Iron-rich tillite

The dark bands seen between the rock layers are goethite, an iron oxide mineral that forms through the oxidation of iron-rich fluids along bedding planes or fractures in the rock.

Located within the Merinjina Tillite Formation, the smaller embedded rocks were likely deposited in this massive matrix by glacial activity. This tillite has since undergone oxidation, and in some areas, has been partially replaced by botryoidal goethite—a rounded form of iron oxide.

Goethite boulders

This group of goethite–quartz boulders may have formed from a hydrothermal seam or vent, where silica and sulfur-rich fluids precipitated quartz and pyrite.  As pyrite oxidizes, it typically forms sulfuric acid, which accelerates iron oxidation, in this case forming goethite. As the surrounding blocky shale erodes, the more resistant goethite-quartz boulders remain – a common sight in the Flinders Ranges.

Continue reading “Goethite boulders”

Muddy limestone turbidite: Nantawarrina

Muddy limestone turbidite, formed from sediment deposits in offshore silty waters during the Cambrian period (around 550 million years ago). The dramatic localised buckling seen here may have occurred in situ during a turbulent underwater event. This rock is part of the Mernmerna Formation in the northern Flinders Ranges.

Glacial geological formation: sedimentary deposits

This striking outcrop near Copley exhibits a range of sedimentary deposits. From the north to south, green shale and blocky siltstone meets weathered sandstone. This is followed by a distinct tillite layer between two dolomite layers, and a thin layer of quartzite. Further along, siltstone layers coloured by iron oxide, and more weathered sandstone.

Recent studies in the area suggest that the northern Flinders Ranges area was a shallow marine or lagoonal setting prior to the climate changing into one of the earth’s most severe glaciations ever recorded (the global Sturtian Glaciation), 720 million years ago . Over these older rocks, we find layers of pebbly, mixed rocks (called diamictites) that were likely deposited by a glacier at its edge, along with some sand layers (Bolla Bollana Tillite). These rock  layers are thought to show the movement of the glacier as it advanced and retreated along the coastline. These layers then change into sandstones and mudstones with large rocks (called dropstones), which probably formed when the ice started to melt, in an area just in front of the retreating glacier (Wilyerpa Formation). After the glacier melted, the layers of rock that formed (Tapley Hill Formation) include thin, layered shales and carbonates that were deposited underwater.

Weathered sandstone:

Continue reading “Glacial geological formation: sedimentary deposits”

Bonney Sandstone Formation

The Bonney Sandstone Formation is the result of deposition of iron-stained sand, silt and mica, eroded from older igneous rocks to the west and transported by rivers into a large delta. This formation has a distinctive reddish colour, and is often seen alongside the harder weathering prominent peaks of Rawnsley Quartzite which was formed from white sands, 600 million years ago. See the essay Legacy of Time by The Royal Geographical Society of South Australia for the riveting story of the formation of the Flinders Ranges.