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Suizhou Meteorite: Mineralogy and Shock Metamorphism

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 me...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autores principales: Xie, Xiande (Autor), Chen, Ming (Autor)
Autor Corporativo: SpringerLink (Online service)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2016.
Edición:1st ed. 2016.
Colección:Springer Geochemistry/Mineralogy,
Temas:
Acceso en línea:Texto Completo

MARC

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245 1 0 |a Suizhou Meteorite: Mineralogy and Shock Metamorphism  |h [electronic resource] /  |c by Xiande Xie, Ming Chen. 
250 |a 1st ed. 2016. 
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300 |a XIV, 258 p. 168 illus., 17 illus. in color.  |b online resource. 
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490 1 |a Springer Geochemistry/Mineralogy,  |x 2194-3184 
505 0 |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. 
520 |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 offers a helpful guide for meteoritics researchers and mineralogists and invaluable resource for specialists working in high-pressure and high-temperature mineralophysics. 
650 0 |a Mineralogy. 
650 0 |a Planetary science. 
650 0 |a Solar system. 
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650 2 4 |a Space Physics. 
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