HR: 14:55h
AN: V43F-06 INVITED [Abstracts]
TI: Integrated Nd, Hf and Pb View of Mantle Evolution
AU: * Vervoort, J D
EM: vervoort@wsu.edu
AF: Washington State University, School of Earth and Environmental Sciences, Pullman, WA
99164-2812, United States
AB:
Recent developments in the 147,146Sm-143,142Nd and 176Lu-177Hf systems during the
past several years have drastically altered our view of the evolutionary history of the early Earth. These new
developments, in particular from 146Sm-142Nd systematics and the changes in the initial
176Hf/177Hf data for early Archean samples using the lower 176Lu decay constant, have
produced a data set that, on face value, appears to be in conflict and require more complicated models for early
planetary differentiation and subsequent evolution. For example, the record of Hf mantle evolution using previous
decay constant of 1.94 e-11 y-1 was entirely congruent with the Nd isotopic record and broadly
characterized by linear trend of radiogenic values today (εHf, εNd of +16 and +10,
respectively) through slightly radiogenic values for the early Archean (εHf, εNd of ~
+4 and +2) and projecting to chondritic values within the first few 100 m.y. of Earth's history. These data seem to
be explained by a rather straight-forward model with differentiation of the mantle and the development of enriched
and depleted reservoirs. Using the most recent 176Lu decay constant estimates, however, the Hf isotope
record of the oldest terrestrial rocks and zircons is characterized by chondritic to negative initial εHf
values. In contrast, the Nd isotopic record of similar rocks are characterized by positive εNd values.
The 143Nd record is now consistent with constraints from the short-lived isotope 146Sm-142Nd
system which indicate very early and widespread differentiation of the mantle and possibly sequestration of the
enriched component to the hidden mantle. The Pb isotopic record of galenas from the Late Archean Abitibi
greenstone belt of the Superior Province also records a pervasive mantle differentiation event in the first hundred
m.y. of Earth's history and therefore are broadly consistent with the 142Nd and 143Nd data. The
apparent decoupling of the Hf systems with the Nd and Pb systems (if the 176Lu decay constant values are
correct) must reflect processes operating during early differentiation of the planet. This differentiation is
responsible for widespread fractionation of Sm/Nd and production of enriched, low Sm/Nd and depleted, high
Sm/Nd reservoirs, but does not fractionate Lu/Hf effectively between these reservoirs. The 146Sm-
142Nd systematics require sequestration of the early enriched reservoir to an unseen part of the mantle.
This is consistent with the positive εNd values that are characteristic of most Archean terranes.
Post-4.0 Ga, the Nd and Hf isotopic systems behave congruently and record the progressive evolution of enriched
and depleted reservoirs due to Lu/Hf and Sm/Nd fractionations such as we see during mantle melting
processes operating on the Earth today.
DE: 1020 Composition of the continental crust
DE: 1021 Composition of the oceanic crust
DE: 1025 Composition of the mantle
SC: Volcanology, Geochemistry, Petrology [V]
MN: 2007 Fall Meeting