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Nature and Origin of Magnetic Lineations Within Valdivia Bank: Ocean Plateau Formation by Complex Seafloor Spreading

  • S. Thoram*
  • , W. W. Sager
  • , K. Gaastra
  • , S. M. Tikoo
  • , C. Carvallo
  • , A. Avery
  • , Arianna V. Del Gaudio
  • , Y. Huang
  • , K. Hoernle
  • , T. W. Höfig
  • , R. Bhutani
  • , D. M. Buchs
  • , C. Class
  • , Y. Dai
  • , G. Dalla Valle
  • , S. Fielding
  • , S. Han
  • , D. E. Heaton
  • , S. Homrighausen
  • , Y. Kubota
  • C. F. Li, W. R. Nelson, E. Petrou, K. E. Potter, S. Pujatti, J. Scholpp, J. W. Shervais, M. Tshiningayamwe, X. J. Wang, M. Widdowson
*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

9 Citations (Scopus)

Abstract

Valdivia Bank (VB) is a Late Cretaceous oceanic plateau formed by volcanism from the Tristan-Gough hotspot at the Mid-Atlantic Ridge (MAR). To better understand its origin and evolution, magnetic data were used to generate a magnetic anomaly grid, which was inverted to determine crustal magnetization. The magnetization model reveals quasi-linear polarity zones crossing the plateau and following expected MAR paleo-locations, implying formation by seafloor spreading over ∼4 Myr during the formation of anomalies C34n-C33r. Paleomagnetism and biostratigraphy data from International Ocean Discovery Program Expedition 391 confirm the magnetic interpretation. Anomaly C33r is split into two negative bands, likely by a westward ridge jump. One of these negative anomalies coincides with deep rift valleys, indicating their age and mechanism of formation. These findings imply that VB originated by seafloor spreading-type volcanism during a plate reorganization, not from a vertical stack of lava flows as expected for a large volcano.

Original languageEnglish
Article numbere2023GL103415
Number of pages11
JournalGeophysical Research Letters
Volume50
Issue number13
DOIs
Publication statusPublished - 16 Jul 2023
Externally publishedYes

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