T. Kuhn et al., ORIGIN OF NEGATIVE CE ANOMALIES IN MIXED HYDROTHERMAL-HYDROGENETIC FE-MN CRUSTS FROM THE CENTRAL INDIAN RIDGE, Earth and planetary science letters, 163(1-4), 1998, pp. 207-220
Layered Fe-Mn crusts from the off-axis region of the first segment of
the Central Indian Ridge north of the Rodrigues Triple Junction were s
tudied geochemically and mineralogically. Vernadite (delta-MnO2) is th
e main mineral oxide phase. Th-230(xs) and Co concentrations suggest h
igh growth rates of up to 29 mm/Myr and a maximum age of the basal cru
st layer of 1 Ma. Whereas most of the major and minor elements show co
ncentrations which are typical of hydrogenetic formation, Co, Pb, Ni a
nd Ti concentrations are strikingly lower. Concentrations and distribu
tion of the strictly trivalent rare-earths and yttrium (REY) are typic
al of hydrogenetic ferromanganese oxide precipitates, but in marked co
ntrast, the crusts are characterized by negative Ce-SN (shale-normaliz
ed) anomalies and (Ce/Pr)(SN) ratios less than unity. Profiles through
the crusts reveal only minor variations of the REY distribution and (
Ce/Pr)(SN) ratios range from 0.45 to 0.68 (compared to ratios of up to
2 for typical hydrogenetic crusts from the Central Indian Basin). The
apparent bulk partition coefficients between the crusts and seawater
suggest that for the strictly trivalent REY the adsorption-desorption
equilibrium has been reached. Positive Ce anomalies in the partition c
oefficient patterns reveal preferential uptake of Ce, but to a lesser
extent than in normal hydrogenetic crusts. A new parameter (excess Ce,
Ce-xs) to quantify the degree of decoupling of Ce from REY(III) is es
tablished on the basis of partition coefficients. Ce-xs/Ce-bulk ratios
suggest that the CIR crusts formed by precipitation of Fe-Mn oxides f
rom a hydrothermal plume and that in hydrothermal plumes and normal se
awater the enrichment of Ce results from the same oxidative sorption p
rocess. The growth rates, calculated with Th-230(xs) data as well as w
ith the Co formula, are inversely related to Ce-xs. (C) 1998 Elsevier
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