| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 4679156 | Earth and Planetary Science Letters | 2009 | 13 Pages |
Abstract
The mantle abundance of W could have been set by single-stage metal-silicate equilibration along the liquidus in a deep peridotite magma ocean at pressures from 20-50 GPa, and at oxygen fugacities consistent with the mantle's present iron budget (IWâ 2 to â 2.5). Equilibration at higher pressure is viable if the core-forming metal contained a significant, but not unreasonable, abundance of carbon (â¼Â 2 wt.%). Recent continuous accretion models involving multi-stage metal-silicate equilibration in a deepening magma ocean with progressive oxidation of the silicate remain permissible given our new treatment of W partitioning data.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Earth and Planetary Sciences (General)
Authors
Elizabeth Cottrell, Michael J. Walter, David Walker,
