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Plagioclase Compositions of Eucrites and Eucrite-Type AchondritesEucrites are basalts, diabases and gabbros composed of ferroan pigeonite and augite, calcic plagioclase, and a silica phase, with accessory amounts of ilmenite, chromite, Ca-phosphate, troilite, metal and olivine. Many of the gabbroic-textured eucrites are cumulates from a mafic magma, while most other eucrites are close to melt compositions. These are referred to as cumulate and basaltic eucrites. Petrologic, compositional and isotopic studies have identified several mafic achondrites with eucritic mineralogy that have anomalous properties, and some of these are considered to have been derived from different parent asteroids than normal eucrites. These are referred to as eucrite-type achondrites, and they include cumulate and basaltic types. Petrologic studies of eucrites often concentrate on pyroxene compositions to reveal the petrogenetic history of the rocks and plagioclase compositions are less utilized. Here I examine Na and K variations of a suite of basaltic and cumulate eucrites and eucrite-type achondrites.
Document ID
20200001771
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Mittlefehldt, David W.
(NASA Johnson Space Center Houston, TX, United States)
Date Acquired
March 19, 2020
Publication Date
March 16, 2020
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
JSC-E-DAA-TN77046
Report Number: JSC-E-DAA-TN77046
Meeting Information
Meeting: Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: United States
Start Date: March 16, 2020
End Date: March 20, 2020
Sponsors: Lunar and Planetary Institute (LPI)
Distribution Limits
Public
Copyright
Public Use Permitted.
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