geodynamics of diamond deposits craig o’neill the university of sydney

15
Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Post on 20-Dec-2015

219 views

Category:

Documents


1 download

TRANSCRIPT

Page 1: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Geodynamics of diamond deposits

Craig O’NeillThe University of Sydney

Page 2: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

New Scientist, 21st September 2002

Page 3: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Formation of diamond deposits: the standard model

Helmstaedt and Gurney, 1995

Page 4: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Southern Africa

Shirey et al. 2002

Page 5: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Southern African geotherms

On-craton

Off-craton

Graphite

Diamond

Page 6: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Clifford’s Rule

Helmstaedt and Gurney, 1995

Page 7: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

AustraliaArgyle: Lamproite

Hall’s Creek mobile belt (Proterozoic), adjacent to Kimberley block (possible Archean basement)

Australia’s diamond occurrences

Merlin: Kimberlite

Central Australian mobile belts

Page 8: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Structure of the Australian Lithosphere

Page 9: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Cross-sections

Page 10: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Numerical Models

Moresi et al., 2000; O’Neill et al., 2002

Page 11: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Numerical Models

Moresi et al., 2000O’Neill et al., 2002

Time in DSF

On-craton

Off-craton

H F

Page 12: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Percentage timegeotherms spend in

DSF

Page 13: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

A. Distance to COB B. Archean cratons

C. Distance from cratons D. Combined

Page 14: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Tomographycross-sectionsthrough Argyle

and Merlin

Page 15: Geodynamics of diamond deposits Craig O’Neill The University of Sydney

Conclusions

Restriction to Archean terranes too stringent• diamond formation may not always be related to formation of cratonic roots• require PT conditions and C source

Inclusion of many stable Proterozoic platforms

Focus on where kimberlite volcanism is likely to occur• Australia example: step changes in lithospheric thicknesses could be important