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  • 1
    Online-Ressource
    Online-Ressource
    Geological Society of America ; 2013
    In:  Geology Vol. 41, No. 5 ( 2013-5), p. 531-534
    In: Geology, Geological Society of America, Vol. 41, No. 5 ( 2013-5), p. 531-534
    Materialart: Online-Ressource
    ISSN: 1943-2682 , 0091-7613
    Sprache: Englisch
    Verlag: Geological Society of America
    Publikationsdatum: 2013
    ZDB Id: 184929-3
    ZDB Id: 2041152-2
    SSG: 13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 2
    Online-Ressource
    Online-Ressource
    American Geophysical Union (AGU) ; 2016
    In:  Journal of Geophysical Research: Planets Vol. 121, No. 6 ( 2016-06), p. 1026-1053
    In: Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 121, No. 6 ( 2016-06), p. 1026-1053
    Kurzfassung: Structural rim uplift is the dominant factor to build up the total amount of the final crater rim Structural rim uplift contributes four fifths to the total elevation of crater rims Target uplift at the position of the final crater rim was established during the excavation stage
    Materialart: Online-Ressource
    ISSN: 2169-9097 , 2169-9100
    URL: Issue
    Sprache: Englisch
    Verlag: American Geophysical Union (AGU)
    Publikationsdatum: 2016
    ZDB Id: 1086497-0
    ZDB Id: 3094268-8
    ZDB Id: 2016810-X
    SSG: 16,13
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 3
    In: Meteoritics & Planetary Science, Wiley, Vol. 52, No. 9 ( 2017-09), p. 1822-1842
    Kurzfassung: The Duolun basin, which is located in Inner Mongolia, China, has been proposed to be an impact structure with an apparent rim diameter of about 70, or even 170 km. The designation as an impact structure was based on its nearly circular topography, consisting of an annular moat that surrounds an inner hummocky region, and the widespread occurrences of various igneous rocks, polymict breccias, and deformed crustal rocks. Critical shock metamorphic evidence is not available to support the impact hypothesis. We conducted two independent reconnaissance field surveys to this area and studied the lithology both within and outside of the ring structure. We collected samples from all lithologies that might contain evidence of shock metamorphism as suggested by their locations, especially those sharing similar appearances with impact breccias, suevites, impact melt rocks, and shatter cones. Field investigation, together with thin‐section examination, discovered that the suspected impact melt rocks are actually Early Cretaceous and Late Jurassic lava flows and pyroclastic deposits of rhyolitic to trachytic compositions, and the interpreted impact glass is typical volcanic glass. Petrographic analyses of all the samples reveal no indications for shock metamorphic overprint. All these lines of evidence suggest that the Duolun basin was not formed through impact cratering. The structural deformation and spatial distribution pattern of the igneous rocks suggest that the Duolun basin is most likely a Jurassic–Cretaceous complex rhyolite caldera system that has been partly filled with sediments forming an annular basin, followed by resurgent doming of the central area.
    Materialart: Online-Ressource
    ISSN: 1086-9379 , 1945-5100
    URL: Issue
    Sprache: Englisch
    Verlag: Wiley
    Publikationsdatum: 2017
    ZDB Id: 2011097-2
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 4
    Online-Ressource
    Online-Ressource
    Wiley ; 2017
    In:  Meteoritics & Planetary Science Vol. 52, No. 7 ( 2017-07), p. 1351-1370
    In: Meteoritics & Planetary Science, Wiley, Vol. 52, No. 7 ( 2017-07), p. 1351-1370
    Kurzfassung: The investigation of terrestrial impact structures is crucial to gain an in‐depth understanding of impact cratering processes in the solar system. Here, we use the impact structure Jebel Waqf as Suwwan, Jordan, as a representative for crater formation into a layered sedimentary target with contrasting rheology. The complex crater is moderately eroded (300–420 m) with an apparent diameter of 6.1 km and an original rim fault diameter of 7 km. Based on extensive field work, IKONOS imagery, and geophysical surveying we present a novel geological map of the entire crater structure that provides the basis for structural analysis. Parametric scaling indicates that the structural uplift (250–350 m) and the depth of the ring syncline ( 〈 200 m) are anomalously low. The very shallow relief of the crater along with a NE vergence of the asymmetric central uplift and the enhanced deformations in the up‐range and down‐range sectors of the annular moat and crater rim suggest that the impact was most likely a very oblique one (~20°). One of the major consequences of the presence of the rheologically anisotropic target was that extensive strata buckling occurred during impact cratering both on the decameter as well as on the hundred‐meter scale. The crater rim is defined by a circumferential normal fault dipping mostly toward the crater. Footwall strata beneath the rim fault are bent‐up in the down‐range sector but appear unaffected in the up‐range sector. The hanging wall displays various synthetic and antithetic rotations in the down‐range sector but always shows antithetic block rotation in the up‐range sector. At greater depth reverse faulting or folding is indicated at the rim indicating that the rim fault was already formed during the excavation stage.
    Materialart: Online-Ressource
    ISSN: 1086-9379 , 1945-5100
    URL: Issue
    Sprache: Englisch
    Verlag: Wiley
    Publikationsdatum: 2017
    ZDB Id: 2011097-2
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 5
    In: Meteoritics & Planetary Science, Wiley, Vol. 54, No. 10 ( 2019-10), p. 2448-2482
    Kurzfassung: The 26 km diameter Nördlinger Ries is a complex impact structure with a ring structure that resembles a peak ring. A first research drilling through this “inner crystalline ring” of the Ries was performed at the Erbisberg hill ( SW Ries) to better understand the internal structure and lithology of this feature, and possibly reveal impact‐induced hydrothermal alteration. The drill core intersected the slope of a 22 m thick postimpact travertine mound, before entering 42 m of blocks and breccias of crystalline rocks excavated from the Variscan basement at 〉 500 m depth. Weakly shocked gneiss blocks that show that shock pressure did not exceed 5 GPa occur above polymict lithic breccias of shock stage Ia (10–20 GPa), with planar fractures and planar deformation features ( PDF s) in quartz. Only a narrow zone at 49.20–50.00 m core depth exhibits strong mosaicism in feldspar and {10 2} PDF s in quartz, which are indicative of shock stage Ib (20–35 GPa). Finally, 2 m of brecciated Keuper sediments at the base of the section point to an inverse layering of strata. While reverse grading of clast sizes in lithic breccias and gneiss blocks is consistent with lateral transport, the absence of diaplectic glass and melt products argues against dynamic overthrusting of material from a collapsing central peak, as seen in the much larger Chicxulub structure. Indeed, weakly shocked gneiss blocks are rather of local provenance (i.e., the transient crater wall), whereas moderately shocked polymict lithic breccias with geochemical composition and 87 Sr/ 86 Sr signature similar to Ries suevite were derived from a position closer to the impact center. Thus, the inner ring of the Ries is formed by moderately shocked polymict lithic breccias likely injected into the transient crater wall during the excavation stage and weakly shocked gneiss blocks of the collapsing transient crater wall that were emplaced during the modification stage. While the presence of an overturned flap is not evident from the Erbisberg drilling, a survey of all drillings at or near the inner ring point to inverted strata throughout its outer limb. Whether the central ring of the Ries represents remains of a collapsed central peak remains to be shown. Postimpact hydrothermal alteration along the Erbisberg section comprises chloritization, sulfide veinlets, and strong carbonatization. In addition, a narrow zone in the lower parts of the polymict lithic breccia sequence shows a positive Eu anomaly in its carbonate phase. The surface expression of this hydrothermal activity, i.e., the travertine mound, comprises subaerial as well as subaquatic growth phases. Intercalated lake sediments equivalent to the early parts of the evolution of the central crater basin succession confirm a persistent impact‐generated hydrothermal activity, although for less time than previously suggested.
    Materialart: Online-Ressource
    ISSN: 1086-9379 , 1945-5100
    URL: Issue
    Sprache: Englisch
    Verlag: Wiley
    Publikationsdatum: 2019
    ZDB Id: 2011097-2
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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  • 6
    Online-Ressource
    Online-Ressource
    Wiley ; 2015
    In:  Meteoritics & Planetary Science Vol. 50, No. 1 ( 2015-01), p. 141-171
    In: Meteoritics & Planetary Science, Wiley, Vol. 50, No. 1 ( 2015-01), p. 141-171
    Kurzfassung: The Ries crater is a well‐preserved, complex impact crater that has been extensively used in the study of impact crater formation processes across the solar system. However, its geologic structure, especially the megablock zone, still poses questions regarding crater formation mechanics. The megablock zone, located between the inner crystalline ring and outer, morphologic crater rim, consists of allochthonous crystalline and sedimentary blocks, Bunte Breccia deposits, patches of suevite, and parautochthonous sedimentary blocks that slumped into the crater during crater modification. Our remote sensing detection method in combination with a shallow drilling campaign and geoelectric measurements at two selected megablocks proved successful in finding new megablock structures ( 〉 25 m mean diameter) within the upper approximately 1.5 m of the subsurface in the megablock zone. We analyzed 1777 megablocks of the megablock zone, 81 of which are new discoveries. In our statistical analysis, we also included 2318 ejecta blocks 〉 25 m beyond the crater rim. Parautochthonous megablocks show an increase in total area and size toward the final crater rim. The sizes of allochthonous megablocks generally decrease with increasing radial range, but inside the megablock zone, the coverage with postimpact sediments obscures this trend. The size‐frequency distribution of all megablocks obeys a power‐law distribution with an exponent between approximately −1.7 and −2.3. We estimated a total volume of 95 km 3 of Bunte Breccia and 47 km 3 of megablocks. Ejecta volume calculations and a palinspastic restoration of the extension within the megablock zone indicate that the transient cavity diameter was probably 14–15 km.
    Materialart: Online-Ressource
    ISSN: 1086-9379 , 1945-5100
    URL: Issue
    Sprache: Englisch
    Verlag: Wiley
    Publikationsdatum: 2015
    ZDB Id: 2011097-2
    SSG: 16,12
    Standort Signatur Einschränkungen Verfügbarkeit
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