期刊
GEOCHEMISTRY GEOPHYSICS GEOSYSTEMS
卷 15, 期 3, 页码 619-633出版社
AMER GEOPHYSICAL UNION
DOI: 10.1002/2013GC005128
关键词
Mantle convection; Viscosity structure; Primordial material; CMB heat flow; thermal evolution
资金
- JSPS [25800254]
- Grants-in-Aid for Scientific Research [25800254] Funding Source: KAKEN
A thermo-chemical mantle convection model with both primordial compositional layering and recycling of mid-ocean ridge basalt (MORB) coupled to a parameterized core heat balance model is used to investigate how the thermo-chemical evolution of the mantle affects the thermal history of the core including primordial material proposed by early Earth hypotheses. The viscosity formulation has been improved from our previous works. The amount of MORB that accumulates above the CMB is strongly dependent on effective Rayleigh number, such that more accumulates at higher Ra (lower viscosity), but a continuous layer of MORB is not obtained here. With initial primordial layering, large-scale thermo-chemical anomalies are found in the deep mantle, which are generated mainly by the primordial material with small amount of segregated basaltic material on top of it, localized in the hot upwelling region. A successful core evolution can only be obtained when initial primordial layering is present. In conclusion, primordial material above the CMB originated from early mantle differentiation might be needed to construct a realistic model of a coupled mantle and core evolution. However, in the current study, the convective vigor is lower than realistic and we only consider the case that primordial material is denser than MORB.
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