The parent material of Sydney laterites
- 1 July 1971
- journal article
- research article
- Published by Taylor & Francis in Journal of the Geological Society of Australia
- Vol. 18 (2) , 159-164
- https://doi.org/10.1080/00167617108728754
Abstract
The petrography of laterites in the Sydney district shows that source rocks range from shales—in which quartz grains are not common and average about 0.03 mm in diameter—to sandstones, with generally abundant quartz grains which may average up to 0.5 mm in diameter. Ferricretes or iron‐cemented duricrusts occur in rocks with coarser quartz grains, such as the Tertiary river gravels of the Maroota area. The porosity and permeability of these rocks have considerably influenced the nature and profiles of the laterites. Two possible sources of sesquioxides in the laterites appear to be the Wianamatta Shale and, perhaps more importantly, basic igneous rocks.Keywords
This publication has 6 references indexed in Scilit:
- Deep weathering and erosion surfaces in the Daly River basin, Northern TerritoryJournal of the Geological Society of Australia, 1963
- STUDIES IN PEDOGENESIS IN NEW SOUTH WALESEuropean Journal of Soil Science, 1953
- Classification and definitions of textures and mineral structures in oresEconomic Geology, 1951
- THE GENESIS OF LATERITESoil Science, 1948
- Solution, transportation, and precipitation of iron and silicaEconomic Geology, 1929
- Occurrence and origin of the bauxite deposits of ArkansasEconomic Geology, 1915