Carbonatites: Classification, Sources, Evolution, and Emplacement
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Yaxley, Greg
Anenburg, Michael
Tappe, Sebastian
Decree, Sophie
Guzmics, Tibor
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Annual Reviews
Abstract
Carbonatites are igneous rocks formed in the crust by fractional crystallization of carbonate-rich parental melts that are mostly mantle derived.
They dominantly consist of carbonate minerals such as calcite, dolomite,
and ankerite, as well as minor phosphates, oxides, and silicates. They are
emplaced in continental intraplate settings such as cratonic interiors and
margins, as well as rift zones, and rarely on oceanic islands. Carbonatites
are cumulate rocks, which are formed by physical separation and accumulation of crystals that crystallize from a melt, and their parental melts
form by either (a) direct partial melting of carbonate-bearing, metasomatized, lithospheric mantle producing alkali-bearing calciodolomitic
melts or (b) silicate-carbonate liquid immiscibility following fractional
crystallization of carbonate-bearing, silica-undersaturated magmas such
as nephelinites, melilitites, or lamprophyres. Their emplacement into
the crust is usually accompanied by fenitization, alkali metasomatism
of wallrock caused by fluids expelled from the crystallizing carbonatite. Carbonatites are major hosts of deposits of the rare earth elements and niobium, and the vast
majority of the global production of these commodities is from carbonatites.
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Carbonatites are igneous rocks formed from carbonate-rich magmas, which ultimately formed in Earth's upper mantle.
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Carbonatites are associated with economic deposits of metals such as the rare earth elements and niobium, which are essential in high-tech applications.
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There are more than 600 carbonatites in the geological record but only one currently active carbonatite volcano, Oldoinyo Lengai in Tanzania.
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Annual Review of Earth and Planetary Sciences
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Free Access via publisher website-http://www.annualreviews.org/eprint/JVDPC4NDH4BAFJNWDAVJ/full/10.1146/annurev-earth-032320-104243
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Restricted until
2099-12-31
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