TY - JOUR
T1 - Tungsten geochemistry and implications for understanding the Earth's interior
AU - Arevalo, Ricardo
AU - McDonough, William F.
N1 - Funding Information:
We would like to thank the Division of Petrology and Volcanology, Department of Mineral Sciences, Smithsonian Institute, especially Leslie Hale, Sorena Sorenson and the late Jim Luhr, for providing us with so many precious samples to conduct this study. We also appreciate the sample donations generously afforded by Michael Garcia, Thomas Ireland, Emily Klein, Charles Langmuir, Gaby Loock, Yaoling Niu, Marc Norman, and Michael Perfit. This study could not have been conducted without the analytical prowess of Richard Ash, who helped us develop the analytical protocol for our LA-ICP-MS method, or the helpful reviews of Rick Carlson, James Day, John Lassiter, Adam Mansur, Carsten Münker, Sune Nielsen, and Richard Walker. Special thanks go to Thorsten Kleine and Tetsuya Yokoyama for their assistance with developing our W isotope dilution procedures. This study was funded by NSF grant # 0337621 and #0739006.
PY - 2008/8/15
Y1 - 2008/8/15
N2 - The concentration of tungsten (W) in basaltic melts provides a window into the behavior of this element during core-mantle separation, crust formation, silicate differentiation, and potentially core-mantle interaction. We have analyzed an extensive suite of modern basalts (n = 86) for their trace element chemistry via laser ablation ICP-MS, with barium (Ba), thorium (Th), uranium (U), and W concentrations typically determined to ≤ 5% (2σ) uncertainty. We find that the partitioning behavior of U mirrors that of W during basalt genesis, whereas Ba and Th both behave more incompatibly. The W/U ratio of our complete sample suite (0.65 ± 0.45, 2σ) is representative of the mean modern mantle, and is indistinguishable from that of mid-ocean ridge basalts (W/UMORB = 0.65 ± 0.41, n = 52), ocean island basalts (W/UOIB = 0.63 ± 0.07, n = 10), and back-arc basin basalts (W/UBABB = 0.62 ± 0.09, n = 12). This ratio is also consistent with the W/U ratio of the continental crust, and thus represents the W/U ratio of the entire silicate portion of the Earth. Assuming a concentration of 20 ± 8 (2σ) ng/g U in the bulk silicate Earth, the abundance of W in the silicate Earth is 13 ± 10 ng/g. Following mass balance, this implies a mean modern mantle and core composition of 8.3 ± 7.1 ng/g W and 500 ± 120 ng/g W, respectively. Additionally, the MORB source is modeled to contain approximately 3.0 ± 2.3 ng/g W, indicating a four-fold depletion of the highly incompatible elements in the MORB source relative to the silicate Earth. Although both the isotopic composition of W and the constancy of the silicate Earth W/U ratio allow for potential insight into core-mantle exchange, both of these proxies are extremely dependent on the chemical composition of the source. A case study of three Hawaiian picrites with enrichments in 186Os-187Os but terrestrial ε182W can be explained by: i) a lack of a core component in the Hawaiian "plume," ii) crustal contamination, or iii) a source composition enriched in incompatible trace elements relative to the bulk silicate Earth.
AB - The concentration of tungsten (W) in basaltic melts provides a window into the behavior of this element during core-mantle separation, crust formation, silicate differentiation, and potentially core-mantle interaction. We have analyzed an extensive suite of modern basalts (n = 86) for their trace element chemistry via laser ablation ICP-MS, with barium (Ba), thorium (Th), uranium (U), and W concentrations typically determined to ≤ 5% (2σ) uncertainty. We find that the partitioning behavior of U mirrors that of W during basalt genesis, whereas Ba and Th both behave more incompatibly. The W/U ratio of our complete sample suite (0.65 ± 0.45, 2σ) is representative of the mean modern mantle, and is indistinguishable from that of mid-ocean ridge basalts (W/UMORB = 0.65 ± 0.41, n = 52), ocean island basalts (W/UOIB = 0.63 ± 0.07, n = 10), and back-arc basin basalts (W/UBABB = 0.62 ± 0.09, n = 12). This ratio is also consistent with the W/U ratio of the continental crust, and thus represents the W/U ratio of the entire silicate portion of the Earth. Assuming a concentration of 20 ± 8 (2σ) ng/g U in the bulk silicate Earth, the abundance of W in the silicate Earth is 13 ± 10 ng/g. Following mass balance, this implies a mean modern mantle and core composition of 8.3 ± 7.1 ng/g W and 500 ± 120 ng/g W, respectively. Additionally, the MORB source is modeled to contain approximately 3.0 ± 2.3 ng/g W, indicating a four-fold depletion of the highly incompatible elements in the MORB source relative to the silicate Earth. Although both the isotopic composition of W and the constancy of the silicate Earth W/U ratio allow for potential insight into core-mantle exchange, both of these proxies are extremely dependent on the chemical composition of the source. A case study of three Hawaiian picrites with enrichments in 186Os-187Os but terrestrial ε182W can be explained by: i) a lack of a core component in the Hawaiian "plume," ii) crustal contamination, or iii) a source composition enriched in incompatible trace elements relative to the bulk silicate Earth.
KW - basalt
KW - concentration ratio
KW - core
KW - mantle
KW - tungsten
KW - uranium
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U2 - 10.1016/j.epsl.2008.05.031
DO - 10.1016/j.epsl.2008.05.031
M3 - Article
AN - SCOPUS:48149102301
SN - 0012-821X
VL - 272
SP - 656
EP - 665
JO - Earth and Planetary Science Letters
JF - Earth and Planetary Science Letters
IS - 3-4
ER -