Lu-Hf and Sm-Nd Isotopic Studies of Shergottites and Nakhlites: Implications for Martian Mantle SourcesWe present a new Lu-Hf and Sm-Nd isotope systematics study of four enriched shergottites (Zagami, Shergotty, NWA856 and Los Angeles), and three nakhlites (Nakhla, MIL03346 and Yamato 000593) in order to further understand processes occurring during the early differentiation of Mars and the crystallization of its magma ocean. Two fractions of the terrestrial petrological analogue of nakhlites, the Archaean Theo's flow (Ontario, Canada) were also measured. The coupling of Nd and Hf isotopes provide direct insights on the mineralogy of the melt sources. In contrast to Sm/Nd, Lu/Hf ratios can be very large in minerals such as garnet. Selective partial melting of garnet bearing mantle sources can therefore lead to characteristic Lu/Hf signatures that can be recognized with Hf-176/Hf-177Hf ratios.
Document ID
20070009871
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
Debaille, V. (Lunar and Planetary Inst. Houston, TX, United States)
Yin, Q.-Z. (California Univ. Davis, CA, United States)
Brandon, A. D. (NASA Johnson Space Center Houston, TX, United States)
Jacobsen, B. (California Univ. Davis, CA, United States)
Treiman, A. H. (Lunar and Planetary Inst. Houston, TX, United States)