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Lithos 70 (2003) 91–110
Very fast exhumation of high-pressure metamorphic rocks with
excess 40Ar and inherited 87Sr, Betic Cordilleras, southern Spain
Koen de Jong*
Department of Isotope Geochemistry, Vrije Universiteit, Amsterdam, The Netherlands
CNRS, UMR 6526 Geosciences Azur, Universite de Nice-Sophia Antipolis, Nice, France
Abstract
In order to attempt to further constrain the age of the early Alpine tectonic evolution of the Mulhacen Complex and to
explore the influence of inherited isotopes, micas from a small number of well-characterised rocks from the Sierra de los
Filabres, with a penetrative tectonic fabric related to the exhumation of eclogite-facies metamorphic rocks, were selected for40Ar/39Ar and Rb–Sr dating.
A single phengite grain from an amphibolite yielded an 40Ar/39Ar laser step heating plateau age of 86.9F 1.2 Ma (2r; 70%39Ar released) and an inverse isochron age of 86.2F 2.4 Ma with an 36Ar/40Ar intercept within error of the atmospheric value.
Induction furnace step heating of a biotite separate from a gabbro relic in an eclogite yielded a weighted mean age of
173.2F 6.3 Ma (2r; 95% 39Ar released). These ages are diagnostic of excess argon (40ArXS) incorporation, as they are older
than independent age estimates for the timing of eclogite-facies metamorphism and intrusion of the gabbros. 40ArXSincorporation probably resulted from restricted fluid mobility in the magmatic rocks during their metamorphic recrystallisation.
Rb–Sr whole-rock–phengite ages of graphite-bearing mica schists from Paleozoic rocks (Secano unit) show a dramatic
variation (66.1F 3.2, 40.6F 2.6 and 14.1F 2.2 Ma). An albite chlorite mica schist from the Mesozoic series of the Nevado–
Lubrın unit has a whole-rock–mica–albite age of 17.2F 1.9 Ma, which is within error of an 40Ar/39Ar plateau age published
previously and of the youngest Rb–Sr age of the Paleozoic series obtained in this study. The significant spread in Rb–Sr ages
implies that progressive partial resetting of an older isotopic system has occurred. The microstructure of the samples with pre-
Miocene Rb–Sr ages reveals incomplete recrystallisation of white mica and inhibited grain growth due to the presence of
graphite particles. This interpretation agrees with previously published, disturbed and slightly dome-shaped 40Ar/39Ar age
spectra that may point similarly to the presence of an older isotope component. The progressively reset Rb–Sr system is a relic
of Variscan metamorphism of the Paleozoic series of the Mulhacen Complex. In contrast, the origin of the ca. 17.2 Ma old
sample from the Mesozoic series precludes any isotopic inheritance, in agreement with its pervasive tectono-metamorphic
recrystallisation during the Miocene.
Exhumation of the eclogite-facies Mulhacen Complex occurred in two stages with contrasting rates of about 22.5 mm/year
during the early phase and 9–10 mm/year during the late phase; the latter with a cooling rate in the order of 330 jC/Ma.
D 2003 Elsevier B.V. All rights reserved.
Keywords: 40Ar/39Ar dating; Excess argon; Isotope inheritance; Phengite; Biotite; Fluids
0024-4937/$ - see front matter D 2003 Elsevier B.V. All rights reserved.
doi:10.1016/S0024-4937(03)00094-X
* Present address. Argon Geochronology Laboratory, Department of Geosciences, National Taiwan University, 245 Choushan Road, Taipei
106, Taiwan, ROC. Tel.: +886-2-3365-1899; fax: +886-2-2363-6095.
E-mail address: [email protected] (K. de Jong).
K. de Jong / Lithos 70 (2003) 91–11092
1. Introduction
Phengite has yielded meaningful 40Ar/39Ar plateau
ages for eclogite-facies metamorphic rocks (Bosse et
al., 2000), but research during the last decade of the
20th century provided a lot of evidence for the incor-
poration of excess argon (40ArXS) in its lattice (e.g.
Tonarini et al., 1993; Li et al., 1994; Arnaud and
Kelley, 1995; Inger et al., 1996; Sherlock et al.,
1999). 40ArXS uptake occurs in association with partial
recrystallisation of high-pressure phengite during sub-
sequent metamorphism at lower temperature and pres-
sure (Hammerschmidt and Franz, 1992; Hannula and
McWilliams, 1995; Ruffet et al., 1995; Reddy et al.,
1996; de Jong et al., 2001). Alternatively, strongly
restricted fluid mobility, leading to the incorporation of
locally derived (inherited) argon, is commonly quoted
as the mechanism responsible for the frequently ob-
served elevated phengite 40ArXS ages in (ultra-) high-
pressure metamorphic rocks (Scaillet, 1996; Boundy et
al., 1997; Li et al., 1999; Giorgis et al., 2000), and is
also seen as the reason for the survival of pre-orogenic
Rb–Sr ages in biotite (Verschure et al., 1980; Kuhn et
Fig. 1. Tectonic map of the eastern Betic Cordilleras, modified after de Jo
(Figs. 2 and 3) are outlined. Stars: samples from the Sierra de Baza (SdB
al., 2000). It appeared that incorporation of argon into
phengite may have been controlled by very low lattice
and grain boundary diffusion under dry, eclogite-facies
conditions and that the gas has been internally derived
from within the eclogite protoliths.
de Jong et al. (2001) attempted to constrain the age
of early Alpine exhumation of the Mulhacen Complex
of the Internal Zone of the Betic Cordilleras of
southern Spain, or Betic Zone (Fig. 1). They obtained
widely scattered 40Ar/39Ar laser step heating plateau
ages between 15.8F 0.4 and 90.1F1.0 Ma (2r) onwell-crystallised single phengite grains from orthog-
neisses in a small area in the easternmost Sierra de los
Filabres (Fig. 2). Age discordance was observed at the
outcrop scale as well as in individual grains. The
authors explained these phenomena by 40ArXS uptake
that seems to be associated with the gneisses, since the
Rb–Sr ages in these rocks are systematically younger
than the K–Ar and 40Ar/39Ar ages. Specific to this
case is the occurrence of hydraulic cracks in the
gneisses, high atmospheric contamination and submi-
croscopic illitisation of phengite, permitting 40ArXSstorage in interlayer vacancies and other lattice imper-
ng (1993a). The sampled areas in the eastern Sierra de los Filabres
) and from Cerro del Almirez (CdA) are discussed.
Fig. 2. Geological map of the easternmost Sierra de los Filabres, modified after de Jong et al. (2001), with the sample locations indicated by
arrows. The Ar/Ar total gas ages obtained by these authors on single phengite grains at different locations (stars) in gneiss body of the Macael–
Chive unit are indicated.
K. de Jong / Lithos 70 (2003) 91–110 93
K. de Jong / Lithos 70 (2003) 91–11094
fections. The oldest phengite was from a coarse-
grained gneiss with closely spaced late-stage hydrau-
lic cracks, which are lacking in fine-grained mylonitic
gneiss that yielded the youngest micas. Hence, the
interaction of meteoric waters with the hot metamor-
phic rocks, phengite recrystallisation and 40ArXS up-
take were much more intense in the coarse-grained
gneiss. Like the fine-grained mylonitic gneisses, mica
schists and mica-bearing foliated amphibolites lack
such extensively developed hydraulic crack networks,
rendering them less liable for the incorporation of40ArXS by this mechanism. Accordingly, white mica
from albite–chlorite–mica schists and marbles with a
penetrative S2 yielded 15.4–17.6 Ma 40Ar/39Ar pla-
teau and total fusion ages (de Jong et al., 1992) that
are not obviously affected by significant levels of
incorporated 40ArXS.
The aim of the present study is to investigate
further the occurrence and source of excess argon as
well as the role of limited fluid mobility in the
incorporation process during the early tectono-meta-
morphic evolution of the Mulhacen Complex in the
Sierra de los Filabres. For this purpose, we used
biotite from a gabbro with a Late Jurassic Rb–Sr
isochron age, in which 40ArXS incorporation has been
established, and that occurs in the core of an eclogite,
which is chemically well characterised. In addition,
we selected a phengite grain from an amphibolite,
which occurs in the same level as the eclogite, and
that acquired a penetrative fabric during the main
tectono-metamorphic phase, D2, subsequent to the
eclogite-facies metamorphism. Also, we applied
Rb–Sr dating to a small number of mica schists with
a tectono-metamorphic fabric that was formed during
D2 and which, in a previous study, yielded 40Ar/39Ar
age spectra that are in part slightly dome-shaped and
in one case flat. Our data set has a large spread in
ages, which is interpreted as due to the occurrence of40ArXS and partially inherited radiogenic 40Ar and87Sr isotopes, but, the least affected samples permitted
to date the timing of exhumation of the Mulhacen
Complex as Middle Miocene.
2. Tectonic setting
The Betic Zone comprises a stack of four nappe
complexes that have overthrust the southernmost
External Zone, which crops out in windows as the
(very) low-grade metamorphic Almagride Complex
(Fig. 1; Simon, 1987; de Jong, 1993a). These are,
from top to bottom: (1) the Malaguide Complex, (2)
Alpujarride Complex, (3) Mulhacen Complex and (4)
Veleta Complex (Egeler and Simon, 1969; Puga and
Diaz de Federıco, 1978; de Jong, 1993a,b; Puga et
al., 1999, 2002). The Alpujarride and Mulhacen
complexes have basal series of graphite-rich metape-
lites and cover series of metapelites and metapsam-
mites with abundant metacarbonates and greenstones
and locally gypsum (Egeler and Simon, 1969; de
Jong and Bakker, 1991; de Jong, 1991). The carbon-
ate series of the Alpujarride Complex are well dated
as Middle to Late Triassic by microfossils (Kozur et
al., 1985; Simon, 1987), whereas the basal series of
some tectonic units yielded Variscan ion-microprobe
zircon ages (Zeck and Williams, 2001, and references
therein). The Mulhacen Complex experienced an
Alpine metamorphism composed of a sequence of
different metamorphic facies (de Roever and Nijhuis,
1963), as well as pre-Alpine recrystallisation, as will
be outlined below. The Malaguide Complex has a
Paleozoic basal series covered by a condensed, but
almost complete Mesozoic and Tertiary section
(Egeler and Simon, 1969). Sediment petrographical
analysis of its Late Paleozoic series implies that it
experienced a Variscan orogeny (Herbig and Statteg-
ger, 1989; Henningsen and Herbig, 1990), although a
major angular unconformity between the Paleozoic
and younger series did not form (Makel, 1988). The
Veleta Complex comprises a monotonous lithological
sequence of graphite-bearing mica schists and quartz-
ites that yielded rare Middle Devonian (Lafuste and
Pavillon, 1976) and Riphean (Gomez-Pugnaire et al.,
1982) fossils. The Alpine tectono-metamorphic
recrystallisation has essentially obliterated the pre-
Alpine fabrics and mineral assemblages, except for
inclusions in chloritoid porphyroblasts in some mica
schists that are very rich in graphite (Puga and Diaz
de Federıco, 1978; Gomez-Pugnaire and Sassi, 1983;
Puga et al., 2002).
2.1. The Mulhacen Complex
The Mulhacen Complex in the Sierra de los
Filabres is composed of three superimposed nappes
(Figs. 2 and 3), each with a probably Paleozoic
Fig. 3. Geological map of the northern part of the central Sierra de los Filabres, modified after de Jong et al. (1992), with arrows indicating the
sampled sites. Thrust slices on top of the Alpujarride Complex consisting of rocks of the Mulhacen Complex, north of Huertecicas Altas, have
been omitted for clarity. Triangles indicate nappe contacts.
K. de Jong / Lithos 70 (2003) 91–110 95
K. de Jong / Lithos 70 (2003) 91–11096
basal series of graphite-rich garnet mica schists that
contain orthogneisses and metagranites in the up-
permost two nappes (de Jong and Bakker, 1991).
The cover series are generally regarded as Triassic
and younger and comprise alternating quartzites and
(albite-bearing) mica schists with marble levels in
the upper parts (de Jong and Bakker, 1991; Tendero
et al., 1993), hereafter called Mesozoic series.
Ultramafic rocks, mainly serpentinites, and abundant
greenstones occur in these higher levels, in part as a
mapable unit of amphibolites and amphibole mica
schists ((Figs. 2 and 3); de Jong and Bakker, 1991,
encl. 1). Early Alpine eclogites occur locally in
these greenstones (Morten et al., 1987; Bakker et
al., 1989; Gomez-Pugnaire et al., 1989; Puga et al.,
1989, 1999), which are wrapped by the main
foliation (S2) in the matrix. Part of the eclogite-
facies metabasites are derived from often cumulitic
gabbros, with partly preserved igneous paragenesis,
a MORB-like chemical composition and 143Nd/144Nd ratios higher than 0.5130 and 87Sr/86Sr ratios
below 0.705 (Puga et al., 2002). Morten et al.
(1987) inferred that crystallisation of the gabbros
occurred at pressures below 1 GPa. A troctolitic
gabbro in the core of an eclogite yielded an Rb–Sr
mineral isochron age of 146F 3 Ma (Hebeda et al.,
1980). The serpentinites are derived from spinel
lherzolites and secondary harzburgites with spini-
fex-like textures, which both contain abundant part-
ly rodingitised dolerite dykes (Puga et al., 2002).
The origin of the greenstone association is still a
matter of debate, with models ranging from a
dismembered ocean floor sequence (Puga et al.,
1989, 1999, 2002) to continental, rift-related mag-
matism (Gomez-Pugnaire et al., 2000). Glauco-
phane-bearing dolerites have locally well-preserved
intrusive contacts with calcite marbles (de Jong and
Bakker, 1991). The greenstone association may
have developed in small oceanic pull-apart basins
situated in a major continental strike-slip zone that
connected Late Jurassic spreading centres in the
Atlantic and Ligurian Oceans (de Jong, 1991,
1993a).
Maximum pressures of 2.0–2.2 GPa have been
estimated for kyanite eclogites (Puga et al., 1999,
2002) and metamorphic ultramafic rocks (Lopez
Sanchez-Vizcaıno et al., 2001) in the Mulhacen
Complex at temperatures of about 700 jC. Strong
decompression concomitant with cooling of the rocks
to 500–600 jC took place during and subsequent to
the main tectono-metamorphic phase, D2, which
occurred at a pressure of about 1.5–1.7 GPa (Puga
et al., 2002) and 0.8–1.2 GPa (Bakker et al., 1989;
de Jong, 1991, 1993a) during the final phase (Fig.
10). This resulted in pervasive amphibolitisation of
the eclogites. Further retrogression is marked by
widespread albite and chlorite growth that occurs
synkinematically with a phase of localised penetra-
tive D3 folding at pressures of about 0.4–0.5 GPa
and temperatures around 400 jC (Fig. 10; de Jong,
1991, 1993a,c). The cooling was followed by pro-
nounced late stage fluid-assisted reheating shown by
the widespread occurrence of rims of oligoclase and
biotite around albite and chlorite, respectively, as
well as by rare and local growth of staurolite and
kyanite during the early stages of D4 in mica schists
of the Mesozoic series of the Nevado–Lubrın unit
(Bakker et al., 1989; de Jong, 1991, 1993a,c). The
absence of garnet constrains the P–T conditions at
around 0.4–0.5 GPa and temperatures of about 500
jC (Fig. 10). The reheating was related to extension
(Bakker et al., 1989; de Jong, 1991, 1993a), which
resulted in recrystallisation, isotope resetting and40ArXS incorporation (de Jong et al., 2001). Ductile
(D5) and brittle–ductile (D6) shear zones, which
developed during retrogression, occur at various
levels within the Mulhacen Complex, but character-
istically at the contact with the overlying Alpujarride
Complex (de Jong, 1991, 1993a,c).
Micas from rocks with a penetrative alpine tectonic
foliation have Rb–Sr ages that generally range be-
tween 12.5 and 16.9 Ma, whereas K–Ar and 40Ar/39Ar
dates span 13.7–90.7 Ma (Monie et al., 1991; de Jong
et al., 1992, 2001). Monie et al. (1991) obtained40Ar/39Ar ages of 24.6F 3.6 and 48.4F 2.2 Ma on
amphibole (Sierra de Baza, Fig. 1). Eleven SHRIMP
U–Pb analysis on nine zircon grains in a pyroxenite
layer in ultramafic rocks (Cerro del Almirez, Fig. 1),
which are characterised by high pressure breakdown
of antigorite to spinifex-textured olivine and ortho-
pyroxene, yielded a mean age of 15.0F 0.6 Ma
(2r) (Lopez Sanchez-Vizcaıno et al., 2001). This
U–Pb zircon age is comparable to the majority of
Rb–Sr ages of white mica and to 40Ar/39Ar ages of
this mineral that are the least affected by 40ArXSuptake. Zircon fission-track ages of the Sierra de los
K. de Jong / Lithos 70 (2003) 91–110 97
Filabres are in the 11–14 Ma range (Johnson et al.,
1997).
2.2. Pre-alpine history of the Mulhacen Complex
Despite the pervasive nature of Alpine tectono-
metamorphic recrystallisation, the basal series of the
Mulhacen Complex contain unambiguous relics of
pre-Alpine tectono-metamorphic evolution. Pre-Al-
pine deformation structures are found in the deeper
part of the complex in the Sierra Nevada, in some
boudins or layers of graphite-bearing mica schists,
which also contain pre-Alpine amphibolite-facies par-
ageneses (Puga et al., 1975, 2002; Puga and Diaz de
Federıco, 1978). The occurrence of chloritoid + al-
mandine, chiastolite + almandine + biotiteF staurolite
parageneses or rare cordierite points to P–T condi-
tions of about 0.2–0.3 GPa and 500–600 jC (Puga et
al., 2002). Elsewhere, studies of the relationship
between mineral growth and superimposed deforma-
tion phases have not yielded any evidence for the
presence of relic minerals that did not form during
Alpine metamorphism (Kampschuur, 1975; Martınez
Martınez, 1980; Bakker et al., 1989; de Jong, 1991).
However, complex inclusion patterns in the cores of
some Alpine porphyroblasts in the Sierra de los
Filabres have been interpreted as due to a pre-Alpine
orogeny (Helmers and Voet, 1967; Vissers, 1977),
especially in garnets and staurolites that are spatially
associated with orthogneisses.
Gneisses and metagranites of the basal series of
this complex in the Sierra de los Filabres have yielded
Rb–Sr errorchrons ranging between 275 and 191 Ma
(Andriessen et al., 1991), which the authors discussed
in the context of partial Alpine resetting and incom-
plete isotope rehomogenisation. A 267F 29 Ma Rb–
Sr age (Andriessen et al., 1991) and a 307F 34 Ma
Sm–Nd isochron (Nieto, 1996) are regarded as the
best estimate of the crystallisation age of the subsol-
vus granites. The country rock to these intrusives is
affected by contact metamorphism, as revealed by the
occurrence of hedenbergite skarn and hornfels bodies
(Helmers, 1982; de Jong and Bakker, 1991). The
petrology of the granites and associated contact meta-
morphic rocks indicates an intrusion depth of at least 6
km (de Jong and Bakker, 1991), which agrees with
P–T estimates for pre-Alpine mineral assemblages
described by Puga et al. (2002).
3. Sample description
3.1. Troctolitic gabbro
Biotite separate ALM 104 (63–125 Am sieve
fraction) has been obtained from a 1-m diameter
massive troctolitic gabbro that occurs in an eclogite,
which yielded a 146F 3 Ma Rb–Sr mineral isochron
age and an initial 87Sr/86Sr ratio of 0.7028F 0.0001
(Hebeda et al., 1980). The biotite separate is known to
have 40ArXS and was used as one of the points that
defined the isochron and was selected for analysis to
better understand this phenomenon. The gabbro is
separated from the underlying albite chlorite mica
schists (Tahal schists, de Jong and Bakker, 1991) by
a fault that was folded during D4 and subsequently
reactivated as a low-angle D6 detachment fault (de
Jong, 1993c). This outcrop is part of a series of
amphibolites and amphibole mica schists of the
Nevado–Lubrın unit (Fig. 2). The course-grained
gabbro has a cumulitic texture with olivine and
labradorite–oligoclase as cumulus phases and clino-
pyroxene as well as minor brown hornblende and
biotite as intercumulus phases.
3.2. Micaceous amphibolite
The slightly elongated (0.75� 1.5 mm) single phen-
gite grain, JK 0, which has been used for 40Ar/39Ar
dating, was obtained from a well-crystallised amphib-
olite with a strongly developed tectonic fabric, from the
same lithological unit as ALM 104 (Fig. 2). Blue-green
hornblende and phengite have a well-developed shape-
preferred orientation with respect to foliation S2,
whereas c-axes of the amphibole are parallel to the
lineation L2. Cores of a number of blue-green horn-
blendes contain relics of glaucophane. The transforma-
tion of glaucophane to blue-green hornblende is a syn-
D2 reaction (Bakker et al., 1989; de Jong, 1991,
1993a,c).
3.3. Mica schists
Mineral separates in the 125–250 Am sieve frac-
tion of four mica schists have been used for Rb–Sr
mineral dating. The same white mica separate of three
of these samples has been analysed by 40Ar/39Ar
furnace step-heating, which yielded a plateau age of
K. de Jong / Lithos 70 (2003) 91–11098
17.3F 0.2 Ma (ALM 270) and in two cases an40Ar/39Ar age spectra with progressively increasing
apparent ages over the main part of degassing that is
somewhat dome shaped as the last important degass-
ing step is slightly younger (Fig. 9). Total gas ages are
19.1F 0.1 (ALM 272) and 25.9F 0.1 Ma (ALM
273). The 40Ar/39Ar isotopic data are given in de
Jong et al. (1992). The samples were chosen to better
understand why some samples yielded disturbed age
spectra and others did not.
The mica schists have a penetrative quartz–mica
differentiated S2 foliation. ALM 272, 273 and 274 are
Table 140Ar/39Ar analytical data of micas from greenstones, Nevado–Lubrın uni
Step 40Aratm (%) 39ArK (10� 13 cm3) 39Ar (%)
ALM 104 (biotite separate, 63–125 lm, 6.0 mg) (furnace step heating) (
450 100.00 6.14 0.06
550 88.31 69.35 0.73
650 75.86 48.22 0.51
700 68.59 51.79 0.54
780 79.80 116.91 1.22
840 39.19 330.87 3.46
880 15.36 648.98 6.79
920 9.74 1428.49 14.95
960 10.60 2128.77 22.28
1000 13.55 1396.01 14.61
1050 13.10 1211.42 12.68
1150 10.99 1994.65 20.88
1350 26.54 120.59 1.26
Fuse 92.55 1.56 0.02
Inverse isochron age steps 450–1150 = 173.2F 8.7 Ma; 40Ar/36Ar interce
JK 0 (single phengite grain) (laser step heating) (J = 0.01709F 1%, 2r)0.35 97.25 110.53 0.65
0.40 92.67 101.01 0.59
0.45 90.65 325.50 1.92
0.56 54.89 4501.07 26.67
0.64 14.24 2846.62 16.86
0.70 14.47 1629.74 9.66
0.82 19.72 2280.95 13.51
0.89 23.11 856.17 5.07
0.99 27.03 838.18 4.96
1.20 23.63 2491.93 14.76
Fuse 19.52 900.83 5.33
Inverse isochron plateau steps (0.35–0.82) = 86.2F 2.4 Ma; 40Ar/36Ar in
Step = temperature (jC) or laser output power (in Watt) for material analys
the atmospheric 40Ar; 40Ar* is the radiogenic argon from natural K-decay39ArK (K-derived argon during irradiation) is based on a mass spectromete
2r level; step ages do not include the errors in J and the age of the flux
measured: 288F 0.5.
graphitic chloritoid garnet mica schists from the
Secano unit (Fig. 3; sensu, Helmers and Voet,
1967). This unit, which resembles the basal series of
the Macael–Chive unit, however, without gneisses, is
separated from the underlying Nevado–Lubrın unit
by a D6 detachment fault (de Jong, 1991). ALM 272
and 273 are taken from the same outcrop within 20 m
from each other. ALM 274 is the most quartz-rich
sample and the least graphite rich. Chloritoid and
garnet porphyroblasts were formed pre- and syn-D2,
during which the main tectonic foliation of the rocks
was formed. Continuous lattice bending and limited
t
37ArCa/39ArK
40Ar*/39ArK Apparent age (Ma)
J = 0.01716F 1%, 2r)3.664 – –
0.000 2.48F 3.79 75.3F 50.3
0.731 5.90F 2.16 174.1F106.6
4.203 5.43F 0.77 160.7F 61.0
0.596 4.96F 0.51 147.3F 21.8
0.325 5.40F 0.35 159.9F 14.4
0.002 5.58F 0.11 165.0F 9.8
0.000 5.57F 0.08 164.6F 3.2
0.081 5.70F 0.11 168.3F 2.2
0.015 5.91F 0.14 174.1F 3.1
0.000 6.17F 0.07 181.5F 3.8
0.000 6.30F 1.10 185.2F 2.0
1.177 12.71F146.52 355.9F 28.0
24.133 40.30F 1.69 948.1F 2681.4
Total age: 174.7F 1.6
pt = 281F 82; MSWD=15
0.045 9.87F 11.82 282.1F 312.6
0.011 3.25F 1.70 98.0F 50.0
0.013 3.13F 0.96 94.3F 28.0
0.001 2.91F 0.08 87.8F 2.4
0.001 2.90F 0.04 87.7F 1.2
0.001 2.86F 0.06 86.3F 1.7
0.001 2.85F 0.04 86.0F 1.4
0.002 2.82F 0.10 85.4F 2.8
0.004 2.76F 0.12 83.5F 3.7
0.006 2.80F 0.06 84.7F 1.6
0.007 3.01F 0.08 90.8F 2.4
Total age: 87.9F 2.2
tercept = 299.0F 4.8; MSWD=0.96
ed with an induction furnace or a laser probe, respectively. 40Aratm is
; 37ArCa is the Ca-derived argon during irradiation. The volume of
r sensitivity of 7� 10� 10 V cm� 3 STP. Uncertainty is quoted at the
monitor. Decay constant 40Ktot = 5.543� 10� 10 year� 1. 40Ar/36Ar
K. de Jong / Lithos 70 (2003) 91–110 99
recrystallisation to strain-free phengite in microfold
hinges is especially prominent in ALM 272 and ALM
273. Continuity between microfold limbs and hinges
is often maintained, and hence, the amount of shape-
preferred orientation of white mica parallel to S2cleavage septa is relatively limited. Such a micro-
structure points to the pinning of mica (sub) grain
boundaries and dislocations on graphite particles.
Cleavage microlithons contain relics of S1.
ALM 270 is an albite chlorite mica schist from the
Mesozoic series of the Nevado–Lubrın unit (La Yedra
Schists and Marbles, de Jong and Bakker, 1991; Fig.
2). The sample is not affected by D3 crenulations, but
chlorite and albite porphyroblasts, which are syn-D3
minerals (de Jong, 1991, 1993a,c), overgrew S2.
Phengite grains are well crystallised and strain-free,
and generally lie with their basal cleavage plane in the
differentiated S2 layering.
Fig. 4. 40Ar/39Ar induction furnace step heating age spectrum (lower
panel) and 37ArCa/39ArK ratio spectrum (upper panel) of biotite
separate ALM 104 from the Mesozoic series of the Nevado–Lubrın
unit. The Rb–Sr mineral isochron age obtained by Hebeda et al.
(1980) is indicated by the grey horizontal line.
4. Experimental procedures and mineral
separation
Single phengite grain JK 0 was selected for40Ar/39Ar incremental heating and separated from
the hand specimen after gentle crushing. It was
carefully selected under a binocular zoom microscope
and subsequently ultrasonically cleaned in demineral-
ised water for 5 min. Mineral separates for Rb–Sr and40Ar/39Ar analyses were prepared from the sieve
fractions by means of a Faul table, a laboratory
overflow centrifuge employing heavy liquids and a
Frantz isodynamic magnetic separator.40Ar/39Ar analyses were made at the University of
Nice-Sophia Antipolis (France) following the proce-
dures outlined in detail by de Jong et al. (2001).
Biotite separate ALM 104 was wrapped in high purity
Al foil and incrementally heated to fusion with a high-
frequency furnace system, whereas phengite single
grain JK 0 was step heated using an argon ion laser
probe with a continuous beam defocused to at least
twice the grain diameter. Homogeneity of the heating
of the grain was monitored with a coupled video-
microscope system. The laser extraction line consists
of an Innova Coherent 70-4 continuous argon ion
laser in combination with a sensitive gas mass spec-
trometer comprising a 12 cm, 120j M.A.S.S.E.Rtube, a Baur-SignerR ion source and an A.E.M.
1000ETPR electron multiplier. A Pyrex cold finger
at � 95 jC and a Zr–Al alloy getter operated at 400
jC purified the extracted gas. System blank runs were
carried out at the start of each laser experiment and
were repeated every third run. Background values
were typically 1�10� 11, 5� 10� 14, 2� 10� 13 and
1�10� 12 cm3 STP for the 40, 39, 37 and 36 argon
isotopes, respectively, and were subtracted from the
subsequent sample analysis results. Samples ALM
104 and JK 0 were irradiated in the Melusine reactor
(Grenoble, France) for 40.95 h together with flux
monitors biotite standard 4B (K–Ar age: 17.25 Ma,
Hall et al., 1984 and subsequent analyses in Nice and
Toronto) and MMHb (K–Ar age: 520.4 Ma, Alexan-
der et al., 1978), respectively, while being rotated
around a vertical axis. The irradiation parameter J was
obtained from the 40Ar*/39ArK ratios measured from
K. de Jong / Lithos 70 (2003) 91–110100
three standards in the tube at the same level as the
samples.
Rb–Sr dating was carried out at the Vrije Uni-
versiteit, Amsterdam, The Netherlands. Pressed pow-
der pellets prepared from splits of whole-rock
powder sample were analysed by X-ray fluorescence
spectrometry for Rb and Sr contents and Rb/Sr ratios
with a Philips PW 1404 automatic spectrometer.
Spiked and unspiked Sr analyses were made on an
automated Finnigan MAT-261 mass spectrometer
with three Faraday cup multicollector system for
Sr. Rb-spiked isotope dilution measurements were
performed using a computer-controlled Teledyne
mass spectrometer with a single Faraday cage col-
lector. For additional analytical details, see footnote
on Table 2.
Mineral ages are calculated using decay constants
given by Steiger and Jager (1977). Plateau, total
fusion and isochron ages include errors in J and the
age of the flux monitor and have errors quoted at the
2r level. Isochron calculations are according to Lud-
wig (2000). Plateau ages were calculated if 60% or
more of the 39Ar was released in three or more
contiguous steps with a probability-of-fit of the
weighted mean of more than 5% (Ludwig, 2000).
All argon isotopic measurements were corrected for
linear extrapolation to gas inlet time, mass discrimi-
nation, atmospheric argon contamination and irradia-
tion-induced contaminant Ar-isotopes derived from
Table 2
Rb–Sr analytical data of white mica; ALM 270, Mesozoic series, Nevad
Estimated errors are 0.5% for X-ray fluorescence spectrometric Rb/Sr an
isotope ratio measurements of whole-rocks and 0.02% for 87Sr/86Sr analy
above mentioned estimated analytical errors. Decay constant of 87Rb = 1.4(1) X-ray fluorescence spectrometric data (whole-rock) and mass-spec(2) Directly measured on unspiked sample (whole-rock) and calculate
Ca and K in the sample; correction factors applied:
(36Ar/37Ar)Ca: 2.79� 10 � 4 (F 3%), (39Ar/37Ar)Ca:
7.06� 10� 4 (F 4%), (40Ar/39Ar)K: 258� 10� 4
(F 3%).
5. Results
The 40Ar/39Ar analytical data of samples ALM 104
and JK 0 are listed in Table 1 and portrayed as age
spectra in Figs. 4 and 6, respectively. Rb–Sr isotopic
analyses of mica schist samples ALM 270, 272, 273
and 274 are given in Table 2.
5.1. 40Ar/39Ar step heating
5.1.1. Biotite separate ALM 104
Induction furnace step heating of biotite separate
ALM 104 yielded an age spectrum with progressively
increasing apparent ages from 147 to 185 Ma, subse-
quent to the first 1% of gas release with irregular
apparent ages (Table 1; Fig. 4, lower panel). The
weighted mean age of the main flat part of the spectrum
(steps 3–12) is 173.2F 6.3Ma. The 37ArCa/39ArK ratio
spectrum is flat, with more Ca-rich compositions
degassing during the first 6.5% and final 2% of gas
release (Fig. 4, upper panel), which probably corre-
spond to impurities. The total fusion age of 174.7F 1.6
Ma and 36Ar/40Ar vs. 39Ar/40Ar inverse isochron age of
o–Lubrın unit; ALM 272, 273, 274 Paleozoic rocks, Secano unit
d isotope dilution measurements of Rb and Sr, 0.01% for 87Sr/86Sr
sis of minerals. The uncertainty is at the 2r level and based on the
2� 10� 11year� 1.
trometric isotope dilution (minerals).
d from analysis of spiked sample (minerals).
Fig. 6. 40Ar/39 Ar laser step heating age spectrum (lower panel) and37ArCa/
39ArK ratio spectrum (upper panel) of single phengite grain
JK 0 from the Mesozoic series of the Nevado–Lubrın unit.
K. de Jong / Lithos 70 (2003) 91–110 101
173.2F 8.7 Ma (Table 1; Fig. 5) are concordant.
However, the large MSWD of 15 renders the meaning
of the isochron age and the 40Ar/36Ar intercept of
281F 82 uncertain.
5.1.2. Phengite single grain JK 0
Laser step heating of a single phengite grain JK 0
yielded a plateau age of 86.9F 0.8 Ma (Fig. 6. lower
panel). The plateau age is concordant to both the
87.9F 2.2 Ma total fusion age and the 86.2F 2.4 Ma36Ar/40Ar vs. 39Ar/40Ar inverse isochron age of the
plateau steps, with an 40Ar/36Ar intercept that is
within error of the atmospheric value (Table 1, Fig.
7). The 37ArCa/39ArK ratio spectrum is flat over the
main part (Fig. 6, upper panel); the high ratio during
the first 3% and the slightly elevated ratio for the final
25% of gas release probably correspond to more Ca-
rich inclusions in the grain.
5.2. Rb–Sr ages
Rb–Sr analyses of phengites frommica schists have
yielded a wide spread of ages (Table 2). Despite un-
favourable enrichment factors of radiogenic 87Sr, sam-
ples ALM 272 and 273 of the Secano unit preserve a
pre-Miocene isotope signal, yielding whole-rock–mi-
ca ages of 66.1F 3.2 and 40.6F 2.6 Ma. ALM 274
(Secano unit) yielded an age of 14.1F 2.2 Ma that is
concordant with the whole-rock–phengite–albite age
Fig. 7. 36Ar/40Ar vs. 39ArK/40Ar correlation plot for single grain JK
0. The open ellipses of steps 8–11 are excluded from the
calculation.
Fig. 5. 36Ar/40Ar vs. 39ArK/40Ar correlation plot for biotite separate
ALM 104. Points 1350 and fuse are excluded from the calculation.
Fig. 8. Rb–Sr albite phengite whole-rock isochron for ALM 270
(Mesozoic series, Nevado–Lubrın unit). The errors are at the 2rlevel.
K. de Jong / Lithos 70 (2003) 91–110102
of 17.2F 1.9 Ma of ALM 270 (Nevado–Lubrın unit,
Fig. 8).
6. Interpretation
The results obtained on samples with the same
tectonic foliation show a wide range of 40Ar/39Ar and
Rb–Sr ages, emphasising the fact that they cannot be
interpreted in terms of a simple cooling history during
exhumation.
6.1. Excess and inherited 40Ar
The 173F 6 Ma 40Ar/39Ar weighted mean age and
virtually all apparent ages of biotite ALM 104 are much
older than the 146F 3Ma Rb–Sr mineral isochron age
of the host gabbro (Fig. 4), which indicates that 40ArXShas been incorporated into the mineral.
The concordant 86.9F 0.8 Ma plateau age and the
86.2F 2.4 Ma isochron age of single phengite grain
JK 0 are much older than the 15.0F 0.6 Ma SHRIMP
U–Pb zircon age obtained by Lopez Sanchez-Viz-
caıno et al. (2001) in Cerro del Almirez (Fig. 1). The
discrepancy between these two estimates for the
timing of high-pressure metamorphism in the Mulha-
cen Complex cannot be accounted for by a polycyclic
Alpine orogeny (e.g. Puga et al., 2002), as the upper
and lower parts of the Nevado–Lubrın unit did not
experience a different tectono-metamorphic evolution,
as would be expected following a re-subduction of the
lower part, as proposed by the latter authors. Accord-
ingly, the best interpretation is that the ca. 87 Ma age
of the phengite is due to the incorporation of 40Ar into
its lattice, which may have been inherited from the
magmatic precursor of the amphibolite that hosted the
white mica and which contained 40ArXS.
The 37ArCa/39ArK ratio and atmospheric contami-
nation of phengite grain JK 0 are fairly constant and
not elevated during the main argon release (Fig. 6,
upper panel; Table 1). It is, therefore, unlikely that40ArXS incorporation was the result of late-stage
illitisation related to fluid ingress via late cracks,
described by de Jong et al. (2001) for phengites in
gneisses, which have an atmospheric contamination
that is well above 30% and 37ArCa/39ArK ratios that
tend to be much higher than those observed for JK 0.
The absence of a dense network of cracks in the
amphibolite emphasizes this.
The fact that the single mica grain yielded a plateau
age that is enhanced by inherited 40Ar implies that Ar
was not released by volume diffusion during in vacuo
step heating. It has been argued that chemical and
structural changes, such as dehydroxylisation of white
mica during step heating, permit the simultaneous
release of 39ArK,40Ar* and 40ArXS from the cores
and rims of crystals, leading to homogenisation of40Ar reservoirs and age gradients (Inger et al., 1996;
Sletten and Onstott, 1998; de Jong et al., 2001).
Trioctahedral micas behave in a similar way (Harrison
et al., 1985; Phillips and Onstott, 1988; Lo and
Onstott, 1989), however, probably due to sample
inhomogeneity, we did not obtain an age plateau for
biotite ALM 104.
In light of the above discussion, the meaning of the
plateau ages of 48.4F 2.2 and 24.6F 3.6 Ma of
barroisitic amphibole and magnesiohornblende, re-
spectively, obtained by Monie et al. (1991) in the
Sierra de Baza (Fig. 1), which both yielded irregular40Ar/39Ar age spectra, cannot be taken at face value.
The barroisitic amphibole grew in an undeformed
metadolerite that contains magmatic plagioclase and
clinopyroxene, making inherited 40Ar likely. The
well-expressed saddle-shaped age spectrum of the
magnesiohornblende clearly points to 40ArXS uptake,
and this sample only yielded a plateau age due to the
very large errors on the individual steps.
K. de Jong / Lithos 70 (2003) 91–110 103
6.2. Trapped argon component
Although 40ArXS often results in 40Ar/36Ar inter-
cepts in isotope correlation diagrams greater than
295.5 (Heizler and Harrison, 1988), examples of
phengite (Inger et al., 1996; Sherlock and Arnaud,
1999; de Jong et al., 2001) and biotite (Foland, 1983;
Ruffet et al., 1995) show that samples with 40ArXSplateau ages can give 40Ar/36Ar intercepts close to the
atmospheric value. The initial 40Ar/36Ar ratio not
necessarily reflects the argon composition immediate-
ly prior to crystallisation, but might equally well
indicate the argon composition added to minerals
during later processes (Roddick, 1978; de Jong et
al., 2001). This may also be the case for ALM 104, as
this sample has an elevated 36ArAIR contamination
corresponding to high 37ArCa/39ArK ratios during the
first 6.5% of 39Ar release. This is most likely related
to impurities of a Ca-rich phase that degasses at low
temperature, like carbonates (500–700 jC: Spray and
Roddick, 1981) and/or chlorite (first degassing peak
< 600 jC: Lo and Onstott, 1989; Ruffet et al., 1991),
which both may have been formed during light
alteration. The K contrast between biotite and submi-
croscopically intergrown chlorite may lead to 39ArKrecoil from the former into the latter, which results in
hump-shaped age spectra with old apparent ages in
the intermediate temperature region (Lo and Onstott,
1989; Ruffet et al., 1991). As we did not observe such
spectra, 39ArK recoil was probably not important and
does not lie behind the scatter of data point in the
isotope correlation diagram and the high MSWD
values for the regression. The isotope correlation
diagram of biotite ALM 104 thus seems to essentially
reflect the mixing of at least three argon reservoirs,
viz: a radiogenic component with two trapped com-
ponents. The first trapped component probably had a
non-atmospheric composition and was incorporated
during crystallisation, whereas the second and domi-
nant component was atmospheric and was added late
in the evolution of the system.
Phengite JK 0 (Table 1, Fig. 6) yielded a statistically
significant inverse isochron age with an 40Ar/36Ar
intercept within error of the atmospheric value. In this
case too, the trapped component may be due to later
processes, rather than have bearing on the trapped
component during recrystallisation of the grain. This
is clearly illustrated by the relatively high 37ArCa/39ArK
ratios and the corresponding elevated atmospheric
contamination.
6.3. Excess 40Ar and restricted fluid mobility
Widely scattered and elevated K–Ar mineral ages
from the gabbro from which biotite ALM 104 was
separated were interpreted by 40ArXS incorporation
(Hebeda et al., 1980). These authors accounted for the
presence of much higher amounts of 40ArXS in the
whole-rock relative to the constituent minerals by its
incorporation in the grain boundary network, fluid
inclusions and lattice defects, acquired during Alpine
metamorphism due to degassing of the surrounding
sediments. Such incipient low-grade metamorphism
during the early stages of subduction affected the
sedimentary rocks, in which argon had accumulated
in minerals since their deposition and diagenesis, and
was present as an inherited argon in detrital grains, but
not the coarse-grained high temperature minerals of
the gabbro. However, the occurrence of 40ArXS in all
the degassing steps of biotite ALM 104 implies
incorporation in the mineral lattice and not in low
retentive sites like cracks, cleavages and defects. The40ArXS uptake may thus have occurred during recrys-
tallisation of the biotite under a high argon activity
during this low-grade event. 40ArXS was probably
incorporated by a carrier fluid without important
recrystallisation of the other magmatic minerals of
the gabbro. This mechanism is in agreement with the
Sr isotopic data. The initial 87Sr/86Sr ratio of 0.7028
(Hebeda et al., 1980) that is close to the primitive
mantle value implies that Alpine recrystallisation did
not affect the Rb–Sr system of the rock. Morten et al.
(1987) noticed a statistically significant increase of the87Sr/86Sr ratio with metamorphic grade during pro-
gressive eclogitisation, which range from 0.703
(gabbros), via 0.705 (garnet-bearing metagabbro), to
about 0.706 (eclogites), in the rock body that yielded
the 146 Ma Rb–Sr age. The data presented by
Gomez-Pugnaire et al. (2000) similarly show higher87Sr/86Sr ratios for dolerites affected by metamorphic
recrystallisation. Morten et al. (1987) explained the
enrichment in radiogenic 87Sr by a limited ingression
of metamorphic fluids derived from the recrystallising
metasedimentary country rocks. Although the very
formation of eclogites is enhanced by fluid infiltration
(Morten et al., 1987; Gomez-Pugnaire et al., 1989), in
Fig. 9. 40Ar/39Ar induction furnace step heating age spectra (lower
panel) and 37ArCa/39ArK ratio spectra (upper panel) of phengite
separates from the eastern Sierra de los Filabres. Data from de Jong
et al. (1992). ALM 270 (Mesozoic series, Nevado–Lubrın unit)
shows a well-developed age plateau, whereas ALM 272 and 273
(Paleozoic series, Secano unit) have disturbed spectra.
K. de Jong / Lithos 70 (2003) 91–110104
agreement with the evolution of the 87Sr/86Sr ratio, the
observed zonation of the metamorphic minerals
implies a state of disequilibrium and a deficit of
cations. Such features suggest that fluid mobility
was limited during eclogitisation, which consequently
conserved the 40ArXS levels in rocks.
The ca. 87 Ma 40Ar/39Ar age of phengite JK 0 is
most likely the consequence of the incorporation of40Ar into the mineral and restricted fluid mobility may
have been instrumental in this process. The amphib-
olite from which single phengite grain JK 0 was
extracted occurs in the same tectono-stratigraphic
level as the 146-Ma-old gabbro ALM 104, which
was plagued by 40ArXS incorporation. Most eclogites
and gabbros in this level are pervasively amphiboli-
tised, pointing to the infiltration of water. Thorough
amphibolitisation of eclogites resulted in changes in
main and trace element chemistry (Morten et al.,
1987). The preferred orientation of mica and blue-
green hornblende in amphibolite JK 0 formed during
thorough recrystallisation that accompanied exhuma-
tion of high-pressure metamorphic rocks during D2.
Yet, the presence of glaucophane relics in the cores of
some hornblendes in this sample implies that disequi-
librium conditions existed during the breakdown of
the blue amphibole during this event. Although the
hydration of eclogites, leading to their amphibolitisa-
tion, resulted in a significant reduction of 40ArXS in
the whole-rock, it was not completely removed, as
shown by the data of Hebeda et al. (1980). This
observation implies that during D2 recrystallisation,
a semi-closed system persisted, in which the argon
activity remained elevated, at least locally. Amphib-
olitisation of gabbros and eclogites under such con-
ditions has led to the local redistribution and
incorporation of 40Ar in newly formed metamorphic
minerals, such as phengite.
6.4. Inherited isotopic components
White micas from the basal series of the Secano
unit yielded Rb–Sr ages that range from 66.1F 3.2 to
14.1F 2.2 Ma (Table 2) and 40Ar/39Ar total gas ages
of 25.9F 0.1 and 19.1F 0.1 Ma (see Section 3),
which imply the progressive resetting of an older
isotopic system. White mica from graphite-rich sam-
ples ALM 272 and 273 has disturbed 40Ar/39Ar age
spectra with apparent ages that are virtually all older
than the 17.3F 0.2 Ma plateau age of ALM 270 of the
Nevado–Lubrın unit (Fig. 9). Disturbed age spectra,
whether dome-shaped or composed of progressively
rising apparent ages, have been interpreted by degass-
ing of mixed micas, one containing an inherited Ar
component due to partial resetting during superim-
posed tectono-metamorphic recrystallisation and a
second that was newly formed during this event, both
of which do not release Ar over the same temperature
interval (Wijbrans and McDougall, 1986; Hammer-
schidt and Frank, 1991; de Jong et al., 1992; West and
Lux, 1993). Consequently, the age spectra of ALM
272 and 273 imply that a relict inherited Ar component
exists in both samples. Their microstructure reveals
incomplete recrystallisation of white mica and the
pinning of its grain boundaries on graphite particles.
K. de Jong / Lithos 70 (2003) 91–110 105
This inclusion-inhibited growth mechanism may sim-
ilarly explain why phengites ALM 272 and 273 have
partially retained an older Rb–Sr isotope signal, as
indicated by their relatively old Rb–Sr ages of 66.1
and 40.6 Ma, respectively. In contrast, the 14.1F 2.2
Ma Rb–Sr age of the most quartz-rich and least
graphite-rich sample ALM 274, which is not affected
by inclusion-inhibited growth of white mica, implies a
complete resetting of its Rb–Sr system. The Rb–Sr
age of this youngest sample of the Secano unit over-
laps with the 17.2F 1.9 Ma Rb–Sr age of ALM 270 of
the Nevado–Lubrın unit. Widespread retrograde
growth of albite and chlorite at the cost of phengite
in ALM 270 implies complete tectono-metamorphic
recrystallisation following D2.
The progressively reset isotopic system in the
Secano unit may be derived from a pre-Miocene
early Alpine signal, or alternatively, its occurrence in
probably Paleozoic rocks implies that it may partially
retain a pre-Alpine history. The ca. 15 Ma U–Pb
SHRIMP zircon age for the high-pressure metamor-
phism (Lopez Sanchez-Vizcaıno et al., 2001) renders
the first option unlikely. In contrast, during the pre-
Alpine evolution of the Mulhacen Complex, the
basal series were metamorphosed up to about 500
jC (Section 2; Fig. 10). Their crystalline nature and
the inhibited recrystallisation of white mica in graph-
ite-rich samples during the Alpine orogeny may lie
behind the inherited pre-Alpine Rb–Sr and K–Ar
systems in these rocks. Their partial survival in white
mica during the Alpine orogeny, when temperatures
of about 500 jC were reached, once again under-
scores that temperature alone is ineffective for iso-
tope resetting, but that fast recrystallisation processes
that affect the ionic bonds in minerals, like tectono-
metamorphic recrystallisation and fluid ingress, are
(Chopin and Maluski, 1980; Verschure et al., 1980;
Wijbrans and McDougall, 1986; Hames and Cheney,
1997; Villa, 1998; Itaya and Fujino, 1999; Kuhn et
al., 2000; de Jong et al., 2001; Dunlap and Kronen-
berg, 2001; Reddy et al., 2001). In contrast, the
occurrence of ALM 270 in the Mesozoic series of
the Nevado–Lubrın unit and its ca. 17.2 Ma40Ar/39Ar plateau and Rb–Sr ages precludes the
presence of any inherited pre-Alpine isotopic com-
ponent. Yet, a small 40ArXS component seems likely,
taking the ca. 15 Ma U–Pb SHRIMP zircon age at
face value.
6.5. Age and rates of exhumation and cooling
Despite the occurrence of inherited isotope systems
and 40ArXS incorporation in white mica and biotite,
our dating sheds light on the timing of exhumation of
the Mulhacen Complex and its rates. Albite in ALM
270 was probably formed from the paragonite com-
ponent in white mica during its recrystallisation at low
pressure during D3. The87Sr/86Sr ratio of this sample
shows that the age information obtained essentially
pertains to albite, as the 87Sr/86Sr ratios of phengite
and the whole-rock are virtually identical (Table 2).
The 17.2F 1.9 Ma whole-rock–mica–albite age con-
sequently has bearing on the decompression to about
0.4–0.5 GPa for D3 (see Section 2.2, Fig. 10).
However, due to the large uncertainty, the age is
within error of the 15.0F 0.6 Ma age estimate of
the high-pressure metamorphism based on the zircon
SHRIMP data of Lopez Sanchez-Vizcaıno et al.
(2001). Subsequent to the D3 cooling phase temper-
atures increased to about 500 jC, whereas the pres-
sure probably did not significantly decrease (Fig. 10).
de Jong et al. (2001) argued that, in conjunction with
this D4 reheating, white mica in the gneisses of the
Macael–Chive unit acquired 40ArXS during submicro-
scopic illitisation, a fluid-assisted recrystallisation
process that probably also affected the Rb–Sr system.
Rb–Sr white mica ages reported by Andriessen et al.
(1991) from the gneisses of the Macael–Chive unit in
the eastern Sierra de los Filabres span the 12.5–15.6
Ma range, with errors of about 2–2.5%. It might be
argued that the youngest Rb–Sr white mica age of
12.5F 0.2 Ma is the result of a thorough recrystalli-
sation during D4, which might imply a decompression
of about 55 km in roughly 2.5 Ma (Fig. 10). The
exhumation rate may consequently be as high as about
22.5 mm/year, about twice the estimate of Lopez
Sanchez-Vizcaıno et al. (2001), who based their value
on an assumed geothermal gradient and not on avail-
able P–T estimates for the late stage evolution.
Fission-track data of Johnson et al. (1997) point to
an accelerated cooling following the first phase of fast
exhumation and cooling. These authors inferred from
an 11 Ma apatite fission-track model age that the
cooling of the uppermost Mulhacen Complex in the
eastern Sierra de los Filabres was essentially complet-
ed by that time. This is consistent with the first
appearance of detritus derived from this part of the
Fig. 10. Pressure–Temperature– time–deformation path and exhumation history of the Mulhacen Complex. P–T determinations by Bakker et
al. (1989), de Jong (1991, 1993a) and Puga et al. (2002). (1) Lower P stability limit of glaucophane after Maruyama et al. (1986); (2)
FeChl +Ms =FeCld +Ann; (3) Cld +AS= St +Chl; (4) FeCld +Ann =Alm+Ms; (5) Cld =Grt + Chl + St; according to Spear and Cheney
(1989); Stability Al-silicate fields after Holdaway and Mukhopadhyay (1993). Mineral abbreviations according to Kretz (1983). Age
constraints: (A) SHRIMP U–Pb mean age of nine zircon grains (Lopez Sanchez-Vizcaıno et al., 2001); (B) youngest Rb–Sr white mica age of
Andriessen et al. (1991); (C) apatite fission-track model age (Johnson et al., 1997).
K. de Jong / Lithos 70 (2003) 91–110106
complex (in part as boulders of the marbles and
gneisses of the Macael–Chive unit) in latest Serraval-
lian to Early Tortonian deposits around the eastern
Sierra de los Filabres (de Jong et al., 2001, and
references in therein). Under the assumption of a
12.5 Ma age for D4 during which temperatures were
in the order of about 500 jC, the final cooling has
taken about 1.5 Ma with a rate of about 330 jC/Ma
and much less fast exhumation rate of 9–12 mm/year
compared to the early exhumation phase.
The Late Miocene cooling has been accounted for
by extension (Johnson et al., 1997). Since the work
of Platt and Vissers (1989), the contact between the
Mulhacen and Alpujarride complexes has been inter-
preted as a major low-angle extensional fault. D5
mylonites and D6 brittle–ductile structures are most
penetratively developed in the uppermost Mulhacen
Complex along the contact with the overlying Alpu-
jarride Complex and show the decreasing tempera-
ture (de Jong, 1991, 1993a) during exhumation. But
also important low-angle brittle–ductile detachments
were formed within the Mulhacen Complex during
this event, like e.g. at the base of the Secano unit
and at the base of the greenstones that contain the
eclogites.
7. Conclusions
Radiometric dating of phengite from rocks with a
tectonic fabric related to the exhumation of high-
pressure metamorphic rocks implies that 40ArXS in-
corporation and isotopic inheritance have occurred
under conditions of restricted fluid mobility and
tectono-metamorphic recrystallisation.
A well-crystallised single phengite grain from an
amphibolite (Nevado–Lubrın unit) has yielded a40Ar/39Ar laser step heating plateau age of 86.9F0.8 (2r; 70% 39Ar released), which is concordant to
its inverse isochron age of 86.2F 2.4 Ma (40Ar/36Ar:
299.0F 4.8). A biotite separate from a gabbro relic in
an eclogite yielded an induction furnace step heating
age spectrum with progressively increasing apparent
ages and a weighted mean age of 173.2F 6.3 Ma (2r;95% 39Ar released). These ages are older than the
eclogite-facies metamorphism (15 Ma) and intrusion
of the gabbros (146 Ma) and, hence, are the result of40ArXS incorporation. 40ArXS uptake by the gabbro
was probably caused by infiltration of fluids derived
from the country rocks during their incipient meta-
morphism at the onset of subduction. 40ArXS incor-
poration in the phengite in the amphibolite was related
K. de Jong / Lithos 70 (2003) 91–110 107
to metamorphic recrystallisation of the magmatic
rocks in an environment with a restricted fluid mo-
bility inherited from the magmatic stage.
Rb–Sr whole-rock–phengite ages of graphite-
bearing mica schists from Paleozoic rocks (Secano
unit) show a dramatic age variation (66.1F 3.2,
40.6F 2.6 and 14.1F 2.2 Ma) that has arisen from
the progressive resetting of an older isotopic system.
This system was probably a remnant of the Variscan
low-grade metamorphism of the basal series of the
Mulhacen Complex. The microstructure of the sam-
ples with pre-Miocene Rb–Sr ages implies that phen-
gite has only partially recrystallised as grain growth
was inhibited by the presence of graphite particles.
This interpretation corroborates previously obtained
disturbed and slightly dome-shaped 40Ar/39Ar age
spectra that reveal the presence of an older isotopic
component. In contrast, the most quartz-rich and least
graphite-rich sample is not affected by inclusion-
inhibited growth of white mica, and has a completely
reset Rb–Sr system, as implied by its 14.1F 2.2 Ma
Rb–Sr age. The latter date overlaps with the
17.2F 1.9 Ma Rb–Sr whole-rock–phengite–albite
age obtained from a schist from the Mesozoic series
of the Nevado–Lubrın unit.
Comparison of our data and literature data reveals
that exhumation of the eclogite-facies Mulhacen Com-
plex occurred at rates in the order of 22.5 mm/year
during the early phase and of 9–12 mm/year during the
late phase. During the latter event, the cooling rate was
of about 330 jC/Ma.
Acknowledgements
I would like to dedicate this article to Prof. W.P. de
Roever, who passed away on 24 September 2000, and
was one of the pioneers in high-pressure petrology just
after World War II. He worked as an undergraduate
student in the area around Lubrın and interpreted the
occurrence of zoned metamorphic minerals by dis-
equilibrium during a succession of different metamor-
phic facies in time (plurifacial metamorphism). Only
much later would such a notion become general with
the reconstruction of P–T– t paths.
I would like to thank Drs. Gilbert Feraud (Geo-
science Azur, Universite de Nice-Sophia Antipolis,
France) and Jan Wijbrans (Department of Isotope
Geochemistry, Faculty of Earth and Life Sciences,
Vrije Universiteit, Amsterdam, The Netherlands) for
the use of analytical facilities and the use of sample
ALM 104 from the mineral separate collection of the
department. Part of the work was carried out while
holding a NATO post-doctoral research fellowship
and The Netherlands Organisation for Scientific
Research (NWO) and the ‘‘Vakgroepfonds Strukturele
Geologie’’ of the University of Amsterdam met travel
costs incurred during the project. Some of the points
addressed in this study came up during a discussion
with Igor Villa. Constructive reviews by Sarah
Sherlock and Richard Spikings contributed to the
clarity of the presentation and the styling of the text.
Daniella Rubatto and Encarnacion Puga are thanked
for providing pre-prints.
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