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6. PROVENANCE OF THE HP-HT UPPER ALLOCHTHON

117

Two-stage depleted mantle model ages (

T

DM

) were

calculated using present day

176

Hf/

177

Hf

=

0.283164

value for average MORB (Chauvel

et al.

, 2008)

which is assumed to be present-day depleted mantle

composition. This value corresponds to an initial

e

Hf

(

t

= 0 Ga)

=

13.4. DM evolution trend was propa-

gated to

e

Hf

(

t

= 4 Ga)

=

0, because the existence of a

voluminous-depleted mantle reservoir during Hadean

is highly speculative (see discussions in Hawkesworth

et al.

, 2010; Kemp

et al.

, 2010 and Zeh

et al.

, 2011).

T

DM

values for all data were calculated using a mean

176

Lu/

177

Hf of 0.0113 (average continental crust;

Rudnick & Gao, 2003).

MORB

176

Hf/

177

Hf interval was taken from the

Atlantic, Pacific and Indian MORB values (excepting

three unusual low values from the Indian Ocean)

reported by Chauvel & Blichert-Toft (2001)

considering a minimum

176

Hf/

177

Hf

=

0.28302

(

e

Hf

(

t

= 0 Ma)

=

8.3) and a maximum

176

Hf/

177

Hf

=

0.28337 (

e

Hf

(

t

= 0 Ma)

=

20.7). These values are prop-

agated to

e

Hf

(

t

= 4 Ga)

=

0, defining a field (blue dis-

continuous lines) around the DM-evolution trend, to

provide an indication of the likely range of DM com-

positions through time.

Sm

Nd whole-rock analyses

Sample preparation and analyses were performed at

the laboratory of Geocronologıa y Geoquımica

Isotopica at the UCM. Whole-rock samples were

dissolved by oven digestion in ultra-pure HF and

HNO

3

acids together with the

149

Sm/

150

Nd spike in

sealed teflon microreactors. Once the samples were

dissolved and dried, HNO

3

was added to eliminate

silica fluorides and then HCl was added to form

chlorine molecules. The sample was then subjected

to a two-stage conventional ion-exchange chro-

matography. The fractions where Sm and Nd were

present in high concentrations were dried and

loaded with H

3

PO

4

on rhenium filaments in triple

disposition, and analysed in a thermal ionization

mass spectrometer TIMS-Phoenix HCT040 follow-

ing a dynamic multicollector method. The measured

143

Nd/

144

Nd isotopic ratios were corrected for pos-

sible isobaric interferences from

142

Ce and

144

Sm

(only for samples with

147

Sm/

144

Sm

<

0.0001) and

normalized to

146

Nd/

144

Nd

=

0.7219 (O’Nions

et al.

,

1977) to correct for mass fractionation. The LaJolla

Nd international isotopic standard was analysed

during sample measurement, and gave an average

value of

143

Nd/

144

Nd

=

0.511847 for nine replicates,

with an internal precision of 0.000008 (2

r

). These val-

ues were used to correct the measured ratios for possible

instrumental bias following reference values from Lug-

mair

et al.

(1983). The analytic errors for

147

Sm/

144

Nd

ratio is 0.1% and for

143

Nd/

144

Nd is 0.006%. CHUR

present-day values considered for this study are

147

Sm/

144

Nd

=

0.1967 (Jacobsen & Wasserburg, 1980)

and

143

Nd/

144

Nd

=

0.512638 (Hamilton

et al.

, 1983).

The DM evolution trend and DM model ages (

T

DM

)

have been calculated as described by DePaolo (1981)

using

147

Sm/

144

Nd ratios and MDAs for each sample

(Fig. 9). A

147

Sm decay constant of 6.539

9

10

11

a

1

has been used, calculated from

147

Sm half-life reported

by Lugmair & Marti (1978) and Begemann

et al.

(2001). MORB epsilon values of

+

7 to

+

12 used are

those reported by DePaolo &Wasserburg (1976).

Fig. 5.

Relative abundance of Banded

Gneisses U

Pb zircon ages for each

significant age population represented as

bar diagrams, for each sample and for the

total U

Pb zircon analyses. Green:

Palaeozoic and Neoproterozoic; yellow:

Mesoproterozoic; pale pink:

Paleoproterozoic; dark pink: Archean

population.

0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1

0

500 1000 1500 2000 2500 3000

Age cumulative probability

(Ma)

GCH-02

GCH-06

GCH-17

GCH-21

GCH-24

Cariño

Gneisses

HP-HT Upper

Allochthon:

IP Upper

Allochthon:

Fig. 6.

Cumulative density plots for each of the HP

HT

Upper Allochthon samples, and for the IP Upper Allochthon.

©

2015 John Wiley & Sons Ltd

PROVENANCE OF THE HP

HT VARISCAN TERRANE

967