The effect of ilmenite viscosity on the dynamics and evolution of an   overturned lunar cumulate mantle

doi:10.1002/2017GL073702

CORC > 北京大学 > 地球与空间科学学院

	The effect of ilmenite viscosity on the dynamics and evolution of an overturned lunar cumulate mantle
	Zhang, Nan ; Dygert, Nick ; Liang, Yan ; Parmentier, E. M.
刊名	GEOPHYSICAL RESEARCH LETTERS
	2017
关键词	GIANT IMPACT MOONS INTERIOR MARE BASALTS SEISMIC DATA ORIGIN CONSTRAINTS CONVECTION MOONQUAKES ASYMMETRY VOLCANISM
DOI	10.1002/2017GL073702
英文摘要	Lunar cumulate mantle overturn and the subsequent upwelling of overturned mantle cumulates provide a potential framework for understanding the first-order thermochemical evolution of the Moon. Upwelling of ilmenite-bearing cumulates (IBCs) after the overturn has a dominant influence on the dynamics and long-term thermal evolution of the lunar mantle. An important parameter determining the stability and convective behavior of the IBC is its viscosity, which was recently constrained through rock deformation experiments. To examine the effect of IBC viscosity on the upwelling of overturned lunar cumulate mantle, here we conduct three-dimensional mantle convection models with an evolving core superposed by an IBC-rich layer, which resulted from mantle overturn after magma ocean solidification. Our modeling shows that a reduction of mantle viscosity by 1 order of magnitude, due to the presence of ilmenite, can dramatically change convective planform and long-term lunar mantle evolution. Our model results suggest a relatively stable partially molten IBC layer that has surrounded the lunar core to the present day. Plain Language Summary The Moon's mantle is locally ilmenite rich. Previous models exploring the convective evolution of the lunar mantle did not consider the effects of ilmenite viscosity. Recent rock deformation experiments demonstrate that Fe-Ti oxide (ilmenite) is a low viscosity phase compared to olivine and other silicate minerals. Our modeling shows that ilmenite changes the lunar mantle plume process. An ilmenite-rich layer around the lunar core would be highly stable throughout geologic time, consistent with a partially molten, low viscosity layer around the core inferred from seismic attenuation and tidal dissipation.; NASA [SSERVI NNA14AB01A]; Jackson School of Geosciences Postdoctoral Fellowship; Peking University; Center for Computation and Visualization at Brown University; Pawsey Supercomputing Centre; Australian Government; Government of Western Australia; SCI(E); ARTICLE; 13; 6543-6552; 44
语种	英语
内容类型	期刊论文
源URL	[http://ir.pku.edu.cn/handle/20.500.11897/472120]
专题	地球与空间科学学院
推荐引用方式 GB/T 7714	Zhang, Nan,Dygert, Nick,Liang, Yan,et al. The effect of ilmenite viscosity on the dynamics and evolution of an overturned lunar cumulate mantle[J]. GEOPHYSICAL RESEARCH LETTERS,2017.
APA	Zhang, Nan,Dygert, Nick,Liang, Yan,&Parmentier, E. M..(2017).The effect of ilmenite viscosity on the dynamics and evolution of an overturned lunar cumulate mantle.GEOPHYSICAL RESEARCH LETTERS.
MLA	Zhang, Nan,et al."The effect of ilmenite viscosity on the dynamics and evolution of an overturned lunar cumulate mantle".GEOPHYSICAL RESEARCH LETTERS (2017).