INTER-PLANETARY DUST - TRACE-ELEMENT ANALYSIS OF INDIVIDUAL PARTICLES BY NEUTRON-ACTIVATION

被引：26

作者：

GANAPATHY, R ^{[1
]}

BROWNLEE, DE ^{[1
]}

机构：

[1] UNIV WASHINGTON, DEPT ASTRON, SEATTLE, WA 98195 USA

来源：

SCIENCE | 1979年 / 206卷 / 4422期

关键词：

D O I：

10.1126/science.206.4422.1075

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Although micrometeorites of cometary origin are thought to be the dominant component of interplanetary dust, it has never been possible to positively identify such micrometer-sized particles. Two such particles have been identified as definitely micrometeorites since their abundances of volatile and nonvolatile trace elements closely match those of primitive solar system material. Copyright © 1979 AAAS.

引用

页码：1075 / 1077

页数：3

共 14 条

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[3] BROWNLEE DE, 1977, P LUNAR PLANET SCI C, V8, P149
[4] FRAUNDORF P, P LUNAR SCI C
[5] GANAPATHY R, UNPUBLISHED
[6] GANAPATHY R, 1970, GEOCHIM COSM SUPPL, V34, P1117
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[8] THERMAL METAMORPHISM OF PRIMITIVE METEORITES .5. 10 TRACE-ELEMENTS IN TIESCHITZ H-3 CHONDRITE HEATED AT 400-1000-DEGREES-C
IKRAMUDDIN, M
MATZA, S
LIPSCHUTZ, ME
[J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 1977, 41 (09) : 1247 - 1256
[9] ABUNDANCE OF 17 TRACE-ELEMENTS IN CARBONACEOUS CHONDRITES
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GANAPATH.R
ANDERS, E
[J]. GEOCHIMICA ET COSMOCHIMICA ACTA, 1973, 37 (05) : 1353 - 1370
[10] Mason B., 1971, HDB ELEMENTAL ABUNDA

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