ORIGIN AND EVOLUTION OF THE NAKHLA METEORITE INFERRED FROM THE SM-ND AND U-PB SYSTEMATICS AND REE, BA, SR, RB AND K ABUNDANCES

被引：126

作者：

NAKAMURA, N

UNRUH, DM

TATSUMOTO, M

HUTCHISON, R

机构：

[1] US GEOL SURVEY, DENVER, CO 80225 USA

[2] BRITISH MUSEUM NAT HIST, DEPT MINERAL, LONDON SW7 5BD, ENGLAND

来源：

关键词：

D O I：

10.1016/0016-7037(82)90314-3

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：

引用

页码：1555 / 1573

页数：19

共 90 条

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[83] Weill D. F., 1975, P LUNAR PLANET SCI C, P1143
[84] WEILL DF, 1974, P LUNAR PLANET SCI C, P1337
[85] WHERE DO METEORITES COME FROM - RE-EVALUATION OF EARTH-CROSSING APOLLO OBJECTS AS SOURCES OF CHONDRITIC METEORITES
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[J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 1976, 40 (11) : 1297 - 1317
[86] Wood C., 1981, LUNAR PLANET SCI, V12, P1197
[87] RARE GASES IN STONY METEORITES
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