Complex Formation History of Highly Evolved Basaltic Shergottite, ZagamiZagami, a basaltic shergottite, contains several kinds of lithologies such as Normal Zagami consisting of Fine-grained (FG) and Coarse-grained (CG), Dark Mottled lithology (DML), and Olivine-rich late-stage melt pocket (DN). Treiman and Sutton concluded that Zagami (Normal Zagami) is a fractional crystallization product from a single magma. It has been suggested that there were two igneous stages (deep magma chamber and shallow magma chamber or surface lava flow) on the basis of chemical zoning features of pyroxenes which have homogeneous Mg-rich cores and FeO, CaO zoning at the rims. Nyquist et al. reported that FG has a different initial Sr isotopic ratio than CG and DML, and suggested the possibility of magma mixing on Mars. Here we report new results of petrology and mineralogy for DML and the Olivine-rich lithology (we do not use DN here), the most evolved lithology in this rock, to understand the relationship among lithologies and reveal Zagami s formation history
Document ID
20120011726
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Niihara, T. (Lunar and Planetary Inst. Houston, TX, United States)
Misawa, K. (National Inst. of Polar Research Tokyo, Japan)
Mikouchi, T. (Tokyo Univ. Japan)
Nyquist, L. E. (NASA Johnson Space Center Houston, TX, United States)
Park, J. (Rutgers Univ. NJ, United States)
Hirata, D. (Museum of Natural History Kanagawa, Japan)
Date Acquired
August 26, 2013
Publication Date
January 1, 2012
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-CN-26537Report Number: JSC-CN-26537
Meeting Information
Meeting: 75th annual Metting of the Meteoritical Society
Location: Cairns
Country: Australia
Start Date: August 12, 2012
End Date: August 17, 2012
Sponsors: Meteoritical Society, NASA Johnson Space Center, Lunar and Planetary Inst.