The similarity of the Lu-Hf and Sm-Nd isotope system during most mantl
e differentiation processes makes the combination of Hf-176/Hf-177 and
Nd-143/Nd-144 a very sensitive indicator of a select number of proces
ses. This paper present new Hf-isotope data for a large number of ocea
n islands and examines the Hf-Nd-Pb isotope relations of oceanic volca
nics. Except for HIMU islands, St. Helena and Tubaii, the Hf and Nd is
otope ratios in ocean island basalts (OIB) are extremely well correlat
ed. It is argued that crustal recycling (by either continental or ocea
nic sediments) most likely did not cause the Hf-Nd variations. The cor
related Hf-176/Hf-177-Nd-143/Nd-144 variations in OIB most likely repr
esent the time integrated fractionations which are the result of melti
ng in the presence of garnet. The Hf-isotope systematics of HIMU-type
OIB are consistent with these basalts representing recycled oceanic cr
ust and thus support the earlier hypothesis on the origins of HIMU bas
alts. Chondrites form an array that is at high angle with the OIB arra
y. This allows a choice in the Nd-143/Nd-144 and( 176)Hf/Hf-177 values
for chondritic bulk earth. With a choice of bulk earth at the extreme
end of the OIB array the shift of OIB to higher Hf-176/Hf-177 can be
explained by either isolation of a significant amount of basalts from
the mantle for several billions of year or by fractionation and isolat
ion of small amounts (< 1%) of perovskite during the early history of
the Earth. The large range in Hf-isotopes for a limited range in Nd-is
otopes in MORE can be explained by addition of small amounts (much les
s than 1%) of the perovskite material back into the MORE mantle. If ch
ondritic BE is chosen to be internal to the OIB the well correlated Hf
-Nd isotope characteristics in OIB argue against the fractionation of
perovskite during the early history of the Earth and the shape of the
MORE field remains an enigma. (C) 1998 Elsevier Science B.V. All right
s reserved.