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Tectonophysics 370 (2003) 49–76
Microstructures, petrofabrics and seismic properties of ultra
high-pressure eclogites from Sulu region, China: implications
for rheology of subducted continental crust and origin
of mantle reflections
Shaocheng Jia,*, Kazuko Saruwataria,1, David Mainpriceb, Richard Wirthc,Zhiqin Xud, Bin Xiae
aDepartement des Genies Civil, Geologique et des Mines, Ecole Polytechnique de Montreal, Succursale Centre-Ville,
Montreal, Quebec, Canada H3C 3A7bLaboratoire de Tectonophysique, Universite de Montpellier II, 34095 Montpellier, Cedex 05, France
cGFZ-Potsdam, Telegrafenberg, D-14473, Potsdam, GermanydChinese Continental Scientific Drilling Program (CCSD), Institute of Geology, Chinese Academy of Geological Sciences, Beijing, PR China
eGuangzhou Institute of Geochemistry, Chinese Academy of Sciences, Wushan, Guangzhou 510640, PR China
Accepted 31 March 2003
Abstract
Ultra high-pressure (UHP) eclogites from Sulu region (China) represent mafic components of the continental crust,
which were first subducted to mantle depths greater than 100 km and then exhumed to the earth’s surface. Detailed
investigation of microstructures, chemical compositions, petrofabrics and seismic properties of the UHP eclogites can
provide important information on the operating deformation mechanisms and rheology of subducted continental crust and
on the origin of seismic reflections within the upper mantle. We present here results from field, optical and TEM
observations, electron back-scattered diffraction (EBSD) measurements and numerical computations of the seismic
properties of UHP eclogites collected from fresh surface outcrops at the drill site (Maobei, Donghai County, Jiangsu
Province) of the Chinese Continental Scientific Drilling Program (CCSD). Two types of eclogites have been distinguished:
Type-1 (coarse-grained) eclogites deformed by recovery-accommodated dislocation creep at the peak metamorphic
conditions, and Type-2 (fine-grained) eclogites which are composed of reworked Type-1 materials during recrystallization-
accommodated dislocation creep in shear zones which were active during the exhumation of the UHP metamorphic rocks.
Both garnet and omphacite in these eclogites deformed plastically and the flow strength contrast between these two
constituent minerals is apparently much less than an order of magnitude under the UHP metamorphic conditions. Plasticity
of eclogites under UHP conditions can effectively facilitate channeled flow along the interplate shear zone. The
0040-1951/03/$ - see front matter D 2003 Elsevier B.V. All rights reserved.
doi:10.1016/S0040-1951(03)00177-X
* Corresponding author. Fax: +1-514-3403970.
E-mail address: [email protected] (S. Ji).1 Present address: Department of Earth Science, Faculty of Science, University of Tokyo, Hongo 7-3-1 Bunkyo-ku Tokyo, Japan.
S. Ji et al. / Tectonophysics 370 (2003) 49–7650
preservation of the relict crustal materials within the continental lithosphere may produce regionally extensive, strong,
seismic reflections in the upper mantle. This may explain the origin of mantle reflections observed in many areas of the
world.
D 2003 Elsevier B.V. All rights reserved.
Keywords: Eclogite; Microstructure; Petrofabrics; Rheology; Subduction; Garnet; Omphacite; Seismic reflection
1. Introduction Wang and Liou, 1991) and diamond (Xu et al., 1992)
Whereas the upper crust is accessible to geological
sampling and mapping, the deeper portions of the crust
and the upper mantle are relatively inaccessible. Much
of our understanding about the composition, structure
and evolution of the deep crust and upper mantle
beneath continents has been derived from various
seismic refraction and reflection measurements. Inter-
pretation of these seismic data is mainly based on our
knowledge of the elastic properties of rocks and rock-
forming minerals, the latter obtained largely from
laboratory measurements of ultrasonic velocities and
density (e.g., Christensen, 1965; Kern and Richter,
1981; Kern, 1990; Ji and Salisbury, 1993; Christensen
and Mooney, 1995; Burlini and Tancredi, 1998; see Ji
et al., 2002, for summary). However, it is not easy to
simulate the pressure and temperature environments of
the earth’s mantle in the laboratory. Thus, theoretical
calculations of seismic properties based on the elastic
theory (Crosson and Lin, 1971; Ji and Mainprice,
1988; Mainprice, 1990) become another way to esti-
mate the anisotropic seismic properties of any kind of
possible rocks when all the physical properties such as
elastic constants, density and crystallographic pre-
ferred orientation (CPO) are known for each constitu-
ent mineral (e.g., Mainprice and Silver, 1993; Ji et al.,
1994; Mainprice et al., 2000; Mauler et al., 2000;
Saruwatari et al., 2001). The CPO measurement of
ultrahigh pressure (UHP) eclogites from former conti-
nental subduction zones has recently been made pos-
sible by technological developments of SEM-based
measurements of minerals of any symmetry, such as
cubic garnet (Prior et al., 2000) and omphacite (Mauler
et al., 2000; Bascou et al., 2002).
The Qinling–Dabie–Sulu ultrahigh pressure (UHP)
metamorphic belt, which is about 1000 km long and
120 km wide, is the largest among seven well-recog-
nized UHP belts in the world and has been investigated
extensively since the discovery of coesite (Xu, 1987;
from the region. The UHP rocks were a part of
lithospheric slab subducted at the intracontinental col-
lision zone between the Sino-Korean and Yangtze
blocks in the Late Triassic or Early Jurassic (e.g., Cong,
1996; Liou, 1999). Previous studies (e.g., Hirajima et
al., 1992; Yang et al., 1993; Zhang et al., 1994) suggest
that the UHP rocks from Dabie and Sulu region was
subducted to a depth up to about 150 km before
being rapidly exhumed to the earth’s surface. Pet-
rologic, mineralogical and geochemical aspects of
these UHP rocks have already been thoroughly
investigated during last decade (e.g., Zhang et al.,
1994; Cong, 1996; Liou, 1999). However, deforma-
tion microstructures of these UHP rocks have re-
ceived little attention although such investigations
may provide important information on deformation
mechanisms, rheological and petrophysical proper-
ties of the continental lithosphere first subducted
into and then exhumed from the upper mantle. In
this paper, we report the results of our investiga-
tions on microstructures, crystallographic preferred
orientation (CPO) and calculated seismic properties
of the UHP-eclogites from the Sulu UHP metamor-
phic terrane. These results are then applied to constrain
deformation mechanism and rheological behavior of
subducted slab and origin of seismic reflections in the
upper mantle.
2. Geological setting
The Sulu UHP metamorphic terrane, which has
been displaced about 530 km by the sinistral, strike–
slip Tanlu fault, is an eastern extension of the
Triassic Qinling–Dabie collision zone (e.g., Wang
and Liou, 1991; Wang et al., 1992). On the north,
the UHP metamorphic terrane is bounded by the
Yantai–Qingdao–Wulian fault with the Proterozoic–
Archean basement (Fig. 1), which is overlain by
Fig. 1. Simplified geological map of the Sulu ultrahigh-pressure (UHP) metamorphic terrane, eastern China. The Sulu region is situated in the
northern Jiangsu and eastern Shandong province. Star symbol represents the drill site (Maobei, Donghai County, Jiangsu Province) of the
Chinese Continental Scientific Drilling Program (CCSD) where eclogite samples were collected. Modified from Zhang et al. (1994).
S. Ji et al. / Tectonophysics 370 (2003) 49–76 51
Paleozoic cratonal cover and the Mesozoic volcano-
clastic rocks (Zhang et al., 1994). On its southern
limit, the high-pressure (HP) terrane includes blues-
chists bounded by the Haizhou–Siyang fault. The
UHP terrane consists of eclogite, gneiss, marble,
quartzite and meta-ultramafic rocks. The eclogite
occurs as sheared lenses, pods and layers ranging
from tens of centimeters to hundreds of meters in
size within foliated ultramafic blocks, metapelites
(garnet-quartz-jadeite gneisses), kyanite quartzites
and marbles. These eclogitic blocks are obviously
tectonic boudins. The age of UHP metamorphism
and the time of collision between the Sino-Korean
and Yangtze blocks is about 210–220 Ma (see Cong,
1996 for summary), as derived from independent
studies including Sm–Nd isochrons (Li et al., 1989,
1992), U–Pb zircon ages (Ames et al., 1993; Li et
al., 1993a,b), 40Ar/Ar39 dating (Hacker and Wang,
1995) and Rb–Sr dating (Cong, 1996). The protolith
of the UHP rocks are considered to be Archean
( = 1.66 Ga, Jahn et al., 1996) or Proterozoic
(f 800 Ma, Li et al., 1993a,b; Jahn et al., 1996).
The present-day crustal structures under the
Dabie–Sulu region are divided into four-layer struc-
tures (i.e., upper, middle, upper lower-crust and
lowermost crust) with an average total thickness of
34 km that is much thinner than the crust (45–70 km)
of western China (Li and Mooney, 1998; Kern et al.,
Fig. 2. Microstructures of the UHP eclogites from Maobei, Donghai, China. (a) Field photograph of compositional banding with alternating
garnet-and omphacite-rich layers. (b) Optical microphotograph of a typical garnetite layer. XZ sections. (c) Optical microphotograph of a coarse-
grained eclogite. Both garnet (Grt) and omphacite (Omp) are flattened and elongated. XZ sections.
S. Ji et al. / Tectonophysics 370 (2003) 49–7652
S. Ji et al. / Tectonophysics 370 (2003) 49–76 53
1999). Both the crustal thinning and exhumation of
the UHP rocks are attributed to an intensive tectonic
extension immediately after the collision between the
Sino-Korean and Yangtze cratons.
P-wave refraction and reflection profiles across the
Sulu UHP terrane from Tangchen to Lianshui (Yang et
al., 1999; Yang and Yu, 2001) have a series of
northwest-dipping reflectors at 0–500, 900–1100
and 3000–4000 m depth. These highly reflective
layers have an average P-wave velocity varying from
6.8 to 7.3 km/s, probably corresponding to a series of
sheared slices of UHP eclogite- and/or garnet lherzo-
lite-bearing felsic gneisses as exposed at the surface.
A high portion of eclogite/lherzolite (30–40 vol.%) is
needed to explain such high P-wave velocities (Kern
et al., 2002).
The studied samples of eclogites were collected
from fresh surface outcrops in stone pits at the drill site
(Maobei, Donghai County, Jiangsu Province) of the
Chinese Continental Scientific Drilling Program
(CCSD). This drill site is located in the southern part
of the Sulu UHP metamorphic terrane, about 30 km
east of the Tanlu fault and approximately 70 km west
of the Yellow sea (Fig. 1). The CCSD drilling started in
July 2001, has reached the depth of 3000 m, and
planned to reach a depth of 5000 m in the year of
2004, penetrating through all the observed seismic
reflectors and high Vp layers within the upper crust
of the region. Petrophysical properties of the studied
coesite-bearing eclogites may provide critical con-
straints on geological interpretations of the seismic
refraction and reflection data obtained from the CCSD,
and further shed light upon the deformation mecha-
nisms of the subducted slab and exhumation of UHP
metamorphic rocks.
Fig. 3. SEM orientation contrast (OC) image (a) and backscattered
electron image (b) of a typical coarse-grained eclogite. XZ sections.
3. Microstructures
3.1. Field, optical and SEM observations
In the field, the UHP eclogites reveal a strong
planar fabric defined by a compositional banding with
alternating garnet- and omphacite-rich layers (Fig. 2a).
These garnet-rich layers, containing more than 85–90
vol.% garnet, can be referred to as garnetite. The
omphacite-rich compositional layers are dominated
by omphacite (>80 vol.%) and can be referred to as
pyroxenite. These layers are 5–80 cm thick. On a
given outcrop, garnetite layers are usually thicker than
pyroxenite layers (Fig. 2a). The stretching lineation is
defined by the elongation of garnet and particularly
omphacite. In thin sections, both garnet and ompha-
cite are flattened and elongated in the eclogites (Fig.
2b and c). The compositional layering (Fig. 2a) is
believed to originate from mass-transfer-related meta-
morphic differentiation.
In thin sections cut parallel to the XZ plane, where
X is parallel to the stretching lineation and Z is nor-
mal to the flattened foliation, garnet grains generally
show a shape of elongate lenses with two smoothly
curved boundaries subparallel to the foliation (Fig. 2b
and c). Intersections of these two boundaries form
two-outward-pointing cusps extending into the folia-
tion plane. Some garnet grains show a well-devel-
oped pinch-and-swell structure. These microstructural
Fig. 4. Grain size distributions of garnet and omphacite in Type-1 (sample 96-MB3C) and Type-2 (sample 96-MB4) eclogites.
S. Ji et al. / Tectonophysics 370 (2003) 49–7654
characteristics provide unambiguous evidence for
garnet plasticity. In the XZ sections, omphacite shows
a mean aspect ratio (2.5–5.0) larger than garnet
(2.0–3.5). In the XY and YZ sections, omphacite also
shows a mean aspect ratio larger than garnet. The
larger aspect ratio of omphacite could be due to a fact
that garnet grains were equidimensional while om-
phacite crystals had a columnar shape prior to de-
Fig. 5. Flinn diagram showing the garnet shape fabrics of Type-1
(solid circle) and Type-2 (open circle) eclogites. X, Y and Z are the
mean crystal lengths in the directions parallel to the stretching
lineation, perpendicular to the stretching lineation and in the
foliation plane and normal to the foliation, respectively.
Fig. 6. SEM orientation contrast (OC) images showing porphyro-
clastic texture of garnetite layers in Type-2 eclogite (sample 96-
MB20D).
S. Ji et al. / Tectonophysics 370 (2003) 49–76 55
formation. It is necessary to note that no strong
deflection of the foliation and layering defined by
flattened omphacite grains has been observed around
garnet crystals (Fig. 2b and c). This fact suggests that
the rheological contrast between garnet and clinopyr-
oxene is much less under the UHP conditions than
those in amphibolite- and granulite-facies mylonites
from the deep crust.
Fig. 7. TEM microphotographs of dislocation substructures in deformed gar
regularly spaced, linear array of straight dislocations. Bright field. Sample 9
polygonal array of dislocations of two (d) or three (c) discrete orientations.
Thin sections which were first polished mechani-
cally and chemically, then coated with carbon and
were examined in a Philips XL30 SEM using a
forescatter detector system to collect orientation con-
trast (OC) images. On these OC images (Fig. 3), grain
boundaries and fractures can be clearly distinguished.
Internal structure such as cellular subdomains of
different crystallographic orientations (Prior et al.,
net grains. (a and b) Dislocation walls defined by well-organized and
6-MB3 (Type-1 eclogite). (c and d) Dislocation networks defined by
Bright field (c) and dark field (d). Sample 96-MB1 (Type-2 eclogite).
S. Ji et al. / Tectonophysics 370 (2003) 49–7656
2000) were occasionally detected in some garnet
grains (Fig. 6b).
Based on grain size, two characteristic types of
UHP eclogites can be identified. The first, referred to
as ‘‘Type-1 eclogites’’, is characterized by coarse-
grained garnet and omphacite. Garnet ranges from
0.15 to 1.4 mm with an average grain size of 0.52
mm, and omphacite (0.32–3.0 mm) has a mean grain
size of 0.93 mm (Fig. 4). Measurements made on thin
sections parallel to XY planes show that garnet and
omphacite have average aspect ratios of 2.06 and
2.58, respectively. On YZ sections, omphacite has a
slightly higher average aspect ratio (1.68) than garnet
(1.46). The garnet grains in Type-1 eclogites have thus
prolate shapes with a Flinn coefficient K = 1.4 (Fig. 5).
The second type of eclogites, referred to as ‘‘Type-2
eclogites’’, is characterized by relatively fine-grained
garnet and omphacite (Fig. 4). Garnet grain size
ranges from 0.03 to 1.4 mm with an average grain
size of 0.28 mm, and omphacite (0.03–1.5 mm) has a
mean grain size of 0.41 mm. Garnet and omphacite on
the XY sections have average aspect ratios of 1.4 and
1.78, respectively. On YZ sections, the average aspect
Fig. 8. TEM (bright field) microphotographs of dislocation substructures
(sample 96-MB3, Type-1 eclogite). (b and c) Dislocation junctions (samp
ratio is 1.56 for omphacite and 1.46 for garnet. The
garnet grains are characterized by quasi-plane-strain
shape with K = 1 in Flinn diagram (Fig. 5). Thus,
Type-1 and Type-2 eclogites can be considered as
LHS and LS tectonites (Helmstaedt et al., 1972),
respectively. The LHS tectonites deformed in the
field of apparent constriction while the LS tectonites
deformed in the field of plane strain and probably
indicates a simple shear deformation (Philippot and
van Roermund, 1992; Godard and van Roermund,
1995; Abalos, 1997; Zulauf, 1997).
Both types of eclogites consist of the same
assemblage of garnet (57F 6 vol.%), omphacite
(f 39F 10 vol.%), rutile (f 1–3%) and phengite
(f 0.5%), and minor amounts (less than 3 vol.%) of
secondary minerals such as amphibole and epidote.
Rutile occurs either as interstitial grains between
garnet and omphacite or as inclusions in these min-
erals. Coesite relicts and their quartz pseudomorphs
occur as inclusions in garnet and omphacite in Type-1
eclogites. Radial extensional fractures from these
inclusions are found in both garnet and omphacite.
Some omphacite grains are rimmed by a very fine-
in deformed garnet grains. (a) Free dislocations within a subgrain
le 96-MB1, Type-2 eclogite).
S. Ji et al. / Tectonophysics 370 (2003) 49–76 57
grained symplectite of plagioclase and Ca-pyroxene
or omphacite with a lower jadeite content. Amphibole
and epidote are the retrograde products which are
restricted to some fractures. Both types of eclogites
are pervasively cracked by extensional fractures
which are predominantly perpendicular to the stretch-
ing lineation (Figs. 2 and 3). These lineation-normal
fractures are very common in granulite facies mylon-
ites and UHP metamorphic rocks and thought to be
formed during the latest stages of the exhumation (Ji
et al., 1997).
When both types of eclogites coexist in the same
blocks, the coarse-grained Type-1 eclogites are
bounded by the fine-grained Type-2 eclogite layers.
The latter represent localized shear zones which over-
printed on the early coarse-grained Type-1 eclogite.
The shear zones are approximately parallel to the
regional penetrative mylonitic foliation in the strongly
deformed wall rocks such as garnet-bearing ultramafic
rocks, UHP paragneiss, quartzite and marble. Fore-
scatter orientation contrast imaging showed that the
Table 1
Bulk compositiona of representative eclogites from Maobei, Donghai Cou
Sample Lithology SiO2 TiO2 Al2O3 FeO+
Fe2O3
Mn
96-MB1B Type-2 eclogite 38.34 3.77 18.74 23.06 0.3
96-MB2 Type-1 eclogite 43.51 0.06 22.01 9.02 0.1
96-MB3C Type-1 eclogite 47.46 1.45 17.97 13.54 0.2
96-MB4 Type-2 eclogite 48.66 0.55 17.88 6.65 0.1
96-MB20D Type-2 eclogite 44.48 0.21 17.74 10.38 0.1
01-MB20 Type-1 eclogite 43.05 0.08 21.23 9.89 0.1
01-MB23 Type-1 eclogite 44.75 0.23 21.92 9.69 0.1
01-MB25 Type-1 eclogite 44.86 0.42 20.33 9.82 0.1
01-MB26 Type-1 eclogite 42.91 0.37 22.11 11.29 0.1
01-MB27 Type-1 eclogite 46.65 0.49 18.53 8.19 0.1
01-MB31 Type-2 eclogite 45.98 1.32 16.64 13.41 0.2
01-MB35 Type-2 eclogite 46.01 1.73 15.91 13.79 0.2
MB98-02 Banded eclogite 43.57
MB98-03 Omp-rich eclogite 46.17
MB98-04 Type-2 eclogite 43.99
MB98-08 Retrograde eclogite 44.34
MB98-19 Garnetite 43.32
D12 Type-1 eclogite 48.65 0.85 19.06 9.03 0.1
a Major oxides are expressed as wt.%.
garnetite layers from Type-2 eclogites developed
porphyroclastic texture with large porphyroclasts en-
closed in a fine-grained matrix (Fig. 6a). The latter
developed a foam structure where grain boundaries
are smoothly curved and aligned 120j triple junctions
(Fig. 6b). No coesite relicts were observed in either
garnet or omphacite from Type-2 eclogites, and quartz
occurs as elongated polycrystalline aggregates be-
tween fine-grained garnet/garnet, garnet/omphacite
or omphacite/omphacite grains. It is thus likely that
Type-2 eclogites resulted from dynamic recrystalliza-
tion of Type-1 eclogites along shear zones which were
active during the exhumation of the UHP metamor-
phic rocks.
3.2. TEM observations
A Philips CM200 transmission electron micro-
scope (TEM, GFZ-Potsdam) operating at 200 kV
was used to characterize the dislocation microstruc-
tures in the eclogites. Dislocation microstructures are
nty, Jiangsu Province
O MgO CaO Na2O K2O P2O5 Total Source
4.2 11.22 1.15 0.02 0.02 100.82 This study
3 12.86 11.57 1.21 0.05 0.03 100.45 This study
6.34 11.03 2.71 0.04 0.15 100.89 This study
2 8.1 15.61 1.48 0.05 0.09 99.19 This study
5 17.41 8.47 0.85 0.12 0.22 100.03 This study
5 14.61 10.11 0.85 0.02 0.03 100.02 This study
5 9.39 11.82 1.95 0.12 0.02 100.04 This study
4 10.87 12.14 2.01 0.07 0.02 100.68 This study
7 11.02 11.56 1.13 0.1 0.03 100.69 This study
1 10.73 12.6 2.66 0.16 0.02 100.14 This study
8 10.26 9.55 3.12 0.01 0.2 100.77 This study
7 10.2 9.42 3.13 0.02 0.08 100.56 This study
Kern et al.,
2002
Kern et al.,
2002
Kern et al.,
2002
Kern et al.,
2002
Kern et al.,
2002
4 8 12.57 0.88 0.19 0.25 99.62 Zhang et al.,
1994
S. Ji et al. / Tectonophysics 370 (2003) 49–7658
similar in garnets from both types of eclogites.
Garnets developed extensively regular dislocation
arrays and dislocation networks. The dislocation
arrays (Fig. 7a and b) can be interpreted as tilt
subgrain boundaries while the dislocation networks
(Fig. 7c and d) imply an activation of more than two
active slip systems. Those well-organized dislocation
microstructures indicate that diffusion-assisted recov-
ery mechanism such as dislocation climb and cross-
Fig. 9. Compositional profiles of pyrope (Prp), grossular (Grs), almandine (
lenticular garnets. (a) Sample 96-MB3C (Type-1 eclogite). (b) Sample 96-M
imageries.
slip efficiently occurred. Within the subgrains sur-
rounded by dislocation walls, free dislocations were
imaged with a density in the range from 1011 to 1012
m� 2 (Fig. 8a). Dislocation junctions, which are
complex intersections (tangles) of several disloca-
tions, were also observed in both types of eclogites
(Fig. 8b and c). The presence of dislocation junctions
indicates that dislocation interactions and conse-
quently the operation of multiple slip systems took
Alm) and spessartine (Sps) contents along two orthogonal profiles of
B4 (Type-2 eclogite). Sketch maps based on backscattered electron
S. Ji et al. / Tectonophysics 370 (2003) 49–76 59
place in the deformed garnet (Voegele et al., 1998;
Wang and Ji, 1999). The above observations agree
with previous TEM investigations on other naturally
deformed garnets (Ando et al., 1993; Ji and Mar-
tignole, 1994; Doukhan et al., 1994; Voegele et al.,
1998; Prior et al., 2000), all suggesting that the
garnet can be deformed plastically as long as tem-
perature, pressure, differential stress and strain rate
are appropriate.
4. Chemical compositions and the metamorphic
temperature
Major elements of 27 UHP eclogites collected from
the region were determined by the X-ray fluorescence
(XRF) in McGill University. The results of 12 repre-
sentative samples are listed in Table 1. Analytical
precision is better than F 1%. The UHP eclogites
Fig. 10. Compositional profiles (b and c) of pyrope, grossular, almandine
garnet porphyroclast (a) from Type-2 eclogite.
have significantly lower contents of K2O, Na2O and
SiO2 compared with typical basalts, indicating that
these relatively mobile components have immigrated
into fluids during the eclogitization. The above chem-
ical composition also reflects a fact that the UHP
eclogites, which have subjected to little retrograde
metamorphism, are mainly bimineralic aggregates of
garnet and omphacite and contains < 1–2% coesite
and/or quartz.
Chemical compositions of garnet and omphacite
were measured using a JEOL 8700 Super-probe,
with an accelerating voltage of 15 kV, a beam
current of 20 nA and a beam diameter of 5 Am.
Each estimation of elements was performed with 20 s
counting time on peaks and 10 s on background. The
precision in the chemical compositions is about
F 1%. Garnet composition varies from sample to
sample; such differences are related to differences in
bulk composition of protoliths. In one garnet-rich
and spessartine contents along profiles AB and CD of an elongated
Fig. 11. Plots of the KD values [Fe2 +/Mg)gt/(Fe2 +/Mg)px] of eclogite
samples versus the grossular content [XCa =Ca/(Ca + Fe +Mg+
Mn)] of garnet. Also shown are the 3.0 GPa isotherms of Ellis and
Green (1979, continuous lines) and Powell (1985, broken lines).
S. Ji et al. / Tectonophysics 370 (2003) 49–7660
layer and in one textural situation in the sample scale,
the garnet grains generally have nearly constant
compositions, varying only by F 3%. For example,
microprobe analyses of 209 garnet grains from sam-
ple 96-MB3C, which is a typical Type-1 eclogite,
yield the ranges of pyrope (38.7–44.5%), grossular
(30.7–36.0%), almandine (22.6–25.6%) and spes-
sartine (0.3–0.7%) with an average composition
Alm24.0F 0.5Prp41.7F 1.1Grs33.7F 1.1Spe0.5F 0.1.
Four typical lenticular garnet grains with length/
width ratios larger than 2 were selected from Type-1
eclogite for compositional X-ray maps of Mg, Ca and
Fe using the electron microprobe. These maps (not
illustrated here) show that each lenticular crystal is
rather homogeneous in compositions and do not
show any clear compositional zoning. Zoning pro-
files from rim to rim through the core were also
carried out along two mutually perpendicular direc-
tions which coincide with the major and minor axes
of several elongated garnet grains in the XZ sections.
These profiles (Fig. 9a) show only slight composi-
tional variations with respect to the uncertainties of
measurements, providing no evidence for the exis-
tence of compositional zoning in garnet grains from
Type-1 eclogites. The absence of compositional zon-
ing in the garnet grains from Type-1 eclogites can be
attributed to homogenization by diffusion at peak
metamorphic conditions (T>800 jC and P>3 GPa,
Zhang et al., 1994) and to the absence of effective
retrogression from the eclogite to granulite or am-
phibolite facies.
In Type-2 eclogites, most of garnet porphyroclasts
do not show significant compositional zoning (Fig.
9b) with some rare exceptions (Fig. 10). When the
compositional zoning occurs, it is characterized by a
relatively low pyrope component at both the center
and the rims while the variation of grossular compo-
nent is reverse (Fig. 10). Higher pyrope component
and lower grossular component occur between the
center and the rims. The almandine and spessartine
components remain generally constant. The zoning
pattern can be interpreted as growth zoning during the
exhumation of the UHP metamorphic terrane. Rapid
exhumation and resultant strain localization might
result in grain boundary migration of garnet and
formation of the compositional zones with distinct
pyrope and grossular components. The radial fractur-
ing around coesite inclusions in Type-1 eclogites and
recrystallization of Type-2 eclogites were probably
contemporaneous with this tectonic uplift. However,
omphacite grains are nearly homogeneous with jadeite
components of Xjd = 0.25–0.60 and show no specific
compositional distinction between these two types of
eclogites.
Equilibrium temperatures were estimated from the
empirical relationship between Ca-content in garnet
[XCa =Ca/(Ca + Fe +Mg+Mn)] and Fe–Mg partition-
ing (KD) between coexisting homogeneous garnet and
omphacite. KD is defined as the ratio of Fe2 +/Mg for
garnet to that for omphacite. Since the existence of
coesite pseudomorphs implies that the garnet and
omphacite assemblage was stable in the coesite sta-
bility field, the peak temperature can be estimated at a
pressure of 3 GPa using the garnet-clinopyroxene
geothermometers of Ellis and Green (1979) and
Powell (1985). These geothermometers generally give
reasonable temperature estimates with garnets of low
to medium grossular components (XGrs < 0.5, Koziol
and Newton, 1989). As shown in Fig. 11, the results
suggest that both types of the eclogites from Maobei
drilling site were equilibrated at the similar tempera-
ture range of 850F 50 jC, consistent with previous
Fig. 12. Garnet compositional variations in an old porphyroclast (profiles AB and CD) and the adjacent matrix of recrystallized new grains
(profiles EF and GH). Type-2 eclogite (sample 96-MB20D).
S. Ji et al. / Tectonophysics 370 (2003) 49–76 61
Fig. 13. Histogram showing density distributions of Type-1 and
Type-2 eclogites.
S. Ji et al. / Tectonophysics 370 (2003) 49–7662
estimates for eclogites from other localities of the Sulu
regions (Zhang et al., 1994).
Compositional variations of garnet relict porphyr-
oclasts and polygonal recrystallized grains were
investigated in sample 96-MB20D, which is a typ-
ical Type-2 eclogite. The results (Fig. 12) are
presented in terms of pyrope, grossular, almandine
and spessartine components. The line drawing (Fig.
12a), which was based on an electron backscattered
image, shows a typical site chosen for microprobe
measurements. The porphyroclast has a serrated
boundary, which is interpreted as the result of grain
boundary migration. The recrystallized matrix sur-
rounding the porphyroclast is characterized by a
mosaic of polygonal fine grains. The pyrope, gros-
sular, almandine and spessartine components display
no variations within the range of uncertainties of
microprobe measurements along two orthogonal
profiles AB and CD in the garnet porphyroclast
(Fig. 12b and c). Along profiles EF and GH, which
started from the rims of the porphyroclast and then
extended progressively to the recrystallized matrix, a
marked continuous decrease in pyrope component
and an increase in both grossular and almandine
components are detected while spessartine content
remains constant (Fig. 12d and e). The observed
tendency of compositional variations has two impli-
cations: (1) the dynamic recrystallization of garnet
took place during uplift of the UHP metamorphic
terrane with continuous decreasing in T and P; and
(2) the dynamic recrystallization of garnet in the
UHP eclogites, which probably occurred through
grain boundary migration, was driven by not only
dislocation strain energy but also by chemical-free
energy.
5. Density data
Densities of the eclogites were measured using
Archimedes methods at ambient conditions. The
densities obtained vary from 3.46 to 4.10 g/cm3
(Fig. 13). The Type-2 eclogites have an average
density of 3.76 g/cm3, which is higher than that
(3.54 g/cm3) of Type-1 eclogites. These mean den-
sities are consistent with the bulk densities of eclo-
gites from Dabie UHP belt (Kern et al., 1999), but
higher than those compiled by Rudnick and Fountain
(1995) (3.43 g/cm3) and Christensen and Mooney
(1995) (3.48 g/cm3).
6. Crystallographic preferred orientations
CPOs were measured on garnet, omphacite and
rutile using electron backscattered diffraction (EBSD),
JEOL JSM 5600 SEM, at Laboratoire de Tectonophy-
sique, Universite de Montpellier II. The CPO dia-
grams were projected in equal area and lower
hemisphere respect to the X, Y and Z directions of
the tectonic framework (Fig. 14).
6.1. Garnet CPO
Each EBSD measurement with more than two
hundreds of garnet grains shows that garnets from
both types of eclogites have weak strengths and
complex CPO patterns with numerous maxima of
h100i, h111i and h110i (Fig. 14). Bulk patterns of
those CPOs cannot be interpreted simply by assum-
ing the activation of any single slip system. The
complex patterns may result from multiple slip of
many systems such as those of 1/2 h111i {110},
{112} or {123}, h100i {010} and h100i {011}.
Activation of these slip systems has been documented
by previous deformation experiments of garnet single
crystals (Garem et al., 1982; Rabier et al., 1976;
Karato et al., 1995; Voegele et al., 1998; Wang and
Ji, 1999). We are not surprised by observing such
weak and complex CPOs for garnets because for a
Fig. 14. Stereographic projections (lower hemisphere equal area) of crystallographic preferred orientations of garnet, omphacite and rutile,
determined by EBSD system. X, Y and Z are defined in the text.
S. Ji et al. / Tectonophysics 370 (2003) 49–76 63
S. Ji et al. / Tectonophysics 370 (2003) 49–7664
given finite strain produced by dislocation slip,
crystals with more active independent slip systems
should develop more complex and weaker CPOs than
those with only single or two active slip systems.
During slip, an unconstrained crystal with five or
more independent slip systems changes its shape but
its lattice may subject to little rotation with respect to
the instantaneous stretching axes of bulk flow. Unlike
triclinic minerals such as plagioclase (Ji and Main-
price, 1988), the bcc garnet has high symmetry and
12 potential slip systems, there is a wide choice of
slip systems. The slip plane does not have to undergo
much rotation before the resolved shear stress
becomes high on another 1/2 h111i {110} slip
system, for example. Even though the slip occurs
predominantly on the {110} planes, it is important to
realize that three {110}-type planes intersect in a
[111] direction and screw dislocations with a 1/2
Fig. 15. Misorientation angle distributions (a) and pole figures of the miso
h111i Burgers vector may move at random on the
{111} planes with high resolved shear stress. Thus,
the weakness of the garnet LPOs cannot provide any
unequivocal evidence for diffusion creep or against
dislocation creep as a deformation mechanism of the
garnet grains in the UHP eclogites (Ji and Mar-
tignole, 1996).
Of note are the data of crystallographic misorien-
tation between two adjacent grains, which may pro-
vide some information for the prevailing deformation
mechanism (Mainprice et al., 1993; Jiang et al.,
2000). The distributions of minimum misorientation
(some times called disorientation) angles and rotation
axes between adjacent garnet grains are presented in
Fig. 15a and b, respectively. There is no clear
distinction between Type-1 and Type-2 eclogites. In
both types of eclogites, the rotation axes are almost
randomly distributed, with no special correlation with
rientation axes (b) of garnet grains in Type-1 and Type-2 eclogites.
S. Ji et al. / Tectonophysics 370 (2003) 49–76 65
the tectonic framework (X–Y–Z axes). The histo-
grams shown in Fig. 15a display a maximum fre-
quency at a disorientation angle of about 45j. For arandom distribution of cubic crystals such as garnet,
the distribution of disorientations has a maximum
peak at exactly 45j (Mackenzie, 1958). Hence, it is
further argument to say that these garnets have a very
weak CPO.
6.2. Omphacite
Both types of eclogites developed strong CPOs
(Fig. 14) with similar preferred orientations of [001],
which is subparallel to the stretching lineation (X).
Both [100] and [010] direction forms girdles perpen-
dicular to the lineation. However, the maximum con-
centrations of the [010] are different for Type-1 and
Type-2 eclogites. The [010] maxima are close to the
Z-direction for Type-1 eclogite while they are located
middle way between the Y and Z directions in the
plane normal to the lineation for Type-2 eclogite. The
omphacite CPO pattern of Type-1 eclogite is very
similar to those of so-called L-type eclogites subjected
to a constriction or coaxial extensional strain (e.g.,
Godard and van Roermund, 1995; Abalos, 1997;
Mauler et al., 2000). The omphacite CPO pattern of
Type-2 eclogite is similar to those observed by Abalos
(1997). Both patterns of the omphacite CPOs have
been reported for eclogites from Western Norway
(Boundy et al., 1992), Western Alps (Philippot and
van Roermund, 1992; Piepenbreier and Stockhert,
2001), Swedish Caledonids and Western France (God-
ard and van Roermund, 1995), NW Spain (Abalos,
1997) and for eclogites xenoliths from East Corolado
Plateau (Kumazawa et al., 1971).
The omphacite CPOs of eclogites (Fig. 14) can be
readily explained according to the recent viscoplastic
self-consistent (VPSC) numerical simulations of Bas-
cou et al. (2002). The simulations were made using
the slip systems observed by TEM in naturally de-
formed omphacite. Slip has been observed on 1/2
h110i {110}, [001] {110} and [001] (100) by van
Roermund and Boland (1981), Buatier et al. (1991), Ji
et al. (1993) and Godard and van Roermund (1995).
Type-1 eclogite has strong point maximum of [001]
with a density of 11.3 m.u.d. subparallel to the
lineation, a girdle of [010] in the YZ plane with a
maximum of 7.6 m.u.d. normal to the foliation (Z) and
more dispersed distribution of [100] in the YZ plane
with a maximum of 3.9 m.u.d. between Y and Z. Both
simple shear and pure shear simulations have these
general characteristics. Deformation of Type-1 eclo-
gite was probably in the constrictional field given the
prolate shape data for omphacite. Type-2 has stronger
point maximum of [001] with a density of 12.9 m.u.d.
subparallel to the lineation, a weaker girdle of [010] in
the YZ plane with a maximum of 6.0 m.u.d. between Y
and Z and stronger concentation of [100] in the YZ
plane with a maximum of 4.7 m.u.d. near Z. The
transtension simulation (Bascou et al., 2002) has these
general characteristics. The transtension used in the
simulation has a kinematic vorticity number of
Wk = 0.9, that is about 90% simple shear with a small
component of tension parallel to the lineation. The
shape data on omphacite for Type-2 is nearly plane
strain which is entirely compatible with a transtension
deformation.
6.3. Rutile
Rutile CPOs are shown in Fig. 14. [001] directions
of rutile in both types of eclogites are concentrated
near the lineation. As rutile is of tetragonal symmetry
where [100] and [010] axes are crystallographically
equal, those axes show similar patterns. [100] and
[010] in Type-1 eclogite show clear girdles perpen-
dicular to the lineation, whereas both these axes in
Type-2 eclogite show relatively dispersing fabric
patterns. Stoichiometric rutile has two principal glide
systems, h101i {101} is active above 600 jC and
[001]{110} above 900 jC (Blanchin et al., 1990).
However, [001] {110} has a critical resolved shear
stress that is twice as high as h101i {101}, hence is
difficult to activate at laboratory strain rates (Blanchin
and Faisant, 1979). As h101i {101} provides only
four slip systems, rutile is extremely difficult to be
fully plastic below 900 jC. Hence, it is likely that the
observed rutile CPO is due either to anisotropic
crystal growth or to the passive rotation of elongate
crystals in the ductile matrix.
7. Seismic wave properties
We calculated the seismic velocities (Vp is re-
ferred to P-wave velocity, and Vs1 and Vs2 are,
S. Ji et al. / Tectonophysics 370 (2003) 49–7666
respectively, the velocities of the first and second
arrived S-waves), shear-wave anisotropy [A(Vs)] and
polarization direction of Vs1 on the basis of the
CPO, density, volume fraction and elastic stiffness
coefficients of each constituent mineral. The elastic
stiffness coefficients of garnet, omphacite and rutile
are derived from Chai et al. (1997), Bhagat et al.
(1992) and Bass (1995), respectively. The seismic
velocities and anisotropies (Fig. 16) have been cal-
culated for each type of eclogite using the Voigt–
Reuss–Hill average. Both types of eclogites yield
comparable Vp anisotropies (1.4–1.5%) with similar
minimum (8.67–8.70 km/s) Vp and maximum
(8.79–8.84 km/s) Vp values. The maximum Vp
occurs at the direction subparallel to the lineation
while the minimum Vp occurs at a high angle to the
lineation. Kern et al. (2002) carried out laboratory
measurements on three fresh UHP eclogite samples
from the same locality as our samples and obtained
mean Vp values at 600 MPa ranging from 8.48 to
8.64 km/s and Vp anisotropies from 1.0% to 2.0%
(Table 2). Although the calculated and measured Vp
anisotropy values are almost the same, the calculated
zero-pressure Vp values of crack-free and retrogres-
sion-free eclogite aggregates are slightly higher than
those values measured at 600 MPa (Table 2). This
fact indicates that the calculated velocity actually
corresponds to a velocity measured at a pressure
above 600 MPa for eclogites. It is not surprising
because the critical pressure over which all pores and
cracks existent within hard rocks such as mantle
xenoliths and eclogites are closed at room tempera-
ture should be significantly higher than 600 MPa
(e.g., Christensen, 1965; Manghnani et al., 1974;
Kern et al., 1999; Wang and Ji, 2001).
Both types of eclogites have almost identical cal-
culated mean Vs1 (4.98–5.00 km/s) and Vs2 (4.96–
4.97 km/s) values, yielding weak Vs anisotropies
( < 1.5%). The low values of A(Vs) are mainly caused
by the volumical predominance of cubic garnet which
Fig. 16. Seismic properties of typical Type-1 and Type-2 eclogites
from the Sulu UHP metamorphic terrane. All the properties were
calculated for the zero-porosity and ambient conditions. Lower
hemisphere projections. Contours for P-wave velocity (Vp), fast S-
wave velocity (Vs1) and slow S-wave velocity (Vs2) are in km/s, S-
wave velocity anisotropy [A(Vs)] is in %. Vs polarization is
indicated by the trace of the fast S-wave vibration plane.
is elastically quasi-isotropic. The calculated values
(Fig. 16) are slightly higher than those values mea-
sured by Kern et al. (2002) at 600 MPa. They yielded
Table 2
Modal compositions, bulk densities and P- and S-wave velocities (at 600 MPa) of UHP eclogites from Maobei, Donghai, China
Sample Description Modal Composition Density Vp(km/s) A(Vp),
%
Vs(km/s) A(Vs),
%
Reference
MB98-02 Banded eclogite Grt57, Omp42, Rt0.6,
Phn0.2, Opq0.3
3.59 8.57 1.0 4.90 1.1 1
MB98-04 Fine-grained eclogite Grt39, Omp58, Hb1.5,
Phn1.0, Rt0.1, Ep.0.1,
Opq0.3
3.52 8.48 1.1 4.80 2.9 1
MB98-19 Garnet-rich eclogite Grt77, Omp14, Ms5,
Phn3, Qtz1
3.62 8.64 2.0 4.93 1.4 1
96-MB3 Coarse-grained eclogite Grt57.5, Omp39.2,
Rt1.5, Qtz1.8
3.54 8.73 1.4 4.97 1.4 2
96-MB4 Fine-grained eclogite Grt62.4, Omp33.7,
Rt2.9, Hb0.8, Opq0.2
3.76 8.77 1.5 4.99 1.3 2
1: experimental data from Kern et al. (2002); 2: calculated data from this study.
Abbreviations: Grt, garnet; Omp, omphacite; Rt, rutile; Phn, phengite; Hb, hornblende; Qtz, quartz; Ms, muscovite; Ep, epidote; Opq, opaques.
S. Ji et al. / Tectonophysics 370 (2003) 49–76 67
the eclogites mean Vs values ranging from 4.80 to 4.93
km/s at this pressure (Table 2). Vs1 fast polarization
directions, as shown in Fig. 16, are similar for Type-1
and Type-2 eclogites except at the Y-direction. The fast
polarization directions are subparallel to the X-direc-
tion for rays parallel to the XY-plane in Type-2 eclogite,
whereas those are oblique to the X-direction for rays
parallel to the Y-direction in Type-1 eclogite.
Fig. 17. Tentative P–T paths for Type-1 and Type-2 eclogites.
Type-1 eclogite deformed under the peak metamorphic conditions
within the wide subduction shear zone at the greater depth while
Type-2 eclogite resulted from reworking of Type-1 eclogite during
the exhumation along some localized narrow shear zones.
8. Discussion
8.1. Transition between constriction and plane strain
In the coarse-grained Type-1 eclogites, both garnet
and omphacite are of prolate shape (LHS), indicating
an apparent constrictional strain (e.g., Godard and van
Roermund, 1995; Zulauf, 1997). In the fine-grained
Type-2 eclogites, however, shapes of either garnet or
omphacite display a plane-strain (LS) which was most
likely related to a non-coaxial shear (e.g., Philippot
and van Roermund, 1992; Abalos, 1997) or trans-
tension as suggested here. It is interesting to discuss
the possible origin of these two types of eclogites.
Field observations show that the deformation fab-
rics of coarse-grained Type-1 eclogite and fine-grained
Type-2 eclogite were not coeval: the early coaxial
fabrics (LHS) were overprinted by the late simple
shear (LS) along the localized shear zones. This feature
implies that the variable microstructures of the UHP
eclogites were not due to heterogeneous and strongly
partitioned deformation—a mechanism proposed by
Henry et al. (1993) for the UHP rocks from the Dora–
Maira massif, Western Alps, Italy. Thus, the distinct
deformation fabrics of the Sulu UHP eclogites should
be formed at different periods of tectonic history and
most likely at different depths (Fig. 17).
S. Ji et al. / Tectonophysics 370 (2003) 49–7668
Systematic analyses of seismic focal mechanisms
led geophysicists to recognize three tectonic strain
regimes along subducting slabs (Isacks and Molnar,
1969, 1971): simple shear at shallow depths ( < 100
km), down-dip extension at intermediate depths
(100–400 km) and down-dip compression at deep
upper mantle depths (400–660 km). The boundaries
between these regimes correspond approximately to
those of phase transformations. At depths greater than
400 km, olivine of the subducting slab is transformed
to spinel while clinopyroxene progressively dissolves
into the garnet structure and finally eclogite complete-
ly transforms to garnetite. Both spinel and garnetite
are denser than olivine and eclogite, resultant negative
buoyancy causes an additional pulling force on the
subducting slab at 100–400 km depth. As the sub-
ducting slab is less dense than perovskite-dominant
lower mantle below the 660 km discontinuity, the
resultant buoyancy will resist against penetration of
the slab into the lower mantle. As a result, the
subducting slab is subject to down-dip compression
at 400–660 km depth. The non-coaxial strain regime
is prevailing along the boundary thrust shear zone
between the subducting slab and its overlying litho-
sphere at depth of the slab bend ( < 100 km). Although
eclogitization of crustal rocks such as amphibolite,
anorthosite and granulite-facies gneiss can start from a
depth of f 40 km, the transformation may not be
fully completed until a depth of f 80 km if the
materials are relatively dry (e.g., Austrheim, 1987;
Andersen et al., 1991).
Type-1 eclogites recorded an apparent constric-
tional strain which could be driven by a slab-pull
mechanism at the depth deeper than the slab bend
(f 100 km), whereas Type-2 eclogites recorded a
plane, non-coaxial strain, predominantly simple shear
which could take place a depths shallower than 100
km deep. This also reasonably explains why both
garnet and omphacite are coarser in Type-1 eclogites
than in Type-2 eclogites and why inclusions of coesite
pseudomorphs surrounded by radial fractures are
observed in Type-1 eclogites rather than in the
recrystallized matrix of Type-2 eclogites. If the above
conclusion is correct, Type-2 eclogites might be
reworked and recrystallized Type-1 eclogites from
shear zones resulted from strain localization during
the uplift of the UHP metamorphic rocks, possibly in
extension as indicated by the transtension interpreta-
tion of omphacite CPOs. It is thus reasonable to
assume that Type-1 eclogite was equilibrated above
the critical pressure for the quartz/coesite transforma-
tion while Type-2 eclogite was equilibrated near or
below this pressure. As the deformation temperatures
estimated from geothermometric mineral assemblages
for both types of eclogites are almost the same (Fig.
11) within the certainties of the geothermometers, the
initial uplift of the UHP metamorphic terrane ap-
peared to be nearly isothermal (Okay, 1993; Zhang
et al., 1994; Wang and Cong, 1999). The existence of
some zoning garnet grains from Type-2 eclogites may
indicate depressurization of these rocks. Furthermore,
the transition from plane, non-coaxial strain (L–S) to
constrictional strain (LHS) within the subducting
slab is believed to occur approximately at the depth
of the transformation of quartz to coesite (f 100 km).
This fabric transition depth, which may depend on
tectonic setting and geothermal gradient, varies from
region to region and may be as shallow as about
40 km depth (e.g., in central European Variscides:
Zulauf, 1997; south Norwegian Caledonides: Ander-
sen et al., 1991).
Previous TEM investigations of the bcc garnets
(e.g., Voegele et al., 1998) revealed that the disloca-
tion slip occurs on several planes, {110}, {111},
{112} and {123} but predominantly in the close-
packed h111i direction. The h111i dislocations are
extensively dissociated into two partials 1/2 h111i,between which a stacking fault is produced. An
extended screw dislocation cannot cross slip unless
the partial dislocations recombine into a perfect dis-
location. The greater the width of the stacking fault,
the difficult it is to produce constrictions in the
stacking fault. An increase in hydrostatic pressure will
tend to reduce partial dislocation separation and in-
crease the possibility of cross-slip (Poirier and Ver-
gobbi, 1978; Montardi and Mainprice, 1987). Because
recovery and recrystallization are two antagonist
(competing) processes, a decrease in hydrostatic pres-
sure due to tectonic exhumation will reduce the ability
of dislocations to cross-slip so that the dislocation
density rises and recrystallization occurs. This may
explain why recovery-accommodated creep is preva-
lent in garnet from Type-1 eclogites which deformed
likely at higher P (= 3.2 GPa), while recrystallization
occurs in garnet from Type-2 eclogite which deformed
likely at lower (P= 2.8 GPa, Fig. 17).
hysics 370 (2003) 49–76 69
8.2. Rheological contrast between garnet and om-
phacite
The studied UHP eclogites are typically two-phase
rocks that are mainly composed of garnet and ompha-
cite. Microstructural observations suggested that the
eclogites can be plastically deformed and are not as
rigid as thought previously. Moreover, plastic flow of
eclogites under UHP conditions may effectively fa-
cilitate channeled flow within the shear zone between
two lithospheric plates. The enhanced counterflow
within a wedge-shaped flow channel can force the
UHP metamorphic rocks to be rapidly exhumed. The
rapid exhumation in turn precludes effective heat
transfer from the surrounding mantle to the wedge,
rendering a cool thermal structure within the sub-
ducted crustal materials (5–10 jC/km, Fig. 17). This
makes the subducted crust possible to preserve the
mineralogic assemblages and deformation microstruc-
tures formed at UHP metamorphic conditions.
Our microstructural observations suggest that the
rheological contrast between garnet and omphacite
under the UHP conditions is lower than that com-
monly observed between garnet and clinopyroxene in
typical deep crustal rocks such as amphibolite or
granulite facies metamorphic rocks (e.g., Ji et al.,
1993). Garnet is most likely several times rather than
several orders stronger than omphacite in UHP eclo-
gites where both garnet and omphacite plastically
deform.
Using a Griggs apparatus, Jin et al. (2001) de-
formed hot-pressed quartz eclogite (50% garnet, 40%
omphacite and 10% quartz), garnet aggregate and
omphacite aggregate. They found that ‘‘the flow
properties of eclogite are very similar to those of
peridotite’’. However, garnet grains in their deformed
samples are extensively fractured rather than flattened,
indicating little plastic deformation of garnet. Eclo-
gites from the Sulu UHP metamorphic terrane show
remarkable evidence of plastic deformation: well-
developed foliation, pronounced stretching lineation
and deformation-metamorphism-induced, alternating
garnet-and omphacite-rich compositional layers (Fig.
2). Both garnet and omphacite grains are flattened and
elongated in the eclogites (Fig. 3). TEM observations
of deformed garnets from the UHP eclogites (Figs. 7
and 8) display well-organized dislocations and regu-
larly spaced subgrain boundaries. EBSD measure-
S. Ji et al. / Tectonop
ments demonstrated that garnet developed complex
CPOs. Furthermore, recrystallization-induced por-
phyroclastic texture is observed in Type-2 eclogites
(Fig. 6). The above observations indicate that garnet
grains in Type-1 and Type-2 eclogites deformed
viably by recovery- and recrystallization-accommo-
dated dislocation creep, respectively.
It is well known that the mechanical strength of a
material strongly depends on operating deformation
mechanisms (e.g., Stockhert and Renner, 1998; Wang
and Ji, 2000). For example, quartz is stronger than
feldspar when quartz deforms by dislocation creep
while feldspar by microfracturing and cataclastic flow,
whereas quartz is weaker than feldspar when both
quartz and feldspar deform by dislocation creep
(Dell’Angelo and Tullis, 1996). Jin et al. (2001)
experiments failed to duplicate the typical microstruc-
tures observed optically and with the TEM in natu-
rally deformed UHP eclogites. Deformation mecha-
nisms in their deformed samples are not the same type
as those operated in natural UHP eclogites from
former subducting slabs. Thus, the mechanical
strength data of the eclogite deformed in the non-
steady-state semibrittle regime cannot be reliably
extrapolated to the UHP eclogites deformed plastical-
ly at much lower natural strain-rate and temperature.
The UHP eclogites from the Sulu region contain
< 50% SiO2 (Table 1) and < 1-2% coesite or quartz
pseudomorphs as inclusions in strong minerals such
as garnet. However, the eclogite specimens studied by
Jin et al. (2001) contain of 10 wt.% intergranular
quartz. The quartz, which did not enter in the stability
field of coesite under their experimental conditions, is
the weakest phase in the eclogite samples and takes
the much greater part of the strain with reference to its
volume fraction. The addition of 10 wt.% quartz into
eclogites as intergranular ‘‘lubricant’’ results in con-
siderable weakening. Therefore, the ‘‘flow’’ strength
of quartz eclogite, reported by Jin et al. (2001), cannot
represent that of bimineralic (garnet and omphacite)
eclogites in the subducting slab.
8.3. Geophysical implications
Seismic reflectors have been observed in the upper
mantle beneath many areas of the world, for example,
the Northwest Territories of Canada (Cook et al.,
1999), the Abitibi–Opatica of the Canadian Superior
S. Ji et al. / Tectonophysics 370 (2003) 49–7670
Province (Calvert et al., 1995) and the north coast of
Scotland (Warner and McGeary, 1987; Warner et al.,
1996). These mantle reflectors are generally gently
dipping and extend from the Moho to at least 110 km
depth. The mantle reflectors display the following
characteristics: (1) Reflection coefficients (Rc) higher
than around 0.1 are needed to cause such reflections
within the upper mantle overlaid by the 40-km-thick
crust (Warner and McGeary, 1987). (2) Seismic
reflectors represent the sharp boundaries (Morgan et
al., 1994; Bostock, 1997). (3) Because seismic re-
flection methods have a vertical and horizontal reso-
lution of about 75 and 3000 m, respectively, at depths
of 40 km (assuming average crustal velocities of 6
km/s and a dominant frequency of 20 Hz), each
mantle reflector must be considered as a zone com-
posed of layered rocks with high impedance contrast.
Such a zone should be regionally extensive, have a
thickness of several hundreds meters to several kilo-
meters and have a sharp, well-defined, continuous
upper surface.
Several models, as discussed below, have been
proposed to interpret the origin of mantle reflections.
(1) Ductile shear zone. The deformed peridotites in a
mantle shear zone have developed strong CPOs of
olivine and pyroxenes and are thus anisotropic,
while the wall rocks are undeformed, have no
CPO and therefore isotropic. The boundary
between deformed and undeformed rocks can be
seismically reflective if the resulting reflection
coefficient is large enough (i.e., Rc >0.5–0.10).
Previous investigations (e.g., Kern et al., 1996; Ji
et al., 1994; Ben Ismaıl and Mainprice, 1998)
show that most of peridotites have a CPO-induced
P-wave anisotropy < 7% with an average value
of f 4%. A simple calculation, assuming that
both deformed and undeformed peridotites have
the same density, can readily demonstrate that the
reflection coefficient related to such an anisotropy
is generally < 0.03. Therefore, the boundary
between sheared (anisotropic) peridotites and
their undeformed (isotropic) protoliths cannot be
a candidate for the observed mantle reflections.
(2) Lithological interfaces between typical mantle
rocks. The presence of water-rich fluids may
cause the upper mantle partially melted. The melts
may crystallize into wehrlite, websterite and
pyroxenite, leaving a residue (harzburgite and
dunite) from partial melting. Although these
lithological units can be interlayered and suffi-
ciently thick (up to several hundred meters), the
boundaries between them will have low reflectiv-
ity for the following reasons: (a) Dunite and
pyroxenite have almost same density although
they are different in average P-wave velocity: 8.40
km/s for dunite and 7.94 km/s for pyroxenite (at a
confining pressure equivalent to 40 km depth,
Christensen and Mooney, 1995). The reflection
coefficient between these two rocks is thus
< 0.04. (b) The wehrlite, websterite and pyrox-
enite occur commonly as subvertical dykes or
veins (Wilshire and Kirby, 1989) which are
difficult to be imaged at mantle depths using
conventional reflection techniques. (c) Contacts
between the lithologic units may not be sharp
enough to be seismically reflective. Furthermore,
spinel lherzolite and garnet harzburgite have
almost the same density, same P-wave velocity
and same anisotropy. The reflection coefficient
between these two rocks is < 0.01. Thus, the
transition boundary from spinel to garnet in
peridotite should not be as reflective, as suggested
by O’Reilly and Griffin (1985).
(3) Transition zone between dislocation and diffusion
creep. Dislocation creep is considered to produce
CPO and thus anisotropy while neither diffusion
nor superplastic process can form CPO and
anisotropy (e.g., Karato and Wu, 1993). However,
the transition zone between the dislocation and
diffusion creep regimes does not cause the strong
reflectivity for the following reasons: (a) typical
maximum seismic anisotropies formed by dis-
location creep in the mantle rocks are f 3–5%
(Mainprice and Silver, 1993; Ji et al., 1994; Kern
et al., 1996; Ben Ismaıl and Mainprice, 1998;
Saruwatari et al., 2001). Even though the
assumption that no CPO is formed in the diffusion
regime is fully correct, the boundary between the
two regimes has a reflection coefficient < 0.02.
(b) Because the average grain size of olivine is
commonly larger than 0.5 mm, as demonstrated
by upper mantle xenoliths, dislocation creep
should be dominated over a thickness of at least
250–300 km (Ji et al., 1994). The transition zone
between dislocation and diffusion creep regimes
Fig. 18. Contents of garnet in HP (high pressure) and UHP
(ultrahigh pressure) eclogites. Data compiled from Birch (1960),
Boundy et al. (1992), Kern and Richter (1981), Kern et al. (1999,
2002), Mauler et al. (2000), Manghnani et al. (1974) and this study.
See Ji et al. (2002) for summary.
S. Ji et al. / Tectonophysics 370 (2003) 49–76 71
should not appear in the depth range of upper
mantle reflectors. (c) The transition zone between
dislocation and diffusion or superplastic creep
regimes may not be sharp enough to produce the
interface transition widths < 200 m required by
the seismic reflection data (Bostock, 1997).
(4) Metasomatized shear zones. Mantle shear zones
developed parallel to a subducting slab in the
mantle wedge above the subducting slab would
provide a favorable conduit for fluids to migrate
upwards. Under high temperature and high
pressure conditions, the fluids react with rocks,
forming seismically slower, less dense hydrated
minerals such as phlogopite and amphibole (e.g.,
Francis, 1976). If the concentration of these
hydrated minerals is higher than about 40% in
metasomatized shear zones, the boundary be-
tween the metasomatized shear zones and their
wall rock has impedance contrasts large enough to
be seismic reflective (Warner and McGeary, 1987;
Calvert et al., 1995). Then the metasomatized
shear zones should be low velocity zones.
However, studies of Morgan et al. (1994), Warner
et al. (1996) and Bostock (1997) suggest that the
mantle reflectors are most likely the faster and
denser layers embedded in the slower and less
denser rocks. Moreover, evidence from mantle
xenoliths (e.g., Francis, 1976) shows that the
concentration of hydrated minerals in metasom-
atized zones is typically only several percent and
much lower than the critical value needed for
causing mantle reflections. All the facts described
above exclude metasomatized shear zones from
the common candidates for the origin of mantle
reflectors.
(5) Boundary between eclogite and peridotite. Pre-
vious researchers (Morgan et al., 1994; Warner et
al., 1996; Calvert et al., 1995) believe that mantle
reflectors represent relict fragments of eclogitic
oceanic crust embedded within the subducted
lithosphere. However, this assumption has not
been fully supported by published petrophysical
data (Ji et al., 2002). According to Christensen
and Mooney (1995), laboratory measurements of
54 mafic eclogite samples at a confining pressure
equivalent to 40 km depth yield an average
density of 3.51 g/cm3 and an average P-wave
velocity of 8.19 km/s, while measurements of 51
peridotite samples under the same conditions gave
an average density of 3.33 and an average Vp of
8.40 km/s. These average values give a reflection
coefficient < 0.02 for the boundary between
eclogite and peridotite, making it unlikely a
candidate for the strong mantle reflectors. Thus,
Fountain and Christensen (1989), Gubbins et al.
(1994), Hynes and Snyder (1995) concluded that
eclogites transformed from mafic rocks are
indistinguishable in both densities and velocities
from peridotitic upper mantle.
S. Ji et al. / Tectonophysics 370 (2003) 49–7672
Eclogites are generally classified into high pres-
sure (HP) and ultrahigh pressure (UHP) ones that
are separated by the quartz-coesite equilibrium (e.g.,
Cong, 1996). The HP and UHP eclogites are also
called ‘‘cold eclogite’’ and ‘‘hot eclogite’’ (Chopin
et al., 1991), respectively. The UHP eclogites (Kern
et al., 1999; Kern et al., 2002; this study) have a
higher mean density and a higher mean Vp than the
HP eclogites (e.g., Fountain et al., 1994; Mauler et
al., 2000) because the first have higher contents of
garnet (Fig. 18) and lower contents of quartz,
amphibole, zoisite and mica than the latter. Thus,
mafic UHP eclogites are believed to be denser and
faster in Vp than typical peridotites while HP
eclogites have similar densities and velocities as the
peridotites.
Field and laboratory studies on lithology, defor-
mation structures and seismic properties of the
Dabie–Sulu UHP metamorphic terrane can provide
some important hints for understanding the origin of
mantle reflections. As stated above, the metamor-
phic terrane consists of interlayered pelitic and felsic
gneisses, quartzite, eclogite, garnet-peridotite and mar-
ble. All these rocks contain coesite as inclusions in
garnet, omphacite, jadeite and zoisite (Wang et al.,
1993; Cong, 1996; Zhang and Liou, 1996; Wang and
Cong, 1999). This suggests that all these rocks, which
could represent continental shelf limestone, quartzo-
feldspathic sandstone (grewacke) and mafic volano-
clastic sediments, were subducted into the upper
mantle at great depths (>90–100 km) and then tecton-
ically exhumed to the earth’s surface, during the
continental collision and post-collision extension. Gar-
net peridotite, on the other hand, may be from the
mantle wedge immediately overriding the subducting
slab.
The UHP eclogites are tectonic boudins since they
occur as pods, layers and blocks, ranging in size
from tens of centimeters to hundreds of meters,
within garnet-peridotite, metapelites (garnet-quartz-
jadeite gneisses), coesite-bearing quartzite and mar-
ble. All the rocks show well-developed foliation,
stretching lineation and compositional layering.
These foliations or compositional layers are generally
subparallel in ultramafic rocks, eclogite layers and
country rocks (gneisses, quartzite and marble), indi-
cating that in-situ contact relations between these
rocks were not considerably disturbed during tecton-
ic emplacement. When such a package of interlay-
ered crustal materials was once subducted and
remains in the upper mantle, a large reflection
coefficient (>0.10) should occur at interfaces be-
tween UHP eclogite or garnet peridotite and their
wall rocks such as quartzite, marble, pelitic and
felsic gneisses. Therefore, the regionally extensive
mantle reflectors probably indicate the preservation
of subducted crustal materials in the lithospheric
upper mantle.
9. Conclusions
The major conclusions of this study are listed
below.
(1) Eclogites from the Sulu region deformed plasti-
cally under the UHP metamorphic conditions and
are not rheologically rigid as thought previously.
Plasticity of eclogites under UHP conditions may
effectively facilitate channeled flow within the
interplate shear zone. The enhanced counterflow
within a wedge-shaped flow channel may force
the subducted crustal rocks to be rapidly ex-
humed.
(2) Observations of optical microstructures, petrofa-
brics and TEM structures suggest that the coarse-
grained (Type-1) and fine-grained (Type-2)
eclogites recorded two distinct plastic deforma-
tions: constrictional strain (LHS) in Type-1
eclogites while plane strain in Type-2 eclogites.
Omphacite, which could be only a few times
lower in flow strength than garnet, deformed
mainly by dislocation creep as demonstrated by
the occurrence of CPOs. Plastic deformation of
garnet in Type-1 eclogites was dominated by
recovery-accommodated dislocation creep as
testified by the pervasive presence of dislocation
walls and networks, whereas garnet in Type-2
eclogites was deformed by recrystallization-
accommodated dislocation creep as indicated by
the presence of porphyroclastic texture. As h111idislocations are commonly dissociated into two
partials 1/2 h111i in bcc garnet (e.g., Voegele et
al., 1998), the cross slip of h111i dislocations,
which is sensitive to the hydrostatic pressure,
may be the factor that controls the transition
S. Ji et al. / Tectonophysics 370 (2003) 49–76 73
from recovery-accommodated dislocation creep
at higher pressures (P>f 3.2 GPa) to recrystal-
lization-accommodated dislocation creep at lower
pressures (P <f 2.8 GPa). Thus, Type-1 eclo-
gites represent the subducted mafic rocks
deformed at the peak metamorphic conditions
while Type-2 eclogites resulted from recrystalli-
zation of Type-1 eclogites along some shear
zones which were active during the exhumation
of the UHP metamorphic rocks.
(3) It is widely accepted that the packages of inter-
layered eclogite, marble, quartzite, pelitic and
felsic gneisses from the Dabie–Sulu belt, which
were pieces of the continental crust, were
subducted to mantle depths greater than 80–100
km and then tectonically exhumed to the earth’s
surface (e.g., Cong, 1996; Liou, 1999; Wang and
Cong, 1999). Field and laboratory studies of these
UHP metamorphic rocks provided some impor-
tant hints for understanding the origin of mantle
reflections. As long as these interlayered UHP
rocks remain within the present upper mantle, the
interfaces between eclogite (or peridotite) and
their wall rocks such as quartzite, marble, pelitic
and felsic gneisses should be strong seismic
reflectors. The continuous boundaries between
garnet- and omphacite-rich layers or between
peridotite and garnet-rich eclogite layers can also
be seismically reflective. Thus, the regionally
extensive seismic reflectors from the upper
mantle may indicate the preservation of relict
crustal materials subducted within the continental
lithosphere.
Acknowledgements
S.C. Ji thanks the NSERC and LITHOPROBE of
Canada for research grants and the Alexander von
Homboldt Stiftung for a visiting fellowship. This is
LITHOPROBE contribution No. 1280. A. Lacombe
and C. Nevardo are thanked for drawing the figures
and for the polished thin sections for the EBSD
analysis, respectively. Crystal orientation measure-
ments were made with Laboratoire de Tectonophysi-
que EBSD/SEM system funded by grants from CNRS/
INSU and Universite Montpellier II (France).
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