38 Time Scales of Denudation: From Catchment to Continent
Wednesday, 27 June 2001
10:00 AM - 4:30 PM
THE ORIGIN OF PASSIVE CONTINENTAL MARGIN ESCARPMENTS: INSIGHTS FROM COMBINING MULTIPLE ANALYTICAL TECHNIQUES
Paper number: 38-2
Program: THEME SESSIONS
Time: 10:20 AM – 10:40 AM
Authors
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Roderick W. BrownUniv of Melbourne, Melbourne, N/A
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Michael A. SummerfieldUniv of Edinburgh, Edinburgh, N/A
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Barry P. KohnUniv of Melbourne, Melbourne, N/A
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Alastair FlemingUniv of Edinburgh, Edinburgh, N/A
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Vicki-Ann DimasUniv of Melbourne, Melbourne, N/A
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David FinkAustralian Nuclear Sci and Technology Organisation, Menai, N/A
Abstract
Recently we demonstrated the benefits of producing an integrated, quantitative record of post-break-up denudation for the south-west African margin in central Namibia (Cockburn et al., 2000). Through the combined use of apatite fission track thermochronology and in-situ-produced cosmogenic isotopes we were able to show that escarpment behaviour in central Namibia was dominated by very slow retreat, ~10m/Ma, for a major portion of the margin’s history. Our results refute a long-standing model of rapid, steady escarpment retreat (~1 km/Ma) for this area and support recent numerical studies that suggest formation of a laterally stable escarpment pinned at an internal drainage divide.
Here we report ongoing studies in southeast Australia and Namibia where we incorporate U-Th/(He) apatite thermonchronometry to provide complementary data to fission track and cosmogenic isotope analysis. Previous research has pointed to slow erosion rates in southeast Australia through the Tertiary, but a range of denudation chronologies still coexist. Preliminary cosmogenic data along a transect across the escarpment at Brown Mt., NSW (36° 45'S), indicate bedrock erosion rates on the escarpment crest >15 m/Ma compared to lower rates both on the inland plateau and coastal plain. These new measurements combined with existing fission track data are inconsistent with a steady retreat model for the southeastern Australian escarpment at this location.
Cockburn, et al., 2000, Earth and Planetary Science Letters, 179, 429-435.