Upcoming Seminars
May 23rd, 2024
Paleomagnetism of Mesoproterozoic mafic dykes of Congo/São Francisco - Implications on transition from Nuna to Rodinia supercontinent
- Johanna Salminen
University of Helsinki, Finland
Reconstructing ancient paleogeography is key to exploring Earth’s evolution in deep time. Currently three supercontinent cycles have been identified and supercontinents have been named from oldest to youngest: Nuna/Columbia, Rodinia, and Pangea. Supercontinents have been suggested to be preceded by the ~200 Myr earlier assembly of smaller landmasses (Wang et al., 2020), such as Umkondia before Rodinia and Gondwana before Pangea. While the Congo-São Francisco (C/SF) craton is a main building block in Gondwana due to its central location and it has been suggested to be part of Umkondia (C/SF-Kalahari-India-Amazonia) (e.g., Choudhary et al., 2019), its connection to Rodinia and Nuna has been controversial.
Here, a paleomagnetic record of Mesoproterozoic mafic dyke swarms in Angola and Brazil is used to reconstruct the paleogeography of C/SF during the supercontinent Nuna cycle. Comparison of the high-quality 1500 Ma Curaça paleomagnetic pole of C/SF (Salminen et al., 2016) with coeval, global robust poles and the large igneous province record indicates the proximity of C/SF with Amazonia-West Africa and Nuna core cratons (Baltica-Laurentia-Siberia), therefore supporting C/SF participation in the construction of the supercontinent Nuna. However, when using the recently obtained 1385 Ma Virei paleomagnetic pole of C/SF (Salminen et al., 2024) together with coeval global poles, a distinct reconstruction is obtained. The 1385 Ma Virei pole requires a substantial transform motion and large-magnitude azimuthal rotation (~85°) of the C/SF craton between 1500 Ma and 1385 Ma, which could be related to an early stage in the Nuna break-up. It also requires a large rotation of C/SF relative to Laurentia between 1385 Ma and the Neoproterozoic assembly of Rodinia.
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