Cardiff University | Prifysgol Caerdydd ORCA
Online Research @ Cardiff 
WelshClear Cookie - decide language by browser settings

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

Darlington, Vicki, Blenkinsop, Thomas G., Dirks, Paul, Salisbury, Jess and Tomkins, Andrew 2016. The Lawn Hill annulus: An Ordovician meteorite impact into water-saturated dolomite. Meteoritics and Planetary Science 10.1111/maps.12734

[thumbnail of LawnHillAnnulus.pdf]
PDF - Accepted Post-Print Version
Download (2MB) | Preview


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).

Item Type: Article
Date Type: Published Online
Status: Published
Schools: Earth and Environmental Sciences
Subjects: Q Science > Q Science (General)
Publisher: Meteoritical Society
ISSN: 1086-9379
Date of First Compliant Deposit: 25 October 2016
Date of Acceptance: 15 August 2016
Last Modified: 21 Oct 2017 07:54

Citation Data

Cited 8 times in Scopus. View in Scopus. Powered By Scopus® Data

Actions (repository staff only)

Edit Item Edit Item


Downloads per month over past year

View more statistics