In
geology, a 'crust' is the outermost layer of a
planet.
The crust of the
Earth is composed of a great variety of
igneous,
metamorphic, and
sedimentary rocks. The crust is underlain by the
mantle. The upper part of the mantle is composed mostly of
peridotite, a rock denser than rocks common in the overlying crust. The boundary between the crust and mantle is conventionally placed at the
Mohorovicic discontinuity, a boundary defined by a contrast in
seismic velocity. Earth's crust occupies less than '1%' of Earth's volume.
The
oceanic crust of the Earth is different from its
continental crust. The
oceanic crust is 5 to 10 km thick and is composed primarily of
basalt,
diabase, and
gabbro. The
continental crust is typically from 30 to 50 km thick, and it is mostly composed of less dense rocks than is the oceanic crust. Some of these less dense rocks, such as
granite, are common in the continental crust but rare to absent in the oceanic crust.
The temperature of the crust increases with depth, reaching values typically in the range from about 500°C to 1000°C at the boundary with the underlying mantle. The crust and underlying relatively rigid mantle make up the
lithosphere. Because of
convection in the underlying
plastic, although non-molten, upper
mantle and
asthenosphere, the lithosphere is broken into
tectonic plates that move.
Origin of the Earth's crust
Earth is considered to have differentiated from an
aggregate of
planetesimals into its core,
mantle and crust within about 100 million years of the formation of the planet, 4.6 billion years ago. The
primordial crust was very thin, and was likely recycled by much more vigorous
plate tectonics and destroyed by significant
asteroid impacts, which were much more common in the early stages of the solar system. There is a theory that the
Moon was formed by one such very large impact.
The Earth has likely always had some form of basaltic oceanic crust, but there is evidence it has also had continental style crust for as long as 3.8 to 3.9 billion years. The oldest crust on Earth is the
Narryer Gneiss Terrane in
Western Australia at 3.9 billion years, and certain parts of the
Canadian Shield and the
Fennoscandian Shield are also of this age.
The majority of the current Earth's continental crust was formed primarily between 4.6 billion years and 3.9 billion years ago, in the
Hadean. The vast majority of rocks of this age are located in
cratons where the crust is up to 70km thick. The lower density of the continental crust as compared to the oceanic crust prevents it being destroyed by
subduction. Crust formation is linked to periods of intense
orogeny or mountain building; these periods coincide with the formation of the
supercontinents such as
Rodinia,
Pangaea and
Gondwana. The crust forms not so much by accumulation of
granite and
metamorphic fold belts, but by depletion of the
mantle to form buoyant lithospheric mantle.
Composition of the crust
The common
rock constituents of the Earth's crust are nearly all
oxides;
chlorine,
sulfur and
fluorine are the only important exceptions to this and their total amount in any rock is usually much less than 1%.
F. W. Clarke calculated that a little more than 47% of the Earth's crust consists of
oxygen. It occurs principally in combination as oxides, of which the chief are
silicon,
aluminium,
iron,
calcium,
magnesium,
potassium and
sodium oxides. Silica is a major constituent of the crust occurring as the
silicate minerals, which are the most common minerals of
igneous and
metamorphic rocks. From a computation based on 1672 analyses of all kinds of rocks Clarke arrived at the following as the average percentage composition by mass:
| Oxide | Percent |
|---|
| SiO2 | 59.71 |
| Al2O3 | 15.41 |
| CaO | 4.90 |
| MgO | 4.36 |
| Na2O | 3.55 |
| FeO | 3.52 |
| K2O | 2.80 |
| Fe2O3 | 2.63 |
| H2O | 1.52 |
| TiO2 | 0.60 |
| P2O5 | 0.22 |
| total | 99.22 |
All the other constituents occur only in very small quantities, and total less than 1%.
See also
★
Continental drift
★
Plate tectonics
References
External links
★
USGS Crust Thickness Map