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School of Engineering and Science - Jacobs University

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modern <strong>and</strong> Archean oceans, as well as for Eu, which indicates a greater contribution to<br />

Archean seawater from high-T hydrothermal fluids (e.g., Figs. 4,5). It should be noted<br />

that the small negative Ce anomaly in the shallow water Holocene reef carbonates<br />

relative to world seawater is not inconsistent, as very shallow seawater <strong>of</strong>ten displays<br />

smaller negative Ce anomalies compared to bulk seawater (e.g., de Baar et al., 1983).<br />

The fact that Archean IFs commonly have seawater-like REY distributions is not<br />

consistent with REY scavenging by Fe-oxyhydroxides in a manner similar to that<br />

observed in modern oceans. As shown in Fig. 8, adsorption-desorption reactions at<br />

equilibrium strongly fractionate the REY between metal-oxides <strong>and</strong> seawater. If<br />

Archean IFs precipitated from seawater as Fe(III) minerals, then their observed REY<br />

distributions would require quantitative scavenging <strong>of</strong> all REY in solution, perhaps in a<br />

manner analogous to the laboratory co-precipitation <strong>of</strong> REE-Fe-oxide phases from<br />

seawater in early studies (e.g., Goldberg et al., 1963). However, the exact nature <strong>of</strong> the<br />

primary IF precipitate remains unresolved, though data presented in Chapter 4 suggests<br />

that initial deposition <strong>of</strong> Fe(II) mineral phases may have been important. Regardless, the<br />

seawater-like REY distributions in Archean IFs, <strong>and</strong> the lack <strong>of</strong> other suitable archives,<br />

indicates that IFs <strong>of</strong>fer the best opportunity for discerning the Nd isotopic composition<br />

<strong>of</strong> >2.7 Ga seawater.<br />

26

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