Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias

Dieter Stöffler; Heinz-Dieter Knöll; W.-U. Reimold; S. Schulien

Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias

Dieter Stöffler
, Heinz-Dieter Knöll
, W.-U. Reimold
, S. Schulien

Universität Münster

Publikation: Beiträge in Sammelwerken › Aufsätze in Konferenzbänden › Forschung › Begutachtung

Abstract

It is found that the clast population of metabreccias 14006, 14311, 14320, and 14321 has the grain size properties of an extremely immature lunar impact detritus, probably developed by reworking. The modal composition of the mineral clast population and the An- and Fe-derived content of plagioclase clasts indicate that the clastic material of the breccias is derived from three types of igneous rocks: KREEP and high-alumina basalt, anorthositic-noritic-troctolitic rocks, and possibly mare-type basalt.

Originalsprache	Englisch
Titel	7th Lunar Science Conference : Proceedings
Redakteure/-innen	Lunar Science Institute
Seitenumfang	21
Band	2
Herausgeber (Verlag)	Pergamon Press
Erscheinungsdatum	1976
Seiten	1965-1985
ISBN (Print)	9780080217710
Publikationsstatus	Erschienen - 1976
Extern publiziert	Ja
Veranstaltung	Lunar and Planetary Science Conference 1976 - Houston, USA / Vereinigte Staaten Dauer: 15.03.1976 → 19.03.1976 Konferenznummer: 7

Fachgebiete und Schlagwörter

Chemie

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http://adsabs.harvard.edu/abs/1976LPSC....7.1965SLizenz: Urheberrechtlich geschützt

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title = "Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias",

abstract = "It is found that the clast population of metabreccias 14006, 14311, 14320, and 14321 has the grain size properties of an extremely immature lunar impact detritus, probably developed by reworking. The modal composition of the mineral clast population and the An- and Fe-derived content of plagioclase clasts indicate that the clastic material of the breccias is derived from three types of igneous rocks: KREEP and high-alumina basalt, anorthositic-noritic-troctolitic rocks, and possibly mare-type basalt.",

keywords = "Chemistry",

author = "Dieter St{\"o}ffler and Heinz-Dieter Kn{\"o}ll and W.-U. Reimold and S. Schulien",

year = "1976",

language = "English",

isbn = "9780080217710",

volume = "2",

pages = "1965--1985",

editor = "\{Lunar Science Institute\}",

booktitle = "7th Lunar Science Conference",

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note = "Lunar and Planetary Science Conference 1976 ; Conference date: 15-03-1976 Through 19-03-1976",

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Stöffler, D, Knöll, H-D, Reimold, W-U & Schulien, S 1976, Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias. in LSI (Hrsg.), 7th Lunar Science Conference: Proceedings. Bd. 2, Pergamon Press, S. 1965-1985, Lunar and Planetary Science Conference 1976 , Houston, USA / Vereinigte Staaten, 15.03.76. <http://adsabs.harvard.edu/abs/1976LPSC....7.1965S>

Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias. / Stöffler, Dieter; Knöll, Heinz-Dieter; Reimold, W.-U. et al.
7th Lunar Science Conference: Proceedings. Hrsg. / Lunar Science Institute. Band 2 Pergamon Press, 1976. S. 1965-1985.

Publikation: Beiträge in Sammelwerken › Aufsätze in Konferenzbänden › Forschung › Begutachtung

TY - CHAP

T1 - Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias

AU - Stöffler, Dieter

AU - Knöll, Heinz-Dieter

AU - Reimold, W.-U.

AU - Schulien, S.

N1 - Conference code: 7

PY - 1976

Y1 - 1976

N2 - It is found that the clast population of metabreccias 14006, 14311, 14320, and 14321 has the grain size properties of an extremely immature lunar impact detritus, probably developed by reworking. The modal composition of the mineral clast population and the An- and Fe-derived content of plagioclase clasts indicate that the clastic material of the breccias is derived from three types of igneous rocks: KREEP and high-alumina basalt, anorthositic-noritic-troctolitic rocks, and possibly mare-type basalt.

AB - It is found that the clast population of metabreccias 14006, 14311, 14320, and 14321 has the grain size properties of an extremely immature lunar impact detritus, probably developed by reworking. The modal composition of the mineral clast population and the An- and Fe-derived content of plagioclase clasts indicate that the clastic material of the breccias is derived from three types of igneous rocks: KREEP and high-alumina basalt, anorthositic-noritic-troctolitic rocks, and possibly mare-type basalt.

KW - Chemistry

UR - http://adsabs.harvard.edu/abs/1976LPSC....7.1965S

M3 - Article in conference proceedings

SN - 9780080217710

VL - 2

SP - 1965

EP - 1985

BT - 7th Lunar Science Conference

A2 - , Lunar Science Institute

PB - Pergamon Press

T2 - Lunar and Planetary Science Conference 1976

Y2 - 15 March 1976 through 19 March 1976

ER -

Grain size statistics, composition and provenance of fragmental particles in some Apollo 14 breccias

Abstract

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