scholarly journals High resolution reconstructions of the Southwest Indian Ridge, 52 Ma to present: Implications for the breakup and absolute motion of the Africa plate

Author(s):  
C DeMets ◽  
S Merkouriev ◽  
D Sauter

Summary We reconstruct the post-52 Ma seafloor spreading history of the Southwest Indian Ridge at 44 distinct times from inversions of ≈20,000 magnetic reversal, fracture zone, and transform fault crossings, spanning major regional tectonic events such as the Arabia-Eurasia continental collision, the Arabia Peninsula’s detachment from Africa, the arrival of the Afar mantle plume below eastern Africa, and the initiation of rifting in eastern Africa. Best-fitting and noise-reduced rotation sequences for the Nubia-Antarctic, Lwandle-Antarctic, and Somalia-Antarctic plate pairs indicate that spreading rates everywhere along the ridge declined gradually by ≈50 percent from ≈31 Ma to 19-18 Ma. A concurrent similar-magnitude slowdown in the component of the Africa plate’s absolute motion parallel to Southwest Indian Ridge spreading suggests that both were caused by a 31-18 Ma change in the forces that drove and resisted Africa’s absolute motion. Possible causes for this change include the effects of the Afar mantle plume on eastern Africa or the Arabia Peninsula’s detachment from the Somalia plate, which culminated at 20-18 Ma with the onset of seafloor spreading in the Gulf of Aden. At earlier times, an apparently robust but previously unknown ≈6-Myr-long period of rapid kinematic change occurred from 43 Ma to 37 Ma, consisting of a ≈50 percent spreading rate slowdown from 43-40 Ma followed by a full spreading rate recovery and 30-40 ○ clockwise rotation of the plate slip direction from 40-37 Ma. Although these kinematic changes coincided with a reconfiguration of the paleoridge geometry, their underlying cause is unknown. Southwest Indian Ridge abyssal hill azimuths are consistent with the slip directions estimated with our newly derived Somalia-Antarctic and Lwandle-Antarctic angular velocities, adding confidence in their reliability. Lwandle-Antarctica plate motion has closely tracked Somalia-Antarctic plate motion since 50 Ma, consistent with slow-to-no motion between the Lwandle and Somalia plates for much of that time. In contrast, Nubia-Somalia rotations estimated from our new Southwest Indian Ridge rotations indicate that 189±34 km of WNW-ESE divergence between Nubia and Somalia has occurred in northern Africa since 40 Ma, including 70-80 km of WNW-ESE divergence since 17-16 Ma, slow to no motion from 26-17 Ma, and 109±38 km of WNW-ESE divergence from 40 Ma to ≈26 Ma absent any deformation within eastern Antarctica before 26 Ma.

2013 ◽  
Vol 5 (2) ◽  
pp. 2449-2482 ◽  
Author(s):  
A. Bronner ◽  
D. Sauter ◽  
M. Munschy ◽  
J. Carlut ◽  
R. Searle ◽  
...  

Abstract. We investigate the magnetic signature of an ultramafic seafloor in the eastern part of the Southwest Indian Ridge (SWIR). There, detachment faulting, continuous over 11 Myrs, exhumed large areas of mantle derived rocks. These exhumed mantle domains occur in the form of a smooth rounded topography with broad ridges locally covered by a thin highly discontinuous volcanic carapace. We present high-resolution data combining deep-tow magnetics, side-scan sonar images and dredged samples collected within two exhumed mantle domains between 62° E and 65° E. We show that, despite an ultraslow spreading rate, volcanic areas within robust magmatic segments are characterized by well defined seafloor spreading anomalies. By contrast, the exhumed mantle domains, including a few thin volcanic patches, reveal a weak and highly variable magnetic pattern. The analysis of the magnetic properties of the dredged samples and careful comparison between the nature of the seafloor, the deep-tow magnetic anomalies and the seafloor equivalent magnetization suggest that the serpentinized peridotites do not carry a sufficiently stable remanent magnetization to produce seafloor spreading magnetic anomalies in exhumed mantle domains.


Solid Earth ◽  
2014 ◽  
Vol 5 (1) ◽  
pp. 339-354 ◽  
Author(s):  
A. Bronner ◽  
D. Sauter ◽  
M. Munschy ◽  
J. Carlut ◽  
R. Searle ◽  
...  

Abstract. We investigate the magnetic signature of ultramafic seafloor in the eastern part of the Southwest Indian Ridge (SWIR). There, detachment faulting, continuous over 11 Myr, exhumed large areas of mantle-derived rocks. These exhumed mantle domains occur in the form of a smooth rounded topography with broad ridges locally covered by a thin highly discontinuous volcanic carapace. We present high-resolution data combining deep-tow magnetics, side-scan sonar images and dredged samples collected within two exhumed mantle domains between 62° E and 65° E. We show that, despite an ultra-slow spreading rate, volcanic areas within robust magmatic segments are characterized by well-defined seafloor spreading anomalies. By contrast, the exhumed mantle domains, including a few thin volcanic patches, reveal a weak and highly variable magnetic pattern. The analysis of the magnetic properties of the dredged samples and careful comparison between the nature of the seafloor, the deep-tow magnetic anomalies and the seafloor equivalent magnetization suggest that the serpentinized peridotites do not carry a sufficiently stable remanent magnetization to produce seafloor spreading magnetic anomalies in exhumed mantle domains.


2008 ◽  
Vol 9 (4) ◽  
pp. n/a-n/a ◽  
Author(s):  
Mathilde Cannat ◽  
Daniel Sauter ◽  
Antoine Bezos ◽  
Christine Meyzen ◽  
Eric Humler ◽  
...  

2021 ◽  
Author(s):  
Vaibhav Vijay Ingale ◽  
Sara Bazin ◽  
Jean-Yves Royer

<p><span><span>In 2018, two earthquake swarms occurred along segments of the ultra-slow Southwest Indian Ridge (spreading rate: 14-15 mm/a). The first swarm is located at the spreading-ridge intersection with the Atlantis Fracture Zone and comprises 9 Mw > 5.0 events (GCMT catalogue) and about 227 lower magnitude events (ISC catalogue), spanning over </span></span><span> </span><span><span>9</span></span><span><span> days (July </span></span><span><span>10</span></span><span><span>-1</span></span><span><span>8</span></span><span><span>).</span></span><span><span> The second crisis is more of a cluster of events focusing near a discontinuity, 220km away from the Indian Triple Junction and comprises 6 Mw > 5 events (GCMT) and 87 lower magnitude events (ISC catalogue), spanning over 30 days (September 2</span></span><span><span>8</span></span><span><span> to October 27). All focal mechanisms (GCMT) indicate normal faulting for both swarms. These two swarms are examined using hydroacoustic records from the OHASISBIO network with 7 to 9 </span></span><span><span>autonomous h</span></span><span><span>ydrophones moored on either side of Southwest Indian Ridge. </span></span></p><p><span><span>The first swarm initiates with a Mw=4.9 event (July 10 2018, 03h55) which triggers numerous events with an average of ~250 events per day for the first three days (July 10</span></span><span><sup></sup></span><span><span>to 12), propagating in the NE direction. After this, the seismic activity ceases down along with a sparse distribution of events until another </span></span><span><span>burst of activity initiating</span></span><span><span> after July 15, last</span></span><span><span>ing</span></span><span><span> for 3 days and comprising of several high intensity events. Overall, this swarm includes ~1100 hydroacoustic events spanning over 13 days.</span></span></p><p><span><span>The second swarm, further east, starts with two events, Mw=5.5 and 5.6 (Sept. 28 2018, 6h21 and 7h06), followed by a few discrete events. After 3 days, a dense cluster of events initiates with a Mw=5.4 event (October 1st, 18h16) and lasts for 7 days (~415 events per day) and decreases till the end of October. Two additional sub-swarms occur on October 1st and on October 6, both propagating towards the NE. Several other high intensity events occur October 10, after which seismic activity propagates towards the SE </span></span><span><span>and fades away until October 27. </span></span><span><span>Overall, this swarm includes ~5000 hydroacoustic events spanning over 33 days.</span></span></p><p><span>The number of events per day is thus larger for the second swarm than for the first one. Also, event source levels are in average smaller in the second crisis than in the first one. Further analyses of these characteristics, along with the different geographical and time distribution of the ~6000 acoustic events (vs ~300 events in the land-based catalogues), provide insights on the onset and on the tectonic or magmatic origin of these two contrasting swarms. </span></p>


2019 ◽  
Vol 220 (2) ◽  
pp. 1149-1171 ◽  
Author(s):  
C DeMets ◽  
S Merkouriev ◽  
S Jade

SUMMARY We reconstruct the movement of the India Plate relative to Eurasia at ≈1-Myr intervals from 20 Ma to the present from GPS site velocities and high-resolution sequences of rotations from the India–Somalia–Antarctic–Nubia–North America–Eurasia Plate circuit. The plate circuit rotations, which are all estimated using the same data fitting functions, magnetic reversal sampling points, calibrations for magnetic reversal outward displacement, and noise mitigation methods, include new India–Somalia rotations estimated from numerous Carlsberg and northern Central Indian ridge plate kinematic data and high-resolution rotations from the Southwest Indian Ridge that account for slow motion between the Nubia and Somalia plates. Our new rotations indicate that India–Somalia plate motion slowed down by 25–30 per cent from 19.7 to 12.5–11.1 Ma, but remained steady since at least 9.8 Ma and possibly 12.5 Ma. Our new India–Eurasia rotations predict a relatively simple plate motion history, consisting of NNE-directed interplate convergence since 19 Ma, a ≈50 per cent convergence rate decrease from 19.7 to 12.5–11.1 Ma, and steady or nearly steady plate motion since 12.5–11.1 Ma. Instantaneous convergence rates estimated with our new India–Eurasia GPS angular velocity are 16 per cent slower than our reconstructed plate kinematic convergence rates for times since 2.6 Ma, implying either a rapid, recent slowdown in the convergence rate or larger than expected errors in our geodetic and/or plate kinematic estimates. During an acceleration of seafloor faulting within the wide India–Capricorn oceanic boundary at 8–7.5 Ma, our new rotations indicate that the motions of the India Plate relative to Somalia and Eurasia remained steady. We infer that forces acting on the Capricorn rather than the India Plate were responsible for the accelerated seafloor deformation, in accord with a previous study. India–Eurasia displacements that are predicted with our new, well-constrained rotations are fit poorly by a recently proposed model that attributes the post-60-Ma slowdown in India–Eurasia convergence rates to the steady resistance of a strong lithospheric mantle below Tibet.


2021 ◽  
Vol 55 (13-14) ◽  
pp. 851-866
Author(s):  
Chong Chen ◽  
Yuru Han ◽  
Jonathan T. Copley ◽  
Yadong Zhou

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