Lamproite

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Sample of lamproite Lamproite photo.jpg
Sample of lamproite

Lamproite is an ultrapotassic mantle-derived volcanic or subvolcanic rock. It has low CaO, Al2O3, Na2O, high K2O/Al2O3, a relatively high MgO content and extreme enrichment in incompatible elements.

Contents

Lamproites are geographically widespread yet are volumetrically insignificant. Unlike kimberlites, which are found exclusively in Archaean cratons, lamproites are found in terrains of varying age, ranging from Archaean in Western Australia, to Palaeozoic and Mesozoic in southern Spain. They also vary widely in age, from Proterozoic to Pleistocene, the youngest known example from Gaussberg in Antarctica being 56,000 ± 5,000 years old.

Lamproite volcanology is varied, with both diatreme styles and cinder cone or cone edifices known.

Petrology

Lamproites form from partially melted mantle at depths exceeding 150 km. The molten material is forced to the surface in volcanic pipes, bringing with it xenoliths and diamonds from the harzburgitic peridotite or eclogite mantle regions where diamond formation is stabilized.

Recent research, for example on the lamproites at Gaussberg in Antarctica, and lead-lead isotope geochemistry have revealed that the source of lamproites may be transition zone melts of subducted lithosphere which has become trapped at the base of the lithospheric mantle. [2] This observation also reconciles the depth of melting with the peculiar geochemistry, which is most easily explained by melting of already felsic material under deep mantle conditions.

Mineralogy

The mineralogy of lamproites is controlled by their peculiar geochemistry, with a predominance of rare silica-deficient mineral species and rare, mantle-derived minerals predominating.

Minerals typical of lamproites include: forsteritic olivine; high iron leucite; titanium-rich aluminium-poor phlogopite; potassium- and titanium-rich richterite; low aluminium diopside; and iron-rich sanidine. A variety of rare trace minerals occur. The rocks are high in potassium with 6 to 8% potassium oxide. High chromium and nickel content is typical. The rocks commonly are altered to talc with carbonate or serpentine, chlorite, and magnetite. Zeolites and quartz may also occur.

Lamproites are characterized by the presence of widely varying amounts (5-90 vol.%) of the following primary phases (Mitchell & Bergman, 1991): [3]

The presence of all the above phases is not required in order to classify a rock as a lamproite. Any one mineral may be dominant, and this, together with the two or three other major minerals present, suffices to determine the petrographic name.

The presence of the following minerals precludes a rock from being classified as a lamproite: primary plagioclase, melilite, monticellite, kalsilite, nepheline, Na-rich alkali feldspar, sodalite, nosean, hauyne, melanite, schorlomite or kimzeyite.

Geochemistry

Lamproites conform to the following chemical characteristics:

Economic importance

The economic significance of lamproite became known with the discovery of Ellendale E4 and E9 lamproite pipes and better known 1979 discovery of the Argyle diamond pipe in Western Australia. This discovery led to the intense study and re-evaluation of other known lamproite occurrences worldwide; previously only kimberlite pipes were considered economically viable sources of diamonds.

The Argyle diamond mine remains the only economically viable source of lamproite diamonds. This deposit differs markedly by having a high content of diamonds but low quality of most stones. Research at Argyle diamond have shown that most stones are of E-type; they originate from eclogite source rocks and were formed under high temperature ~1,400 °C (2,600 °F). The Argyle diamond mine is the main source of rare pink diamonds.

Olivine lamproite pyroclastic rocks and dikes are sometimes hosts for diamonds. The diamonds occur as xenocrysts that have been carried to the surface or to shallow depths by the lamproite diapiric intrusions.

The diamonds of Crater of Diamonds State Park near Murfreesboro, Arkansas are found in a lamproite host.

Nomenclature

Lamproites, as a group, were known by a variety of localised names because their mineralogy is quite variable, and because of their rarity often few examples of the following lamproite variants were known. Modern terminology classes all as lamproites but modifies this term with the mineral abundances as per the standard IUGS rules.

HistoricModern
Wyomingite diopside-leucite-phlogopite lamproite
Orenditediopside-sanidine-phlogopite lamproite
Madupitediopside madupitic lamproite
Cedricitediopside-leucite lamproite
Mamiliteleucite-richterite lamproite
Wolgiditediopside-leucite-richterite madupitic lamproite
Fitzroyiteleucite-phlogopite lamproite
Veritehyalo-olivine-diopside-phlogopite lamproit
Jumilliteolivine-diopside-richterite madupitic lamproite
Fortunitehyalo-enstatite-phlogopite lamproite
Cancaliteenstatite-sanidine-phlogopite lamproite

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<span class="mw-page-title-main">Compatibility diagram</span> Depicts coexisting mineral phases in a metamorphic rock

In metamorphic geology, a compatibility diagram shows how the mineral assemblage of a metamorphic rock in thermodynamic equilibrium varies with composition at a fixed temperature and pressure. Compatibility diagrams provide an excellent way to analyze how variations in the rock's composition affect the mineral paragenesis that develops in a rock at particular pressure and temperature conditions. Because of the difficulty of depicting more than three components, usually only the three most important components are plotted, though occasionally a compatibility diagram for four components is plotted as a projected tetrahedron.

References

  1. "Rock Library". Mars Exploration Rover Mission. NASA Jet Propulsion Laboratory. Archived from the original on 19 November 2005. Retrieved 2 June 2014.
  2. Mirnejad, H.; Bell, K. (2006). "Origin and source evolution of the Leucite Hills lamproites: Evidence from Sr–Nd–Pb–O isotopic compositions". Journal of Petrology. 47 (12): 2463–2489. Bibcode:2006JPet...47.2463M. CiteSeerX   10.1.1.573.872 . doi:10.1093/petrology/egl051.
  3. Mitchell, R. H.; Bergman, S. C. (1991). Petrology of lamproites. New York: Plenum Press. ISBN   978-0-306-43556-0.

Further reading