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Ultramafic rocks also referred to as ultrabasic rocks although the terms are not wholly equivalent are igneous and meta

Ultramafic

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Ultramafic
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Ultramafic rocks (also referred to as ultrabasic rocks, although the terms are not wholly equivalent) are igneous and meta-igneous rocks with a very low silica content (less than 45%), generally >18% MgO, high FeO, low potassium, and are usually composed of greater than 90% mafic minerals (dark colored, high magnesium and iron content). Earth's mantle is composed of ultramafic rocks. Ultrabasic is a more inclusive term that includes igneous rocks with low silica content that may not be extremely enriched in Fe and Mg, such as carbonatites and ultrapotassic igneous rocks.

image
Peridotite, a type of ultramafic rock

Intrusive ultramafic rocks

image
IUGS Classification diagram for intrusive ultramafic rocks based on modal percentages of mafic minerals. Green area represents typical mantle peridotite.

Intrusive ultramafic rocks are often found in large, layered ultramafic intrusions where differentiated rock types often occur in layers. Such cumulate rock types do not represent the chemistry of the magma from which they crystallized. The ultramafic intrusives include the dunites, peridotites and pyroxenites. Other rare varieties include troctolite which has a greater percentage of calcic plagioclase. These grade into the anorthosites. Gabbro and norite often occur in the upper portions of the layered ultramafic sequences. Hornblendite and, rarely phlogopite, are also found.

Volcanic ultramafic rocks on Earth

Volcanic ultramafic rocks are rare outside of the Archaean and are essentially restricted to the Neoproterozoic or earlier. Subvolcanic ultramafic rocks and dykes persist longer, but are also rare. There is evidence of ultramafic rocks elsewhere in the Solar System.

Examples include komatiite and picritic basalt. Komatiites can be host to ore deposits of nickel.

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 dikes, diatremes, lopoliths or laccoliths, and very rarely, intrusions. Most kimberlite and lamproite occurrences occur as volcanic and subvolcanic diatremes and maars; lavas are virtually unknown.

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 chlorite-serpentine-amphibole type assemblages.

Distribution in space and time

The majority of ultramafic rocks are exposed in orogenic belts, and predominate in Archaean and Proterozoic terranes. Ultramafic magmas in the Phanerozoic are rarer, and there are very few recognised true ultramafic lavas in the Phanerozoic.[citation needed]

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, regolith, and biology

Serpentine soil is a magnesium rich, calcium, potassium and phosphorus poor soil that develops on the regolith derived from ultramafic rocks. Ultramafic rocks also contain elevated amounts of chromium and nickel which may be toxic to plants. As a result, a distinctive type of vegetation develops on these soils. Examples are the ultramafic woodlands and barrens of the Appalachian Mountains and piedmont, the "wet maquis" of the New Caledonia rain forests, and the ultramafic forests of Mount Kinabalu and other peaks in Sabah, Malaysia. Vegetation is typically stunted, and sometimes includes endemic species adapted to the soils.

Often thick, magnesite-calcrete caprock, laterite and duricrust forms over ultramafic rocks in tropical and subtropical environments. Particular floral assemblages associated with highly nickeliferous ultramafic rocks are indicative tools for mineral exploration.

Weathered ultramafic rocks may form lateritic nickel ore deposits.

Lichen communities on ultramafic rocks show distinctive characteristics, including the unusual co-presence of species that typically grow on either acidic or calcium-rich rocks, due to the rocks' unique chemical composition. While some lichen species appear to be characteristic of ultramafic environments within specific geographical regions, very few species are found exclusively on these rocks. Studies have shown that lichen communities on ultramafic rocks can be more diverse than those on adjacent mafic rocks, with some localities showing notably higher species counts on serpentinites compared to other rock types. These communities often display xerophytic characteristics and may include species with disjunct distribution patterns. The weathering action of lichens on ultramafic rocks can promote biogeochemical processes, including the complete depletion of magnesium from serpentine minerals beneath lichen thalli and the formation of secondary minerals common in serpentine soils.

Other celestial bodies

Io

Ultramafic lava may have been detected on Io, a moon of Jupiter, because heat-mapping of Io's surface found ultra-hot areas with temperatures in excess of 1,200 °C (2,190 °F). The magma immediately below these hot spots is probably about 200 °C (360 °F) hotter, based on surface-to-subsurface temperature differences observed for lava on Earth. A temperature of 1,400 °C (2,550 °F) is thought to indicate the presence of ultramafic magma.

Mercury

Mercury appears to have ultramafic volcanic rock.

Mars

The undifferentiated crust of Mars is largely composed of mafic and ultramafic rocks. Dark lobate flows of upper Hesperian and early Amazonian age, probably extruded from a regional network of extension faults, can be traced in the Ladon Basin. Spectral analysis data confirm the ultramafic character of these flows and the underlying rocks.

Trappist-1 b

Mid-infrared (12.8 μm) observations have shown that the exoplanet's measured flux is consistent with a surface model of ultramafic rocks.

See also

  • Chromitite
  • Magnetite
  • Kambalda type komatiitic nickel ore deposits
  • Fractional crystallization (geology)
  • Volcanism on Io, a moon of Jupiter

References

  1. 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.
  2. Hill R.E.T, Barnes S.J., Gole M.J., and Dowling S.E., 1990. Physical volcanology of komatiites; A field guide to the komatiites of the Norseman-Wiluna Greenstone Belt, Eastern Goldfields Province, Yilgarn Block, Western Australia., Geological Society of Australia. ISBN 0-909869-55-3
  3. Lesher, C.M., Arndt, N.T., and Groves, D.I., 1984, Genesis of komatiite-associated nickel sulfide deposits at 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.
  4. Golightly, J.P. (1981): Nickeliferous Laterite Deposits. Economic Geology 75, pp. 710–735
  5. Schellmann, W. (1983): Geochemical principles of lateritic nickel ore formation. Proceedings of the 2. International Seminar on Lateritisation Processes, São Paulo, pp. 119–135
  6. Favero-Longo, Sergio E.; Isocrono, Deborah; Piervittori, Rosanna (2004). "Lichens and ultramafic rocks: a review". The Lichenologist. 36 (6): 391–404. doi:10.1017/S0024282904014215.
  7. "Space Volcanoes". Horizon. No. Series 54, Episode 6. BBC. 7 July 2018. Retrieved 6 March 2019.
  8. Lopes, Rosaly M. C.; Williams, David A. (2015-01-01), Sigurdsson, Haraldur (ed.), "Chapter 43 - Volcanism on Io", The Encyclopedia of Volcanoes (Second Edition), Amsterdam: Academic Press, pp. 747–762, ISBN 978-0-12-385938-9, retrieved 2025-05-17
  9. Charlier, B.; Grove, T.L.; Zuber, M.T. (2013). "Phase equilibria of ultramafic compositions on Mercury and the origin of the compositional dichotomy" (PDF). Earth and Planetary Science Letters. 363: 50–60. Bibcode:2013E&PSL.363...50C. doi:10.1016/j.epsl.2012.12.021.
  10. Müntener, Othmar (2010-10-01). "Serpentine and serpentinization: A link between planet formation and life". Geology. 38 (10): 959–960. doi:10.1130/focus102010.1. ISSN 0091-7613.
  11. Mège, Daniel; Gurgurewicz, Joanna; Massironi, Matteo; Pozzobon, Riccardo; Tognon, Gloria; Pajola, Maurizio; Tornabene, Livio L.; Lucchetti, Alice; Baschetti, Beatrice; Davis, Joel M.; Hauber, Ernst; De Toffoli, Barbara; Douté, Sylvain; Keszthelyi, Laszlo; Marinangeli, Lucia (2023). "Hydrothermal Alteration of Ultramafic Rocks in Ladon Basin, Mars—Insights From CaSSIS, HiRISE, CRISM, and CTX". Journal of Geophysical Research: Planets. 128 (1): e2022JE007223. doi:10.1029/2022JE007223. ISSN 2169-9100.
  12. Shrestha, Sabnam (2025-03-26). "The enigma of Trappist-1 b: a thick atmosphere or airless rock?". Physics World. Retrieved 2025-05-17.

Author: www.NiNa.Az

Publication date: May 26, 2025 / 06:18

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Ultramafic rocks also referred to as ultrabasic rocks although the terms are not wholly equivalent are igneous and meta igneous rocks with a very low silica content less than 45 generally gt 18 MgO high FeO low potassium and are usually composed of greater than 90 mafic minerals dark colored high magnesium and iron content Earth s mantle is composed of ultramafic rocks Ultrabasic is a more inclusive term that includes igneous rocks with low silica content that may not be extremely enriched in Fe and Mg such as carbonatites and ultrapotassic igneous rocks Peridotite a type of ultramafic rockIntrusive ultramafic rocksIUGS Classification diagram for intrusive ultramafic rocks based on modal percentages of mafic minerals Green area represents typical mantle peridotite Intrusive ultramafic rocks are often found in large layered ultramafic intrusions where differentiated rock types often occur in layers Such cumulate rock types do not represent the chemistry of the magma from which they crystallized The ultramafic intrusives include the dunites peridotites and pyroxenites Other rare varieties include troctolite which has a greater percentage of calcic plagioclase These grade into the anorthosites Gabbro and norite often occur in the upper portions of the layered ultramafic sequences Hornblendite and rarely phlogopite are also found Volcanic ultramafic rocks on EarthVolcanic ultramafic rocks are rare outside of the Archaean and are essentially restricted to the Neoproterozoic or earlier Subvolcanic ultramafic rocks and dykes persist longer but are also rare There is evidence of ultramafic rocks elsewhere in the Solar System Examples include komatiite and picritic basalt Komatiites can be host to ore deposits of nickel 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 rocksTechnically 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 gt 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 dikes diatremes lopoliths or laccoliths and very rarely intrusions Most kimberlite and lamproite occurrences occur as volcanic and subvolcanic diatremes and maars lavas are virtually unknown 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 rocksMetamorphism 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 chlorite serpentine amphibole type assemblages Distribution in space and timeThe majority of ultramafic rocks are exposed in orogenic belts and predominate in Archaean and Proterozoic terranes Ultramafic magmas in the Phanerozoic are rarer and there are very few recognised true ultramafic lavas in the Phanerozoic citation needed 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 regolith and biologySerpentine soil is a magnesium rich calcium potassium and phosphorus poor soil that develops on the regolith derived from ultramafic rocks Ultramafic rocks also contain elevated amounts of chromium and nickel which may be toxic to plants As a result a distinctive type of vegetation develops on these soils Examples are the ultramafic woodlands and barrens of the Appalachian Mountains and piedmont the wet maquis of the New Caledonia rain forests and the ultramafic forests of Mount Kinabalu and other peaks in Sabah Malaysia Vegetation is typically stunted and sometimes includes endemic species adapted to the soils Often thick magnesite calcrete caprock laterite and duricrust forms over ultramafic rocks in tropical and subtropical environments Particular floral assemblages associated with highly nickeliferous ultramafic rocks are indicative tools for mineral exploration Weathered ultramafic rocks may form lateritic nickel ore deposits Lichen communities on ultramafic rocks show distinctive characteristics including the unusual co presence of species that typically grow on either acidic or calcium rich rocks due to the rocks unique chemical composition While some lichen species appear to be characteristic of ultramafic environments within specific geographical regions very few species are found exclusively on these rocks Studies have shown that lichen communities on ultramafic rocks can be more diverse than those on adjacent mafic rocks with some localities showing notably higher species counts on serpentinites compared to other rock types These communities often display xerophytic characteristics and may include species with disjunct distribution patterns The weathering action of lichens on ultramafic rocks can promote biogeochemical processes including the complete depletion of magnesium from serpentine minerals beneath lichen thalli and the formation of secondary minerals common in serpentine soils Other celestial bodiesIo Ultramafic lava may have been detected on Io a moon of Jupiter because heat mapping of Io s surface found ultra hot areas with temperatures in excess of 1 200 C 2 190 F The magma immediately below these hot spots is probably about 200 C 360 F hotter based on surface to subsurface temperature differences observed for lava on Earth A temperature of 1 400 C 2 550 F is thought to indicate the presence of ultramafic magma Mercury Mercury appears to have ultramafic volcanic rock Mars The undifferentiated crust of Mars is largely composed of mafic and ultramafic rocks Dark lobate flows of upper Hesperian and early Amazonian age probably extruded from a regional network of extension faults can be traced in the Ladon Basin Spectral analysis data confirm the ultramafic character of these flows and the underlying rocks Trappist 1 b Mid infrared 12 8 mm observations have shown that the exoplanet s measured flux is consistent with a surface model of ultramafic rocks See alsoChromitite Magnetite Kambalda type komatiitic nickel ore deposits Fractional crystallization geology Volcanism on Io a moon of JupiterReferencesBallhaus C G amp Glikson A Y 1995 Petrology of layered mafic ultramafic intrusions of the Giles Complex western Musgrave Block central Australia AGSO Journal 16 1 amp 2 69 90 Hill R E T Barnes S J Gole M J and Dowling S E 1990 Physical volcanology of komatiites A field guide to the komatiites of the Norseman Wiluna Greenstone Belt Eastern Goldfields Province Yilgarn Block Western Australia Geological Society of Australia ISBN 0 909869 55 3 Lesher C M Arndt N T and Groves D I 1984 Genesis of komatiite associated nickel sulfide deposits at 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 pp 710 735 Schellmann W 1983 Geochemical principles of lateritic nickel ore formation Proceedings of the 2 International Seminar on Lateritisation Processes Sao Paulo pp 119 135 Favero Longo Sergio E Isocrono Deborah Piervittori Rosanna 2004 Lichens and ultramafic rocks a review The Lichenologist 36 6 391 404 doi 10 1017 S0024282904014215 Space Volcanoes Horizon No Series 54 Episode 6 BBC 7 July 2018 Retrieved 6 March 2019 Lopes Rosaly M C Williams David A 2015 01 01 Sigurdsson Haraldur ed Chapter 43 Volcanism on Io The Encyclopedia of Volcanoes Second Edition Amsterdam Academic Press pp 747 762 ISBN 978 0 12 385938 9 retrieved 2025 05 17 Charlier B Grove T L Zuber M T 2013 Phase equilibria of ultramafic compositions on Mercury and the origin of the compositional dichotomy PDF Earth and Planetary Science Letters 363 50 60 Bibcode 2013E amp PSL 363 50C doi 10 1016 j epsl 2012 12 021 Muntener Othmar 2010 10 01 Serpentine and serpentinization A link between planet formation and life Geology 38 10 959 960 doi 10 1130 focus102010 1 ISSN 0091 7613 Mege Daniel Gurgurewicz Joanna Massironi Matteo Pozzobon Riccardo Tognon Gloria Pajola Maurizio Tornabene Livio L Lucchetti Alice Baschetti Beatrice Davis Joel M Hauber Ernst De Toffoli Barbara Doute Sylvain Keszthelyi Laszlo Marinangeli Lucia 2023 Hydrothermal Alteration of Ultramafic Rocks in Ladon Basin Mars Insights From CaSSIS HiRISE CRISM and CTX Journal of Geophysical Research Planets 128 1 e2022JE007223 doi 10 1029 2022JE007223 ISSN 2169 9100 Shrestha Sabnam 2025 03 26 The enigma of Trappist 1 b a thick atmosphere or airless rock Physics World Retrieved 2025 05 17

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