A 70m long continental sediment record was recovered at Darwin Crater in western Tasmania, Australia. The sediment succession includes a pre-lake silty sand deposit overlain by lacustrine silts that have accumulated in the ~ 816 ka meteorite impact crater. A total of 160m of overlapping sediment cores were drilled from three closely spaced holes. Here we report on the drilling operations at Darwin Crater and present the first results from petrophysical whole core logging, lithological core description, and multi-proxy pilot analysis of core end samples. The multi-proxy dataset includes spectrophotometry, grain size, natural gamma rays, paleoand rock magnetism, loss on ignition, and pollen analyses. The results provide clear signatures of alternating, distinctly different lithologies likely representing glacial and interglacial sediment facies. Initial paleomagnetic analysis indicate normal magnetic polarity in the deepest core at Hole B. If acquired at the time of deposition, this result indicates that the sediment 1m below commencement of lacustrine deposition post-date the Matuyama- Brunhes geomagnetic reversal ~ 773 ka.
Funding
This project is funded by the Australian Research Council (ARC) Discovery Indigenous project IN170100062 to Michael S. Fletcher and Agathe Lisé-Pronovost. Agathe Lisé-Pronovost is supported by a McKenzie Fellowship at the University of Melbourne and funding from La Trobe University's Deputy Vice Chancellor Research (DVCR). Tom Mallett is supported by a La Trobe University Postgraduate Research Scholarship. Joel B. Pedro acknowledges support from the European Research Council under the European Union's Seventh Framework Programme (FP7/2007-2013) and ERC grant agreement no. 610055 (the ice2ice project).