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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Bibliographic Details
Main Author: Valdes, Maria
Other Authors: Debaille, Vinciane
Format: Doctoral Thesis
Language:en
Published: Universite Libre de Bruxelles 2018
Subjects:
Online Access:http://hdl.handle.net/2013/ULB-DIPOT:oai:dipot.ulb.ac.be:2013/276866
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spelling 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
collection NDLTD
language en
format Doctoral Thesis
sources NDLTD
topic Géochimie
Système solaire
Géologie
Géologie et minéralogie
Minéralogie
Pétrologie
Géochronologie
Geochemistry
Cosmochemistry
Calcium isotopes
Mass spectrometry
Layered complex
Meteorites
Moon
Lunar
Isotopes
spellingShingle 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
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