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Tectonophysics, 184 (1990) 219-296
Elsevier Science Publishers B.V., Amsterdam
279
Alpine tectonics and rotation pole evolution of Iberia
Koen de Jong
Instrtute for Earth Sciences, Free Unruersity, P.O. Box 7161, 1007 MC Amsterdam (The Netherlands)
(Received April 20,1989; revised version accepted January 26. 1990)
ABSTRACT
De Jong, K., 1990. Alpine tectonics and rotation pole evolution of Iberia. In: G. Boillot and J.M. Fontbote (Editors), Alpine
Evolution of Iberia and its Continental Margins. Tectonophysics, 184: 279-296.
The geological evolution of the Betic Cordilleras and Pyrenees reflects the Cretaceous and Tertiary rotation pole and
kinematic evolution of the Iberian and African plates. New constraints on the Alpine tectonic evolution of the Iberian plate
are provided by P-T-t data and regionally consistent stretching lineations from the metamorphic parts of the Betic
Cordilleras.
High-pressure low-temperature metamorphism in the Betic Cordilleras resulted from continent-continent collision which
caused subduction to a maximum depth of 37 km. A preliminary 116 + 10 Ma radiometric age for this event corresponds to
the initiation of seafloor spreading to the west of Iberia which lasted until about 80 Ma. Intracontinental thrusting in the
Betics between 99 Ma and 83 Ma took place after subduction ended. E-W to ESE-WNW trending stretching lineations
indicate the direction of thrusting, which resulted in extensional strains of 200-600%. The timing of thrusting in the Betics
coincides with a 95-80 Ma tectonic phase in northern Africa, during which E-W stretching lineations were formed. The
stretching Iineations are coincident with the 110-80 Ma motion vector of Africa-Iberia with respect to Eurasia. Thrusting in
the Betics and deformation in northern Africa was driven by convergence of Africa-Iberia and Eurasia. Cretaceous
deformation is further recorded by terrigeneous sedimentation in the Mauritanian Flysch and by the tectosedimentary
evolution of the Malaguide Complex. Crustal thinning, magmatism and metamorphism in the Pyrenees during the 110-85 Ma
period is governed by a left-lateral strike-slip of Africa-Iberia with respect to Eurasia around the same rotation pole as
thrusting in the Betics.
During the 80-54 Ma period the rotation pole was situated west of Gibraltar, near the previous active collision zone. This
inhibited large-scale overthrusting and related penetrative deformation in northern Africa and the Betic Cordilleras.
Deformation was instead transferred to the northern boundary of Iberia, now acting as an African promontory. From the
Campanian on wards, oblique convergence took place around the combined Gibraltar rotation pole. Deformation culminated
in the late Eocene, corresponding to spreading in the Norwegian-Greenland Sea at 55 Ma which induced an additional
compression in western Eurasia. During the Pyrenean collision, high-pressure metamorphic rocks in the Betic Cordilleras were
exhumed and they cooled substantially. The cooling trend was disturbed by Oligocene extensional deformation and
introduction of a transient heat source, which correlates with the mantle being uplifted during extension. Heating culminated
at the Oligocene-Miocene boundary in the Betic Cordilleras and in northern Africa. This evolution agrees with the
development of a plate boundary between Iberia and Africa at 30 Ma, after completion of the Pyrenean collision. The new
plate boundary was connected to the western European rift system.
Renewal of compression and overthrusting in the Betic Zone took place after 20 Ma. Overthrusting is succeeded by two
phases of wrenching, juxtaposing crustal segments with different Moho depths inherited from the late Oligocene to Early
Miocene extension.
Introduction
The Iberian peninsula (Fig. 1) is bordered by
two Alpine foldbelts, the Pyrenees to the north
and the Betic Cordilleras to the south. These belts
separate the Iberian plate from, respectively, the
Eurasian plate and the African plate. The Creta-
ceous to Tertiary tectonic evolution of the Pyrenees
has been well documented (Mattauer and Henry,
1974; Puigdefabregas and Souquet, 1986; Soula et
al., 1986). Until now the Betic Cordilleras has
most often been regarded as a Tertiary orogen,
mainly on the basis of important Tertiary defor-
mation in the non-metamorphic parts (Rondeel
and Simon, 1974; De Smet, 1984). A Mesozoic age
for the early deformation has, however, been sug-
0040-1951/90/$03.50 0 1990 - Elsevier Science Publishers B.V.
280
gested by Kampschuur and Rondeel(l975) owing to the Mesozoic age of the flysch deposits in the western Betics. New data discussed in this paper also suggest important Cretaceous tectonics in the metamorphic Internal Zone of the Betic Cordilleras. Ceochronological studies in the Al- pine collision belt of northern Africa (Monie et al., 1984a; 1988) show a tectonic evolution which is comparable to that of the Betics-Cretaceous metamo~~c ages and an important Tertiary re- setting. This paper aims at tying the new tectonic model for the Betic Zone and the thermotectonic evolution of the northern African belt to the well- constrained tectonic evolution of the Pyrenees. The tectonic evolution of the erogenic belts bordering the Iberian plate will be shown to be consistent with the Cretaceous and Tertiary rota- tion pole and kinematic evolution of the Iberian and African plates discussed by Savostin et al.
K. DE JONG
(1986) Srivastava and Tapscott (1986) and Klit- gord and Schouten (1986).
Regionally consistent stretching lineations which were formed during early Alpine thrusting at lower crustal levels are a salient feature of the tectonic evolution of the Internal Zone. They coincide with the mid-Cretaceous motion vector of
Savostin et al. (1986) of the African plate (includ- ing Iberia at that time) with respect to Eurasia. Because stretching lineations appro~mate the movement direction in shear zones (Esscher and Watterson, 1974) they probably also trace plate motion directions. A relationship between the di- rection of thrusting and plate motion has been suggested for an number of orogens (Shackleton and Ries, 1984), including the Alps (Baird and Dewey, 1986; Choukroune et al., 1986). During the later stages of the tectonic evolution of the arcuate western Alps, radial thrusting occurred
IBERIAN MESETA
GULF DE LION
Infernal Zones of the Betlc Cordilleras and Rlf
;:
D IAbne metamorphic rocks)
a
Fig. 1. Sketch map of the westernmost Mediterranean area (modified after Ricou et al., 1986) showing the major Alpine structural
provinces. The eastern Betic Cordilleras of southern Spain are delineated.
ALPINE TECTONICS AND ROTATION POLE EVOLUTION OF IBERIA 281
(Choukroune et al., 1986) at higher crustal levels,
this thrusting clearly bearing no relationship to
plate motion vectors. Relatively large finite dis-
placements and rotations during such a stage will
disturb the original pattern of older stretching
lineations formed at deeper levels. The eastern
part of the Betic Cordilleras does not demonstrate
an arcuate form, and therefore no pervasive re-
orientation of older structures is to be expected.
Palaeostress analyses in stable forelands do not
usually suffer the disadvantage of reorientation, as
finite strain is in general small. A clear relation-
ship between (successive) palaeostress directions
and plate motion vectors is therefore recorded in
the Alpine foreland (Letouzey, 1986; Bergerat,
1987). However, in Iberia the Mesozoic palaeos-
tress directions do not mimic the plate vector very
accurately (Malod, 1989). This is partly the result
of reorientation and heterogeneities induced by
pre-existing faults. Therefore, the regionally con-
sistent stretching lineations in the Internal Zone
are considered as an important constraint in the
early kinematic evolution of the Iberian plate.
Motions around different rotation pole positions
during orogeny will, due to overprinting and re-
orientation, not be recorded by successive genera-
tions of stretching lineations. Shifting of rotation
poles has, however, a marked effect on tectonics in
metamorphic belts, as will be discussed later.
Evolution of the tectonic zones bordering Iberia
The Alpine collision belts bordering Iberia are
characterized by Jurassic to Early Cretaceous ex-
tensional deformation and related strike-slip de-
formation. A Middle to Late Jurassic strike-slip
fault between Iberia-Africa is indicated by plate
reconstructions (Savostin et al., 1986; Klitgord
and Schouten, 1986). The occurrence of a frag-
ment of an ophiolite sequence of Late Jurassic age
in northern Africa (Bouillin et al., 1977) accords
with these reconstructions. Continuing motion into
the Cretaceous is indicated by flysch deposits
culminating in Aptian-Albian times in the Flysch
Domain (Bouillin et al., 1986). The non-metamor-
phic External Zones of Iberia and northern Africa
are palaeogeographically unrelated (Bouillin et al.,
1986) this also indicating their initial separation.
In the External Zone of the Betic Cordilleras an
algal platform broke up at the Middle to Late
Jurassic boundary (Geel, 1979) resulting in strong
palaeogeographical differentiation (Hermes, 1978).
An extensional tectonic regime is indicated by
pillow basalt intrusions in the Sub-Betic (Hermes,
1978; De Smet, 1984). Important hiatuses, turbi-
dite deposits and the occurrence of Middle Jurassic
lithoclasts in Albian-Aptian marls (Hermes, 1978)
indicate important vertical motions continuing into
the Cretaceous. Basaltic intrusion in the Internal
Zone of the Betics is of Jurassic age (146 + 3 Ma,
Rb/Sr age, Hebeda et al., 1980; 200 f 5 Ma,
K/Ar biotite age, Besems and Simon, 1982).
At the northern boundary of Iberia, in the
future Pyrenees, carbonate platform breakup oc-
curred in the Early to Middle Jurassic
(Puigdefabregas and Souquet, 1986). At the north-
western margin of Iberia, Late Jurassic rifting
possibly occurred; important rifting started in the
Berriasian to earliest Valanginian (144-140 Ma,
Boillot et al., 1989). The end of emplacement of
ultramafic rocks by ductile normal faulting has
been dated at 122 f 0.6 Ma (Feraud et al., 1988).
Final emplacement by brittle deformation oc-
curred before the late Aptian breakup unconfor-
mity (around 115 Ma), which marks the onset of
seafloor spreading (Boillot and Malod, 1988; Boil-
lot et al., 1989; Malod, 1989). Opening of the Bay
of Biscay occurred between the Aptian and
Campanian and induced several hundred kilo-
metres of strike-slip on the North Pyrenean Fault
(Le Pichon et al., 1971; Choukroune and Mat-
tauer, 1978; Savostin et al., 1986; Srivastava and
Tapscott, 1986; Klitgord and Schouten, 1986;
Boillot and Malod, 1988; Malod, 1989). Deforma-
tion coincided with a general change in the sedi-
mentation pattern in Aptian times (Souquet et al.,
1985) and Pyrenean magmatism and metamor-
phism between 110 and 85 Ma (Albarede and
Michard-Vitrac, 1978; Montigny et al., 1986).
During this period the North Pyrenean Fault zone
was characterized by high heat flow in response to
crustal thinning related to strike-slip tectonics
(Choukroune and Mattauer, 1978; Vielzeuf and
Kornprobst, 1984; Golberg et al., 1986). Early
Cretaceous metamorphic ages are also well re-
corded by the 4oAr-39Ar stepwise heating method
2x2 K. DE JDNG
of samples from mylonite zones in the eastern
Pyrenees (110-100 Ma and 90 Ma, Costa and
Maluski 1988) and in strike-slip basins at the
northwestern termination of the Iberic Cordillera
(100 Ma, Golberg et al., 1988).
The extensional regime in the Pyrenees changed
to compression in the latest Cretaceous (Vielzeuf
and Kornprobst, 1984); oblique convergence
started in the Campanian (PuigdefBbregas and
Souquet, 1986). Strike-slip ceased dr~atically
during the middle Eocene, when major thrusts
were developed parallel to the mylonite zones
(Soula et al., 1986). The northern Spanish passive
margin was converted into an active margin in the
Paleocene-Eocene interval as a result of plate
convergence (Boillot and Malod, 1988). During
convergence, Variscan and Early Cretaceous faults
were reactivated (Soula et al., 1986; McCaig and
Miller, 1986; Majoor, 1988). Radiometric ages in
mylonite zones indicate a latest Cretaceous to
middle Eocene age for reactivation (McCaig and
Miller, 1986; Costa and Maluski, 1988;Majoor,
1988). Compressional deformation in the non-
metamo~hi~ zones cul~nated in the Eocene
(Mattauer and Henry, 1974; Puigdefabregas and
Souquet, 1986). Piggy-back thrusting in the central
southern Pyrenees migrated southward with time
(Williams, 1985), concomitant with the progressive
southward development of molasse basins (Mat-
tauer and Henry, 1974) and their incorporation in
subsequently formed thrust units (Puigdef~bregas
and Souquet, 1986). Flexure modelling ildb shown
that the Ebro foreland basin formed as a result of
the Pyrenees, Catalan Coastal Range and Iberic
Cordillera loads (Zoetemeijer et al., 1990). It con-
tains Paleocene and thick Eocene-Oligocene de-
posits, recording erosion of rising mountain chains
(Mattauer and Henry, 1974; Nagtegaal and De
Weerd, 1985). The southward propagating defor-
mation front reached the Ebro Basin after deposi-
tion of the Oligocene molasse (Williams, 1985).
The interiors of the Iberian plate also experi-
enced extensional phases during the Late Jurassic
to Early Cretaceous period, which accord well
with phases of spreading in the North Atlantic
(Malod, 1989). Late Eocene to late Oligocene
northward compression reactivated Variscan and
Mesozoic faults (GuimerB, 1984; Viallard, 1985).
Raising of geotherms during extension caused ef-
fective weakening of the lithosphere, which is also
a si~ificant factor in the localization of in-
tracontinental Tertiary compression (Zoetemeijer
et al., 1990).
The External Zone of the Betic Cordilleras
records only relatively small increments of the
Pyrenean collision (De Ruig, this issue). This colli-
sion resulted in differential block movements dur-
ing the Paleocene and Eocene (Kenter et al., 1990).
The main compression occurred at the Middle to
Late Miocene boundary (Simon, 1987) during
northward thin-skinned tectonics with intermit-
tant strike-slip deformation (De Ruig et al., 1987).
Compression also began in the Middle Miocene in
the Tell and External Rif of northern Africa.
In the following I present indications of an
important phase of tectonism in the Internal Zone
of the Betic Cordilleras between the Barremian
and Campanian.
Tectonic evolution of the Internal Zone of the
Betic Cordilleras
Regionaf scale structure
The Internal Zone occurs to the south of the
External Zone, which constitutes the margin of
Iberia characterized by Mesozoic rifting (Hermes,
1978). These two zones are presently separated by
a strike-slip fault of Miocene age (Hermes, 1978;
Le Blanc and Olivier, 1984; De Smet. 1984). The
Triassic stratigraphy of the overthrust units in the
Internal Zone bears no resemblance to the Triassic
stratigraphy of the External Zone (Simon, 1987).
The Internal Zone can thus be considered as alloc-
hthonous to Iberia. (Very) low grade Triassic
metarno~~c rocks of the Almagride Complex
occur in windows below the Alpujarride Complex
of the Internal Zone (Fig. 2); they show striking
similarities with Triassic rocks of the eastern Sub-
Betic (Besems and Simon, 1982; Simon, 1987).
This indicates an original overthrust contact be-
tween the Internal Zone and rocks that were prob-
ably separated from the External Zone during
Mesozoic rifting. The Miocene strike-slip fault
between the Betic Zone and the External Zone can
not therefore be interpreted as a plate boundary,
EXTE
RML
ZONE
SdA
=
Ster
ra
ck
Alm
ogro
S
.&i
E
z S
ierr
a cf
e ‘O
S
Esr
onci
as
Sdi
.F=
Sie
rrc
de
lo5
F”i/s
bres
S
.N
= S
,err
a N
l??V
CJC
iCl
d 0
10
50
1OO
km
I-
t _l
__l._
_-
-_
.._._
- 1”
P
Y
0’
Fig
. 2.
Tec
toni
c sk
etch
m
ap
of t
he
east
ern
Bet
ic
C’o
rdill
eras
sh
owin
g th
e di
stri
butio
n of
m
ajor
te
cton
ic
com
plex
es
(aft
er
Bak
ker
et a
l.,
1989
).
I.ow
er
hem
isph
ere
proj
ectlo
ns
indi
cate
D
,
stre
tchn
g Im
eati
ons
on
Hal
-lyi
ng
mai
n fo
liati
on,
exce
pt
(e)
whi
ch
indi
cate
s D
, ,
stre
tchi
ng
linea
tiuns
. m
ainl
y fr
om
a 5.
5 km
’ gn
eiss
bo
dy.
Loc
atio
n (f
) In
dica
tes
L,
from
th
e
Alm
anzo
ra
Uni
t; sp
read
ing
resu
lts in
th
e Si
erra
de
ias
Fa
tanc
ias
(h
and
i) b
y su
bseq
uent
m
odcr
ate
defo
rmat
ion.
284 K. DE JONG
but as a later structure of relatively minor impor.
tance. The Internal Zone consists of four stacked
crustal segments. The lowest segment, the Veleta Complex, is characterized by low-pressure, low- temperature (LP/LT) metamorphism (Puga and Diaz de Federico; 1978), for which recently a pre-Alpine age has been suggested (Gomez- Pugnaire and Franz, 1989). This complex has been overthrust by the Mulhacen Complex, which bears evidence of early Alpine high-pressure, low-tem- perature (HP/LT) metamorphism partially over- printed by medium-grade metamorphism (Gomez -Pugnaire and Femandez-Soler, 1987; Bakker et al., 1989). The Alpujarride Complex occurs on top of the Mulhacen Complex and is also char- acterized by early H P/LT met~o~~srn (Bakker et al., 1989; GoffC et al., 1989). In the western Betics the Alpujarride Complex experienced high- temperature metamo~~sm at high to low pres- sure related to emplacement of ultramafic rocks (Westerhof, 1977) of Early Miocene age (Priem et al.. 1979; Zindler et al., 1983). The uppermost tectonic unit, the Malaguide (Ghoma~de in north- ern Africa) Complex, is almost entirely non-meta- morphic (Egeler and Simon, 1969). Condensed, but continuous, Mesozoic and Paleogene stratigra- phy (Roep, 1980) indicates that this crustal do- main has always retained near the crustal surface. The Dot-sale calcaire and Pre-dorsalian Zone rep- resent the margin of this Malaguide/Ghomaride domain with dominant Triassic and Jurassic shelf and slope sedimentation (Bouillin et al., 1986).
3,
10
09
08
P Oi IGFQ,
06
05
04
03
02
01
‘-F
1
j 300 4cxJ 500 600
T(C”)
Fig. 3. P-T-r paths of the Mulhacen Complex (light stipple)
and the Almanzora Unit (dark stipple). Tourmahne K/Ar.ages
for D, and D,_t are indicated. Ages (Ma) of deformation
phases used to constrain exhumation are indicated by circles,
inferred ages by diamonds. Boxes indicate P-T conditions
(after Bakker et al., 1989). (I ) albite-jadeite + quartz (Newton
and Kennedy, 1968); (2) glaucophane stability (Maresch,
1977); (3) staurolite-in (Hoschek, 1969); (4) anorthite+HzO
= kyanite f zoisite + quartz (Newton and Kennedy, 1963); (5)
Al-silicate triple point (Holdaway, 1971).
Tectonometamorphic evolution
The pressure temperature (P-T) and tectonic evolution of the Mulhacen Complex and the Al- manzora Unit of the Alpujarride Complex has been reconstructed by Bakker et al. (1989) by relating deformation and metamorphism and P-T determinations by microprobe analyses.
Both complexes are characterized by initial HP/LT metamorphism, indicating the dis- turbance of the pre-existing pattern of isotherms by subduction. The maximum metamorphic pres-
sures in the Mulhacen Complex (1 GPa) (Fig. 3) occur in the western Sierra Nevada to the eastern Sierra de 10s Filabres (Velilla and Fen011 Hach-Ali, 1986; Gomez-Pugnaire and Fernandez-Soler, 1987; Bakker et al., 1989). The Almanzora Unit experi- enced a pressure of 0.7 GPa (Bakker et al., 1989), which agrees with the maximum pressure in the other Alpujarride units (GoffC et al., 1989). Subse- quent isobaric heating in both units indicates the starting relaxation of the disturbed pattern of iso- therms and cessation of further underthrusting of cooler crustal segments (England and Thompson, 1984). At the end of the isobaric heating trajectory the first phase of penetrative deformation (D,_,) took place. The most penetrative deformation (D,) occurred at peak temperature conditions of about
ALPINE TECTONICS AND ROTATION POLE EVOLUTION OF IBERIA
570” C in the Mulhacen Complex and 450 o C in
the Almanzora Unit (Fig. 3) (Bakker et al., 1989).
D, effectively transposed all earlier fabrics. In
the Almanzora Unit D,_, deformation fabrics
were only left as internal fabrics in glaucophane
and crossite crystals. In the Mulhacen Complex
penetrative D,._, fabrics were left unaffected only
locally in glaucophane schist facies amphibolites,
local conglomerate bodies and in the core of a 5.5
km3 gneiss body. D, _ 1 is characterized by E-W to
ESE-WNW trending stretching lineations (Fig. 2)
on flat-lying foliations. Strain analyses on con-
glomerate pebbles indicates extensional strains of
lOO-300% (Fig. 4A). Borradaile (1976) inferred
ESE-WNW extensional strains in excess of 150%
in the gneisses. Top-to-the-west shear is indicated
by asymmetric tails at the extremities of K-felds-
par porphyroclasts. Ductile D,_ 1 deformation was
the result of thrusting within the Mulhacen Com-
plex (Bakker et al., 1989). D, is also characterized
by important regionally consistent E-W to ESE-
WNW stretching (Fig. 2) paralleling axes of lo-
cally pronounced sheath-like folds. Plagioclase
porphyroclasts in amphibolites record extensional
strains of 200-600% (Fig. 4B) which, however,
might contain an unknown D,_, component. A
minimum D, stretching amount is provided by the
rotation of syn-D, garnets. Rotation angles of
90-110” indicate a shear strain of 3.5 using the
Rosenfeld (1970) equation. If this rotation is
B
285
formed during plane strain, the shear strain indt-
cates 250% extension. Vissers (1989) arrived at a
similar strain estimate. Because the contact be-
tween the internal garnet fabric and the external
fabric is lost most often during post-blastesis D,
deformation and garnets have been boundinaged,
this amount is a minimum estimate. Strain analyses
on pebbles in quartzites with a penetrative D,
fabric in the Alpujarride Complex indicate 300-
600% extension (Fig. 4C). Similarity of main phase
deformation fabrics in both complexes combined
with comparable amounts and directions of
stretching directions indicate a similar tectonic
history. Strain in the Alpujarride Complex is
much more heterogeneously developed, the core of
the conglomerate body indicating maximum ex-
tension of 125% (Fig. 4C).
On the basis of the models of Davy and Gillet
(1986) the P-T-t path of the Alpujarride Com-
plex is explicable by a screening effect of the
underlying Mulhacen Complex and heating to-
gether with loading by overlying crustal segments
during D,. In the last stages of D, the Mulhacen
Complex overthrust the Veleta Complex (Fig. 5B),
the latter never having experienced very deep
tectonic burial. The contact zone is characterized
by mylonites with E-W trending stretching linea-
tions (Fig. 2). Preferred orientations of quartz-c-
axes indicate top-to-the-west shear (De Jong, in
prep.). Large-scale imbrication occurred in a crust
Fig. 4. Log-strain diagram (Wood, 1974) presenting strain analyses from the Internal Zone; averages indicated by triangles. (A) D,_ 1 quartz pebbles, Mulhacen Complex, location (c) in Fig. 2, central Sierra de 10s Filabres. (B) D, elongated plagioclase porphyroclasts
in amphibolites, Mulhacen Complex, location (d) in Fig. 2, eastern Sierra de 10s Filabres. (C) D, quartz pebbles, high strain area
indicated by crosses, low strain area by dots, Alpujarride Complex, location (i) in Fig. 2, central Sierra de las Estancias; the single
square displays one determination from the Almanzora Unit near location (8).
2X6 K. DE JONG
A LD, CONFIGURATION 1 AU MC
i- T--r 80-85 Ma
6 Lb+, CONFIGURATION c T--r
‘i
w \
33 Ma
E
0
Fig. 5. (A) Crustal configuration during the 85-80 Ma phase of crustal scale imbrication a peak thermal conditions during D, (insets
arc P-T-f paths). (B) Oligocene extension of the crustal wedge. juxtaposing the Almanzora Unit (AU) and the Mulhacen Complex
(MC) during D, + ,
that had already been largely thermally equi-
librated after initial thermal disturbance by sub-
duction. The Almagride Complex is also char-
acterized by ESE-WNW trending stretching lin-
eations (Fig. 2) in carbonate mylonites, which
record top-to-the-west shearing by asymmetric
pull-apart structures.
After D,, decompression and cooling dominates
the thermal evolution, in the absence of any
penetrative deformation. The form of the P-T-t
trajectory precludes rapid exhumation of the In-
ternal Zone. Continued thermal equilibration to-
wards a new steady-state isotherm generates an
increasing apparent geothermal gradient, which
reaches about 35O/km. Erosional unroofing pre-
sumably played an important role during this
trajectory.
The Almanzora Unit was placed on top of the
Mulhacen Complex along a low-angle ductile nor-
mal shear zone during D,, ,, which represents a
phase of heterogeneous crustal thinning and ex-
tension (Bakker et al., 1989). The latter authors
estimated the excision of a 6 km thick crustal
section along a single shear zone during eastward
slip of the hangingwall. Thermal consequences of
extension were retarded; temperature increase
started during Dx+* and culminated during the
D X+3 second thermal peak at 525 o C (Bakker et
al., 1989). Retardation of heating at a particular
crustal level with respect to the timing of exten-
sion is also shown by thermomechanical models of
crustal extension (Crough and Thompson, 1976;
Thompson, 1981; Moretti and Froideveaux, 1986).
Crustal thickening by large-scale S-verging D, +Z
ALPINE TECTONICS AND ROTATION POLE EVOLUTION OF IBERIA 287
folding and associated thrusting enhanced this.
The second thermal peak may indicate the effect
of magma addition (Thompson, 1981) or introduc-
tion of magmatic fluids (England and Thompson,
1984) at higher crustal levels. The large amount of
heating, about 100 o C (Fig. 3) indicates the intro-
duction of a transient heat source in the Internal
Zone; this was the consequence of crustal and
lithospheric mantle extension and resulted in em-
placement of ultramafic rocks in the western Bet-
its (Platt, 1987; Bakker et al., 1989; Doblas and
Oyarzun, 1989) in the Early Miocene (22 + 4 Ma,
Priem et al., 1979; 21.5 + 1.8 Ma, Zindler et al.,
1983). The timing is coincident with intrusions of
similar rocks in the Rif in Morocco (Ben Othman
et al., 1984). The Dx+3 thermal peak in the eastern
Internal Zone is consequently an Early Miocene
feature. The regional importance of this event is
indicated by widespread resetting of radioisotope
systems at the Oligocene-Miocene boundary in
the Kabylian Massifs in northern Algeria and the
External Rif (MoniC et al., 1984a, b, 1988).
Timing of tectonic events in the Mulhacen Com-
plex
In order to constrain the tectonic evolution of
the Betic Zone we need to know the ages of the
various tectonometamorphic phases. However,
only very limited radiometric data on metamor-
phic minerals are available. For the Mulhacen
Complex an average muscovite Rb/Sr age of 13.8
Ma has been calculated from data reported by
Priem et al. (1966) and Andriessen et al. (1989).
The latter authors also report a 12.8 Ma biotite
Rb/Sr age. In addition, in the context of a feasi-
bility study of K/Ar dating of tourmalines three
ages of 80-85 jI 8 Ma and one age of 116 f 10 Ma
have been reported (Andriessen et al., 1989). The
suggested blocking temperature for tourmaline of
above 600” C (Andriessen et al., 1989) well ex-
ceeds the maximum metamorphic temperature in
the Mulhacen Complex. These ages can therefore
be interpreted as metamorphic crystallization ages.
The 80-85 Ma ages (averaging 83 Ma) are ob-
tained from gneisses with a D, mylonite fabric, in
which synkinematic growth of tourmaline has oc-
curred. This suggests an age of 83 Ma for D,. For
the 116 Ma age, excess Ar might be put forward as
an explanation as this component has a widespread
occurrence (Hebeda et al., 1980); in addition, this
is an explanation which is difficult to disprove.
Alternatively, this age can reflect pre-D, ~, or D, _. ,
metamorphism. It will be shown that the 116 Ma
age is actually in accordance with the time scale
for the establishment of the Mulhacen Complex
P-T-t path, and can be geologically relevant.
A point which constrains the P-T-t path of
the Mulhacen Complex is D,, which occurs at a
depth of 31 km with an inferred age of 83 Ma.
Another point is D, + 3, with an inferred age of 22
Ma at about 7.5 km depth. Combination of these
two P-T-t points provides an exhumation of 23.5
km in 61 Ma; which is an exhumation rate of 0.39
km/Ma. As the depths of the other deformation
phases are known (Fig. 3) their age can be esti-
mated by using a first-order approach of uniform
exhumation with time. As the Mulhacen Complex
experienced five phases of penetrative deforma-
tion related to translations, this reasoning is cer-
tainly a simplification: it should only be used as
an initial guide. D, + 1 and Dx+Z have an inferred
age of 33 Ma and 26 Ma respectively. The age of
D x-1 is approximated at 99 Ma, using the post-D,
exhumation rate for the D,-D,-, trajectory too.
The 119 Ma age for initial HP/LT metamor-
phism is obtained by adding 20 Ma to the age of
D x_,r which is consistent with estimates for iso-
baric heating of HP/LT metamorphics from
modelling by Richardson and England (1979) and
England and Thompson (1984). The 116 Ma ra-
diametric age is thus in accordance with the ther-
mal evolution of. HP/LT metamorphic crustal
segments. An alternative correlation of the 116
Ma age with D,-, would result in a very slow
uplift of 0.2 km/Ma between D, and D,- ,. Such
a slow uplift certainly would have erased all evi-
dence of HP/LT metamorphism due to long-term
recrystallization near the thermal peak D,; this
does not accord with the observed partial over-
printing. Another consequence of the uniform ex-
humation approach is a period of about 50 Ma
without penetrative deformation between D, and
D, + , This is the consequence of the rotation pole
evolution, which will be discussed in the next
section.
288
The tentative 99 and 83 Ma ages for the first
two phases of penetrative deformation in the east-
ern Internal Zone accord with well-established
95-80 Ma 40Ar-39Ar ages for deformation in
northern Africa; this deformation is also char-
acterized by important E-W stretching (Monie et
al., 1984a, b). Stepwise heating experiments fur-
ther record a thermotectonic event at 28-25 Ma
(MoniC et al., 1984a, b, 1988), which accords with
heating in the Betics after 26 Ma, culminating at
22 Ma. The 13.8 Ma and 12.8 Ma Rb/Sr mica
ages indicate cooling after the Early Miocene ther-
mal peak.
Rotation pole evolution and tectonics in the west-
ernmost Mediterranean
Collision in the Internal Zone
Early Cretaceous rifting and rotation of Iberia
occurred independent of the motion of Africa and
North America (Savostin et al., 1986). Coinci-
dence of the Iberian and African rotation poles in
the late Aptian has been explained by the collision
of these two plates (Savostin et al., 1986). The
timing closely coincides with the proposed 116 +
10 Ma age for initial HP/LT metamorphism and
subduction in the Internal Zone. Data from Klit-
gord and Schouten (1986) and Srivastava and
Tapscott (1986) indicate that Iberia formed part
of Africa directly from the initial rifting from
North America, after 123 Ma. HP/LT metamor-
‘5”’ ’ ‘OO’ ”
K DE JONG
phism in the Betics in this model would be ini-
tiated by collision of Africa-Iberia with another
continental fragment. In both models initiation of
oceanic spreading to the west of Iberia, at about
115 Ma (Boillot et al., 1989; Malod, 1989) is
coeval with collision and subduction to the east of
Iberia. This timing of collision agrees with a num-
ber of geological features indicative of tectonism
at this time, and heavy terrigeneous sedimentation
of Aptian age in the Mauritanian flysch unit in
northern Africa, which comprises turbidites with a
northern provenance (Dercourt et al., 1986)
accords with collision to the north in the Betics.
Widespread erosion and faulting characterizes the
Aptian to late Albian in the Malaguide Complex
(Roep, 1980).
Intracontinental thrusting in the Internal Zone
D x_ 1 and D, structures were tentatively formed
at 99 Ma and 83 Ma respectively, during post-sub-
duction intracontinental thrusting of segments of
various metamorphic grade and burial histories
(Fig. 5a). Regionally consistent D,_, and D,
ESE-WNW trending stretching lineations are
coincident with the 110-80 Ma motion vector in
the Betics around the combined African-Iberian
rotation pole of Savostin et al. (1986) (Figs. 2 and
6). Coincidence of the plate motion vector and the
movement and stretching direction in a crustal
scale imbricate stack suggests that thrusting at
lower crustal depths is directly driven by plate
motion vector
,P. 1 loo.
Fig. 6. The 110-80 Ma position of the combined rotation pole position of Africa and Iberia, motion vector around this pole for
southeastern Spain indicated by the ESE-WNW trending bar, which coincides with similarly trending stretching lineations. Positions
of rotation poles (Ib = Iberia; A/= Afica) and continents at 80 Ma after Savostin et al. (1986), Apulia schematically indicated.
ALPINE TEC-TONICS ‘AND ROTATION POLE EVOLUTION OF IBERIA 289
convergence. The length of the 110-80 Ma plate
motion vector (Savostin et al., 1986) indicates
appro~mately 600 km of motion at the latitude of
southern Spain. If motion has been steady through
time this suggests 400 km of convergence between
99 and 83 Ma. which constrains the maximum
amount of overthrusting in the Internal Zone. The
map (Fig. 2) indicates a minimum D, overthrust-
ing of 150 km of the Mulhacen Complex over the
Veleta Complex parallel to the stretching linea-
tion. To this estimate a few tens of kilometres of
D,_, thrusting within the Mulhacen Complex
(Bakker et al., 1989) must be added. Total over-
thrusting is about 200 km. The amount of over-
thrusting of the Alpujarride Complex must be
simultaneously considered. However, the original
relationship between the Alpujar~de Complex and
the underlying Mulhacen Complex is disturbed by
a low-angle ductile normal shear zone of Oligo-
cene age (Fig. 5B). This makes it impossible to
establish the amount of Cretaceous overthrusting.
Furthermore, part of the overthrusting of the Al-
pujarride Complex might already have been
accomplished during subduction. The balancing
approach is certainly a simplification, as it does
not include the possible role of Cretaceous strike-
slip motions between the Internal and External
Zones of the Betic Cordilleras and in northern
Africa. It does indicate, however, the importance
and magnitude of westward directed overthrusting
driven by plate convergence.
As the motion vector defines the relative mo-
tion between Africa-Iberia and stable Eurasia,
one of the crustal segments involved in thrusting
was attached to stable Eurasia. Two models can
be envisaged. In the first model the entire Internal
Zone belongs to Eurasia and the External Zone to
Iberia. In a second mode1 the Internal Zone also
belongs to Iberia (and thus to Africa). In both
models the Eurasian promontory is connected via
the Sardinia-Corsica crust with main Eurasia. The
first model predicts strong differential motions
between the allochthonous Internal Zone and Ex-
ternal Zone. ESE-WNW trending stretching lin-
eations in the Almagride Complex indicate in-
volvement of a rifted part of the External Zone in
Cretaceous thrustingIn the second model the In-
ternal Zone was subducted and overthrust by a
segment of Eurasia; strong differential motion has
taken place between this upper plate, presumably
a Kabylian type of segment, and Iberia. In the
second model the differential motion between the
Internal and External Zones of the Betic
Cordilleras is much more limited. Flysch deposits
to the south of the Kabylian Massifs (Bouillin et
al., 1986) indicate important motion between these
massifs and Africa. The Kabylian Massifs experi-
ence E-W stretching and shearing during the 95-
80 Ma period (Mom& et al., 1984a, 1988). This
direction fits the plate motion vector in the area at
this time, indicating that the Kabylian segment
was involved in the Cretaceous collision. Sub-
marine faulting in late Turonian to early Senonian
times and widespread erosion in the Cenomanian
to early Turonian in the Malaguide Complex
(Roep, 1980) occur contemporaneously with
thrusting at depth.
The 110-85 Ma tectonic regime at the northern
boundary of Iberia (the Galicia Margin and the
future Pyrenees) resulted from left-lateral motion
of Africa-Iberia with respect to Eurasia (Savostin
et al., 1986; Srivastava and Tapscott, 1986; Klit-
gord and Schouten, 1986; Malod, 1989). The North
Pyrenean Fault can be approximated by a small
circle around the same rotation pole as that for
the movement direction of the collisional tectonics
in the Internal Zone, indicating a coupling be-
tween both motions.
Pyrenean collision and tectonic quiescence in the
Internal Zone
A new position of the combined African-
Iberian rotation pole after 80 Ma near the Straits
of Gibraltar (Savostin et al., 1986) (Fig. 7a) re-
sulted in a dramatic change in the tectonic regime
in the Pyrenees and in the Betics. The formerly
thinned, heated and consequently weakened
Pyrenean domain was thickened in compression.
Flexure modelling of the Ebro Basin at the south-
ern boundary of the Pyrenees confirmed that colli-
sion was intracontinental in nature (Zoetemeijer et
al., 1990). Oblique convergence started in the
Campanian (Puigdefabregas and Souquet, 1986)
mimicking the rotation pole evolution very accu-
rately. Deformation culminated in the Eocene
290 K. DE JONG
Fig. 7. Positions of the African ( Af )-Iberian (16) combined rotation pole after Savostin et al. (1986). (a) Quadrangles indicate the 80-65 Ma and circles the 65-54 Ma position close to the previous collision zone: Apulia schemetically indicated. (b) Positions of the
separated African and Iberian poles for the 54-35 Ma period. Iberia is part of the Eurasian continent at 35 Ma.
(Mattauer and Henry, 1974; Puigdefabregas and
Souquet, 1986), during continuing convergence be-
tween Africa and Eurasia around the Gibraltar
pole. Savostin et al. (1986) indicate that motion
around this pole resulted in about 100 km of
shortening in the Pyrenees; this accords with the
analysis of the ECORS profile (Rome et al., 1989).
Thermal disturbances at 60-55 Ma in the Pyrenean
shear zones {Costa and Malt&i, 1988) and at the
northwestern termination of the Iberic Cordillera
(Golberg et al., 1988) coincide with initiation of
spreading in the Norwegian-Greenland Sea
(Srivastava and Tapscott, 1986; Klitgord and
Schouten, 1986; Savostin et al., 1986). This in-
duced an additional compressional component in
western Eurasia.
Because Iberia was attached to Africa it acted
as an African promontory during collison with
Eurasia in the Pyrenees. It suffered relatively in-
tense deformation by reactivation of Variscan and
Mesozoic faults (Guimera, 1984; Viallard, 1985) in
a weakened lithosphere by Cretaceous extension
(Zoetemeijer et al., 1990). Convergence resulted in
limited riot-later~ motion of main Iberia with
respect to the Iberic Cordillera and the Ebro Basin
(Malod, 1982) and left-lateral motion in the Cata-
lan Coastal Range (Guimera, 1984). A subhori-
zontal NW-directed main compression direction
u1 in the Catalan Coastal Range (Guimera, 1984)
coincides with the motion direction around the
Gibraltar poie.
During the Pyrenean collision the Internal Zone
was tectonically relatively quiet, as is evident from
the absence of penetrative deformation for about
50 Ma, between 83 Ma and 33 Ma. This is in close
agreement with the geochronological evolution of
the Kabylian Massifs in northern Algeria. The
location of the African-Iberian rotation pole near
the Cretaceous Betic collision zone (Fig. 7a) in-
bibited large-scale motions in this zone after 80
Ma. Minor tectonics is documented in the Exter-
nal Zone of the Betics in the form of relative uplift
between 68 Ma and 60 Ma; this probably resulted
from compression caused by African-Eurasian
convergence (Kenter et al., 1990).
After 54 Ma the African rotation pole was
separated from the Iberian pole and shifted north-
ward (Savostin et al., 1986) (Fig. 7b). Shifting
might be partly explained by the Pyrenean colli-
sion, forcing the African plate to pivot around a
different pole. The effect of this new rotation pole
position is the starting of limited differential mo-
tion between Africa and Iberia, resulting in the
tectonism which has been well documented in the
Betic Cordilleras. The External Zone records a
second period of uplift at about 50 Ma (Kenter et
al., 1990). The Malaguide Complex shows an ero-
sional contact between the Maastrichtian and the
Early Eocene (Roep, 1980). Because the metamor-
phic zones of southern Spain and northern Africa
do not record penetrative deformation and meta-
morphism, this tectonic activity is probably of
ALPINE TECTONICS AND ROTATION POLE EVOLUTION OF IBERIA 291
minor importance. Northerly to north-northeast-
erly compression is detected in the late Eocene in
the Catalan Coastal Range (Guimera, 1984) and
the External Betics (De Ruig, this issue) and in
other areas in Spain (Letouzey, 1986; Bergerat,
1987). The main compression direction is coinci-
dent with the motion vector around the 54-35 Ma
African rotation pole of Savostin et al. (1986)
(Fig. 7b). The mountain ranges of northern Africa
also experienced compression during this episode
(Letouzey, 1986; Dercourt et al., 1986) presuma-
bly connected with the Pyrenean collision. The
Pyrenean collision ended at about 35 Ma, after
which no independent lberian rotation pole may
be detected (Savostin et al., 1986). Klitgord and
Schouten (1986) concluded that the final
amalgamation of Iberia with Eurasia occurred at
about 30 Ma.
Extensional tectonics
Savostin et al. (1986) demonstrate a dramatic
shift of the African rotation pole to a new position
in the South Atlantic at 35 Ma as a consequence
of 40% decrease in spreading rate between the
African and North American plates; no change
occurred in Eurasia-North America spreading.
This kinematic pattern is, however, not supported
by the central Atlantic magnetic anomaly pattern
(Klitgord and Schouten, 1986) or by North
Atlantic and Arctic data (Srivastava and Tapscott,
1986). Klitgord and Schouten (1986) indicate a
shift of the African-Eurasian plate boundary from
the northern side of Iberia to the southern side of
it, separating Iberia from Africa by the Azores-
Gibraltar fracture zone after 30 Ma. The establish-
ment of a new plate boundary between Iberia and
Africa accords with timing of extensional defor-
mation and heating in the Internal Zone and
northern Africa. Regionally consistent southeast-
erly slip of the hangingwall towards ultramafic
rocks in the western Betics (Tubia and Cuevas,
1986) and the Rif (Saddiqi et al., 1988) suggests a
SE-NW extensional component on the plate
boundary. Extension is further attested by an Early
Miocene basaltic dike-swarm (Torres-Roldan et
al., 1986). The timing of extension and magmatism
accords well with the tectonic evolution of the
Gulf of Lion and the Balearic Basin, which opened
in Oligocene to Aquitanian times (Alvarez et al.,
1974; Rehault et al., 1984). Deformation in this
area spread southward with time (Mauffret and
Gennesseaux, 1989). Extension resulted in pro-
gressive crustal thinning in northeastern Spain to-
wards the Balearic Basin (Banda, 1987). Strong
crustal thinning in the eastern part of the Internal
Zone (Banda and Ansorge, 1980) is also attributed
to this Oligo-Aquitanian crustal thinning and ex-
tension. Extensional deformation to the east of
Iberia links the African-Eurasian plate boundary
with the western European rift system (Bresse-
Rhine graben) which experienced extension up to
the latest Oligocene (Bergerat, 1987). The shift of
the African rotation pole at 35 Ma accords well
with renewal of deformation in the Betics and
northern Africa. However, the motion around this
pole (Savostin et al., 1986) generates northwesterly
compression between Africa and Eurasia and
hence cannot explain the observed extension.
The 20 Ma position of the African rotation
pole to the northwest of Portugal (Savostin et al.,
1986) resulted in cessation of extensional deforma-
tion and induced a northeasterly relative motion
of Africa with respect to Eurasia, resulting in
NE-SW directed compression (Letouzey, 1986;
Bergerat, 1987). Compression caused thickening of
the previously thinned and weakened crustal do-
main to the south of Iberia, this being demon-
strated by NNE-directed thrusting in the Mulha-
ten Complex (Bakker et al., 1989) and reactivation
of the original contact between the Alpujarride
and Mulhacen Complexes. The Alpujarride Com-
plex has moved northwards on a shear zone with
respect to the underlying Mulhacen Complex (Platt
et al., 1983) which already contains the imprints
of the 22 Ma Dx+3 thermal peak. Behrmann (1984)
concluded on the basis of palaeostress and strain
rate estimates that ductile deformation in this
shear zone lasted 4 Ma. Consequently, ductile
thrusting stopped during the Burdigalian. This
accords with the superposition of the Malaguide
Complex onto the already quite well developed
Alpujarride Complex around the Aquitanian-
Burdigalian boundary (Makel, 1981) and with
sealing of thrusts in the Malaguide Complex by
Burdigalian sediments (MacGillavry et al., 1963;
292 K DE JONG
Torres-Roldan et al., 1986). Burdigalian sedimen-
tation in large parts of the Internal Zone occurred
in a tectonically quiet environment (Volk, 1967).
The compression direction after 20 Ma enables
early left-lateral motion on ENE-WSW to NE-
SW trending strike-slip faults crossing the Betic
Zone. Middle Miocene strike-slip motion has been
described by Sanz de Galdeano et al. (1985) and
by Bon et al. (1989). The 10 Ma to present rota-
tion pole position of Africa, to the west of
Gibraltar (Savostin et al., 1986) enables the
northwesterly to northerly compression detected
by Montenat et al. (1987) in the Betics. The posi-
tion of the main compression axes in the obtuse
angle of a set of NE-SW and NNE-SSW trend-
ing strike-slip faults (Montenat et al., 1987) points
to a reactivation of an earlier fault system. The
position of the rotation pole relatively close to the
strike-slip fault system only allows limited dis-
placements. About 20 km of left-lateral slip has
been argued by Veeken (1983) for the NNE-
trending Palomares Fault. Both phases of strike-
slip motion juxtapose crustal segments with differ-
ent Moho depths, the latter inherited from late
Oligocene to Aquitanian extension. Present-day
compression and intraplate seismicity (Udias et
al., 1976) is localized in the thinned Alboran Sea
and southern Spain.
Conclusions
The tectonic evolution of the Alpine collision
belts bordering Iberia is in accordance with
kinematics of the Iberian and African plates and
their rotation pole evolution.
Subduction and HP/LT metamorphism in the
Betics at 116 + 10 Ma coincide with initiation of
seafloor spreading at the northwestern margin of
Iberia and the Bay of Biscay. This phase also
coincides with heavy terrigeneous sedimentation
in the Mauritanian flysch in northern Africa and
the tectosedimentary evolution of the Malaguide
Complex.
A period of intracontinental thrusting between
99 Ma and 83 Ma in the Internal Zone of the
Betics occurred during continuing spreading to the
west of Iberia and progressive opening of the Bay
of Biscay. Regionally consistent ESE-WNW
trending stretching lineations in the Internal Zone,
which were formed during thrusting at lower
crustal levels, are coincident with the motion di-
rection of Africa-Iberia with respect to Eurasia.
At least 200 km of thrusting in the Internal Zone
was driven by the convergence of Africa-Iberia
with respect to Eurasia. Strike-slip motion of
Africa-Iberia with respect to Eurasia along the
North Pyrenean Fault took place around the same
rotation pole as thrusting in the Betics.
At 80 Ma, shifting of the African-Iberian rota-
tion pole to a position near the Betic collision
zone resulted in cessation of penetrative deforma-
tion in the Internal Zone and northern Africa.
Collision of Africa-Iberia with Eurasia was trans-
ferred to the Pyrenees. Iberia acted as an African
promontory by motion around the rotation pole
near Gibraltar. Pyrenean collision culminated at
60-55 Ma by an additional compression generated
by seafloor spreading in the Norwegian-Green-
land Sea.
After completion of the Pyrenean collision at
35-30 Ma, penetrative deformation and heating
again took place in the Internal Zone and north-
ern Africa by establishment of the Azores-
Gibraltar fracture zone, which interacted with the
Cretaceous collision system. The new plate
boundary was connected via the Balearic rift sys-
tem with the western European rift. Deformation
was initiated by late Oligocene crustal and litho-
spheric mantle extension, resulting in Early
Miocene emplacement of ultramafic rocks with
associated heating.
Compression after 20 Ma was initiated by mo-
tion around a rotation pole to the west of Iberia.
Crustal thickening was localized in the previously
extended and heated and consequently weakened
Internal Zone. This process resulted in overthrust-
ing in the Internal Zone, which was completed
before the end of the Burdigalian. Middle and
Late Miocene strike-slip motion was initiated dur-
ing continuing convergence and juxtaposed crustal
segments of differing Moho depths, the latter hav-
ing been inherited from late Oligocene to Early
Miocene extension.
Acknowledgements
I thank Sierd Cloetingh for constructive criti-
cism on the manuscript and Henk Helmers for
ALPINE TECTONK’S AND ROTATION POLE EVOLUTION OF IBERIA 293
placing the strain data on plagioclase porphyro-
clasts at my disposal. Jacques Malod, Paul
Andriessen and Reini Zoetemeier are thanked for
providing preprints. The technical assistance of
Fred Kievits during the preparation of the figures
is aiso acknowledged. Part of the field work was
financed by a grant from the “Stichting
Molengraaff-fonds”.
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