Kimberlite Diamond Deposits
by B.A. Kjarsgaard
Contents of this page:
Abstract
Definition
Distribution
Grade, Tonnage, and Value Statistics
Geological Attributes
Key Exploration Criteria
Knowledge Gaps
Areas of High Diamond Potential in Canada
Acknowledgements
References
Tables
Figures
Diamonds have formed over a signifi cant period of the Earth’s history, from ca. 3.57 Ga to 88 Ma, and probably to present day. Macrodiamonds are interpreted to crystallize from low-density fl uids, or carbon- and water-rich melts at pressures >~4.0 GPa and temperatures <~1350°C. These P?T conditions are met within thick, old lithospheric mantle roots that have low paleogeothermal gradients, and these roots lie under ancient continental nuclei. Kimberlite-hosted diamond mines occur in these cratonic shield regions that are older than 2.5 Ga. Macrodiamonds are transported as xenocrysts from the mantle to the surface by kimberlite magmas. The initiation of kimberlite magmatism is at depth in the asthenospheric mantle (>150 km), although the initiation and generation of kimberlite magma is poorly understood. Kimberlites magmas generate a range of rocks that form a wide variety of landforms and intrusions, in many aspects similar to that generated by small-volume alkali basaltic volcanic systems. Kimberlite bodies typically form from multiple intrusive and/or extrusive events; these discrete events form distinct kimberlite phases. These individual kimberlite phases are characterized by differing textures, mineralogy and geochemistry, and diamond grade, size populations and morphology, and value.
Figure 10: Figure 19: Figure 20: Figure 21: カナダ地質調査所(Geological Survey of Canada)による『Mineral Deposits of Canada Maps of deposits and resources(world)』から |