Recent from talks
Nothing was collected or created yet.
Dunite
View on WikipediaDunite (/ˈduːnaɪt, ˈdʌnaɪt/), also known as olivinite (not to be confused with the mineral olivenite), is an intrusive igneous rock of ultramafic composition and with phaneritic (coarse-grained) texture. The mineral assemblage is greater than 90% olivine, with minor amounts of other minerals such as pyroxene, chromite, magnetite, and pyrope. Dunite is the olivine-rich endmember of the peridotite group of mantle-derived rocks.
Dunite and other peridotite rocks are considered the major constituents of the Earth's mantle above a depth of about 400 km (250 mi). Dunite is rarely found within continental rocks, but where it is found, it typically occurs at the base of ophiolite sequences where slabs of mantle rock from a subduction zone have been thrust onto continental crust by obduction during continental or island arc collisions (orogeny). It is also found in alpine peridotite massifs that represent slivers of sub-continental mantle exposed during collisional orogeny. Dunite typically undergoes retrograde metamorphism in near-surface environments and is altered to serpentinite and soapstone.

The type of dunite found in the lowermost parts of ophiolites, alpine peridotite massifs, and xenoliths may represent the refractory residue left after the extraction of basaltic magmas in the upper mantle. However, a more likely method of dunite formation in mantle sections is by interaction between lherzolite or harzburgite and percolating silicate melts, which dissolve orthopyroxene from the surrounding rock, leaving a progressively olivine-enriched residue.
Dunite may also form by the accumulation of olivine crystals on the floor of large basaltic or picritic magma chambers. These "cumulate" dunites typically occur in thick layers in layered intrusions, associated with cumulate layers of wehrlite, olivine pyroxenite, harzburgite, and even chromitite (a cumulate rock consisting largely of chromite). Small layered intrusions may be of any geologic age, for example, the Triassic Palisades Sill in New York and the larger Eocene Skaergaard complex in Greenland. The largest layered mafic intrusions are tens of kilometers in size and almost all are Proterozoic in age, e.g. the Stillwater igneous complex (Montana), the Muskox intrusion (Canada), and the Great Dyke (Zimbabwe). Cumulate dunite may also be found in ophiolite complexes, associated with layers of wehrlite, pyroxenite, and gabbro.
Dunite was named by the Austrian geologist Ferdinand von Hochstetter in 1859, after Dun Mountain near Nelson, New Zealand.[1] Dun Mountain was given its name because of the dun colour of the underlying ultramafic rocks. This color results from surface weathering that oxidizes the iron in olivine in temperate climates (weathering in tropical climates creates a deep red soil). The dunite from Dun Mountain is part of the ultramafic section of the Dun Mountain Ophiolite Belt.
A massive exposure of dunite in the United States can be found as Twin Sisters Mountain, near Mount Baker in the northern Cascade Range of Washington. In Europe it occurs in the Troodos Mountains of Cyprus. In southern British Columbia, Canada dunite rocks form the core of an ultramafic rock complex located near the small community of Tulameen. The rocks are locally enriched in platinum group metals, chromite and magnetite.
Carbon sequestration potential
[edit]Dunite could be used to sequester CO2 and help mitigate global climate change via accelerated chemical rock weathering. This would involve the mining of dunite rocks in quarries followed by crushing and grinding to create fine ground rock that would react with the atmospheric carbon dioxide. The resulting products are magnesite and silica which could be commercialized.[2][3]
References
[edit]- ^ Johnston, M. R. (2007). "Nineteenth-century observations of the Dun Mountain Ophiolite Belt, Nelson, New Zealand and trans-Tasman correlations". Geological Society, London, Special Publications. 287 (1). Geological Society of London: 375–87. Bibcode:2007GSLSP.287..375J. doi:10.1144/SP287.27. S2CID 129776536.
- ^ Danae A. Voormeij, George J. Simandl, Bill O'Connor - A systematic assessment of ultramafic rocks and their suitability for mineral sequestration of CO2 Archived 2015-02-12 at the Wayback Machine
- ^ Peter Köhler, Jens Hartmann, and Dieter A. Wolf-Gladrow. 2010. Geoengineering potential of artificially enhanced silicate weathering of olivine. PNAS ∣ November 23, 2010 ∣ vol. 107 ∣ no. 47 | 20228–20233
- Dunite
- Blatt, Harvey and Robert J. Tracy, 1996, Petrology, 2nd ed., W. H. Freeman, ISBN 0-7167-2438-3
Dunite
View on GrokipediaEtymology and History
Discovery and Naming
Dunite was named in 1859 by Austrian geologist Ferdinand von Hochstetter following his examination of ultramafic rocks during the Austrian Novara expedition's geological survey of New Zealand.[11][12] He designated the term for the olivine-dominated rock observed at its type locality on Dun Mountain (also known as Maungatapu), a peak near Nelson in New Zealand's South Island.[13][14] This naming reflected the mountain's distinctive dun (dull brownish) coloration, resulting from surface weathering that oxidizes iron in the olivine to produce a yellowish-orange rind over the fresh green interior.[13][15] The Dun Mountain occurrence forms part of a larger Permian-age ophiolite sequence, where dunite represents a mantle-derived peridotite body intruded or tectonically emplaced amid mafic and sedimentary rocks.[16] Hochstetter's description established dunite as a distinct lithology, characterized by over 90% modal olivine (forsterite-rich Mg-endmember), distinguishing it from broader peridotites.[3] Early recognition of such rocks predated formal naming, with similar olivine-rich masses noted in European localities, but Dun Mountain provided the eponymous prototype due to its accessibility and purity.[14] Subsequent mining for chromite in the area further highlighted the deposit's economic potential, though initial surveys focused on petrological classification.[15]Early Petrological Studies
The petrological study of dunite began with Ferdinand von Hochstetter's fieldwork in New Zealand during the Austrian Novara Expedition in 1859, where he examined exposures at Dun Mountain near Nelson. Hochstetter identified the rock as consisting predominantly of olivine crystals, distinguishing it from the surrounding serpentinized ultramafics by its fresh, coarse-grained texture and lack of pervasive alteration. He described it as a novel igneous rock type, nearly pure olivine forming an extensive mass, and formally named it "dunite" based on the mountain's characteristic dun-colored weathering.[17][18] Hochstetter's initial analysis relied on hand-specimen examination and early microscopic techniques, noting the olivine grains' granular fabric and accessory chromite, while tentatively proposing an eruptive origin emplaced during Jurassic volcanism within a broader ophiolitic sequence. His observations, communicated in letters to colleague Julius von Haast, emphasized the rock's uniformity and rarity as a "pure olivine" lithology, unprecedented in European petrology at the time. Following Hochstetter's departure in 1860, von Haast extended mapping efforts along the Dun Mountain belt, corroborating the olivine dominance through field descriptions and integrating dunite into regional stratigraphic interpretations as an ultrabasic intrusive body associated with serpentinites.[19][18] By the early 20th century, petrological examinations incorporated more systematic modal analyses, as in the 1911 survey by Bell, Clarke, and Marshall, which detailed the Dun Mountain dunite's textural variations but lacked chemical compositions, relying instead on qualitative olivine abundance estimates exceeding 90 volume percent. These studies affirmed dunite's ultramafic nature and igneous character, though debates persisted on its precise emplacement mechanism, with some attributing it to differentiation from basaltic magmas rather than primary mantle material. Early interpretations generally viewed dunite as a fractionated end-member of peridotite suites, setting the stage for later geochemical validations.[20]Petrological Characteristics
Mineral Composition
Dunite consists predominantly of the mineral olivine, which typically comprises more than 90% of its volume, distinguishing it from other peridotites like harzburgite that contain significant orthopyroxene.[21] The olivine is magnesium-rich, often with forsterite contents (Fo, defined as molar Mg/(Mg+Fe)) ranging from Fo90 to Fo93, as observed in alpine-type peridotites.[22] This high Fo value reflects derivation from mantle sources with elevated Mg/Fe ratios, minimizing iron enrichment during crystallization.[22] Accessory minerals, constituting less than 10% of the rock, include orthopyroxene (primarily enstatite), clinopyroxene (such as chromian diopside), and members of the spinel group like chromite.[23] Chromite occurs as disseminated euhedral to subhedral grains, often with elevated Cr/(Cr+Al+Fe3+) ratios (0.30–0.75), influencing the rock's potential for chromite enrichment in certain deposits.[22][24] Rare phases such as plagioclase or amphibole may appear but are typically absent or secondary, resulting from alteration rather than primary igneous processes.[25] The monomineralic nature arises from extreme fractional crystallization or melt-rock reaction in ultramafic systems, concentrating olivine while depleting other silicates.[26]| Mineral | Typical Modal Abundance | Key Characteristics |
|---|---|---|
| Olivine | >90 vol.% | Forsterite-rich (Fo90–Fo93), coarse-grained, equant to anhedral |
| Orthopyroxene (enstatite) | <5 vol.% | Accessory, often altered to serpentine |
| Clinopyroxene (chromediopside) | <5 vol.% | Trace, Cr-bearing |
| Chromite/spinel | <1–2 vol.% | Euhedral grains, high Cr# |