Cratons are large areas of thick continental
lithosphere that have been stable for long periods of geological
time, generally since the Archean. Most cratons are characterized
by low heat flow and no or few earthquakes. Many
have a thick mantle root or tectosphere, characterized seismologically
and from xenolith studies to be cold and refractory,
having had basaltic melt extracted from it during the Archean.
Seismological studies have shown that many parts of the tectosphere
are strongly deformed with most of the minerals oriented
in planar or linear fabrics. Current understanding about
the origin of stable continental cratons and their roots hinges
upon recognizing which processes change the volume and
composition of continental lithosphere with time, and how
and when juvenile crust evolved into stable continental crust.
Despite decades of study, several major unresolved questions
remain concerning Archean tectosphere: (1) how is it formed?
Large quantities of melt extraction (komatiite in composition,
if melting occurred in a single event) are required from petrological
observations, yet little of this melt is preserved in
Archean cratons, which are characterized by highly evolved
crust compositions. (2) In what tectonic settings is it formed?
Hypotheses range from intraplate, plume-generated settings to
convergent margin environments. (3) Finally, once formed,
does the chemical buoyancy and inferred rheological strength
of the tectosphere preserve it from disruption? Until recently,
most scientists would argue that cratonic roots last forever—
isotopic investigations of mantle xenoliths from the Kaapvaal,
Siberian, Tanzanian, and Slave cratons document the longevity
of the tectosphere in these regions. However, the roots of
some cratons are now known to have been lost, including the
North China craton, and the processes of the loss of the tectosphere
are as enigmatic as the processes that form the roots.
See also ARCHEAN; CRATONS; PLATE TECTONICS.














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