1987
DOI: 10.1007/bf01821089
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The ševĚtín astrobleme, southern Bohemia, Czechoslovakia

Abstract: Geologische, geomorphologische, petrologische und geophysikallsche Daten, die tiber die 46 km im Durchmesset aufweisende Rundstruktur von ~ev~tin in Stidb6hmen (49~ 14~ ermittelt wurden, entsprechen der Charakteristik mittelm~ig erodierten Strukturen, die infolge des Einschlags eines grof~en Meteoriten yon Hypergeschwindigkeit entstanden sin& Das Astroblem wird als oberkretazisch (wahrscheinlich yon Coniac-his Santonalter, ~85-75 Mill. Jahre) geologisch datiert. Es ist durch Brtiche in Radialsegmente aufgeglie… Show more

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Cited by 6 publications
(3 citation statements)
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“…These occur in either primary or reworked impact ejecta and are postulated to have formed within the turbulent ejecta cloud (Pope et al, 1999). First recognized from the Ries crater (Graup, 1981), they have since been described associated with the Sevetin (Vrana, 1987), Azuara (Ernstson and Fiebag, 1992), Alamo (Warme and Kuehner, 1998), and Chicxulub (Ocampo et al, 1996;Pope et al, 1999) impact sites. Accreted grains from the latter three sites are composed largely or completely of fi ne carbonate fragments in a carbonate matrix, refl ecting bedrock at the impact sites.…”
Section: Accreted Grains In Other Settingsmentioning
confidence: 99%
See 1 more Smart Citation
“…These occur in either primary or reworked impact ejecta and are postulated to have formed within the turbulent ejecta cloud (Pope et al, 1999). First recognized from the Ries crater (Graup, 1981), they have since been described associated with the Sevetin (Vrana, 1987), Azuara (Ernstson and Fiebag, 1992), Alamo (Warme and Kuehner, 1998), and Chicxulub (Ocampo et al, 1996;Pope et al, 1999) impact sites. Accreted grains from the latter three sites are composed largely or completely of fi ne carbonate fragments in a carbonate matrix, refl ecting bedrock at the impact sites.…”
Section: Accreted Grains In Other Settingsmentioning
confidence: 99%
“…Calcite is also present in accreted grains at Ries although it is described as being a secondary infi ltration (Graup, 1981). No carbonate is present at Sevetin, but the impact breccia there is silicifi ed (Vrana, 1987), and thus its original composition is uncertain. These examples are from ancient impact sites and the composition of the contemporaneous cement is not known.…”
Section: Accreted Grains In Other Settingsmentioning
confidence: 99%
“…However, using a standard petrographic microscope, it can be difficult to distinguish between PDFs and nonshock‐related planar microstructures in quartz. On several occasions, lamellar microstructures in quartz have been identified as PDFs, but have subsequently been disproved to be shock‐related, or they remain controversial (e.g., Vrána 1987 versus Cordier et al. 1994; Surenian 1988 versus Leroux and Doukhan 1993; Ernstson and Fiebag 1992 versus Langenhorst and Deutsch 1996; Becker et al.…”
Section: Introductionmentioning
confidence: 99%