Welcome to the new version of CaltechAUTHORS. Login is currently restricted to library staff. If you notice any issues, please email coda@library.caltech.edu
Published March 15, 2020 | Supplemental Material
Journal Article Open

Reversible subsidence on the North West Shelf of Australia

Abstract

The Northwest Shelf (NWS) of Australia is characterized by offshore basins associated with Permian and Jurassic rifting and was only slowly subsiding by the Neogene. International Ocean Discovery Program (IODP) Expedition 356 targeted this region by coring four sites in the Northern Carnarvon and Roebuck Basins and two sites in the Perth Basin to the south on the Australian western margin. We use detailed lithological, physical property and age data with paleobathymetric interpretations, to infer tectonic subsidence apparently confined to the NWS that reverses (uplifts) with about the same amplitude and rate as an earlier subsidence event. About 300 m of tectonic subsidence occurred over one million years from 6 to 5 million years ago and then reverses when 300 m of tectonic uplift occurred from 2 to 1 Ma. The along strike extent of this subsidence pattern is ∼ 400 km. The similarity of magnitude and duration of the subsidence and uplift phases suggest that the subsidence is reversible. The results cannot be explained by glacial eustatic variability nor can the uplift event be attributed to sediments filling the accommodation space generated earlier. Reversible subsidence is a key fingerprint of dynamic topography. Although the rates of subsidence and uplift are roughly ∼ 300 m/Myr, a substantial portion of the changes occur over less than 1 Myr and the rates inferred from a detailed least squares analysis can reach up to about 500 m/Myr. These rates are incompatible with dynamic topography associated with motion of Australia over large-scale convection (10 to 40 m/Myr) or that associated with instability of the base of the lithosphere (<15 m/Myr). The vertical motions are too large to be associated with simple flexure of a plate and plate buckling in that the required amplitudes would lead to permanent deformation of the plate. A new geodynamic mechanism is required to fit the observations.

Additional Information

© 2020 Elsevier B.V. Received 13 April 2019, Revised 2 November 2019, Accepted 4 January 2020, Available online 17 January 2020. USSSP supported the participation of MG and MK on IODP Expedition 356 as well as with post expedition awards. MG was also supported by the NSF through EAR-1645775. Funding to SJG was provided by the Australian IODP office and the ARC Basins Genesis Hub (IH130200012). The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Attached Files

Supplemental Material - 1-s2.0-S0012821X20300133-mmc1.pdf

Files

1-s2.0-S0012821X20300133-mmc1.pdf
Files (7.5 MB)
Name Size Download all
md5:d1040314dd7133ce7752da8dcf71be0a
7.5 MB Preview Download

Additional details

Created:
August 22, 2023
Modified:
October 19, 2023