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Coevolution of craton margins and interiors during continental break-up
Many cratonic continental fragments dispersed during the rifting and break-up of Gondwana are bound by steep topographic landforms known as ‘great escarpments’ 1 – 4 , which rim elevated plateaus in the craton interior 5 , 6 . In terms of formation, escarpments and plateaus are traditionally conside...
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Published in: | Nature (London) 2024-08, Vol.632 (8024), p.327-335 |
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Main Authors: | , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites |
Online Access: | Get full text |
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Summary: | Many cratonic continental fragments dispersed during the rifting and break-up of Gondwana are bound by steep topographic landforms known as ‘great escarpments’
1
–
4
, which rim elevated plateaus in the craton interior
5
,
6
. In terms of formation, escarpments and plateaus are traditionally considered distinct owing to their spatial separation, occasionally spanning more than a thousand kilometres. Here we integrate geological observations, statistical analysis, geodynamic simulations and landscape-evolution models to develop a physical model that mechanistically links both phenomena to continental rifting. Escarpments primarily initiate at rift-border faults and slowly retreat at about 1 km Myr
−1
through headward erosion. Simultaneously, rifting generates convective instabilities in the mantle
7
–
10
that migrate cratonward at a faster rate of about 15–20 km Myr
−1
along the lithospheric root, progressively removing cratonic keels
11
, driving isostatic uplift of craton interiors and forming a stable, elevated plateau. This process forces a synchronized wave of denudation, documented in thermochronology studies, which persists for tens of millions of years and migrates across the craton at a comparable or slower pace. We interpret the observed sequence of rifting, escarpment formation and exhumation of craton interiors as an evolving record of geodynamic mantle processes tied to continental break-up, upending the prevailing notion of cratons as geologically stable terrains.
By integrating geological observations, statistical analysis, geodynamic simulations and landscape-evolution models, a physical model is proposed to link the coevolution of craton margins and interiors with continental rifting. |
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ISSN: | 0028-0836 1476-4687 1476-4687 |
DOI: | 10.1038/s41586-024-07717-1 |