Abstract:Abstract-The Kärdla crater is a 4 km-wide impact structure of Late Ordovician age located on Hiiumaa Island, Estonia. The 455 Ma-old buried crater was formed in shallow seawater in Precambrian crystalline target rocks that were covered with sedimentary rocks. Basement and breccia samples from 13 drill cores were studied mineralogically, petrographically, and geochemically. Geochemical analyses of major and trace elements were performed on 90 samples from allochthonous breccias, sub-crater and surrounding basem… Show more
“…The vertical lines show the average density contrast for marine craters (1 and 3) and for craters formed on land (2 and 4). than 100 m (Puura et al 2004), whereas Tv‰ren and Lockne formed in a water depth of at least 100 m (Ormˆ and Lindstrˆm 2000). From our observations of drill cores from the K‰rdla structure, we conclude that open fractures here are rather rare, but not as rare as in Lockne and Tv‰ren.…”
Section: Comparisons To Other Impact Cratersmentioning
Abstract-The Lockne and Tv‰ren impact craters in Sweden formed in a marine environment during the Ordovician. The contrast in density between the impact breccias and the surrounding target rock of these two craters is significantly lower than what has been found in craters formed in crystalline targets on land. Another marine-target structure, the Estonian K‰rdla structure, demonstrates intermediate contrast in impact breccia and target rock, which we attribute to the interpreted shallowness of the sea at the K‰rdla impact site. We conclude that the main cause for these low-density contrasts is pore and fracture filling of calcite with subordinate quartz and fluorite. Calcite is the most abundant cement, and its density differs most from that of fractured and brecciated bedrock with a low degree of cementation. Furthermore, from the studied cases, it is concluded that the target rock to impact rock contrast is generally the highest in craters formed on land in crystalline targets and the lowest in craters formed at sea, while craters formed on land in sedimentary targets are intermediate. The low density contrasts should decrease the negative gravity anomalies of marine craters.
“…The vertical lines show the average density contrast for marine craters (1 and 3) and for craters formed on land (2 and 4). than 100 m (Puura et al 2004), whereas Tv‰ren and Lockne formed in a water depth of at least 100 m (Ormˆ and Lindstrˆm 2000). From our observations of drill cores from the K‰rdla structure, we conclude that open fractures here are rather rare, but not as rare as in Lockne and Tv‰ren.…”
Section: Comparisons To Other Impact Cratersmentioning
Abstract-The Lockne and Tv‰ren impact craters in Sweden formed in a marine environment during the Ordovician. The contrast in density between the impact breccias and the surrounding target rock of these two craters is significantly lower than what has been found in craters formed in crystalline targets on land. Another marine-target structure, the Estonian K‰rdla structure, demonstrates intermediate contrast in impact breccia and target rock, which we attribute to the interpreted shallowness of the sea at the K‰rdla impact site. We conclude that the main cause for these low-density contrasts is pore and fracture filling of calcite with subordinate quartz and fluorite. Calcite is the most abundant cement, and its density differs most from that of fractured and brecciated bedrock with a low degree of cementation. Furthermore, from the studied cases, it is concluded that the target rock to impact rock contrast is generally the highest in craters formed on land in crystalline targets and the lowest in craters formed at sea, while craters formed on land in sedimentary targets are intermediate. The low density contrasts should decrease the negative gravity anomalies of marine craters.
“…Only samples L-37X and L-6B have substantially lower Na contents relative to K, similar to the samples reported from melt rocks at Brent (Grieve 1978) and Ames (Koeberl et al 1997) impact structures. Moderately enriched values of K, compared to Na, may be the result of vaporization or post-impact hydrothermal processes, as discussed in detail by Puura et al (2004). In our samples, indications of a post-impact hydrothermal influence are ambiguous because the high Cr and Ni abundances in all analyzed samples are associated with rather low levels of As, elevated values of which might indicate hydrothermal activity.…”
Abstract-The Lonar crater, India, is the only well-preserved simple crater on Earth in continental flood basalts; it is excavated in the Deccan trap basalts of Cretaceous-Tertiary age. A representative set of target basalts, including the basalt flows excavated by the crater, and a variety of impact breccias and impact glasses, were analyzed for their major and trace element compositions. Impact glasses and breccias were found inside and outside the crater rim in a variety of morphological forms and shapes. Comparable geochemical patterns of immobile elements (e.g., REEs) for glass, melt rock and basalt indicates minimal fractionation between the target rocks and the impactites. We found only little indication of post-impact hydrothermal alteration in terms of volatile trace element changes. No clear indication of an extraterrestrial component was found in any of our breccias and impact glasses, indicating either a low level of contamination, or a non-chondritic or otherwise iridium-poor impactor.
“…Despite the extensive petrographic observation indicating a Kmetasomatic event, our geochemical data do not reveal any strong substitution of K for Na or Ca. This indicates that K redistribution occurred at a scale of less than sample size, unlike, for example, at the Kärdla crater, where a distinct Kfeldspar enrichment was observed exchanging for Ca and Na feldspars (see Puura et al 2004).…”
Abstract-Approximately 100 m of impactites were retrieved from the ICDP borehole Yaxcopoil-1 (Yax-1), located ~60 km south-southwest from the center of the Chicxulub impact crater on the Yucatán Peninsula of Mexico. Here, we characterize and discuss this impact breccia interval according to its geochemical characteristics. Chemical analysis of samples from all five recognized breccia units reveals that the impactites are of heterogeneous composition with regard to both major and trace elements at the single sample (8-16 cm 3 ) scale. This is primarily due to a strong mixing relationship between carbonate and silicate fractions. However, averaged compositions for suevitic units 1 to 3 are similar, and the silicate fraction (after removal of the carbonate component) indicates thorough mixing and homogenization. Analysis of the green melt breccia horizon, unit 4, indicates that it contains a distinct mafic component. Large brown melt particles (in units 2, 3, and 4) represent a mixture of feldspathic and mafic components, with high CaO abundances. Unit 5 shows the greatest compositional diversity, with highly variable abundances of SiO 2 , CaO, and MgO.Inter-sample heterogeneity is the result of small sample size combined with inherent heterogeneous lithological compositions, highly variable particle size of melt and lithic components, and post-depositional alteration. In contrast to samples from the Y6 borehole from closer to the center of the structure, Yax-1 impactites have a strong carbonate component. Elevated loss on ignition, Rb, and Cs contents in the upper two impactite units indicate strong interaction with seawater. The contents of the siderophile elements, including Ni, Co, Ir, and Cr, do not indicate the presence of a significant extraterrestrial component in the Yax-1 impactites.
scite is a Brooklyn-based organization that helps researchers better discover and understand research articles through Smart Citations–citations that display the context of the citation and describe whether the article provides supporting or contrasting evidence. scite is used by students and researchers from around the world and is funded in part by the National Science Foundation and the National Institute on Drug Abuse of the National Institutes of Health.