Paleomagnetic investigation of the basal Maieberg Formation (Namibia) cap carbonate sequence (635 Ma): Implications for Snowball Earth postglacial dynamics

Author(s)

Pescarini, Thales ; Trindade, Ricardo I. F. ; Hoffman, Paul F. ; Sant'Anna, Lucy Gomes

• Document type: Journal article
• Source: GEOLOGICAL SOCIETY OF AMERICA BULLETIN; v. N/A, p. 23-pg., 2024-04-23.

Abstract

In this study, we investigate the paleomagnetism of the basal Maieberg Formation (Namibia) cap carbonate sequence to elucidate its magnetic properties and paleolatitude of deposition, establish global correlations, and contribute to the understanding of Snowball Earth postglacial dynamics. Two distinct magnetization components, C-1 and C-2 , were identified. C-1 is interpreted as a depositional or post-depositional remanent magnetization carried by detrital pseudo-single domain (PSD) magnetite, while the C-2 component is a thermochemical remanent magnetization carried by fine authigenic single domain (SD)-PSD magnetite. The deposition paleolatitude provided by C-1 is 33.3 degrees +/- 3.2 degrees , which gives an initial quantitative approximation of the paleolatitude for the underlying Marinoan Ghaub diamictites. The thickness of the Keilberg Member cap dolostone is anomalously high for the paleolatitude calculated with C-1 , which suggests that other factors besides the influence of the paleolatitude on carbonate oversaturation may have influenced the sedimentary production of cap dolostones and the overall thickness of the flooding cap carbonate sequence. Possible explanations could include the influence of alkalinity input combined with local tectonic subsidence during a long glacial period with unusually low sedimentation rates, which appear to be in a favorable configuration for the substantial thickness of the Keilberg Member. Paleomagnetic field reversals at the Keilberg cap dolostone and analogous units globally suggest a longer duration of marine transgression than energy-balance deglaciation models and sedimentological-geochemical observations have constrained. Factors such as ocean warming, thermal expansion, and local glacio-isostatic adjustments imply extended marine transgressions beyond the deglaciation period. Still, magnetostratigraphic estimates for postglacial transgressive sequences require longer time scales by a factor of five or more. Thus, the conflict arising between estimates derived from paleomagnetic data and the constraints imposed by climate physics underscores uncertainties regarding an unconventional field state or a remanence acquisition mechanism within these cap carbonates that is not fully understood. Importantly, if such a phenomenon proves to be primary and global, the widespread occurrence of these stratigraphically compressed reversals would support the precise temporal correlation between Marinoan cap dolostones. The C-2 pole correlates with Cambrian remagnetization poles observed in carbonates from West Gondwana, which now extend to the Congo craton. The remanence acquisition of C-2 likely stems from diagenesis-related low-temperature authigenic magnetite formation after the conversion of iron-rich smectite to iron-poor illite. Cooling associated with the Kaoko orogen's exhumation and tectonic uplift possibly locked the magnetic system at ca. 520 Ma, supported by the C-2 pole position on the West Gondwana apparent polar wander path, although other explanations remain valid. (AU)

• FAPESP's process: 20/03347-5 - Magnetic and cyclostratigraphy of the Nama group, Namibia: tectonic and chronologic implications for the Kalahari craton in the Ediacaran - Cambrian transition
• Grantee: Thales Pescarini
• Support Opportunities: Scholarships in Brazil - Doctorate (Direct)
• FAPESP's process: 16/06114-6 - The Neoproterozoic Earth System and the rise of biological complexity
• Grantee: Ricardo Ivan Ferreira da Trindade
• Support Opportunities: Research Projects - Thematic Grants