1887
ASEG2009 - 20th Geophysical Conference
  • ISSN: 2202-0586
  • E-ISSN:

Abstract

Summary

Lamproites are peralkaline, typically ultrapotassic (6 to 8% KO) and magnesia-rich lamprophyric rocks of volcanic or hypabyssal origin and are now considered to crystallize from a distinct type of magma. Most lamproites occur in irregular, asymmetric craters that are generally rather shallow, usually less than 300 metres in depth, often in the shape of a champagne glass with crater diameters ranging from a few hundred metres to 1500 metres. An unusual feature is that volcaniclastic rocks in many lamproite craters are intruded by a magmatic phase that forms lava lakes or domes. Lamproite forms from a very explosive volatile-rich magma that forms deep down within the Earth (greater than 150 km) and rises rapidly to the surface because of the high fluid pressure. As it rises, it fractures the surrounding rock explosively and most lamproites contain numerous xenoliths from all levels of the mantle and crust that the lamproite has passed through on its way to the surface. The initial explosive phreatomagmatic stage of the eruption, powered by gases or boiling ground water, corrodes the hosting rock to form the champagne-glass shape. Particles of ash, lapilli, and pumice partially fill the crater and form a tuff ring and finally the crater fills with a lava pond from the degassed lamproite magma. These are typical maar-type diatremes, formed by an explosive reaction induced when hot, rising magma came into contact with subterranean water.

Lamproites are small-volume magmas and there are relatively few lamproites known world wide, with less than 20 geological provinces, of which only seven are diamondiferous. Only olivine lamproites are diamondiferous, other varieties such as leucite lamproites presumably did not originate deep enough in the mantle to contain significant diamond content. Olivine lamproite pyroclastic rocks and dikes are the usual source of diamonds whereas diamonds are rarely found in the magmatic equivalents. Diamonds do not crystallize from the lamproite magma but are brought to the surface as the magma ascends rapidly to the surface, collecting fragments of the mantle and crust en route. The Kimberley region of Western Australia contains the only two lamproite-hosted diamond mines in the world (the Argvle Diamond Mine in the East Kimberley and Kimberley Diamond Company’s Ellendale 9, in the West Kimberley).

Loading

Article metrics loading...

/content/journals/10.1071/ASEG2009ab111
2009-12-01
2026-01-19
Loading full text...

Full text loading...

References

  1. Cooper, G.R.J., and Cowan, D.R., 2003, Feature detection using sunshading: Extended abstracts, ASEG 16th Geophysical Conference and Exhibition, February 2003, Adelaide.
  2. Cooper, G.R.J., and Cowan, D.R., 2004a, The use of textural analysis to locate features in geophysical data: Extended abstracts, ASEG 17th Geophysical Conference and Exhibition, August 2004, Sydney.
  3. Cooper, G.R.J., and Cowan, D.R. 2004b, The detection of circular features in irregularly spaced data, Computers & Geosciences, 30, 101-105.
  4. Cowan, D.R., Tompkins, L.A., and Cowan, S. 2000, Screening kimberlite magnetic anomalies in magnetically active areas, Exploration Geophysics 31, 66-72.
  5. ASEG 20th Geophysical Conference and Exhibition, February 2009, Adelaide
  6. Jenke, G., and Cowan, D.R., 1994, Geophysical signature of the Ellendale lamproite pipes, Western Australia. In ‘Geophysical Signatures of Western Australian Mineral Deposits’, Geology & Geophysics Department (Key Centre) & UWA Extension, The University of Western Australia, Publication No 26, 1994, 403-414
  7. Keating, P., 1995, A simple technique for identifying magnetic anomalies due to kimberlite pipes, Exp lor. Mining Geol. 4, 121-125
/content/journals/10.1071/ASEG2009ab111
Loading
This is a required field
Please enter a valid email address
Approval was a Success
Invalid data
An Error Occurred
Approval was partially successful, following selected items could not be processed due to error