Insufficient Energy From MgO Exsolution to Power Early Geodynamo
- Carnegie Inst. of Washington, Washington, DC (United States)
- Carnegie Inst. of Washington, Washington, DC (United States); Smithsonian Inst., Washington, DC (United States). National Museum of Natural History
- Yale Univ., New Haven, CT (United States)
- Univ. of Chicago, IL (United States). Center for Advanced Radiation Sources (CARS)
The origin of Earth's ancient magnetic field is an outstanding problem. It has recently been proposed that exsolution of MgO from the core may provide sufficient energy to drive an early geodynamo. Here, in this work, we present new experiments on Mg partitioning between iron-rich liquids and silicate/oxide melts. Our results indicate that Mg partitioning depends strongly on the oxygen content in the iron-rich liquid, in contrast to previous findings that it depends only on temperature. Consequently, MgO exsolution during core cooling is drastically reduced and insufficient to drive an early geodynamo alone. Using the new experimental data, our thermal model predicts inner core nucleation at ~850 Ma and a nearly constant paleointensity.
- Research Organization:
- Argonne National Laboratory (ANL), Argonne, IL (United States). Advanced Photon Source (APS)
- Sponsoring Organization:
- Carnegie Fellowship; National Science Foundation (NSF); USDOE Office of Science (SC), Basic Energy Sciences (BES). Chemical Sciences, Geosciences, and Biosciences Division
- Grant/Contract Number:
- EAR-1447311; EAR-1321956; EAR-1551348; EAR-1128799; FG02-94ER14466; AC02-06CH11357; AC02‐06CH11357
- OSTI ID:
- 1423342
- Alternate ID(s):
- OSTI ID: 1410579
- Journal Information:
- Geophysical Research Letters, Vol. 44, Issue 22; ISSN 0094-8276
- Publisher:
- American Geophysical UnionCopyright Statement
- Country of Publication:
- United States
- Language:
- ENGLISH
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