Computer Science
Scientific paper
Mar 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27...81b&link_type=abstract
Lunar and Planetary Science, volume 27, page 81
Computer Science
Basalt: Mare, Isotopes: Hafnium, Mantle
Scientific paper
The Lu-Hf isotopic system is ideally suited for determining the mineralogy of source regions because of the large mineral dependent Lu-Hf fractionations that occur during partial melting and crystallization. However, because of the analytical challenges of Hf isotopic analysis the Lu-Hf isotope system has not been widely applied to studies of petrogenesis. We have developed a new technique for Hf isotopic analysis and Lu and Hf concentration determination by isotope dilution mass-spectrometry that is ideally suited for Lu-Hf isotopic analysis of high-Ti basaltic rocks. Using this technique we have analyzed 5 high-Ti mare basalts; 2 Apollo 11 samples with high epsilon (sub)Nd values and 3 Apollo 17 samples with low epsilon (sub)Nd values. These new data complement the existing Hf isotopic analyses of high-Ti basalts, which consist of 4 Apollo 11 samples with low epsilon (sub)Nd values and 3 Apollo 17 samples with high epsilon (sub)Nd values. This combined data set clearly demonstrates that the Hf isotopic composition of high-Ti basalts is relatively constant over a range of epsilon (sub)Nd values. The Hf - Nd isotopic array of high-Ti basalts is in marked contrast to the Hf - Nd isotopic data of low-Ti basalts which defines a strong positive correlation with epsilon (sub)Hf = 4epislon (sub)Nd. The differences for the Hf and Nd isotopic arrays of low- and high-Ti basalts implies that the low- and high-Ti basalt source regions have been distinct over nearly the entire history of the Moon. Moreover, these source regions must have formed with distinctly different mineralogies.
Beard Brian L.
Johnson Matthew C.
Scherer Erik E.
Snyder Glenn A.
Taylor Lawrence A.
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