期刊
METEORITICS & PLANETARY SCIENCE
卷 51, 期 9, 页码 1588-1610出版社
WILEY
DOI: 10.1111/maps.12684
关键词
-
资金
- Department of Space, Government of India
- [MLP-6513-28-EVB]
- [INDEX-WP-2.1]
Tissint, a new unaltered piece of Martian volcanic materials, is the most silica-poor and Mg-Fe-rich igneous rock among the depleted olivine-phyric shergottites. Fe-Mg zoning of olivine suggests equilibrium growth (<0.1 degrees Ch(-1)) in the range of Fo(80-56) and olivine overgrowth (Fo(55-18)) through a process of rapid disequilibrium (similar to 1.0-5.0 degrees Ch(-1)). The spatially extended (up to 600 m) flat-top Fe-Mg profiles of olivine indicates that the early-stage cooling rate of Tissint was slower than the other shergottites. The chemically metastable outer rim of olivine (
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