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The Kharamai kimberlite field, Siberia: modification of the lithospheric mantle by the Siberian Trap event
Authors:WL Griffin  LM Natapov  SY O'Reilly  E van Achterbergh  AF Cherenkova  VG Cherenkov
Institution:

aGEMOC ARC National Key Centre, Department of Earth and Planetary Sciences, Macquarie University, NSW 2109, Australia

bCSIRO Exploration and Mining, North Ryde, NSW 2113, Australia

cAerogeologia, Enterprise of Russian Ministry of Natural Resources, 35 Leninsky Prospect,119071, Moscow, Russia

Abstract:The kimberlites of the Kharamai field intruded through the Siberian Traps shortly after their eruption in Permo-Triassic time. The composition and thermal state of the subcontinental lithospheric mantle (SCLM) beneath the Kharamai field in lower Triassic time have been reconstructed using major- and trace-element analyses of 345 Cr-pyrope garnet xenocrysts from six of the kimberlites, supplemented by a small suite of mantle-derived peridotite xenoliths. The data define a geotherm lying near a 38 mW/m2 conductive model to a depth of ca 170 km, where the base of the depleted lithosphere is defined by a marked increase in melt-related metasomatism and by an inflected geotherm. Compared to the SCLM sampled by Devonian (pre-Trap) kimberlites in the same and adjacent terranes, the Kharamai SCLM in Triassic time was warmer and was cooling from a previous thermal high. It was also thinner than the SCLM beneath the Daldyn and Alakit kimberlite fields, and had been strongly metasomatised. The metasomatism lowered the mean Fo content of olivine (from ≥Fo93 to Fo92), greatly reduced the proportion of subcalcic harzburgites, and increased the proportion of fertile lherzolites, especially in the depth range of 80–130 km. The overall pattern of metasomatism is similar to that observed in the SCLM sampled by the Group I kimberlites of the SW Kaapvaal Craton, and inferred to be related to the Karoo thermal event. These observations suggest that events such as the eruption of the Karoo basalts and Siberian Traps change the composition of the SCLM, but do not necessarily destroy it, at distances of several hundred kilometres from the main eruption centres.
Keywords:Kharamai kimberlite field  Permo-Triassic time  Metasomatism
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