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-List Of Titles -Inclusions in diamonds from the K14 and K10 kimberlites, Buffalo Hills, Alberta, Canada : diamond growth in a plume?

Please use this identifier to cite or link to this item: http://hdl.handle.net/1959.14/40007

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Title
Inclusions in diamonds from the K14 and K10 kimberlites, Buffalo Hills, Alberta, Canada : diamond growth in a plume?
Related
Lithos, Vol. 77, Issue 1-4, p.99-111
DOI
10.1016/j.lithos.2004.04.008
Publisher
Elsevier Science
Date
2004
FoR/RFCD Code(s)
040299 Geochemistry not elsewhere classified  040313 Tectonics
Author/Creator
Davies, Rondi M
Author/Creator
Griffin, William L
Author/Creator
O'Reilly, Suzanne Y
Author/Creator
McCandless, Tom E
Description
Analyses of mineral inclusions, carbon isotopes, nitrogen contents and nitrogen aggregation states in 29 diamonds from two Buffalo Hills kimberlites in northern Alberta, Canada were conducted. From 25 inclusion bearing diamonds, the following paragenetic abundances were found: peridotitic (48%), eclogitic (32%), eclogitic/websteritic (8%), websteritic (4%), ultradeep? (4%) and unknown (4%). Diamonds containing mineral inclusions of ferropericlase, and mixed eclogitic-asthenospheric-websteritic and eclogitic-websteritic mineral associations suggests the possibility of diamond growth over a range of depths and in a variety of mantle environments (lithosphere, asthenosphere and possibly lower mantle). Eclogitic diamonds have a broad range of C-isotopic composition (δ¹³C=−21‰ to −5‰). Peridotitic, websteritic and ultradeep diamonds have typical mantle C-isotope values (δ¹³C=−4.9‰ av.), except for two ¹³C-depleted peridotitic (δ¹³C=−11.8‰, −14.6‰) and one ¹³C-depleted websteritic diamond (δ¹³C=−11.9‰). Infrared spectra from 29 diamonds identified two diamond groups: 75% are nitrogen-free (Type II) or have fully aggregated nitrogen defects (Type IaB) with platelet degradation and low to moderate nitrogen contents (av. 330 ppm-N); 25% have lower nitrogen aggregation states and higher nitrogen contents (~30% IaB; <1600 ppm-N). The combined evidence suggests two generations of diamond growth. Type II and Type IaB diamonds with ultradeep, peridotitic, eclogitic and websteritic inclusions crystallised from eclogitic and peridotitic rocks while moving in a dynamic environment from the asthenosphere and possibly the lower mantle to the base of the lithosphere. Mechanisms for diamond movement through the mantle could be by mantle convection, or an ascending plume. The interaction of partial melts with eclogitic and peridotitic lithologies may have produced the intermediate websteritic inclusion compositions, and can explain diamonds of mixed parageneses, and the overlap in C-isotope values between parageneses. Strong deformation and extremely high nitrogen aggregation states in some diamonds may indicate high mantle storage temperatures and strain in the diamond growth environment. A second diamond group, with Type IaA–IaB nitrogen aggregation and peridotitic inclusions, crystallised at the base of the cratonic lithosphere. All diamonds were subsequently sampled by kimberlites and transported to the Earth's surface.
Description
13 page(s)
Subject Keyword
040299 Geochemistry not elsewhere classified
Subject Keyword
040313 Tectonics
Subject Keyword
inclusions in diamond
Subject Keyword
Alberta diamonds
Subject Keyword
Buffalo Hills
Subject Keyword
carbon isotopes
Subject Keyword
nitrogen contents
Subject Keyword
nitrogen aggregation states
Resource Type
journal article
Organisation
Macquarie University. Dept. of Earth and Planetary Sciences
Organisation
Macquarie University. National Key Centre for Geochemical Evolution and Metallogeny of Continents (GEMOC)

Identifier
http://hdl.handle.net/1959.14/40007
Identifier
ISSN:0024-4937
Identifier
mq-rm-2004020678
Language
eng
Reviewed
Reviewed
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Citation Format
E-mail Address
Subject
"Lithos"
 
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