Ajw. Markwick et H. Downes, Lower crustal granulite xenoliths from the Arkhangelsk kimberlite pipes: petrological, geochemical and geophysical results, LITHOS, 51(1-2), 2000, pp. 135-151
Five mafic garnet granulite xenoliths have been obtained from Devonian kimb
erlite hosts from the Pachuga field, Arkhangelsk, NW Russia. Whole rock maj
or and trace element data, Sr and Nd isotopic analyses, mineral chemistry,
calculated compressional wave velocities and densities of the xenoliths are
reported here. The xenoliths are medium grained and are reasonably fresh w
ith well-developed granoblastic fabrics. Primary mineralogy consists of alm
andine-pyrope-rich garnet, diopside, oligoclase plagioclase and scapolite;
minor phases include rutile and ilmenite. One sample contains only garnet a
nd metasomatic pargasitic amphibole, pseudomorphing primary diopside. All a
nalysed samples have sub-alkaline basaltic compositions. REE patterns show
variable LREE-enrichment (La-N/Yb-N = 13 to 1.4) and small negative and pos
itive Eu anomalies (0.87-1.32), indicating that both plagioclase fractionat
ion and accumulation have occurred. Present-day Sr-87/Sr-86 and Nd-143/Nd-1
44 isotope ratios are very low (0.70272-0.70378 and 0.511736-0.512225, resp
ectively), suggesting that both assimilation of Archaean continental crust
and removal of Rb, possibly related to granulite-facies metamorphism, took
place early in the history of these rocks. P/T estimates (670-730 degrees C
, 1.4-1.6 GPa) indicate equilibration depths of up to 50 km. Calculated com
pressional wave velocities range from 6.94 to 7.70 km/s and densities from
3.2 to 3.5 Mg/m(3), assuming P/T conditions of 500 degrees C and 1.4 GPa. T
hese values support an origin in the deep continental crust. T-DM model age
s are 1.7 to 1.9 Ga and may represent the time of extraction from the mantl
e during the mid-Proterozoic. These xenoliths may represent the in situ maf
ic lower crust beneath Arkhangelsk, formed as a result of basaltic underpla
ting during the mid-Proterozoic. (C) 2000 Published by Elsevier Science B.V
. All rights reserved.