ISOTOPE SYSTEMATICS AND SHOCK-WAVE METAMORPHISM .1. U-PB IN ZIRCON, TITANITE, AND MONAZITE, SHOCKED EXPERIMENTALLY UP TO 59 GPA

被引:61
作者
DEUTSCH, A
SCHARER, U
机构
[1] UNIV QUEBEC,DEPT SCI TERRE,MONTREAL H3C 3P8,QUEBEC,CANADA
[2] UNIV QUEBEC,GEOTOP,MONTREAL H3C 3P8,QUEBEC,CANADA
基金
加拿大自然科学与工程研究理事会;
关键词
D O I
10.1016/0016-7037(90)90295-V
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
This study reports the first U-Pb isotope analyses on experimentally shocked zircon, titanite, and monazite from Proterozoic granitoid rocks. In all three types of minerals, shock-waves produce drastic changes in the crystal lattices, causing strong lowering of birefringence, turbidization, and decolorization of the individual grains. Moreover, X-ray patterns indicate transition of the crystals into polycrystalline aggregates of < 10(-5) mm block-size. Precisely dated grains with concordant or nearly concordant ages were embedded in KBr and shocked at 35, 47.5, and 59 GPa. U-Pb isotope analyses on these grains show that shock metamorphism does not fractionate Pb isotopes within the analytical precision of +/- 0.1%. As far as chemical fractionation is concerned, there is no difference in degree of concordancy between shocked and unshocked monazite, and small degrees (< 2%) of relative U/Pb fractionation in shocked zircon and titanite are due to time-integrated Pb-loss and not to shock experiment. In consequence, the data document that shock-wave metamorphism alone does not measurably effect the U-Pb chronometer, questioning the view that lower intercept ages of discordant U-Pb data reflect shock-induced re-equilibration of the chronometer in moderately to highly shocked, rapidly cooling rocks.
引用
收藏
页码:3427 / 3434
页数:8
相关论文
共 50 条
[1]  
ABERG G, 1985, EARTH PLANET SC LETT, V74, P347, DOI 10.1016/S0012-821X(85)80006-6
[2]   SHOCK EFFECTS AND ARGON LOSS IN SAMPLES OF THE LEEDEY L6 CHONDRITE EXPERIMENTALLY SHOCKED TO 29-70 GPA PRESSURES [J].
BOGARD, D ;
HORZ, F ;
JOHNSON, P .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1987, 51 (07) :2035-2044
[3]   NOBLE-GAS CONTENTS OF SHERGOTTITES AND IMPLICATIONS FOR THE MARTIAN ORIGIN OF SNC METEORITES [J].
BOGARD, DD ;
NYQUIST, LE ;
JOHNSON, P .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1984, 48 (09) :1723-1739
[4]  
BOGARD DD, 1989, GEOCHIM COSMOCHIM AC, V52, P2639
[5]   FORMATION AGES AND EVOLUTION OF SHERGOTTY AND ITS PARENT PLANET FROM U-TH-PB SYSTEMATICS [J].
CHEN, JH ;
WASSERBURG, GJ .
GEOCHIMICA ET COSMOCHIMICA ACTA, 1986, 50 (06) :955-968
[6]  
Compston W., 1984, J GEOPHYS RES, V89, pB525, DOI DOI 10.1029/JB089IS02P0B525
[7]   STRONTIUM-ISOTOPIC AND NEODYMIUM-ISOTOPIC CHARACTERISTICS OF A HETEROLITHIC BRECCIA IN THE BASEMENT OF THE SUDBURY IMPACT STRUCTURE, CANADA [J].
DEUTSCH, A ;
LAKOMY, R ;
BUHL, D .
EARTH AND PLANETARY SCIENCE LETTERS, 1989, 93 (3-4) :359-370
[8]  
DEUTSCH A, 1989, EUROP J MINERAL S, V1, P31
[9]  
DEUTSCH A, 1987, LUNAR PLANET SCI C, V18, P237
[10]  
Dressler B.O., 1984, GEOL ORE DEPOSIT+, V1, P97