- 1European Institute for Marine Studies, Laboratoire Geo-Ocean, Brest, France (remisharajeev@gmail.com)
- 2Laboratoire de Géologie, CNRS - Ecole Normale Supérieure - Paris Sciences & Lettres, Paris, France
The Mid-Atlantic Ridge (MAR) north of the Kane Transform Fault (MARNOK) provides an
ideal setting to investigate the interplay between magma supply, faulting, and lithospheric
structure at a slow-spreading mid-ocean ridge (MOR). Along this section, two orthogonal
segments and four oblique segments bounded by non-transform discontinuities show
contrasting accretion styles. Orthogonal segments 1 and 6, located at the southern and
northern ends of the study area, show symmetrical spreading, and progressive thinning of the
crust with decreasing distance to the axis (from 8-9 km in ~1.12-Myr old lithosphere to 6-7 km
on-axis). These segments also display closely spaced, elongated normal faults, and their
Mantle Bouguer anomaly (MBA) and Residual Mantle Bouguer anomaly (RMBA) are lower
than that of the adjacent oblique segments. The lack of axial volcanic ridges in segments 1
and 6 along with the decreasing crustal thickness towards the axis indicate a reduction in melt
supply in recent geological time, and possible fluctuations of the magma supply on
characteristic time scales of ~1.12 Myr in this part of the MAR.
The oblique segments (Segments 2 to 5) show a mixed tectono-magmatic regime that reflects
the structural complexity of the MARNOK region. Detachment faults at the inside corners of
segments 2 and 5 along with thin crust indicate earlier asymmetrical, low-magma accretion
typical of oblique MAR segments. Present-day magmatism forms discontinuous, sigmoidal,
and locally focused axial volcanic ridges that resemble those observed on other oblique MOR
segments such as Mohns ridge, and certain oblique areas of the Southwest Indian Ridge.
Short, widely spaced faults and irregular volcanic constructions indicate that magma is
currently contributing to plate separation. Even though the axial volcanic ridges are aligned
with the strike of orthogonal segments 1 and 6, the melt budget of segments 2–5 does not
appear sufficient to reorganize these segments into orthogonal spreading.
Petrological observations reveal that melt–rock interaction is pronounced in tectonically
dominated MARNOK domains. This result along with structural and gravity, observations
indicating transient, localized melt focusing occurs within the MARNOK mantle. These
findings support observations from other slow and ultraslow ridges showing that magmatic
accretion is highly variable and controlled by mantle fertility, detachment-related cooling, and
intermittent melt supply. Overall, the results indicate that crustal formation in the MARNOK
region is shaped not simply by spreading rate, but by the combined influence of obliquity, melt
availability, faulting, and thermal structure. This integrated tectono-magmatic framework
provides new insight into how slow-spreading lithosphere evolves north of the Kane Transform
Fault and highlights the rapid temporal and spatial variability that characterizes magmatic and
tectonic processes at the Mid-Atlantic Ridge.
How to cite: Rajeevan, R., Maia, M., Rospabé, M., Pelleter, E., Besson, F., Olive, J.-A., Principaud, M., and Alix, A.-S.: Accretion Dynamics of the Oblique section of the Mid-Atlantic Ridge North of the Kane Transform Fault (23°50’N-25°15’N) , EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-393, https://doi.org/10.5194/egusphere-egu26-393, 2026.