horizon.png Jiří Otava TRACING THE ORIGIN OF CAVE SANDS: STATE OF THE ART IN THE MORAVIAN KARST 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY I:\1OWNPAPERS\2017\SYDNEY\toSYDNEY\jpg\Otava_154_fig1.jpg.JPG Variscan Europe and Moravian Karst, Czech Republic horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY …it is very easy to know the provenance of cave sands near the ponor… horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY …but it is sometimes very difficult to recognize the sources of cave sediments when you are deep inside the limestone massif: horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY I:\1OWNPAPERS\2017\SYDNEY\toSYDNEY\jpg\Otava_154_fig1.jpg.JPG Assemblages coming from the western sources (Neoproterozoic granitoids and Devonian clastics): Translucent heavy mineral assemblage derived directly from Devonian clastics and granitoids of the Brno Massif, locality 1 on fig. 1, Suchdolský ponor, Dóm Juniorů. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY I:\1OWNPAPERS\2017\SYDNEY\toSYDNEY\jpg\Otava_154_fig1.jpg.JPG Assemblages coming from the northern sources: Lower Carboniferous, Mississippian (greywackes of the Protivanov F.): Translucent heavy mineral assemblage of the northern Culmian greywacke, locality 2 on fig. 1, Helišova skála. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY I:\1OWNPAPERS\2017\SYDNEY\toSYDNEY\jpg\Otava_154_fig1.jpg.JPG Assemblages coming from the eastern sources Lower Carboniferous, Mississippian (greywackes of the Rozstání and Myslejovice Fms.): Translucent heavy mineral assemblage of the Culmian greywacke at NE, locality 3 on fig. 1, Krasovský potok Valley. Translucent heavy mineral assemblage of the Culmian greywacke easterly from the Moravian Karst, locality 4 on fig. 1, Habrůvka Village. Translucent heavy mineral assemblage of the Culmian greywacke SE from the Moravian Karst, locality 5 on fig. 1, Hádek near Ochoz. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY I:\1OWNPAPERS\2017\SYDNEY\toSYDNEY\jpg\Otava_154_fig1.jpg.JPG Assemblages coming from the paleokarst fill, Cretaceous, Cenomanian (sands of the Rudice Formation): Translucent heavy mineral assemblage of the Cretaceous sands, locality 6 on fig. 1, Rudice-Seč. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Assemblages coming from the lower Miocene sands: Translucent heavy mineral assemblage of the terrestric Miocene, locality 7 on fig. 1, Ostrov, borehole OM3. ZTR means ultrastable minerals zircon + tourmaline + rutile. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Distiguishing of source of cave sands in the northern part of the Moravian Karst: terrestric Miocene source; eastern Culmian source; western and northern sources. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Cave sands of the Macocha Abyss and its closest vicinity are divided in two groups with different provenance: The first one ( ) comes from Cretaceous paleokarst fill (staurolite, kyanite, tourmaline, rutile), while the other one ( ) comes mainly from the western vicinity of the Moravian karst ((epidote, amphibole) with various admixture of the eastern source (garnets). horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Cretaceous (Cenomanian) kaolinic quartz sands in a palokarst depression, locality 6 on fig. 1, Rudice-Seč horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Kyanite – one of the most characteristic heavy mineral of the Cretaceous paleokarst fill. Photo in crossed polars. horizon.png 17TH INTERNATIONAL CONGRESS OF SPELEOLOGY, SYDNEY, AUSTRALIA 2017 JULY Conclusions •The metod of translucent heavy mineral analyses has been used to trace the provenance af cave sands in the Moravian karst. •Several examples of distiguishing the source of sands in enigmatic positions are presented. •The first one shows differences between cave sands coming from W and N, i.e. from granitoids and old Culmian, from E (younger Culmian) and from terrestric miocene •The other example was taken from cave sands in the close vicinity of the Macocha Abyss. •The result shows mixing of prevailing western source with minor share of easten source and another clearly different source – the products of Cretaceous paleokarst fill. •One of main goals of the analyses is to establish the paleohydrography of the karst and to show possibilities of new discoveries