Ultramafic rock
Ultramafic rocks (also referred to as ultrabasic rocks, although the terms are not wholly equivalent) are
Intrusive ultramafic rocks
Intrusive ultramafic rocks are often found in large, layered
Volcanic ultramafic rocks on Earth
Examples include
Ultramafic tuff
Ultramafic tuff is extremely rare. It has a characteristic abundance of olivine or serpentine and a scarcity or absence of feldspar and quartz. Rare occurrences may include unusual surface deposits of maars of kimberlites in the diamond fields of southern Africa and other regions.
Ultrapotassic ultramafic rocks
Technically ultrapotassic rocks and melilitic rocks are considered a separate group, based on melting model criteria, but there are ultrapotassic and highly silica-under-saturated rocks with >18% MgO which can be considered "ultramafic".
Ultrapotassic, ultramafic igneous rocks such as lamprophyre, lamproite and kimberlite are known to have reached the surface of the Earth. Although no modern eruptions have been observed, analogues are preserved.
Most of these rocks occur as
Vents of Proterozoic lamproite (Argyle diamond mine), and Cenozoic lamproite (Gaussberg, Antarctica) are known, as are vents of Devonian lamprophyre (Scotland). Kimberlite pipes in Canada, Russia and South Africa have incompletely preserved tephra and agglomerate facies.
These are generally diatreme events and as such are not lava flows although tephra and ash deposits are partially preserved. These represent low-volume volatile melts and attain their ultramafic chemistry via a different process than typical ultramafic rocks.
Metamorphic ultramafic rocks
Metamorphism of ultramafic rocks in the presence of water and/or carbon dioxide results in two main classes of metamorphic ultramafic rock; talc carbonate and serpentinite.
Talc carbonation reactions occur in ultramafic rocks at lower greenschist through to granulite facies metamorphism when the rock in question is subjected to metamorphism and the metamorphic fluid has more than 10% molar proportion of CO2 (carbon dioxide).
When such metamorphic fluids have less than 10% molar proportion of CO2, reactions favor serpentinisation, resulting in
Distribution in space and time
The majority of ultramafic rocks are exposed in
Many surface exposures of ultramafic rocks occur in ophiolite complexes where deep mantle-derived rocks have been obducted onto continental crust along and above subduction zones.
Soil and regolith
Often thick,
Weathered ultramafic rocks may form lateritic nickel ore deposits.[4][5]
Other celestial bodies
Io
Ultramafic lava may have been detected on
Mercury
Mercury appears to have ultramafic volcanic rock.[7]
See also
- Chromitite
- Magnetite
- Kambalda type komatiitic nickel ore deposits
- Fractional crystallization (geology)
- Volcanism on Io, a moon of Jupiter
References
- ^ Ballhaus, C.G. & Glikson, A.Y., 1995, Petrology of layered mafic-ultramafic intrusions of the Giles Complex, western Musgrave Block, central Australia. AGSO Journal, 16/1&2: 69-90.
- ISBN 0-909869-55-3
- Kambalda, Western Australia: A distal volcanic model, in Buchanan, D.L., and Jones, M.J. (Editors), Sulphide Deposits in Mafic and Ultramafic Rocks, Institution of Mining and Metallurgy, London, p. 70-80.
- ^ Golightly, J.P. (1981): Nickeliferous Laterite Deposits. Economic Geology 75, 710-735
- Sao Paulo, 119-135
- ^ "Space Volcanoes". Horizon. No. Series 54, Episode 6. BBC. 7 July 2018. Retrieved 6 March 2019.
- .