2008
DOI: 10.1016/j.epsl.2007.10.009
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Where on Earth is the enriched Hadean reservoir?

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Cited by 50 publications
(35 citation statements)
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“…An EER is only needed if the BSE has chondritic relative abundances of refractory lithophile elements (Figure 2). This study and previous studies have identified no geochemical evidence that any surface rock has been derived from the EER [e.g., Boyet and Carlson, 2006;Caro et al, 2006;Andreasen et al, 2008;Murphy et al, 2010]. Either the EER has been convectively isolated from participating in surface magmatism throughout Earth history, or there is no EER and the BSE does not have chondritic relative abundances of the refractory lithophile elements.…”
Section: Resultsmentioning
confidence: 87%
“…An EER is only needed if the BSE has chondritic relative abundances of refractory lithophile elements (Figure 2). This study and previous studies have identified no geochemical evidence that any surface rock has been derived from the EER [e.g., Boyet and Carlson, 2006;Caro et al, 2006;Andreasen et al, 2008;Murphy et al, 2010]. Either the EER has been convectively isolated from participating in surface magmatism throughout Earth history, or there is no EER and the BSE does not have chondritic relative abundances of the refractory lithophile elements.…”
Section: Resultsmentioning
confidence: 87%
“…The reported differences in the isotopic abundances of refractory elements such as barium (Andreasen et al 2008;Carlson et al 2007;Ranen & Jacobsen 2006), neodymium, and samarium (Andreasen & Sharma 2006;Boyet & Carlson 2005;Carlson et al 2007) between bulk meteorites and the Earth, suggest that heterogeneity in the solar nebula was preserved through part of the accretion process. These recent observations support earlier barium isotope measurements of chondrite leaches by Hidaka et al (2003) and contrast to some degree with predictions based on dynamical models that mixing and homogenization of the nebula was highly efficient (cf.…”
Section: Introductionmentioning
confidence: 99%
“…Though the suggestion has been made (Andreasen et al 2008), there is not yet any convincing evidence that the REE will gain siderophile or chalcophile tendencies at the high pressures and temperatures expected for terrestrial core formation. Thus, the abundance of REE in the core is expected to be very low with the implication that fractionation of Sm from Nd by core formation is unlikely.…”
mentioning
confidence: 99%