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ELKINS-TANTON, Linda T., PARMENTIER, E. M., HESS, P. C. (2003) Magma ocean fractional crystallization and cumulate overturn in terrestrial planets: Implications for Mars. Meteoritics & Planetary Science, 38 (12) 1753-1771 doi:10.1111/j.1945-5100.2003.tb00013.x

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Reference TypeJournal (article/letter/editorial)
TitleMagma ocean fractional crystallization and cumulate overturn in terrestrial planets: Implications for Mars
JournalMeteoritics & Planetary Science
AuthorsELKINS-TANTON, Linda T.Author
PARMENTIER, E. M.Author
HESS, P. C.Author
Year2003 (December)Volume38
Issue12
PublisherWiley
DOIdoi:10.1111/j.1945-5100.2003.tb00013.xSearch in ResearchGate
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Mindat Ref. ID332104Long-form Identifiermindat:1:5:332104:5
GUID0
Full ReferenceELKINS-TANTON, Linda T., PARMENTIER, E. M., HESS, P. C. (2003) Magma ocean fractional crystallization and cumulate overturn in terrestrial planets: Implications for Mars. Meteoritics & Planetary Science, 38 (12) 1753-1771 doi:10.1111/j.1945-5100.2003.tb00013.x
Plain TextELKINS-TANTON, Linda T., PARMENTIER, E. M., HESS, P. C. (2003) Magma ocean fractional crystallization and cumulate overturn in terrestrial planets: Implications for Mars. Meteoritics & Planetary Science, 38 (12) 1753-1771 doi:10.1111/j.1945-5100.2003.tb00013.x
In(2003, December) Meteoritics & Planetary Science Vol. 38 (12) Wiley

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Elkins-Tanton, L.T., Zaranek, S.E., Parmentier, E.M., Hess, P.C. (2005) Early magnetic field and magmatic activity on Mars from magma ocean cumulate overturn. Earth and Planetary Science Letters, 236 (1) 1-12 doi:10.1016/j.epsl.2005.04.044
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Mandler, Ben E., Elkins-Tanton, Linda T. (2013) The origin of eucrites, diogenites, and olivine diogenites: Magma ocean crystallization and shallow magma chamber processes on Vesta. Meteoritics & Planetary Science, 48 (11) 2333-2349 doi:10.1111/maps.12135
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Brown, Stephanie M., Elkins-Tanton, Linda T., Walker, Richard J. (2014) Effects of magma ocean crystallization and overturn on the development of 142Nd and 182W isotopic heterogeneities in the primordial mantle. Earth and Planetary Science Letters, 408. 319-330 doi:10.1016/j.epsl.2014.10.025
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