نتایج جستجو برای: breccia

تعداد نتایج: 715  

2003
L. Hecht R. T. Schmitt A. Wittmann

Introduction. About 100 m of impactites (suevitetype breccias) have been drilled at the ICDP drill site Yax-1 within the Chicxulub impact structure (see [1] for more information). Post-impact hydrothermal alteration including alkali metasomatism and devitrification of impact melt glass has significantly modified the mineralogy and chemistry of the impact breccia lithologies. Hydrothermal altera...

2009
B. L. Jolliff R. L. Korotev R. A. Zeigler T. H. Prettyman

Introduction: Lunar meteorite Dhofar 961, a complex, lithic-clast-rich impact breccia [1,2], was called out by [3-6] as a candidate for an origin in the South Pole – Aitken (SPA) Basin region of the Moon (the SPA Terrane) on the basis of its relatively mafic, but nonmare lithologic and major-element chemical composition. It also has an incompatible-element signature that differs from the KREEP-...

2003
B. L. Jolliff R. L. Korotev R. A. Zeigler C. Floss

Introduction: Northwest Africa 773 is one of the more unusual lunar meteorites found in recent years because it contains a prominent clast lithology, which appears to be an olivine-rich cumulate [1-4] and because it is a very-low-Ti (VLT) mare breccia with relatively high incompatible-trace-element concentrations and LREE/HREE enrichment [3]. A lunar origin was verified by Fagan and coworkers [...

2009
K. E. Gibson B. L. Jolliff R. A. Zeigler R. L. Korotev

Figure 1: In this x-ray composite image made with the electron microprobe, red represents aluminum, green, magnesium, and blue, iron. A glassy impact-melt vein with several large vesicles cuts through the breccia on the right side. Bx=Breccia, OPB=Olivine Phyric Basalt, OGC=Olivine Gabbro Cumulate TESTING PETROGENETIC RELATIONSHIPS OF THE LUNAR NWA773 METEORITE CLAN WITH NICKEL & COBALT IN OLIV...

2008
Robert W. Kay

The Beaverhead impact structure, in southwestern Montana (44°36-N;112°58'W), was identified recently by the presence of shatter cones and impactitcs in outcrops of Proterozoic sandstones of the Belt Supergroup [1]. The cones occur over an area > 100 km. Because the geologic and tectonic history of this region is long and complex, the outline of the original impact crater is no longer identifiab...

2007
Ludovic FERRIÈRE Christian KOEBERL Wolf Uwe REIMOLD

available online at http://meteoritics.org Drill core LB-08A, Bosumtwi impact structure, Ghana: Petrographic and shock metamorphic studies of material from the central uplift Ludovic FERRIÈRE1*, Christian KOEBERL1, and Wolf Uwe REIMOLD2 1Department of Geological Sciences, University of Vienna, Althanstrasse 14, A-1090 Vienna, Austria 2Mineralogy, Museum of Natural History, Humboldt University, ...

Journal: :Science 2004
Andrew Glikson

Nearly a decade ago, Gorter (1) suggested that the Bedout basement high, offshore Western Australia, might represent an impact structure, in view of the site_s well-defined circular Bouguer anomaly and seismic reflection data indicating a possible ring syncline. Recently, Becker et al. (2), as part of the search for the cause or causes of the mass extinction that marks the Permian-Triassic (P-T...

Journal: :Science 2004
Edwin Gnos Beda A Hofmann Ali Al-Kathiri Silvio Lorenzetti Otto Eugster Martin J Whitehouse Igor M Villa A J Timothy Jull Jost Eikenberg Bernhard Spettel Urs Krähenbühl Ian A Franchi Richard C Greenwood

The lunar meteorite Sayh al Uhaymir 169 consists of an impact melt breccia extremely enriched with potassium, rare earth elements, and phosphorus [thorium, 32.7 parts per million (ppm); uranium, 8.6 ppm; potassium oxide, 0.54 weight percent], and adherent regolith. The isotope systematics of the meteorite record four lunar impact events at 3909 +/- 13 million years ago (Ma), approximately 2800 ...

2005
M. Smith M. M. Grady

The Open University's repository of research publications and other research outputs Halite and stable chlorine isotopes in the Zag H3-6 breccia Journal Article

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