Igneous processes of the early solar system

Thesis (Ph. D. in Geochemistry)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, February 2004.

Bibliographic Details
Main Author: Singletary, Steven J. (Steven James), 1973-
Other Authors: Timothy L. Grove.
Format: Thesis
Language:eng
Published: Massachusetts Institute of Technology 2010
Subjects:
Online Access:http://hdl.handle.net/1721.1/58444
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author Singletary, Steven J. (Steven James), 1973-
author2 Timothy L. Grove.
author_facet Timothy L. Grove.
Singletary, Steven J. (Steven James), 1973-
author_sort Singletary, Steven J. (Steven James), 1973-
collection MIT
description Thesis (Ph. D. in Geochemistry)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, February 2004.
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spelling mit-1721.1/584442019-04-10T18:06:22Z Igneous processes of the early solar system Singletary, Steven J. (Steven James), 1973- Timothy L. Grove. Massachusetts Institute of Technology. Technology, Dept. of Earth, Atmospheric, and Planetary Sciences. Massachusetts Institute of Technology. Technology, Dept. of Earth, Atmospheric, and Planetary Sciences. Technology, Earth, Atmospheric, and Planetary Sciences. Thesis (Ph. D. in Geochemistry)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, February 2004. Includes bibliographical references. Experimental, petrographic and numerical methods are used to explore the igneous evolution of the early solar system. Chapters 1 and 2 detail the results of petrographic and experimental studies of a suite of primitive achondritic meteorites, the ureilites. The first chapter presents data that reveal correlations between mineral modal proportions and mineral chemistry that are used to guide experiments and models of ureilite petrogenesis. Chapter 2 details and applies the experimental results to describe ureilite petrogenesis as the result of progressive heating of a primitive carbon-rich body. The experiments place temperature and depth constraints on uteilite formation of 1100 to 13000C and 5 to 13 MPa - equivalent to the central pressure of an asteroid with a radius of 130 km. Chapter 3 reports the results of melting experiments of Allende carbonaceous chondrite at temperatures and pressures that would be expected on small bodies in the early solar system (up to 1300⁰C and 2.5 to 15 IPa) heated by decay of short lived isotopes. The results are then applied to ureilite petrogenesis and assembly of larger planetary bodies. The final chapter is an experimental study to test a hybridized source region for the high titanium lunar ultramafic glasses. Two models are presented that invoke either a heterogeneous source region or sinking and reaction of an ultramafic, titanium rich magma with underlying mantle regions. by Steven J. Singletary. Ph.D.in Geochemistry 2010-09-03T18:52:52Z 2010-09-03T18:52:52Z 2003 2004 Thesis http://hdl.handle.net/1721.1/58444 61047605 eng M.I.T. theses are protected by copyright. They may be viewed from this source for any purpose, but reproduction or distribution in any format is prohibited without written permission. See provided URL for inquiries about permission. http://dspace.mit.edu/handle/1721.1/7582 172 leaves application/pdf Massachusetts Institute of Technology
spellingShingle Technology, Earth, Atmospheric, and Planetary Sciences.
Singletary, Steven J. (Steven James), 1973-
Igneous processes of the early solar system
title Igneous processes of the early solar system
title_full Igneous processes of the early solar system
title_fullStr Igneous processes of the early solar system
title_full_unstemmed Igneous processes of the early solar system
title_short Igneous processes of the early solar system
title_sort igneous processes of the early solar system
topic Technology, Earth, Atmospheric, and Planetary Sciences.
url http://hdl.handle.net/1721.1/58444
work_keys_str_mv AT singletarystevenjstevenjames1973 igneousprocessesoftheearlysolarsystem