LEADER 04009nam 22006735 450 001 9910254103903321 005 20200702152203.0 010 $a3-662-48479-X 024 7 $a10.1007/978-3-662-48479-1 035 $a(CKB)3710000000484427 035 $a(EBL)4092237 035 $a(SSID)ssj0001584520 035 $a(PQKBManifestationID)16265360 035 $a(PQKBTitleCode)TC0001584520 035 $a(PQKBWorkID)14864010 035 $a(PQKB)10589529 035 $a(DE-He213)978-3-662-48479-1 035 $a(MiAaPQ)EBC4092237 035 $a(PPN)190524685 035 $a(EXLCZ)993710000000484427 100 $a20150930d2016 u| 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aSuizhou Meteorite: Mineralogy and Shock Metamorphism /$fby Xiande Xie, Ming Chen 205 $a1st ed. 2016. 210 1$aBerlin, Heidelberg :$cSpringer Berlin Heidelberg :$cImprint: Springer,$d2016. 215 $a1 online resource (268 p.) 225 1 $aSpringer Geochemistry/Mineralogy,$x2194-3176 300 $aDescription based upon print version of record. 311 $a3-662-48477-3 320 $aIncludes bibliographical references at the end of each chapters. 327 $aGeneral 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. 330 $aThis book introduces the unusual shock-related mineralogical features of the shocked Suizhou L6 (S5) meteorite. The olivine and pyroxene in Suizhou display a mosaic shock feature, while most of plagioclase grains have transformed to glassy maskelynite. A few of the shock-induced melt veins in the meteorite are the simplest, straightest and thinnest ones among all shock-vein-bearing meteorites, and contain the most abundant high-pressure mineral species. Among the 11 identified species, tuite, xieite, and the post-spinel CF-phase of chromite are new minerals. The meteorite experienced a peak shock pressure up to 24 GPa and temperatures of up to 1000° C. Locally developed shock veins were formed at the same pressure, but at an elevated temperature of about 2000° C that was produced by localized shear-friction stress. The rapid cooling of the extremely thin shock veins is the main reason why 11 shock-induced high-pressure mineral phases could be preserved in them so well. This book offers a helpful guide for meteoritics researchers and mineralogists and invaluable resource for specialists working in high-pressure and high-temperature mineralophysics. 410 0$aSpringer Geochemistry/Mineralogy,$x2194-3176 606 $aMineralogy 606 $aPlanetology 606 $aSpace sciences 606 $aMineralogy$3https://scigraph.springernature.com/ontologies/product-market-codes/G38000 606 $aPlanetology$3https://scigraph.springernature.com/ontologies/product-market-codes/G18010 606 $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030 615 0$aMineralogy. 615 0$aPlanetology. 615 0$aSpace sciences. 615 14$aMineralogy. 615 24$aPlanetology. 615 24$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics). 676 $a549 700 $aXie$b Xiande$4aut$4http://id.loc.gov/vocabulary/relators/aut$0890793 702 $aChen$b Ming$4aut$4http://id.loc.gov/vocabulary/relators/aut 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910254103903321 996 $aSuizhou Meteorite: Mineralogy and Shock Metamorphism$92505879 997 $aUNINA