EGU24-13004, updated on 09 Mar 2024
https://doi.org/10.5194/egusphere-egu24-13004
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Evolution history of the Knipovich-Mohns ridge intersection (Artic Ocean) during the last 20 Ma

Eleonora Ficini1, Cuffaro Marco1, Ligi Marco2, Miglio Edie3, and Sanfilippo Alessio4
Eleonora Ficini et al.
  • 1Istituto di Geologia Ambientale e Geoingegneria, Consiglio Nazionale delle Ricerche, Rome, Italy (eleonora.ficini@igag.cnr.it)
  • 2Istituto di Scienze Marine, Consiglio Nazionale delle Ricerche, Bologna, Italy
  • 3Dipartimento di Matematica, Politecnico di Milano, Milan, Italy
  • 4Dipartimento di Scienze della Terra e dell'Ambiente, Università di Pavia, Pavia, Italy

Mid-ocean ridges (MORs) form as a result of upwelling and partial melting of the underlying mantle, leading to seafloor spreading and new lithosphere formation. They result from an interplay between different geological forces shaping ocean seafloors and offer insights into Earth's mantle convection and lithospheric evolution. Recent advances in numerical models contributed to describe oceanic rift processes, although complex geodynamic settings remain relatively unexplored.
Knipovich and Mohns ultraslow spreading ridges are located in the Arctic Ocean, separated from Kolbensey and Gakkel ridges by the Jan Mayen transform and Lena Trough. They do not present any evidence of transform fault along their entire length and are characterized by a high obliquity (~35°-50°) with respect to their spreading direction, constituting some of the most intriguing MORs worldwide. At their intersection, geophysical data revealed a focused mantle upwelling along a narrow, oblique, and strongly asymmetric zone, coinciding with uneven surface uplift. These asymmetrical features have been associated to i) the control on passive upwelling of slow and asymmetric motion of the North America and Eurasia plates, or ii) the results of a major spreading reorganization in the area. However, asymmetries are tipically observed in other geodynamic settings, such as for example subduction zones, where they have been related to the relative motion of lithospheric plates with respect to the asthenosphere. In this work we carried out 3D numerical models reproducing the geodynamic evolution of a ~800-km long segment of the Knipovich and Mohns ridges (extending from ~76°N to ~71°N), including their migration with respect to the asthenosphere. The model uses a visco-plastic rheology which approximate both the asthenospheric and the lithospheric mantle, providing information on the temperature and deformation patterns within the mantle. We also computed the degrees of melting beneath each area of the MOR segment. In agreement with previous geophysical and petrological data, our results suggest that mantle upwelling is focused in a narrow zone, where the MOR makes a sharp bend, providing the inferred asymmetric patterns. On this basis, we propose a mechanism which could have led to the asymmetrical features (e.g., topography, spreading rate, mantle temperature and composition, etc.) characterizing the Knipovich-Mohns segments area. 

How to cite: Ficini, E., Marco, C., Marco, L., Edie, M., and Alessio, S.: Evolution history of the Knipovich-Mohns ridge intersection (Artic Ocean) during the last 20 Ma, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-13004, https://doi.org/10.5194/egusphere-egu24-13004, 2024.