Geochemistry and Cosmochemistry of Calcium Stable Isotopes |
title_sort |
geochemistry and cosmochemistry of calcium stable isotopes |
publisher |
Universite Libre de Bruxelles |
publishDate |
2018 |
url |
http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/276866 |
work_keys_str_mv |
AT valdesmaria geochemistryandcosmochemistryofcalciumstableisotopes |
_version_ |
1718757352702738432 |