EGU24-7543, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-7543
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Magma-induced tectonics at the East Pacific Rise 9º50’N: Evidence from high-resolution characterization of seafloor and subseafloor 

Milena Marjanovic1,2, Jie Chen1, Javier Escartín3, Ross Parnell-Turner2, and Jyun-nai Wu2
Milena Marjanovic et al.
  • 1Institut de Physique du Globe de Paris, Marine Geosciences, Paris, France (marjanovic@ipgp.fr)
  • 2Institute of Geophysics and Planetary Physics, Scripps Institution of Oceanography, University of California, San Diego, La Jolla, CA, USA
  • 3Laboratoire de Géologie, École Normale Supérieure/CNRS UMR 8538, PSL Research University, Paris, France

Mid-ocean ridges host the most extensive magmatic system on Earth, where ~60% of the lithosphere is formed. Fast spreading segments such as the East Pacific Rise (EPR) 9º50’N (full spreading rate >80 mm/yr) represent only ~20% of the global ridge network, but contribute ~50% of the total oceanic crustal accretion.  At these ridge segments, magma accumulates in on-axis, quasi-steady-state axial magmatic lenses (AML), typically found 1-2 km below the seafloor, 2 km wide on average, and <0.1 km thick. AMLs are highly three-dimensional in geometry, marked by alternating lineated ridges and troughs where dikes originate and connect with the seafloor through the systems of the faults and fissures (Marjanović et al., 2023). A couple of kilometers away from the ridge axis, the seafloor is dominated by abyssal hills, which are bounded by faults resulting from unbending, cooling, and extension of the lithosphere. Within the critical region between the axial summit trough (AST) and the first abyssal hill bounding faults, sparse mapping has shown that prominent faults can exist, but the mechanism for their origin and contribution to tectonic strain has remained elusive.

At the EPR 9º50’N, we combine meter-scale bathymetric mapping with the highest-resolution seismic imagery of an AML to date (horizontal resolution 25 x 25 m2) to reveal a remarkable vertical alignment between the AML and seafloor fault scarps. This genetic link we observe for four distinct cases. Each AML-fault pair is aligned asymmetrically with respect to the ridge axis and is associated with confirmed and possible records of hydrothermal venting observed in the results of recent seafloor and water column mapping (Wu et al., 2023). Along most of such faults’ scarps, the emplacement of magma through various eruption episodes is evident, helping build the crust outside the AST. Our observations at 9º48’N support a mechanism by which these asymmetric, tectonic-magmatic features originate from shallow magma injection sites. After initial magma injection, the surrounding crustal stresses are perturbed thus promoting further crack propagation aligned with the orientation of the underlying magma body. Finally, by joint analyses of faults exposed on the seafloor and seismically-imaged in the subsurface, we also show that their collective contribution to the overall tectonic component of seafloor spreading is less than 0.5%, with a close to negligible role of the lava-covered faults, much smaller than previously proposed.

Marjanović, M. et al., 2023, Insights into dike nucleation and eruption dynamics from high-resolution seismic imaging of magmatic system at the East Pacific Rise: Science advances, v. 9, p. eadi2698, doi:10.1126/sciadv.adi2698.

Wu, J.-N., Parnell-Turner, R., Fornari, D.J., Barreyre, T., and McDermott, J., 2023a, Oceanic heat transfer by diffuse and focused flow through off-axis vents at 9°50’N, East Pacific Rise, in AGU Fall Meeting Abstracts, v. 2023, p. V43B-0174.

How to cite: Marjanovic, M., Chen, J., Escartín, J., Parnell-Turner, R., and Wu, J.: Magma-induced tectonics at the East Pacific Rise 9º50’N: Evidence from high-resolution characterization of seafloor and subseafloor , EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-7543, https://doi.org/10.5194/egusphere-egu24-7543, 2024.