Research output: Contribution to journal › Article › peer-review
The New Massadou Diamondiferous Kimberlite Field in Guinea. / Afanasiev, V. P.; Nikolenko, E. I.; Glushkova, N. V. et al.
In: Geology of Ore Deposits, Vol. 61, No. 4, 01.07.2019, p. 381-390.Research output: Contribution to journal › Article › peer-review
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TY - JOUR
T1 - The New Massadou Diamondiferous Kimberlite Field in Guinea
AU - Afanasiev, V. P.
AU - Nikolenko, E. I.
AU - Glushkova, N. V.
AU - Zolnikov, I. D.
PY - 2019/7/1
Y1 - 2019/7/1
N2 - Abstract: A new Massadou kimberlite field, was discovered in southeastern Guinea, near the town of Macenta. It consists of 16 poorly diamondiferous kimberlite dikes, ~1 m thick on average. The ore-controlling zone has a width of around 600 m, its orientation corresponds to the K-4 trend after S. Haggerty, and it is quite well detectable in satellite images. A thick laterite weathering profile has developed on the kimberlites. The main indicator minerals are pyrope, chromite, and ilmenite. Ilmenite grains have a zoned structure with a high-Fe core (hemoilmenite) overgrown by a parallel-columnar aggregate of Mg-ilmente rim resulting from interaction of the core phase with kimberlitic melt. The age of kimberlites is estimated as 140–145 Ma by analogy with those in adjacent areas. Dikes occur as an independent form of kimberlite magmatism in the Guinean–Liberian shield, rather than being roots of kimberlite pipes; therefore, the erosion cutout is relatively small and large-scale diamond placers should not be expected.
AB - Abstract: A new Massadou kimberlite field, was discovered in southeastern Guinea, near the town of Macenta. It consists of 16 poorly diamondiferous kimberlite dikes, ~1 m thick on average. The ore-controlling zone has a width of around 600 m, its orientation corresponds to the K-4 trend after S. Haggerty, and it is quite well detectable in satellite images. A thick laterite weathering profile has developed on the kimberlites. The main indicator minerals are pyrope, chromite, and ilmenite. Ilmenite grains have a zoned structure with a high-Fe core (hemoilmenite) overgrown by a parallel-columnar aggregate of Mg-ilmente rim resulting from interaction of the core phase with kimberlitic melt. The age of kimberlites is estimated as 140–145 Ma by analogy with those in adjacent areas. Dikes occur as an independent form of kimberlite magmatism in the Guinean–Liberian shield, rather than being roots of kimberlite pipes; therefore, the erosion cutout is relatively small and large-scale diamond placers should not be expected.
KW - diamond
KW - Guinean–Liberian shield
KW - kimberlite
KW - kimberlite indicator minerals
KW - tectonic control of kimberlites
KW - Guinean-Liberian shield
UR - http://www.scopus.com/inward/record.url?scp=85071993765&partnerID=8YFLogxK
U2 - 10.1134/S1075701519030024
DO - 10.1134/S1075701519030024
M3 - Article
AN - SCOPUS:85071993765
VL - 61
SP - 381
EP - 390
JO - Geology of Ore Deposits
JF - Geology of Ore Deposits
SN - 1075-7015
IS - 4
ER -
ID: 21472605