Fault growth and propagation during incipient continental rifting: Insights from a combined aeromagnetic and Shuttle Radar Topography Mission digital elevation model investigation of the Okavango Rift Zone, northwest Botswana
Abstract:Digital Elevation Models (DEM) extracted from the Shuttle Radar Topography Mission (SRTM) data and high‐resolution aeromagnetic data are used to characterize the growth and propagation of faults associated with the early stages of continental extension in the Okavango Rift Zone (ORZ), northwest Botswana. Significant differences in the height of fault scarps and the throws across the faults in the basement indicate extended fault histories accompanied by sediment accumulation within the rift graben. Faults in t… Show more
“…The plate is thick and comparatively strong, and the stress accumulation required to cause fault slip may take 10 3 -10 5 a, based on sparse paleo-trenching studies (e.g., Zielke and Strecker, 2009;Machette et al, 1998). All or large parts of long border-fault systems that develop very early in basin evolution slip in large magnitude earthquakes (e.g., Kinabo et al, 2008;Craig et al, 2011), and intrabasinal faulting may also be seismogenic (e.g., Biggs et al, 2011). The interseismic cycle is barely detectable with GPS, suggesting that nearly all strain occurs during rifting episodes.…”
Section: Rifting Periodicity: From Seconds To Geological Time Scalesmentioning
The rifting cycle initiates with stress buildup, release as earthquakes and/or magma intrusions/eruptions, and visco-elastic rebound, multiple episodes of which combine to produce the observed, time-averaged rift zone architecture. The aim of our synthesis of current research initiatives into continental rifting-to-rupture processes is to quantify the time and length scales of faulting and magmatism that produce the time-averaged rift structures imaged in failed rifts and passive margins worldwide. We compare and contrast seismic and geodetic strain patterns during discrete, intense rifting episodes in magmatic and amagmatic sectors of the East African rift zone that span early-to late-stage rifting. We also examine the longer term rifting cycle and its relation to changing far-fi eld extension directions with examples from the Rio Grande rift zone and other cratonic rifts. Over time periods of millions of years, periods of rotating regional stress fi elds are marked by a lull in magmatic activity and a temporary halt to tectonic rift opening. Admittedly, rifting cycle comparisons are biased by the short time scale of global seismic and geodetic measurements, which span a small fraction of the 10 2 -10 5 year rifting cycle. Within rift sectors with upper crustal magma chambers beneath the central rift valley (e.g., Main Ethiopian, Afar, and Eastern or Gregory rifts) seismic energy release accounts for a small fraction of the deformation; most of the strain is accommodated by magma intrusion and slowslip. Magma intrusion processes appear to decrease the time period between rifting episodes, effectively accelerating the rift to rupture process. Thus, the inter-seismic period in rift zones with crustal magma reservoirs is strongly dependent upon the
“…The plate is thick and comparatively strong, and the stress accumulation required to cause fault slip may take 10 3 -10 5 a, based on sparse paleo-trenching studies (e.g., Zielke and Strecker, 2009;Machette et al, 1998). All or large parts of long border-fault systems that develop very early in basin evolution slip in large magnitude earthquakes (e.g., Kinabo et al, 2008;Craig et al, 2011), and intrabasinal faulting may also be seismogenic (e.g., Biggs et al, 2011). The interseismic cycle is barely detectable with GPS, suggesting that nearly all strain occurs during rifting episodes.…”
Section: Rifting Periodicity: From Seconds To Geological Time Scalesmentioning
The rifting cycle initiates with stress buildup, release as earthquakes and/or magma intrusions/eruptions, and visco-elastic rebound, multiple episodes of which combine to produce the observed, time-averaged rift zone architecture. The aim of our synthesis of current research initiatives into continental rifting-to-rupture processes is to quantify the time and length scales of faulting and magmatism that produce the time-averaged rift structures imaged in failed rifts and passive margins worldwide. We compare and contrast seismic and geodetic strain patterns during discrete, intense rifting episodes in magmatic and amagmatic sectors of the East African rift zone that span early-to late-stage rifting. We also examine the longer term rifting cycle and its relation to changing far-fi eld extension directions with examples from the Rio Grande rift zone and other cratonic rifts. Over time periods of millions of years, periods of rotating regional stress fi elds are marked by a lull in magmatic activity and a temporary halt to tectonic rift opening. Admittedly, rifting cycle comparisons are biased by the short time scale of global seismic and geodetic measurements, which span a small fraction of the 10 2 -10 5 year rifting cycle. Within rift sectors with upper crustal magma chambers beneath the central rift valley (e.g., Main Ethiopian, Afar, and Eastern or Gregory rifts) seismic energy release accounts for a small fraction of the deformation; most of the strain is accommodated by magma intrusion and slowslip. Magma intrusion processes appear to decrease the time period between rifting episodes, effectively accelerating the rift to rupture process. Thus, the inter-seismic period in rift zones with crustal magma reservoirs is strongly dependent upon the
“…The development of the ORZ is thought to be taking place within a large structural depression known as the Makgadikgadi-OkavangoZambezi basin (MOZ) and is characterized by northeasterly trending folds and faults of the Ghanzi-Chobe belt (Cooke, 1984). The strike of the main bounding rift-related faults is 030 -050 o in the north and 060 -070 o in the south (Kinabo et al, 2007;2008). The orientation of the faults on the surface is influenced by pre-existing faults and folds of the basement rocks Kinabo et al, 2007;2008).…”
Section: The Okavango Rift Zonementioning
confidence: 99%
“…In addition, comparison of the throw on the basement surface with the throw on the topographic fault scarp demonstrates many of the faults have extended histories. Most of the faults suggest evidence for multiple episodes of faulting with concomitant sedimentation along the down thrown block and erosion of the fault scarps (Kinabo et al, 2008).…”
Section: Faulting In the Areamentioning
confidence: 99%
“…The strike of the main bounding rift-related faults is 030 -050 o in the north and 060 -070 o in the south (Kinabo et al, 2007;2008). The orientation of the faults on the surface is influenced by pre-existing faults and folds of the basement rocks Kinabo et al, 2007;2008). The MOZ basin comprised of both alluvial fan deposits and deeper palaeo-lake sediments in structural depressions or sub-basins Shaw and Nash 1998).…”
Section: The Okavango Rift Zonementioning
confidence: 99%
“…It occurs in an intercratonic zone between the Congo craton to the northwest and the Kalahari craton (consisting of the Zimbabwe and Kaapvaal cratons) to the www.intechopen.com Geomorphic Landforms and Tectonic Controls Along the Eastern Margin of the Okavango Rift Zone, North Western Botswana as Deduced From Geophysical Data in the Area 171 east-southeast (e.g., Kinabo et al, 2007;2008). The development of the ORZ is thought to be taking place within a large structural depression known as the Makgadikgadi-OkavangoZambezi basin (MOZ) and is characterized by northeasterly trending folds and faults of the Ghanzi-Chobe belt (Cooke, 1984).…”
We used aeromagnetic and gravity data to investigate the thermal structure beneath the incipient Okavango Rift Zone (ORZ) in northwestern Botswana in order to understand its role in strain localization during rift initiation. We used three-dimensional (3-D) inversion of aeromagnetic data to estimate the Curie Point Depth (CPD) and heat flow under the rift and surrounding basement. We also used two-dimensional (2-D) power-density spectrum analysis of gravity data to estimate the Moho depth. Our results reveal shallow CPD values (8-15 km) and high heat flow (60-90 mW m À2 ) beneath a~60 km wide NE-trending zone coincident with major rift-related border faults and the boundary between Proterozoic orogenic belts. This is accompanied by thin crust (<30 km) in the northeastern and southwestern parts of the ORZ. Within the Precambrian basement areas, the CPD values are deeper (16-30 km) and the heat flow estimates are lower (30-50 mW m À2 ), corresponding to thicker crust (~40-50 km). We interpret the thermal structure under the ORZ as due to upward migration of hot mantle fluids through the lithospheric column that utilized the presence of Precambrian lithospheric shear zones as conduits. These fluids weaken the crust, enhancing rift nucleation. Our interpretation is supported by 2-D forward modeling of gravity data suggesting the presence of a wedge of altered lithospheric mantle centered beneath the ORZ. If our interpretation is correct, it may result in a potential paradigm shift in which strain localization at continental rift initiation could be achieved through fluid-assisted lithospheric weakening without asthenospheric involvement.
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