GREAT DIKE OF ZIMBABWE
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| Plate T-34 |
Map |
Southern Africa contains extensive exposures of the African Shield, a
cratonic complex
consisting of accreted arcs and microplates that have built up from collisional
terranes.
These terranes are replete with sutures, infolded sedimentary rocks, and
intrusions of
granitic rock. Isotopic ages range from 3800 to 500 Ma. The Plate scene shows
the
southern Zimbabwe (Rhodesian) Craton and one of the most remarkable intrusive
bodies in
the world, the Great Dike of Zimbabwe (also referred to in older reports as the
Great Dyke
of Rhodesia).
On the south, the Limpopo Mobile Belt, a 900-km long, 200-km wide
ancient mountain belt (including metasediments as old as 3.8 Ga and clastic
sediments as young as 2.5 Ga), separates the Zimbabwe Craton from the Kaapvaal
Craton in the Transvaal of South Africa (plate T-33). Highly deformed
greenschists, anorthosites, and gneisses (seen on the index map at A and B) were
thrust from the south against the Zimbabwe Craton about 2700 Ma ago.
The Zimbabwe cratonic terrane is an excellent example of an Archean
greenstone/granodioritic complex (MacGregor, 1951). Volcanic rocks,
graywackes, cherts, banded iron formation, and other sedimentary rocks have been
metamorphosed into low-grade schists and amphibolites. These comprise
strongly deformed, arcuate, synformal belts enclosed within older rocks.
"Gregarious batholiths" (MacGregor, 1951), diapiric granites/
tonalites, including the Chibi batholith at C and segments of the Shangani and
Malopo batholiths at D and E, occupy large parts of the image.
The Plate scene and Figure T-34.1, another
Landsat frame that depicts the craton around Salisbury and to the east,
illustrate the terrain typical of the region. The greenstone belts (Sebakwian
Group (~3.3 Ga), Bulawayan Group (2.7 Ga); with contorted infolds at F,
G, H, and I; Shamvaian Group (2.65 Ga)) are conspicuous, but the gneisses,
granulates, and granites form featureless low-relief topography. The
savannah veld contains obscuring patterns of land use, including large
light-toned cleared areas that superficially resemble plutons. In Figure T-34.2, the northeast corner of Zimbabwe,
circular clusters of castle kopjes (degenerate bornhardts) -rocky hills of
resistant granite- are remnants of several plutons (e.g., Mtoko near the
center). The arrangement of the kopjes suggests that weathering and erosion
proceeded along fractures (joints) that enlarged over time.
The Great Dike itself, conspicuous on the image and in an aerial photograph
(Figure T-34.2), is a topographic ridge of low
relief with linear outer ridges developed on cumulate layers that dip gently
inward near the contact of the dike with the country rock. The dike (average
width of 6 to 8 km) runs about N15°E for nearly 500 km across Zimbabwe. The
term "dike" for this structure is somewhat misleading in a strict
sense. The narrow linear dark band seen in the Plate is actually the feeder
conduit for four contiguous lopoliths intruded about 2.5 Ga ago into several
north-trending fractures within the craton during an extensional tectonic
phase. The intrusions spread subhorizontally in one or more thick, dense units.
Later faulting (normal with some strike-slips along west-northwest or
east-west trends) offsets the lopoliths and their feeders, easily seen in
the Plate (at J, K, L, M). Subsequent deep erosion over the last 2.5 Ga has
stripped off most of the spread-out lopolithic mass, leaving only its feeder
roots in the form of the largest "dike" known on Earth. Smaller
subsidiary dikes, Umvimeela and East, also served as feeders.
Each of the lopoliths' feeder segments, the Wedza and Selukwe complexes in
the Plate and the Hartley and Musengezi Complexes to the north, is characterized
by similar distinctive petrology and internal structure. Where exposed or
drilled, each of the lopoliths is layered with a gentle syncline bend
perpendicular to the dike axis. The topmost unit is usually gabbroic, seen in
the Landsat images as patches of lighter toned rock. Lower units consist of
cyclic bands (cumulates, often many meters thick) of orthopyroxenite, picrite,
harzburgite, and chromite seams. Structural relations and gravity distribution
suggest that
the "dike" is a permissive intrusion with vertical contacts emplaced
in an extensional stress field; it seemingly is not the initial phase of
continental rifting.
The Zimbabwe shield ends abruptly along a suture line against the Zambesi
belt to the
north. This is strikingly evident in a Landsat image (Figure T-34.3) that shows darker tones where the
Zambesi belt meets the shield. An escarpment marks the contact, and both
topography and structural grain are somewhat different in this northern terrane.
(The irregular light-toned patches result from land cultivation practices.)
The Zambezi River here flows eastward from Zambia to Mozambique. (NMS)
Additional References: Bichan (1970), Furon (1963), MacGregor (1951),
Pritchard (1979), Stagman (1978), Worst
(1960). Landsat 10103-07291-7, November 5, 1972.
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