SPHENE AND TiO2 ASSEMBLAGES IN THE CHICXULUB PEAK RING: U-Pb SYSTEMATICS AND IMPLICATIONS FOR SHOCK PRESSURES, TEMPERATURES, AND CRATER COOLING

被引:0
|
作者
Schmieder, M. [1 ,2 ]
Kring, D. A. [1 ,2 ]
Lapen, T. J. [3 ]
Gulick, S. P. S. [4 ]
Stockli, D. F. [4 ]
Rasmussen, C. [5 ]
Rae, A. S. P. [6 ]
Ferriere, L. [7 ]
Poelchau, M. [8 ]
Xiao, L. [9 ]
Wittmann, A. [10 ]
机构
[1] Lunar & Planetary Inst, 3303 NASA Rd 1, Houston, TX 77058 USA
[2] NASA, SSERVI, Moffett Field, CA USA
[3] Univ Houston, Houston, TX 77004 USA
[4] Univ Texas Austin, Austin, TX 78712 USA
[5] Univ Utah, Salt Lake City, UT USA
[6] Imperial Coll, London, England
[7] Natl Hist Museum, Vienna, Austria
[8] Univ Freiburg, Freiburg, Germany
[9] China Univ Geosci, Wuhan, Hubei, Peoples R China
[10] Arizona State Univ, Tempe, AZ USA
关键词
POLYMORPH; RUTILE; COMPRESSION;
D O I
暂无
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
6134
引用
收藏
页码:A308 / A308
页数:1
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