Description
The beginning of our Solar System, including events such as the formation of the first solids as well as the accretion and differentiation of planetary bodies, is recorded in meteoritic material. This record can be deciphered using petrographic, geochemical and isotopic investigations of different classes of meteorites and their components.
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Contributors
- Mane, Prajkta (Author)
- Wadhwa, Meenakshi (Thesis advisor)
- Hervig, Richard (Committee member)
- Desch, Steven (Committee member)
- Garvie, Laurence (Committee member)
- Bell, James (Committee member)
- Arizona State University (Publisher)
Date Created
The date the item was original created (prior to any relationship with the ASU Digital Repositories.)
2016
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Note
- Partial requirement for: Ph.D., Arizona State University, 2016Note typethesis
- Includes bibliographical references (pages 134-154)Note typebibliography
- Field of study: Geological sciences
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Statement of Responsibility
by Prajkta Mane