Abstract
The volcanic structure of the Seymour Sewell seamount appears to have formed over a relatively long time in at least two stages. Its main massif was formed as a result of volcanic activity in the axial zone of the Central Indian Ridge about 16.3 Ma ago for about 0.5 Ma. Then the volcanic process temporarily stopped and the seamount drifted 260 km southwest along with the supporting African plate. In the last epoch of direct magnetic polarity (Brunes, 680 ka ago), as a result of a new cycle of volcanotectonic activity, the southeastern segment of the seamount collapsed. At this time, a new portion of magmatic material with a high ferrous mineral content was erupted here, reflected in the more intense magnetic anomaly confined to this part of the seamount.
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Funding
The study was carried within a state task (topic no. 0128-2021-0005, O.V. Levchenko, I.A. Veklich, and A.N. Ivanenko; and topic no. 0135-2019-0076, N.N. Turko); it was supported by the Russian Foundation for Basic Research (project no. 19-05-00680).
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Levchenko, O.V., Veklich, I.A., Ivanenko, A.N. et al. Geophysical Studies of the Seymour Sewell Seamount on the Flank of the Central Indian Ridge. Oceanology 62, 550–560 (2022). https://doi.org/10.1134/S0001437022040075
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DOI: https://doi.org/10.1134/S0001437022040075