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151215 ||| eng |
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|a 9783662484791
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|a Xie, Xiande
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245 |
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|a Suizhou Meteorite: Mineralogy and Shock Metamorphism
|h Elektronische Ressource
|c by Xiande Xie, Ming Chen
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250 |
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|a 1st ed. 2016
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260 |
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|a Berlin, Heidelberg
|b Springer Berlin Heidelberg
|c 2016, 2016
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300 |
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|a XIV, 258 p. 168 illus., 17 illus. in color
|b online resource
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|a General introduction of the Suizhou meteorite -- Micro-mineralogical investigative techniques -- Mineralogy of unmelted chondritic rock -- Distinct morphological and petrological features of the Suizhou shock veins.- Mineralogy of Suizhou shock veins -- Shock-induced redistribution of trace elements.- Evaluation of shock stage for Suizhou meteorite -- P-T history of the Suizhou meteorite
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653 |
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|a Planetary Science
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653 |
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|a Planetary science
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653 |
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|a Mineralogy
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653 |
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|a Space Physics
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653 |
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|a Solar system
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700 |
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|a Chen, Ming
|e [author]
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|a eng
|2 ISO 639-2
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|b Springer
|a Springer eBooks 2005-
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|a Springer Geochemistry/Mineralogy
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|a 10.1007/978-3-662-48479-1
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|u https://doi.org/10.1007/978-3-662-48479-1?nosfx=y
|x Verlag
|3 Volltext
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|a 549
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|a This book introduces the unusual shock-related mineralogical features of the shocked Suizhou L6 (S5) meteorite. The olivine and pyroxene in Suizhou display a mosaic shock feature, while most of plagioclase grains have transformed to glassy maskelynite. A few of the shock-induced melt veins in the meteorite are the simplest, straightest and thinnest ones among all shock-vein-bearing meteorites, and contain the most abundant high-pressure mineral species. Among the 11 identified species, tuite, xieite, and the post-spinel CF-phase of chromite are new minerals. The meteorite experienced a peak shock pressure up to 24 GPa and temperatures of up to 1000° C. Locally developed shock veins were formed at the same pressure, but at an elevated temperature of about 2000° C that was produced by localized shear-friction stress. The rapid cooling of the extremely thin shock veins is the main reason why 11 shock-induced high-pressure mineral phases could be preserved in them so well. This book offersa helpful guide for meteoritics researchers and mineralogists and invaluable resource for specialists working in high-pressure and high-temperature mineralophysics
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