Chemical and Isotopic Consequences of Lunar Formation via Giant Impact

Chemical and Isotopic Consequences of Lunar Formation via Giant Impact

There is near consensus in the planetary science community that the origin of the Moon can be traced to a massive interplanetary collision between a roughly Mars-sized object and the growing Earth towards the end of planetary accretion. Many in the geochemical community, however, have rightly expre...

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Bibliographic Details
Main Author: Pahlevan, Kaveh
Format: Others
Published: 2010
Online Access:https://thesis.library.caltech.edu/5937/1/thesis-final.pdf
Pahlevan, Kaveh (2010) Chemical and Isotopic Consequences of Lunar Formation via Giant Impact. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/YPP1-AQ73. https://resolver.caltech.edu/CaltechTHESIS:06082010-072824369 <https://resolver.caltech.edu/CaltechTHESIS:06082010-072824369>

Internet

https://thesis.library.caltech.edu/5937/1/thesis-final.pdf
Pahlevan, Kaveh (2010) Chemical and Isotopic Consequences of Lunar Formation via Giant Impact. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/YPP1-AQ73. https://resolver.caltech.edu/CaltechTHESIS:06082010-072824369 <https://resolver.caltech.edu/CaltechTHESIS:06082010-072824369>

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