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Transcript of The Origin of m Langes Cautionary Tales From Indonesia 2013 Journal of Asian Earth Sciences
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8/16/2019 The Origin of m Langes Cautionary Tales From Indonesia 2013 Journal of Asian Earth Sciences
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The origin of mélanges: Cautionary tales from Indonesia
A.J. Barber ⇑
Department of Earth Sciences, Royal Holloway, University of London, Egham, Surrey TW20 0EX, UK
a r t i c l e i n f o
Article history:
Available online 8 January 2013
Keywords:
Mélange
Mud diapirs
Mud volcanoes
Timor
Sumba
Nias
a b s t r a c t
The origin of block-in-matrix mélanges has been the subject of intense speculation by structural and tec-
tonic geologists working in accretionary complexes since their first recognition in the early twentieth
century. Because of their enigmatic nature, a number of important international meetings and a largenumber of publications have been devoted to the problem of the origin of mélanges. As mélanges show
the effects of the disruption of lithological units to form separate blocks, and also apparently show the
effects shearing in the scaly fabric of the matrix, a tectonic origin has often been preferred. Then it
was suggested that the disruption to form the blocks in mélanges could also occur in a sedimentary envi-
ronment due to the collapse of submarine fault scarps to form olistostromes, upon which deformation
could be superimposed tectonically. Subsequently it has proposed that some mélanges have originated
by overpressured clays rising buoyantly towards the surface, incorporating blocks of the overlying rocks
in mud or shale diapirs and mud volcanoes.
Two well-known examples of mélanges from the Banda and Sunda arcs are described, to which tectonic
and sedimentary origins were confidently ascribed, which proved on subsequent examination to have
been formed due to mud diapirism, in a dynamically active environment, as the result of tectonism only
indirectly. Evidence from the Australian continental Shelf to the south of Sumba shows that large quan-
tities of diapiric mélange were generated before the diapirs were incorporated in the accretionary com-
plex. Comparable diapirs can be recognised in Timor accreted at an earlier stage. Evidence from both
Timor and Nias shows that diapiric mélange can be generated well after the initial accretion process
was completed.The problem is: Why, when diapirism is so abundantly found in present convergent margins, is it so
rarely reported from older orogenic belts? Many occurrences of mélanges throughout the world to which
tectonic and/or sedimentary and origins have been ascribed, may in future investigations prove to have
had a diapiric origin.
It is emphasised that although the examples of diapiric mélange described here may contain ophiolitic
blocks, they were developed in shelf or continental margin environments, and do not contain blocks of
high grade metamorphic rocks in a serpentinous matrix; such mélanges originate diapirically during sub-
duction in a mantle environment, as previous authors have suggested.
2013 Elsevier Ltd. All rights reserved.
1. Introduction
When Greenly (1919) described a chaotic unit in the GwnaGroup of Anglesey as ‘mélange’, containing a variety of blocks of
ocean floor and continental shelf materials, such as spilitic pillow
lava and tuff, red jasper chert, manganiferous limestone, shale,
quartzite and grey limestone in a fine-grained matrix, it seemed
obvious that this mélange had been disrupted and sheared during
a process of tectonic deformation. Later Beneo (1955) described
extensive deposits of mélange in Sicily in the western Mediterra-
nean, which he interpreted as having been formed in a sedimen-
tary environment as the product of large-scale submarine
landslides. This interpretation has been used frequently to account
for the large-scale mélanges of the Argille Scagliose throughout
Italy. In the discussion following Beneo’s (1955) paper, Floresintroduced the terms olistostrome for these deposits, and olistoliths
for the included blocks. Although Hsü (1968, 1974) recognised tec-
tonic and olistostromal mélanges he suggested that the term
‘mélange’ should be restricted to those formed tectonically, in
practice, due to the difficulty of determining their origins, the term
has been used to describe all ‘block in matrix’ mélange deposits
worldwide, however they may have originated.
Subsequently both tectonic and sedimentary interpretations,
sometimes in combination, have been offered for many other
occurrences, especially where mélanges are found in association
with accretionary complexes, formed in subduction trenches from
oceanic material scraped off downgoing oceanic plates (e.g. Aalto,
1367-9120/$ - see front matter 2013 Elsevier Ltd. All rights reserved.http://dx.doi.org/10.1016/j.jseaes.2012.12.021
⇑ Tel.: +44 020 7228 1897.
E-mail address: [email protected]
Journal of Asian Earth Sciences 76 (2013) 428–438
Contents lists available at SciVerse ScienceDirect
Journal of Asian Earth Sciences
j o u r n a l h o m e p a g e : w w w . e l s e v i e r . c o m / l o c a t e / j s e a e s
http://dx.doi.org/10.1016/j.jseaes.2012.12.021mailto:[email protected]://dx.doi.org/10.1016/j.jseaes.2012.12.021http://www.sciencedirect.com/science/journal/13679120http://www.elsevier.com/locate/jseaeshttp://www.elsevier.com/locate/jseaeshttp://www.sciencedirect.com/science/journal/13679120http://dx.doi.org/10.1016/j.jseaes.2012.12.021mailto:[email protected]://dx.doi.org/10.1016/j.jseaes.2012.12.021http://crossmark.crossref.org/dialog/?doi=10.1016/j.jseaes.2012.12.021&domain=pdf
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1981; Cowan, 1985; Collins and Robertson, 1997; Ogawa, 1998;
Robertson and Pickett, 2000; Robertson and Ustaömer, 2011).
Meanwhile, geologists using seismic reflection profiling and dril-
ling for oil in deltaic deposits, frequently encountered salt diapirs
and shale diapirs containing block-in-matrix deposits in deltas on
passive margins, attributed to the mobilisation of salt and shale
units due to overpressure generated in areas with very high sedi-
mentation rates, e.g. Nile Delta (Loncke et al., 2006), Niger Delta(Morley and Guerin, 1996) Baram Delta (Morley et al., 1998; Mor-
ley, 2003). Shale diapirs are also encountered on active continental
margins, where the overpressuring and mobilisation of shales is
attributed to the stacking of thrust slices, e.g. Barbados (Brown
and Westbrook, 1988; Stride et al., 1982; Westbrook and Smith,
1983), the Makran (Stöcklin, 1990; Grando and McClay, 2007), Ara-
kan, Burma (Maurin and Rangin, 2009). Much effort has been ex-
pended in defining criteria by which tectonic, olistostromal and
diapiric mélanges might be distinguished (e.g. Barber et al., 1986;
Camerlenghi and Pini, 2009; Codegone et al., 2012b; Cowan, 1985;
Dilek et al., 2012; Festa et al., 2010; Festa, 2011; Lash, 1987; Or-
ange, 1985; Pini, 1999; Raymond, 1984; Silver and Beutner,
1980; Sengör, 2003; Wakabayashi, 2011).
Experience gained during study of mélanges regions of present
day active tectonics in the Outer Banda Arc and the Outer Sunda
Arc in Indonesia, to which both tectonic and olistostromal origins
have been attributed, but for which substantive evidence of diapir-
ism has been subsequently obtained, suggests that diapiric
mélange is much more common than many structural and tectonic
geologists have appreciated: Diapirism should be considered as an
origin for mélanges, before tectonism or submarine slumping are
automatically assumed.
2. Mélange in the Outer Banda Arc
The island of Timor in eastern Indonesia, just to north of Austra-
lia, forms part of the Outer Banda Arc ( Fig. 1). The island was
formed from Australian Precambrian basement and continental
margin sediments, ranging in age from the Permian to the Pliocene,
imbricated in accretionary complexes and thrust beneath an ophi-
olite nappe, during the collision between the northern continental
margin of Australia and the Banda Volcanic Arc (Barber et al., 1977;
Charlton et al., 1991). The eastern part of Timor (Timor Leste) was
mapped geologically by Audley-Charles (1968), and the strati-
graphic units he established were later adopted by the IndonesianGeological Survey when they mapped the western part of the is-
land (Rosidi et al., 1981) (Fig. 2). During the mapping Audley-
Charles (1965, 1968) recognised an extensive mélange deposit,
the Bobonaro Scaly Clay, containing a variety of blocks in a scaly
clay matrix (Fig. 3) which, following Beneo (1955), he interpreted
as olistostromes, the product of large-scale submarine slumping.
This interpretation was accepted by Hutchison (2007) in his ac-
count of the geology of Timor in the textbook Geological Evolution
of South-east Asia (p. 58).
Audley-Charles (1968) and Carter et al. (1976) regarded the
Bobonaro Scaly Clay as a distinct stratigraphic unit, formed at a
specific period of time, Early Pliocene, N19-20 in Blow’s (1969)
foraminiferal zonal scheme, although Pleistocene forams were
identified in the scaly clay matrix, these were interpreted as being
incorporated by soil creep from overlying raised coral reefs. They
visualised that slumping had occurred by the collapse of submar-
ine fault scarps developed in the accretionary complex, with the
deposition of the blocks into adjacent troughs, where deep-water
clays, which now form the scaly clay matrix, were being deposited.
These escarpments were formed as the result of thrusting during
the subduction/collision between the northern margin of the Aus-
tralian continent and the Banda Arcs.
Later, Hamilton (1979) visited West Timor and described and
illustrated the Bobonaro Scaly Clay Mélange. In the outcrops that
he visited, Hamilton observed that the fabric of the scaly clay ma-
trix had a predominantly northerly dip and suggested that the
mélange had been generated tectonically by southerly-directed
118°E 120° 122° 124° 126° 128° 130° 132° 134°
8°
10°
6°S
12°
14°
118° 120° 122° 124° 126° 128° 130° 132° 134°
Sumba
Savu
Semau
Timor
Tanimbar
Aru
Kai
Banda
V o l c a n i c
A r c
BANDA SEA
Darwin
AUSTRALIA
INDIANOCEANFLOOR
AUSTRALIAN MARGINAL SEDIMENTS
A U S T R
A L I A N
C O N T
I N E N T A
L S H E
L F
1 0 0 0 m 5
0 0 0
m
d e f o r m
a t i o n f r o
n t b a c k t h r u
s t
Accretionary and Collisional Complex
Active mud volcano fields
Volcanic Ar c
6°
8°
10°
12°
14°
1000m
FLORES SEA
Fig. 1. The Banda Arcs Eastern Indonesia, with the island of Timor formed by the collision between the northern margin of Australia and the volcanic arc showing thedistribution of active mud diapirs and mud volcanoes around the Outer Arc (Barber and Brown, 1988).
A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438 429
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overthrusting, during the collision between the northern Austra-
lian margin and the Banda Arc.
Subsequently, in a geophysical cruise in Eastern Indonesia by
the Hawaiian Institute of Geophysics, the Research Vessel KanaKeoki surveyed the Timor accretionary complex and the Australian
Continental Shelf to the south of Timor. The survey mapped the
bathymetry, recorded seismic profiles and used the side-scan sonar
SeaMarc II system (Blackington et al., 1983) to image the Timor
slope, the Timor Trough and the northern part of the Australian
shelf. The seismic section showed that sediments from the Timor
Trough and the Australian margin had been uplifted into the accre-
tionary complex along bedding parallel thrust planes which stee-
pen toward the surface and generate fault-bend folds in the
overlying sediments (Karig et al., 1987) (Fig. 4). Earlier, Upper Pli-
ocene to Recent sediments had been drilled in DSPD 262 on the
floor of the Timor Trough and showed that sediments on the floor
of the trough, to a depth of 400+ m, consist of unlithified radiolar-
ian and clay-rich nanno ooze (Heirtzler et al., 1973). The SeaMARCII side-scan imagery showed fault scarps, both on the Australian
margin and on the Timor slope, together with slumps, débris and
mud flows and sediment-filled slope basins (Fig. 5), as postulated
by Audley-Charles (1965), but the seismic section shows that the
surface of the Australian slope and the accretionary complex is
composed only of recently deposited soft sediments of Pliocene
to Recent age, with no major fault scarps uplifting the underlying
continental shelf sequence from which blocks of lithified sedi-
ments could be derived, to form olistostromes, as postulated by
Audley-Charles (1965, 1968) to account for the Bobonaro Scaly
Clay Mélange on Timor.
A similar survey was conducted by the R.V. Kana Keoki furtherwest, to the south of the island of Sumba, across the accretionary
complex, the trench and the Australian margin (Breen et al.,
1986). SeaMARC II side-scan sonar imagery, together with bathym-
etry and seismic reflection profiling, showed that the surface of the
sea floor on the Australian continental shelf, immediately to the
south of the deformation front of the accretionary complex, is cov-
ered by mounds and ridges (Fig. 6). Neither the side-scan sonar
imagery nor the seismic profiles show any large-scale fault scarps
in the accretionary complex; the upper slopes of the complex are
covered by a thin drape of undisturbed Recent sediments, and
are devoid of structural features (Breen et al., 1986, Fig. 7). Seismic
sections obtained south of the deformation front show that at
intervals of 10 km or so, the regular horizontal reflections in the
bedded sedimentary sequence are disrupted by transparent zones,devoid of reflections, capped by the mounds on the sea floor. These
transparent zones are interpreted as vertical mud diapirs and the
mounds are interpreted as mud volcanoes (Fig. 6).
Breen et al. (1986) correlated the sequence represented in the
profiles with the undisturbed Australian continental marginal se-
quence encountered in boreholes on the Scott Reef ( Rad and Exon,
1982). The deepest reflection (E) is identified as the top of the clas-
tic sequence, which marks the break-up unconformity in the pas-
sive margin of the NW Australian Shelf. A transparent zone
between (E) and (C) is identified as Lower Cretaceous hemipelagic
marine shale deposited on the subsided ocean floor. Overlying
reflectors between (E) and (A) are identified as lithified Upper Cre-
taceous to Miocene pelagic carbonates, with interbedded marls,
deposited on a prograding carbonate shelf, and the zone from (A)to the surface, as Pliocene to Recent pelagic marls. The vertical
124°E 125° 126° 127°
5°
10°
127°126°125°124°E
5°S
10°
0 10 20 30 40 50km
WEST TIMOR
EAST TIMOR
KupangKolbano
Dili
Post-collision Units
Bobonaro Scaly Clay
Pre-Collision Units
Late Miocene-Recent
Permian-Late Miocene
Melange &mud volcanoes
Fig. 2. Geological map of Timor, Eastern Indonesia, showing the extent of the Bobonaro Scaly Clay Mélange: East Timor (Timor Leste) from Audley-Charles (1968); West
Timor from Rosidi et al. (1981).
Fig. 3. Landscape in West Timor with scattered blocks of a variety of lithologies,
some the size of houses, due to the erosion of the clay matrix from an outcrop of
Bobonaro Scaly Clay Mélange.
430 A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438
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transparent zones seen in the seismic sections rise from the level of
the Lower Cretaceous shale at a depth of 1.5 km, and cut across the
bedded reflectors to the base of the surface mounds (Fig. 6). In
passing through the overlying bedded sequence the mobilised clay
is likely to have incorporated blocks of the lithified carbonate units
to form a mélange of Upper Cretaceous to Miocene limestone
blocks in a hemipelagic clay matrix. Scattered occasional reflec-
tions in the transparent zones may from larger blocks. The largest
of the ridges on the sea floor is 200–300 m high, 18 km long with a
width of 2.5 km and extends to a depth of 1.5 km, representing avolume of 70 km3 of mélange.
A subsequent survey by the R.V. Charles Darwin using the GLO-
RIA side-scan sonar system showed that the diapir field extends
over an area of 100 km 50 km on the Australian continental shelf
(Masson et al., 1991). The seismic sections show that continental
margin sediments incorporating the diapirs and the mud volca-
noes, including many hundred cubic kilometres of mélange, are
in the process of incorporation into the toe of the accretionary
complex (Fig. 6).
Westbrook and Smith (1983), in a comparable situation in
Barbados, where mud diapirs and mud volcanoes occur in OrinocoFan sediments on the oceanward side of the deformation front,
passive margin
sediments
syn-rift sediments
br eak -up unc onf or mity
AUSTRALIA TIMORSE NW
2.0
3.0
4.0
5.0
6.0
s e c o n d s t w o - w a y t i m e
2.0
6.0
5.0
4.0
3.0
s e c on d s
t w o-w a y t i m e
0 10 20km
trough fill
slope sediments deformation front
Australian slope Timor TroughTimor slope
Pliocene-Recent
Upper Jurassic - Miocene
Permian -Upper Jurassic
Fig. 4. Interpreted seismic section from the Australian continental shelf across the Timor Trough and the Timor accretionary complex showing that only the most recent
sediments are exposed; the shelf sequence is not exposed and cannot provide blocks to form olistostromes (Karig et al., 1987).
sediment lobes
T I M O R
S L O P E
A U S T
R A L I A
N S L
O P E
1000m
1700
1700
2300
2300
2000
1600
1600
600
1000
1500
1800
1800
2000
2300
2300
2000
124°00’123°45’
123°45’E 124°00’ 124°15’
10°30S
10°45’
11°00’
10°30’
10°45’
11°00’
0 10 20km
floor of Timor Trough
deformation front (inactive)
slump scars
slope basins
normal faults
deformationfront (inactive)
turbiditechannels
anticlines
normal faults
back thrust
Fig. 5. Interpretation of SeaMARC II imagery of the accretionary complex south of Timor shows slumping of soft sediment from the most recent deposits from the Timor
Trough, with no olistostromes containing blocks derived from the underlying continental margin sequence (reinterpreted after Charlton (1987) and personal communication
2012). N.B. The subduction system in the Timor Trough is no longer active. GPS measurements show that Timor Island is accreted to the Australian Plate and is moving NE-
wards at 7.7 cm/yr together with Australia (Genrich et al., 1996).
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before they were activated by the overpressure generated by the
accretion process.
During mapping in West Timor the Geological Survey of Indone-
sia identified twenty-one mud volcano fields and cross-cutting
mud diapirs, intruded through the other rocks, as the Bobonaro
Scaly Clay Mélange (Rosidi et al., 1981) (Fig. 2). In the Kolbano area,
and in other areas in the southern part of the island, imbricated
and folded Late Cretaceous to Miocene carbonates, form a Late Ter-tiary accretionary complex and are cut by mud diapirs composed of
red scaly clay containing manganese nodules and blocks of Late
Cretaceous to Miocene limestones, forming a mélange (Barber
et al., 1986, Fig. 2). Hydrofracturing of the blocks, with films of
the matrix injected along joints and fractures indicate that the
mud matrix in the diapirs was overpressured (Barber et al., 1986;
Barber and Brown, 1988). Yassir (1987) has demonstrated experi-
mentally that the fabric in scaly clay matrix in mélanges develops
in overpressured clays, without the addition of superimposed
shearing.
The Cretaceous to Miocene limestones and the accompanying
mélange in Kolbano and other areas in the southern part of Timor,
correspond to the Australian marginal sediments and diapirs south
of Sumba, which were incorporated at an earlier stage in the island
arc-continental collision, along a décollement at a level near the
break-up unconformity. There are no active mud volcanoes in this
part of Timor, evidently the diapiric system is now inactive. The
collision commenced in the region of East Timor, and has since ex-
tended to both east and west.
In the island of Semau (Barber et al., 1986) (Fig. 8) and in other
areas in the northern part of Timor (Fig. 2), active mud volcano ex-
trude fluid mud and bubbles of methane and have an oily scum on
the surface of mud pools. Mud in the volcanoes and scaly clay in
the diapirs were derived from Permo-Triassic red shale horizons
and carry blocks of Permo-Triassic sandstone and limestone (Figs. 9
and 10). Evidently, the Permo-Triassic rocks were uplifted into the
accretionary complex from a décollement surface near the base-
ment unconformity with the Australian basement in a process of
underplating (Charlton et al., 1991). Hutchison (2007, p. 320), fol-lowing Audley-Charles (1968), noted that ‘ultramafic’ rocks are
also included in the mélange, showing that some of the diapirs
had intruded the overlying ophiolite nappe. Other diapirs and
mud volcanoes contain blocks of reef material and were intruded
through Pleistocene coral reefs (Barber et al., 1986). The evidence
from the incorporation of the coral blocks and active mud volca-
nism, indicates that compression, overthrusting and the generation
of fluid overpressures continues within the collision complex in the
northern part of Timor to the present day.
Diapirs and active mud volcanoes occur extensively on all the
Banda Outer Arc islands between Timor and Seram (Fig. 1). The
process of the formation of mélanges must be occurring on a very
large scale today as the result of the collision between Australiaand the Banda Arcs.
Fig. 8. The mud volcano field showing small-scale mud volcanoes up to 3 m high,
with fluid mud flows and scattered blocks, in the crater of the 1 km diameter large
mud volcano forming Palau Kambing, SW of Kupang, West Timor. The crater wall in
the background is littered with blocks. The soft clays are eroded during the rainy
season and washed out through a gap in the crater wall (see Barber et al., 1986,Fig. 3).
Fig. 9. Cross-section of a mud diapir containing lensiod and irregular blocks of
limestone and sandstone in a scaly clay matrix in roadside quarry, near Takari, West
Timor. The matrix is intruded along fractures in the blocks, indicating high
overpressures, and the foliar structure of the scaly clay matrix is attributed to flow
rather that to shearing.
Fig. 10. Bedded block of Permian sandstone in varicoloured scaly clay matrix
derived from Permo-Triassic red marls in a mud diapir, exposed by river erosion in
the Noil Toko, near Nenas, West Timor. Patrick Bird provides scale. The location is
shown in Fig. 4 of Barber et al. (1986). (For interpretation of the references to colour
in this figure legend, the reader is referred to the web version of this article.)
A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438 433
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3. Mélange in the Outer Sunda Arc
Outcrops of mélange were mapped in the outer arc islands of
Nias, Simeulue, Siberut, Sipora and Pagai, associated with subduc-
tion of the Indian Ocean floor beneath Sumatra. (Andi Mangga and
Burhan, 1994; Budhitrisna and Andi Mangga, 1990; Endharto and
Sukido, 1994). The mélange contains blocks of serpentinite, gabbro,
basalt, chert, calcilutite, Eocene limestone with foraminifera, gra-nitic and metamorphic rocks together with abundant greywacke
shale and claystone in a scaly clay matrix.
In the 1970s the Scripps Institution of Oceanography (SIO) ob-
tained seismic sections from the Indian Ocean floor, the Sunda
Trench and the Outer Arc Ridge to the SW of Sumatra ( Moore
and Curray, 1980) (Fig. 11A). Karig et al. (1980) made a detailed
study of the trench and the accretionary complex from the SIO
seismic profiles, and then completed a series of traverses across
the Outer Arc Ridge where it is exposed on the island of Nias
(Moore et al., 1980b; Moore and Karig, 1980). On Nias the mélange
deposits, termed the Oyo Complex, occur as a series of NW–SE
trending linear belts parallel to the length of the island, several
hundred metres wide and kilometres in length, alternating with
bedded turbidites of Early Miocene to Early Pliocene age, termed
the Nias Beds (Fig. 12).
In the early 1990s Nias Island was mapped in detail by Samuel
(1994; Samuel et al., 1997) (Fig. 12) with the ages of the rocks very
tightly controlled by detailed microfossil analysis, supported by
petrographic, mineralogical and geochemical analyses. In particu-
lar a systematic study was made of the Oyo Mélange and the rela-
tionships to the bedded units.
From their study of the seismic sections, Moore and Karig
(1976) and Karig et al. (1979) developed a model for the evolution
of the accretionary complex, the development of the forearc ridge
and the geology and structure of Nias. They speculated that the
Oyo Mélange was developed as a trench-fill deposit composed of
fragments of ocean crust and turbidites which slumped down the
face of the accretionary complex as debris flows (olistostromes)
and were subsequently accreted at the toe of the complex (Mooreand Karig, 1980). Further debris flows were derived from fault
scarps developed on the NE side of slope basins formed on top of
the accretionary complex. The resolution of the 1970s seismic
reflection imaging was not sufficiently clear to either confirm or
contradict these interpretations (Fig. 11). Neither debris flows
nor diapirs are seen in the seismic profiles across the Sunda Trench
(Fig. 11A and B). It may require swath mapping or 3D seismic sur-
veys across the trench and the accretionary complex to identify
such flows (e.g. Gee et al., 2007). Karig et al. (1979) further specu-
lated that the chaotic and sheared appearance of the mélange was
due to the dynamic tectonic environment within the developing
accretionary complex, in which original thrust surfaces were con-
tinually reactivated, with the development of new thrust planes,
disrupting the accreted oceanic material and breaking it into
blocks. They were unable to determine the age of the mélange di-
rectly, but inferred that the age was indicated by the youngest
dateable included blocks, the Eocene limestones.
Although no depositional contacts were observed, Moore et al.
(1980a) and Moore and Karig (1980) suggested that the Oyo
Mélange was the oldest unit on Nias, on which the Nias Beds were
deposited unconformably. They suggested that the Nias Beds had
0
1
2
3
4
5
6
NEsecondstwo-way-time
SUNDA TRENCH
Deformation front
Indian Ocean Crust
Accretionary Complex
Outer Arc RidgeMentawai Fault Forearc Basin
0 10 20km
Vertical exaggeration 6.1 X
2000
3000
4000
5000
6000
7000
8000
9000
10000
11000
D e p t h i n m
26 28 30
Distance along profile in km32 34 36 38 40
(A) Nias Transect
(B) South Sumatra Transect
42 44 46 48 50 52 54 56 58 60 62 64 66 68
Indian Ocean Crust
Deformation front
Accretionary Complex
Outer Arc Ridge
NE
SW
SW
SUNDA TRENCH
Vertical exaggeration 1.5 X
slope basins
Fig. 11. (A) NE–SW line drawing from seismic profile to the south of Nias, from the Indian Ocean Floor across the Sunda Trench, the accretionary complex and the Outer Arc
Ridge to the Sumatran Forearc Basin (redrawn from Moore et al. (1980b)). (B) NE–SW line drawing from a seismic section offshore South Sumatra. The original section is inKopp and Kukowski (2003).
434 A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438
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been deposited in slope basins on the accretionary complex and
were uplifted and compressed during thrusting, with the growth
of the complex, until they were exposed in Nias.
On the other hand Samuel et al. (1995) found that the bedded
sediments on Nias had been deposited in basins developed on
top of the accretionary complex, bounded to the NE by syn-depo-
sitional extensional faults. They also found that the Upper Palaeo-
gene and Neogene stratigraphic sequences on Nias correspond
with the same sequences in the Banyak and Batu islands, which
lie within the forearc basin to the northeast of Nias, and also in
boreholes in the forearc basin itself. These sequences resemble in
stratigraphy and lithology the units on Nias. Samuel et al. (1995)
therefore concluded from the occurrence of well-rounded quartzpebbles and metamorphic clasts, in the Oligocene and Lower
Miocene sandstones and conglomerates, that the sediments on
Nias were derived from a mature continental provenance, either
basement uplifts in the forearc or the mainland of Sumatra, and
that prior to the Pleistocene, sedimentation extended continuously
from Sumatra across the present forearc basin onto the outer arc
islands, and do not correspond to the deposits in the Sunda Trench.
Samuel (1994) found that in addition to ophiolitic material, ser-
pentinite, gabbro, basalt, calcilutite and chert of ocean floor prove-
nance, at least 50%, and commonly 90% of the blocks in the
mélange had been derived from the bedded Oligocene and Lower
Miocene units, while some outcrops contained clasts of Upper Mio-
cene and even Pleistocene units. He also found that the mud matrix
contained the same microfossils, had the same mineral composi-tion and the same thermal history, yielding the same range of
reefs
reefs
reefs
Gunungsitoli Formation (Plio-Pleistocene)
Ophiolitic basement (B)
C
1°00
1°15'
1°30'N
97°45'97°30'97°15'E
97°15'E 97°30'
1°00'
0°45'
B
B
B
B
B
GUNUNG- SITOLI
TELUKDALAM
Fault
Anticline
Syncline
Lineament
Thrust
Alluvium
Oyo Mélange (blocks in scaly clay)
* Mud volcanoes
))
0 10 20km
Gomo Formation )
Lelematua Formation
Conglomerate Member (Late Oligocene-Early Miocene)
'Nias Beds' (Early Miocene-Early Pliocene)
*
*
1°15'
97°45'
B
C
B
B
B
C
I N D I A N O C E A N
Pagai
S U M A T
R A
6°N 6°
0° 0°
6°6°S
200km100°
100°E
S u n d a T
r e n c h
Simeulue
NIAS
Siberut F i g
. 1 1 A
SUMATRAN FOREARC
F i g . 1 1 B
Fig. 12. Geological and structural map of the Island of Nias, Outer Arc, showing outcrops of the Oyo Mélange and the location of mud volcano fields. Locations marked ‘B’ are
outcrops of coherent ophiolitic basement, in contrast to ophiolitic blocks in the mélange (based on Djamal et al. (1994) and Samuel (1994)). The thrusts shown on the SW side
of the mélange outcrops may not be correct, see text. Inset map shows location of Nias in the Sumatran Forearc and the position of the seismic lines in Fig. 11A and B.
A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438 435
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vitrinite values, as mudstones in the Oligocene to Lower Miocene
succession.Samuel (1994) found that the scaly fabric that pervades the
mélange matrix is commonly vertical, but may be folded and
wrapped around the enclosed clasts, and at the contacts, the fabric
is parallel to the margins of the mélange outcrop (Fig. 13). Karig
et al. (1980) observed that as mélange units are traced along strike
they are in contact with different units of the Nias Beds, and are
sheared and mixed into the mélange. But as we have seen already,
a shearing process is not necessary to impart the scaly fabric to the
clay matrix of the mélanges (Yassir, 1987). Karig et al. (1980) inter-
preted these contacts as high angle reverse faults. However, Sam-
uel et al. (1997) observed that the contacts between the mélange
and the adjacent bedded units are always intrusive, with the ma-
trix penetrating along the bedding planes and fractures in the bed-
ded units. If these observations are correct, the thrusts shownalong the SW margins of the mélange outcrops in geological map
(Fig. 12) are probably erroneous. The mélange was observed to
cut units of all ages from Oligocene to Recent. It appears that the
main period of mélange formation occurred during the Pliocene,
but mélange production continues to the present day, as shown
by the eruption of mud volcano fields (Fig. 12), extruding blocks
in a grey mud slurry, identical in composition and ages to the ma-
trix of the mélange.
Similar mélanges, have been mapped on the other Sumatran
Outer Islands of Simeulue, Siberut, Sipora and Pagai, commonly
with circular outcrops, and associated with active mud volcanoes
(Endharto and Sukido, 1994; Andi Mangga and Burhan, 1994;
Budhitrisna and Andi Mangga, 1990). Evidently as in Timor and
the other island of the Outer Banda Arc System, the outer arc ridge
in the Sunda Arc system continues to be compressed, causing over-
pressure and the mobilisation of clays to form mud diapirs and
mud volcanoes.
4. Conclusions
Contrary to the hypothesis of Audley-Charles (1965), evidence
from Sumba and Timor indicates that there are no débris flows
containing continental shelf blocks, associated with the develop-
ment of the accretionary complex forming at the present day,
which could account for the Bobonaro Scaly Clay Mélange on Ti-
mor. Evidence from Sumba indicates that large volumes of
mélange, in the form of diapirs, were generated by overpressured
fluids in the Australian continental marginal sediments, beforethey were incorporated into the accretionary complex. The
experimental work of Yassir (1987) shows that the presence of a
scaly clay fabric does not necessarily indicate tectonic deformation,
as Hamilton (1979) assumed. However, it is possible for deforma-
tion to be superimposed on mélanges after accretion has ceased,
e.g. Barber et al. (1986) describe mélange sheared along strike-slip
faults in West Timor, and Harris et al. (1998) has suggested that the
mélanges occur along the base of major thrusts developed during
the progress of the collision. It may be that the diapiric mélangeshave provided weak zones along which the thrust planes were
developed. Evidence from Timor and the islands to the east, indi-
cates that compression and thrusting to produce overpressure,
with the formation of mud diapirs and mud volcanoes in the Outer
Banda Arc, due to the collision with Australia, continues to the
present day.
The seismic sections across the Sunda Trench, the accretionary
complex and the Outer Arc Ridge offshore Sumatra show no evi-
dence of mud diapirism from the Nicobar Fan sediments on the In-
dian Ocean floor (Fig. 11A and B), in contrast to the Northwest
Australian Shelf south of Sumba, where the sequence contains a
permeable clastic sequence overlain by impermeable clays which
could be mobilised by overpressures generated by the loading of
the accretionary complex. Although the presence of débris flows
in the Sunda Trench or in slope basins on the developing accretion-
ary complex in the Sunda Arc system, as proposed by Karig et al.
(1979), nor the disruption and break-up of units by thrusts within
the accretionary complex, cannot definitely be ruled out, Samuel’s
(1994; Samuel et al., 1995, 1997) study of the geology of the island
of Nias has shown conclusively that these processes were not
responsible for the formation of the mélanges on Nias. Samuel
(1994) found that the Oyo Mélange Complex was formed as mud
diapirs within extensional sedimentary basins, formed on top of
the accretionary complex. Nor were the mélanges deformed as
the result of the continual reactivation of the accretionary com-
plex, causing the development of thrust planes with further dis-
ruption and the formation of the scaly fabric, as Moore and Karig
(1980) had suggested. As we have seen the occurrence of mud vol-
cano fields on Nias and the other Sunda Outer Arc islands indicatesthat compression-generated overpressures forming diapiric
mélange is still in the process of formation at the present day.
Nevertheless, the olistostromal and tectonic models for the for-
mation of mélanges proposed by Karig et al. (1979) has been so im-
mensely persuasive and influential that it has been invoked as an
explanation for the occurrence of mélanges all over the world;
e.g. Turkey and the Himalayas (Collins and Robertson, 1997; Rob-
ertson and Pickett, 2000; Robertson and Ustaömer, 2011). Hamil-
ton (1979), as a Californian geologist, would have been well
aware of the work at Scripps, which led him to the interpretation
of the Bobonaro Scaly Mélange of West Timor as of tectonic origin,
formed by the process visualised by Karig et al. (1979).
As far as the author is aware no clasts of blueschist or eclogite
have been recorded from the mélanges on Timor or on the OuterSunda Arc islands, which as has been explained originated as dia-
pirs on a continental shelf or in an active continental margin envi-
ronment. Clasts of ophiolitic materials are found in the mélanges
on both Timor and Nias but these have been incorporated when
diapirs have penetrated overlying accreted slices of ocean crust.
Mélanges that contain clasts of blueschists, eclogites and other
high grade metamorphic rocks, often in a serpentinous matrix such
as those in the Franciscan Mélange of California and the Peleru
Mélange Complex of Central Sulawesi have risen diapirically up
the subduction zone from the mantle, as earlier authors have sug-
gested (Cloos, 1984, 1985; Parkinson, 1996).
In a landmark paper, Kopf (2002, Fig. 1) building on an earlier
review by Higgins and Saunders (1967) catalogued the occurrence
of mud volcanism and mud diapirism throughout the world; henoted that they are especially developed on convergent plate
Fig. 13. The margin of a mud diapir exposed in the bank of a tributary stream of the
Oyo River, showing the grey scaly clay matrix, with a fabric parallel to the margin,
cutting and injected along joint fractures in a greywacke sandstone bed, Oyo
Mélange, Nias, Sumatran Outer Arc. Notebook 110 150 mm.
436 A.J. Barber / Journal of Asian Earth Sciences 76 (2013) 428–438
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margins. Mud diapirs and mud volcanoes are particularly abundant
in the collision zone between Africa and Eurasia and in the subduc-
tion and collision zones between the Indian and Australian plates
and Southeast Asia. The floor of the Mediterranean Sea has been
particularly well studied by marine geophysical surveys in the past
two decades (see Camerlenghi and Pini, 2009, Fig. 4). Kopf (2002)
claims that is ‘‘arguably the region with the highest abundance
of MVs (mud volcanoes) and diapirs on Earth’’. Several hundredmud volcanoes and mud diapirs have been discovered on Mediter-
ranean Ridge accretionary complex to the south of Crete, formed
by the subduction of the African Plate beneath the European Plate.
The mud volcanoes have been imaged by seismic surveys and
swath mapping and have been sampled by coring, deep drilling
and the use of submersibles, with study of the blocks and the clay
matrix. It is a remarkable anomaly that although mélanges occur
commonly on the adjacent land areas of Greece, Crete, Cyprus
and Southern Turkey they are invariably attributed to the pro-
cesses of submarine slumping and tectonism, not to mud diapirism
(Camerlenghi and Pini, 2009, Fig. 3). Although mud diapirs may be
difficult to recognise in older mélanges on land because diagnostic
features such as mud volcanoes have long since been eroded away,
and the cross-cutting relationships have been modified or de-
stroyed by later tectonism. However, examples are known where
mélanges are incorporated into metamorphic complexes and have
been deformed and recrystallised to form schists, in which blocks
flattened in the foliation planes are injected by the matrix, showing
evidence of overpressure, as seen in diapiric mélange. Structural
and tectonic geologists working on mélanges on land should con-
sider more seriously the possibility that mud diapirism may have
played a role in their formation. In the recent Special Issue of Tec-
tonophysics (Dilek et al., 2012) there is evidence in the papers by
Festa et al. (2012), Codegone et al. (2012a), Codegone et al.
(2012b) and Wakita (2012) that this possibility is beginning to
be appreciated.
Acknowledgements
The author is indebted to Dr. Tim Charlton for his companion-
ship and support over many years of work on the geology of Timor.
He is also thanked for reinterpreting the side-scan sonar imagery
across the Timor Trough, shown as Fig. 5 in this paper, to clarify
some ambiguities in the original interpretation prepared for his
Ph.D. Thesis in 1987.
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