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NSF Forms - Ridge 2000 Program

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PROJECT SUMMARY<br />

Intellectual Merit: We propose an intensive U-series study of volcanics from the Lau<br />

back-arc basin, which is an Integrated Study Site (ISS) for the <strong>Ridge</strong><strong>2000</strong> program. The Eastern<br />

Lau Spreading Center provides a natural experiment thanks to progressive change in the distance<br />

of the spreading center from the trench from south to north. Recent cruises have led to detailed<br />

maps, the discovery and characterization of five new vent fields, and closely spaced rock<br />

sampling. The rock sampling has led to the best sampled back-arc basin spreading center, with<br />

precisely located, axial samples in a well determined tectonic context. Extensive major element,<br />

trace element, volatile element and isotopic data have been obtained for these samples. This<br />

exceptional sample collection, the new comprehensive data set, and the unique tectonic context of<br />

the Lau spreading centers provide new opportunities for U-series studies.<br />

We propose measurements of U, Th and Ra isotopes with two major goals: (1) To constrain<br />

the origin and transport time of subduction components. Excesses akin to convergent margin<br />

lavas are a characteristic aspect of back-arc basin lavas and distinguish them from open ocean<br />

spreading centers. Published data from convergent margins appear to require distinct time scales<br />

from U-Th and Ra-Th isotopes, and have correlations of 238 U and 226 Ra excesses with subduction<br />

signatures such as Ba/Th. Further from the trench at back-arcs, the time scales for fluid transport<br />

should differ. We have the entire range of U/Th ratios at diverse distances from the arc. Do<br />

these relationships between U-series excesses and subduction components change with arc<br />

distance, and can they be used to constrain fluid transport times from slab to surface? Our<br />

existing geochemical data also provide evidence for two distinct fluid compositions, and<br />

systematic correlations between U-Th systematics and long-lived radiogenic isotopes. Thus we<br />

have the potential to further constrain both the origin of the U-series excesses, and the timing<br />

between creation of these excesses and surface eruption. (2) To provide the necessary age<br />

constraints for further development and understanding of the ISS. Age constraints are essential to<br />

relate volcanic activity to tectonics, variations in the underlying magma chamber reflector, and<br />

temporal changes in lava compositions. They also are an essential link between the volcanic<br />

system and the hydrothermal and biological activities that are supported and impacted by<br />

fluctuations in volcanism. Questions such as whether segments have been recently active,<br />

whether there is a relationship between lava age and the presence of magma chamber reflectors,<br />

how age distribution may vary with subduction input cannot begin to be addressed without age<br />

constraints. While “model ages” as applied on the EPR may not be applicable in this region, age<br />

constraints from U-series can still be obtained, and are essential for a host of questions and<br />

hypotheses for the <strong>Ridge</strong> system from mantle to microbe. We thus propose measurement of 40<br />

samples for U-Th-Ra measurements, and 5-10 samples for 210 Pb measurements to identify<br />

eruptions that may be

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