| タイトル | Mineralogy and Petrology of EK-459-5-1, A Type B1 CAI from Allende |
| 本文（外部サイト） | http://hdl.handle.net/2060/20150001952 |
| 著者（英） | Andreasen, R.; Righter, M.; Ross, D. K.; Lapen, T. J.; Kerekgyarto, A. G.; Jeffcoat, C. R. |
| 著者所属（英） | NASA Johnson Space Center |
| 発行日 | 2015-03-16 |
| 言語 | eng |
| 内容記述 | Calcium-aluminum-rich inclusions (CAIs) are a type of coarse-grained clast composed of Ca-, Al-, and Mg-rich silicates and oxides found in chondrite meteorites. Type B (CAIs) are exclusively found in the CV chondrite meteorites and are the most well studied type of inclusion found in chondritic meteorites. Type B1 CAIs are distinguished by a nearly monomineralic rim of melilite that surrounds an interior predominantly composed of melilite, fassaite (Ti and Al-rich clinopyroxene), anorthite, and spinel with varying amounts of other minor primary and secondary phases. The formation of Type B CAIs has received considerable attention in the course of CAI research and quantitative models, experimental results and observations from Type B inclusions remain largely in disagreement. Recent experimental results and quantitative models have shown that the formation of B1 mantles could have occurred by the evaporative loss of Si and Mg during the crystallization of these objects. However, comparative studies suggest that the lower bulk SiO2 compositions in B1s result in more prior melilite crystallization before the onset of fassaite and anorthite crystallization leading to the formation of thick melilite rich rims in B1 inclusions. Detailed petrographic and cosmochemical studies of these inclusions will further our understanding of these complex objects. |
| NASA分類 | Geosciences (General); Earth Resources and Remote Sensing; Lunar and Planetary Science and Exploration |
| レポートNO | JSC-CN-32839 |
| 権利 | Copyright, Distribution under U.S. Government purpose rights |
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