Ra. Cliff et al., GEOCHRONOLOGICAL STUDIES OF PROTEROZOIC CRUSTAL EVOLUTION IN THE NORTHERN OUTER HEBRIDES, Precambrian research, 91(3-4), 1998, pp. 401-418
New data on the Proterozoic thermal and tectonic crustal history of th
e Lewisian complex have been determined using Sm-Nd and Ar-40-Ar-39 is
otopic analyses. Igneous assemblages from two mafic/ultramafic masses
indicate crystallization at 2.54 and 2.14 Ga from magmas with initial
Nd isotopic composition lower than predicted depleted mantle at those
times. Sm-Nd isotope systematics (T-DM=2.45 Ga) in two samples of meta
sediment from the Leverburgh Belt imply that they contain a significan
t post-Archaean component and cannot therefore be part of an Archaean
stratigraphic sequence. Sm-Nd mineral isotope data on three samples co
nfirm the Proterozoic age of high-pressure granulite facies metamorphi
sm in the South Harris igneous complex; the most precise estimate is 1
.827 +/- 0.016 Ga on a metagabbro which was intruded after deformation
of the host anorthosite under granulite facies conditions. Localized
granulite facies assemblages in Younger Basic bodies further north are
significantly younger at 1.63 Ga. Whole rock Sm-Nd data on two sample
s from the 1.7 Ga granite injection complex of South Harris indicate e
psilon(Nd) between -11.5 and -13.7 at the time of intrusion, providing
a strong indication that they were produced by remelting of pre-exist
ing crust similar to the exposed grey gneisses which had values close
to -12 at that time. Ar-40-Ar-39 data from 13 hornblendes generally sh
ow complex argon release patterns with indications of excess argon in
most samples. Flat sections of the spectra range in age between 1.63 a
nd 1.78 Ga. Previous Rb-Sr data on biotite showed a distinct break in
age pattern across the Langavat Belt. There is no indication of such a
break in the hornblende data and it is inferred that despite variatio
ns in the timing of peak metamorphism the whole of the northern Outer
Hebrides cooled through hornblende closure temperatures in the interva
l 1.7-1.6 Ga. (C) 1998 Elsevier Science B.V.