4 research outputs found

    The Lawn Hill annulus: An Ordovician meteorite impact into water-saturated dolomite

    Get PDF
    The Lawn Hill Impact Structure (LHIS) is located 250 km N of Mt Isa in NW Queensland, Australia, and is marked by a highly deformed dolomite annulus with an outer diameter of ~18 km, overlying low metamorphic grade siltstone, sandstone, and shale, along the NE margin of the Georgina Basin. This study provides detailed field observations from sections of the Lawn Hill annulus and adjacent areas that demonstrate a clear link between the deformation of the dolomite and the Lawn Hill impact. 40Ar-39Ar dating of impact-related melt particles provides a time of impact in the Ordovician (472 ± 8 Ma) when the Georgina Basin was an active depocenter. The timing and stratigraphic thickness of the dolomite sequence in the annulus suggest that there was possibly up to 300 m of additional sedimentary rocks on top of the currently exposed Thorntonia Limestone at the time of impact. The exposed annulus is remarkably well preserved, with preservation attributed to postimpact sedimentation. The LHIS has an atypical crater morphology with no central uplift. The heterogeneous target materials at Lawn Hill were probably low-strength, porous, and water-saturated, with all three properties affecting the crater morphology. The water-saturated nature of the carbonate unit at the time of impact is thought to have influenced the highly brecciated nature of the annulus, and restricted melt production. The impact timing raises the possibility that the Lawn Hill structure may be a member of a group of impacts resulting from an asteroid breakup that occurred in the mid-Ordovician (470 ± 6 Ma)

    When a bolide hits a world class Pb/Zn deposit : new insights into the Lawn Hill impact structure

    No full text
    The Lawn Hill Impact Structure is situated approximately 240km NNW of Mt Isa in north eastern Queensland, and consists of a ring of low Cambrian limestone hills overlying very weakly metamorphosed Proterozoic shales and other sediments. The world class Century Pb/Zn deposit sits at the margin of the structure and is hosted within the Proterozoic basement. The deposit exhibits strong indications of impact related brecciation previously attributed to other causes, or left unexplained. These include a variety of breccia textures, some incorporating the much younger Cambrian limestone, and ranging from micro to mega scale, including a one million tonne "megaclast" of Century-like ore encapsulated with Cambrian limestone adjacent to the main deposit. Other interpreted impact effects include milled limestone "breccia dykes" injected deep into the deposit and impact related hydrothermal remobilisation of ore minerals with small galena deposits observed within the Cambrian limestone. These were possibly formed through a process similar to Mississippi Valley Type Pb/Zn deposits. Additional results from a fluid inclusion study indicate that temperatures and fluid composition were within tolerances for remobilisation of Pb and Zn during impact-related fluid flow; however, sealing of flow paths and short lived convection may limit the size of possible impact-generated ore deposits. New constraints are placed on the age of the impact structure through 40 Ar/39 Ar dating of impact melt from the central uplift.1 page(s
    corecore