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Author's personal copy Neogene development of the Savu Forearc Basin, Indonesia James W.D. Rigg 1 , Robert Hall * SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London, Egham Hill, Egham, Surrey TW20 0EX, UK article info Article history: Received 12 July 2011 Received in revised form 23 October 2011 Accepted 4 November 2011 Available online 18 November 2011 Keywords: Indonesia Sunda arc Banda arc Seismic Extension abstract The Savu Basin is situated in the SundaeBanda forearc where there is now a change from oceanic subduction to continentearc collision. It records Middle Miocene initiation of subduction of the Banda oceanic embayment, subsequent arc volcanism, and Pliocene to Recent collision of the Australian continent and Banda forearc. New seismic data provide insights into its Neogene development. Four major units can be recognised offshore and correlated with geology on land. Unit 1 is underlain by continental crust and Cretaceous-Paleogene arc rocks capped by Oligocene to Lower Miocene shallow water carbonates. Subduction rollback-induced extension in the Middle Miocene caused subsidence to depths of several kilometres. Units 2 to 4 include Middle Miocene to Pliocene arc-derived volcaniclastic turbidites and deep water carbonates that thin northwards into the basin, and Pliocene to Recent sediments that thicken northwards due to slumping from the south. Apart from tilting and slumping the Savu Basin is little deformed and there are no thrusts within it. Only at its southern edge is there signicant deformation close to the Savu and Roti Thrusts, which do not form part of a single through- going thrust zone. There are two ridges at the south side of the basin. The Sumba Ridge was elevated as Australian margin continental crust underthrust the forearc to form a broad exure tilting older units and causing debris ows and turbidites to ow northwards into the basin. The SavueRoti Ridge is composed of a pre-collision Banda forearc accretionary complex and Australian margin sedimentary cover. It is partly bounded by north-vergent and south-vergent thrust zones and has risen from depths of more than 2 km since 2 Ma. Most of the basin is undeformed but remains a high-risk area for hydro- carbons although there are a few indications which may be prospective in shallower areas. Ó 2011 Elsevier Ltd. All rights reserved. 1. Introduction The Savu Basin is part of the forearc of the SundaeBanda volcanic arc at the southern Eurasian margin (Fig. 1). It is located just north of the position where there is a change from subduction of Indian Ocean crust at the Java Trench in the west to collision between the Australian continental margin and the Banda forearc to the east. There are hydrocarbon provinces in the area surrounding the Savu Basin and current interest in exploration in this frontier region. The productive oil and gas elds of the northern Browse Basin and Bonaparte Gulf Basin are located in the Australian NW Shelf southeast of the Savu Basin. These are situated within the relatively undeformed rocks of the Australian continental margin, which are juxtaposed to the north against the highly deformed rocks of the Banda ArceAustralian collision complex, notably in Timor. There is considerable exploration interest in the Banda region (e.g. Charlton, 2004; Satyana and Purwaningsih, 2011), where hydrocarbon seeps have long been known, but petroleum systems are complicated by a number of factors, including uncer- tainty about the nature of the underlying crust, its complex tectonic setting, and the consequences of Neogene deformation. The Savu Basin has been very little explored although recently acquired seismic data from the basin show a number of features which may be associated with hydrocarbons, and seeps have been identied from satellite mapping (Toothill and Lamb, 2009). The basin has been the subject of speculation concerning its origin because of its position and unusual shape, especially the way in which it widens westwards towards the forearc island of Sumba (e.g. Chamalaun et al., 1982; Audley-Charles, 1985; van der Werff, 1995a; Ruth- erford et al., 2001). The islands surrounding the basin (Sumba, Flores, Wetar, Timor, Roti and Savu) have been the source of most information for its interpretation. The Savu Basin is bounded to the west by the island of Sumba and a submarine ridge (the Sumba Ridge) that crosses the forearc obliquely in an NWeSE direction. It narrows from its greatest width * Corresponding author. Tel.: þ44 1784 443897; fax: þ44 1784 434716. E-mail address: [email protected] (R. Hall). 1 Now at: CGGVeritas, Crompton Way, Manor Royal Estate, Crawley, West Sussex RH10 9QN, UK. Contents lists available at SciVerse ScienceDirect Marine and Petroleum Geology journal homepage: www.elsevier.com/locate/marpetgeo 0264-8172/$ e see front matter Ó 2011 Elsevier Ltd. All rights reserved. doi:10.1016/j.marpetgeo.2011.11.002 Marine and Petroleum Geology 32 (2012) 76e94

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Neogene development of the Savu Forearc Basin, Indonesia

James W.D. Rigg 1, Robert Hall*

SE Asia Research Group, Department of Earth Sciences, Royal Holloway University of London, Egham Hill, Egham, Surrey TW20 0EX, UK

a r t i c l e i n f o

Article history:Received 12 July 2011Received in revised form23 October 2011Accepted 4 November 2011Available online 18 November 2011

Keywords:IndonesiaSunda arcBanda arcSeismicExtension

a b s t r a c t

The Savu Basin is situated in the SundaeBanda forearc where there is now a change from oceanicsubduction to continentearc collision. It records Middle Miocene initiation of subduction of the Bandaoceanic embayment, subsequent arc volcanism, and Pliocene to Recent collision of the Australiancontinent and Banda forearc. New seismic data provide insights into its Neogene development. Fourmajor units can be recognised offshore and correlated with geology on land. Unit 1 is underlain bycontinental crust and Cretaceous-Paleogene arc rocks capped by Oligocene to Lower Miocene shallowwater carbonates. Subduction rollback-induced extension in the Middle Miocene caused subsidence todepths of several kilometres. Units 2 to 4 include Middle Miocene to Pliocene arc-derived volcaniclasticturbidites and deep water carbonates that thin northwards into the basin, and Pliocene to Recentsediments that thicken northwards due to slumping from the south. Apart from tilting and slumping theSavu Basin is little deformed and there are no thrusts within it. Only at its southern edge is theresignificant deformation close to the Savu and Roti Thrusts, which do not form part of a single through-going thrust zone. There are two ridges at the south side of the basin. The Sumba Ridge was elevated asAustralian margin continental crust underthrust the forearc to form a broad flexure tilting older unitsand causing debris flows and turbidites to flow northwards into the basin. The SavueRoti Ridge iscomposed of a pre-collision Banda forearc accretionary complex and Australian margin sedimentarycover. It is partly bounded by north-vergent and south-vergent thrust zones and has risen from depths ofmore than 2 km since 2 Ma. Most of the basin is undeformed but remains a high-risk area for hydro-carbons although there are a few indications which may be prospective in shallower areas.

� 2011 Elsevier Ltd. All rights reserved.

1. Introduction

The Savu Basin is part of the forearc of the SundaeBandavolcanic arc at the southern Eurasian margin (Fig. 1). It is locatedjust north of the position where there is a change from subductionof Indian Ocean crust at the Java Trench in the west to collisionbetween the Australian continental margin and the Banda forearcto the east.

There are hydrocarbon provinces in the area surrounding theSavu Basin and current interest in exploration in this frontierregion. The productive oil and gas fields of the northern BrowseBasin and Bonaparte Gulf Basin are located in the Australian NWShelf southeast of the Savu Basin. These are situated within therelatively undeformed rocks of the Australian continental margin,which are juxtaposed to the north against the highly deformed

rocks of the Banda ArceAustralian collision complex, notably inTimor. There is considerable exploration interest in the Bandaregion (e.g. Charlton, 2004; Satyana and Purwaningsih, 2011),where hydrocarbon seeps have long been known, but petroleumsystems are complicated by a number of factors, including uncer-tainty about the nature of the underlying crust, its complex tectonicsetting, and the consequences of Neogene deformation. The SavuBasin has been very little explored although recently acquiredseismic data from the basin show a number of features which maybe associated with hydrocarbons, and seeps have been identifiedfrom satellite mapping (Toothill and Lamb, 2009). The basin hasbeen the subject of speculation concerning its origin because of itsposition and unusual shape, especially the way in which it widenswestwards towards the forearc island of Sumba (e.g. Chamalaunet al., 1982; Audley-Charles, 1985; van der Werff, 1995a; Ruth-erford et al., 2001). The islands surrounding the basin (Sumba,Flores, Wetar, Timor, Roti and Savu) have been the source of mostinformation for its interpretation.

The Savu Basin is bounded to the west by the island of Sumbaand a submarine ridge (the Sumba Ridge) that crosses the forearcobliquely in an NWeSE direction. It narrows from its greatest width

* Corresponding author. Tel.: þ44 1784 443897; fax: þ44 1784 434716.E-mail address: [email protected] (R. Hall).

1 Now at: CGGVeritas, Crompton Way, Manor Royal Estate, Crawley, West SussexRH10 9QN, UK.

Contents lists available at SciVerse ScienceDirect

Marine and Petroleum Geology

journal homepage: www.elsevier .com/locate/marpetgeo

0264-8172/$ e see front matter � 2011 Elsevier Ltd. All rights reserved.doi:10.1016/j.marpetgeo.2011.11.002

Marine and Petroleum Geology 32 (2012) 76e94

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of c.200 km to approximately 20 km in the east north of Timor andin the west to approximately 50 km north of Sumba (Fig. 2). To thenorth is the active volcanic arc including the island of Flores whichpasses east into an extinct sector of the Banda arc between Alor andWetar. Volcanic activity in this sector ceased by about 2e3 Ma(Abbott and Chamalaun, 1981; Scotney et al., 2005; Herringtonet al., 2011). Although there are several volcanoes on Flores,Wheller et al. (1987) noted that those in western Flores, north ofSumba, may also be extinct although activity must have ceasedquite recently as several deeply eroded Quaternary strato-volcanoes remain. To the north of these extinct sectors there isnorthward-directed thrusting in the backarc region north of Floresand Wetar (Fig. 2) that has been interpreted as indicating subduc-tion polarity reversal (e.g. Silver et al., 1983; Snyder et al., 1996).However, north of the active arc segment in eastern Flores, in thesector immediately north of the central Savu Basin, there is nobackarc thrusting (Silver et al., 1983).

At the eastern end of the Savu Basin the forearc narrows to lessthan 50 km between the collision complex on Timor and theinactive Banda volcanic arc islands of Alor and Wetar to the north.To the south of the Savu Basin are the small islands of Savu and Rotiand to the south of them is a sinuous bathymetric trough thatconnects the Timor Trough to the Java Trench. Debate continuesabout the significance of the trough (e.g. Fitch, 1970, 1972; Audley-Charles and Milsom, 1974; Fitch and Hamilton, 1974; Hamilton,1979; Audley-Charles, 1986b, 2004; Harris, 1991; Lorenzo et al.,1998; Tandon et al., 2000; Spakman and Hall, 2010) and the timingof collision (e.g. Audley-Charles, 1986a, 2011; Hall and Wilson,2000; Keep et al., 2003; Harris et al., 2009).

There has been little information from the Savu Basin itself. Asmall number of marine geophysical cruises and hydrocarbonexploration investigations crossed the basin in the 1970s and1980s and acquired bathymetric, gravity, magnetic and seismic

data (e.g. Hamilton, 1979; Silver et al., 1983; Karig et al., 1987;Fortuin et al., 1992; van der Werff et al., 1994; van der Werff,1995a,b; Harris et al., 2009). For most of the seismic lines dataquality is relatively poor and penetration is typically 1 or 2 s TWTat best. Toothill and Lamb (2009) illustrated seismic sections fromsurveys in 2002 and 2007 which collected new gravity and seismicdata. CGGVeritas kindly provided the seismic lines acquired duringthose surveys which provided the basis for this study of the SavuBasin.

2. Dataset and previous stratigraphic studies

The seismic data (Fig. 2) consists of 32 2D seismic lines, of whichthe longest is 535 km, covering the southern and western parts ofthe Savu Basin, with a total area of 50,000 km2, which wereacquired and processed by CGGVeritas. The results of two surveyswere combined for this study. The first dataset was acquired in2002 and comprises 2740 km of long-offset 2D data to a depth of12 s TWT. The secondwas acquired in 2007 and comprises 3000 kmof long-offset 2D data to a depth of 8 s TWT (Toothill and Lamb,2009).

No wells have been drilled in the basin. The only well in thestudy area was a dry hole drilled on north Savu in 1975 (Savu #1 ofHarris et al., 2009) with TD at 1227 m. This well reveals melangesand repetition due to thrusting, but cannot be used to correlate intothe basin. Although there are no wells it is possible to correlate thestratigraphy offshore with that on land in some of the surroundingislands. To the north, no correlation with Flores is possible. Onlya few of the lines approach within 30e50 km of the south coast ofthe island and most terminate more than 100 km south of Flores.Regional bathymetry (Gebco, 2003; Sandwell and Smith, 2009),and the few available older lines that do approach Flores (Hamilton,1979; Karig et al., 1987), show there is an abrupt bathymetric

Figure 1. Location of the Savu Basin in SE Asia. Bathymetry simplified from Gebco (2003) with contours in metres. Red triangles are active and Quaternary volcanoes (Siebert andSimkin, 2002). Box outlines area of Figure 2. (For interpretation of the references to colour in this figure legend, the reader is referred to the web version of this article.)

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change south of the islandwith water depths rising frommore than3 km, at the northern ends of the new seismic lines, to almost sealevel over a distance of 10e15 kmwhich we suggest is a major fault(see below). However, the lines do provide good coverage close tothe island of Sumba, as well as Timor, Savu and Roti, although thesethree islands are separated from the main basin by thrust zones. Allthese islands emerged in the Pliocene or Pleistocene.

The stratigraphy and structure of Sumba has been well docu-mented (e.g. van Bemmelen, 1949; Burollet and Salle, 1981, 1982;von der Borch et al., 1983; Effendi and Apandi, 1993; Fortuinet al., 1992, 1994, 1997), it is relatively undeformed, and theseismic lines close to Sumba cross sequences that are also littledeformed. There are no major structures separating Sumba fromthe sequences seen in the Savu Basin which makes it possible tocorrelate from land to the offshore area. The oldest rocks reportedfrom Sumba (Roggeveen, 1929) are Jurassic sands and shales withInoceramus and ammonite fragments. Cretaceous marine tuffa-ceous sandstones and mudstones associated with basalt flows andbasaltic-andesitic agglomerates are intruded by a suite of igneousrocks including granodiorites and gabbros. The older rocks areunconformably overlain by Paleocene and Eocene volcanic rocks,and non-marine to shallowmarine conglomerates, sandstones, andmudstones. Above these are widespread shallow water carbonate

deposits of Late Oligocene to Early Miocene age which are overlainby thick deep marine volcaniclastic sedimentary rocks. The strati-graphic column (Fig. 3) shows the strata present in the eastern partof Sumba (Fortuin et al., 1992, 1994) and correlation with theseismic sequences identified in this study.

To the east of the Savu Basin metamorphic rocks and a sedi-mentary cover sequence derived from the Banda forearc wereemplaced as thrust sheets on Timor during the late Neogene andhave become known as the Banda Terrane (Audley-Charles andHarris, 1990; Harris, 1991; Audley-Charles, 2011). The meta-morphic rocks are assigned to the Mutis Metamorphic Complex inWest Timor (Earle, 1981; Brown and Earle, 1983) and correlatedwith the Lolotoi Metamorphic Complex of East Timor (Audley-Charles, 1968; Barber and Audley-Charles, 1976) which Standleyand Harris (2009) have shown includes an Upper Cretaceoussedimentary protolith and records an Eocene metamorphic eventinterpreted to have occurred in the forearc.

Audley-Charles (1985) summarised the stratigraphy of theBanda Terrane cover sequences in West Timor based onearlier studies by Tappenbeck (1940), Audley-Charles and Carter(1972), Audley-Charles et al. (1974), Haile et al. (1979), Rosidi et al.(1996), and Earle (1981). The Palelo Group includes UpperJurassic agglomerates and tuffs, Lower Cretaceous cherts and

Figure 2. Geographical features of Savu Basin and surrounding area. A. DEM of satellite gravity-derived bathymetry combined with SRTM topography (Sandwell and Smith, 2009).SR is Sumba Ridge and SRR is Sumba-Roti Ridge. B. Contoured bathymetry in metres (Gebco, 2003) and location of seismic lines. Red triangles are active and Quaternary volcanoes.Flores andWetar Thrusts from Silver et al. (1983). Small red box north of Savu shows the area of the seismic grid of Harris et al. (2009). (For interpretation of the references to colourin this figure legend, the reader is referred to the web version of this article.)

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pelagic limestones, and a Paleocene sequence of volcanics andvolcaniclastics, resting with an angular unconformity on theCretaceous rocks. Eocene shallow water limestones with an Asiancharacter (Lunt, 2003) locally overlie the Mutis MetamorphicComplex in West Timor with faulted and possible unconformablecontacts and there are widespread Upper Oligocene-LowerMiocene shallow water limestones assigned to the Cablac Lime-stone that rest unconformably on theMutis Metamorphic Complex,locally with a basal conglomerate. Mio-Pliocene volcanic rocks,including tuffs, are the youngest parts of the Banda Terrane.Audley-Charles (1985) drew attention to the similarity of the WestTimor and Sumba sequences despite a separation of more than400 km, and noted that Miocene volcanism seemed more impor-tant in Sumba than Timor.

To the south of the Savu Basin studies on and close to Savu andRoti (Rosidi et al., 1996; Harris et al., 2009; Roosmawati and Harris,2009) also provide valuable information that has aided interpre-tation of the offshore data, although both these islands, and theoffshore areas close to the islands are much more deformed thanthe areas to the north in the basin itself, and it is not possible tocorrelate from them into the basin. Marine geophysical investiga-tions combined with gravity and tomographic modelling haverecently been used to interpret the deep crustal structure alonga regional transect crossing the central part of the Savu Basin(Shulgin et al., 2009). The combination of information fromprevious studies with the new seismic data set offshore providedthe basis for our interpretation of the stratigraphy offshore and thehistory of the forearc.

3. Offshore and onshore stratigraphy

Four major units can be mapped through the basin (Figs. 4e6)and most of the adjacent offshore areas and can be correlated withsequences on land. The units have been described in Rigg and Hall(2011) and only key points are repeated here.

3.1. Unit 1

Unit 1 is the deepest unit with a package of bright reflectors upto 0.4 s TWT thick at its top that can be mapped throughout theentire area as a continuous feature despite offsets by extensionalfaults (Fig. 4). We suggest this bright package correlates withEocene to Lower Miocene Nummulites and shallow water lime-stones observed on Sumba (von der Borch et al., 1983; Fortuin et al.,1992, 1997; van der Werff et al., 1994) and Timor (Audley-Charles,1985). The field relationships described by Fortuin et al. (1992,1994) from Sumba with tilted fault blocks capped by discontin-uous carbonates, all overlain unconformably by Middle Mioceneand younger strata, closely resemble features seen in the seismiclines. On Sumba thin conglomerates containing older shallowwater limestone clasts mark a probable Late Burdigalian uncon-formity that passes up into chalks and marls (Fig. 3). Fortuin et al.(1994) suggest these conglomerates correspond to breakup ofa carbonate platform and rapid subsidence in the early MiddleMiocene. If our correlation is correct, and the reflectors that can betraced into the deepest parts of the basin are Lower Miocene andolder shallow water carbonates, the Savu Basin is very unlikely tobe underlain by young oceanic crust (Fleury et al., 2009) or bea Paleogene marginal basin (Harris, 2003).

Unit 1 can on some lines be split into two. In some places there isno clear boundary between the upper and lower parts whereaselsewhere there is a sharp boundary. The upper part containslocalised sub-parallel reflectors, and the faults that cut the top ofUnit 1 cannot be traced downwards, whereas the lower part ischaracterised by laterally discontinuous bedding which can betraced for distances of up to 20 km.We suggest that the lower part ofUnit 1 can be correlatedwithMesozoic rocks on land, and the upperpart is probably Paleogene. On Sumba there are shallow marineJurassic sediments (Roggeveen, 1929), Cretaceous marine siltstonesand sandstones (Burollet and Salle, 1981, 1982) interpreted assubmarine fan deposits (von der Borch et al., 1983) and arc rocks

Figure 3. Seismic stratigraphy of the Savu Basin and correlation with stratigraphy of east Sumba (Fortuin et al., 1992). The colours shown next to the seismic section for the fourunits are those used on figures of other seismic profiles. The vertical scale of seismic sections is two way travel time (TWT) in seconds. (For interpretation of the references to colourin this figure legend, the reader is referred to the web version of this article.)

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that include volcaniclastics cross-cut by intrusive igneous bodies(Effendi and Apandi, 1993; Fortuin et al., 1994, 1997; Abdullah et al.,2000). These are overlain unconformably by non-marine to shallowmarine Paleogene conglomerates, sandstones, and mudstones,foraminiferal limestones, tuffs and ignimbrites (von der Borch et al.,1983; Effendi and Apandi, 1993; Abdullah et al., 2000).

3.2. Unit 2

Above the distinctive reflectors at the top of Unit 1 is Unit 2(Figs. 4e6) with a thickness up to 1.6 s TWT which fills the depres-sions created by the extensional faulting andonlaps the faults. Its topis a prominent unconformity that can be mapped throughout thebasin at thebaseofUnit 3.Unit 2 is variable in character. It commonlylacks the well bedded character of the overlying Units 3 and 4.Reflectors are clearest where the unit is thin and are typically bright,sub-parallel and discontinuous, whereas thicker parts of Unit 2 arecharacterised by a transparent seismic character.

We suggest Unit 2 can be correlated with volcaniclastic turbi-dites on Sumba (Fortuin et al., 1992, 1994) above the Late Burdi-galian unconformity. Locally well bedded parts of Unit 2 passlaterally into unreflective packages consistent with a transitionfrom bedded turbidites to rapid deposited disorganised volcani-clastic material. On land these rocks are poorly dated due toreworking and absence of microfossils but are considered toexplosive island arc volcanism between 14.8 and 5.5Ma that wanedduring the Tortonian and revived during the Messinian (Fortuinet al., 1994, 1997). Fortuin et al. (1997) suggested subsidencebelow a carbonate compensation depth of 4e5 km during the

Middle Miocene in east Sumba and during the Late Miocene incentral Sumba based on dissolution of carbonate in some samplesbut the presence of calcareous nannofossils in others.

3.3. Unit 3

Unit 3 is a very distinctive sequence characterised by closelyspaced strong reflectors particularly on seismic lines crossing thesouthern part of the basin. It has a maximum thickness of 1.8 s TWTand is typically about 1 s thick. On the NWeSE-trending SumbaRidge Unit 3 is flat lying and conformable on Unit 2 but to the northof the ridge there are a series of northward-dipping planar pack-ages. In many places Unit 3 appears to downlap onto an uncon-formity at its base (Fig. 4) and in the deeper parts of the basin itrests locally on Unit 1, and Unit 2 is missing (Fig. 7). On the fewundeformed sections south of the Sumba Ridge a similar downlaponto underlying units can be seen. Unit 3 thickens north from theSumba Ridge into the deep Savu Basin and further north becomesthinner, suggesting it was derived from the south. On the SumbaRidge it is cut bymany high angle small displacement normal faults,with a spacing of 8e10 km.

There are a number of slumped packages within Unit 3, wellimaged by marked contrasts in reflector character (Fig. 7). Theyhave a chaotic internal structure compared to adjacent well beddedsequences and thicknesses commonly between 0.1 and 0.35 s TWT.The thinnest slumps cannot be mapped between lines indicatingthey have a lateral extent of less than a few kilometres, but largerslumps can be mapped within an area of about 25 km radius. Thevariation in the thickness and number of slumps contributes to

Figure 4. Seismic line fromwestern part of Savu Basin showing relationships between Units 1 to 4. Half graben at base of Unit 2 are clear at this location. High angle normal faults inUnit 3 are well imaged.

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Figure 6. Approximately north-south line crossing the Savu Basin. At the south end Unit 1 is uplifted and thrust northwards towards the basin and Units 2, 3 and 4 are largelymissing and interpreted to have been redeposited in the basin as Unit 4.

Figure 5. In the centre of the Savu Basin many high angle normal faults cut Unit 1 with local small half graben at the base of Unit 2. Units 2 and 3 are thin. Unit 4 can be subdividedinto several sub-units with prominent unconformities between them, which separate phases of deposition and slumping.

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lateral thickness changes in Unit 3. They are most common at thesouthern edges of the basin and indicate repeated failures at thebasin margins as Sumba, Savu and Roti were uplifted.

We interpret Unit 3 as equivalent to the Tortonian to Plioceneforaminiferal chalks, marls, hemipelagic nannofossil oozes andvolcanogenic muds with some thickly bedded volcanic mass flowdeposits on Sumba (von der Borch et al., 1983; Fortuin et al., 1992,1994, 1997). The fan of sediment was derived from the southwestand deposited in the deeper area of the central Savu Basin, and canbe traced at least 75 km northwards from the present southernedge of the basin. This implies the Sumba Ridge was a slightlyelevated feature at the south edge of the basin when the fan beganto develop. The fan prograded northwards and beds downlap ontoolder units. Local onlap between layers resembles features inter-preted on Sumba by Fortuin et al. (1997) to be the result of shiftingfan lobes which may contribute to thickness variations in Unit 3.The present dip of beds (up to 5e6�) is unlikely to relate to anoriginal depositional slope for fine grained sediments and wesuggest this apparent downlap north of the Sumba Ridge is theresult of uplift of the ridge and rotation of beds. This implies thatuplift of the ridge began during deposition of Unit 3, supported byincreasing abundance of slumps up section.

3.4. Unit 4

Unit 4 can bemapped throughout the area north of Sumba Ridge(Figs. 4 to 8) but it is not possible to correlate across the ridge to the

south because Units 2 to 4 now thin towards the ridge and areabsent on it. Locally Unit 4 onlaps Unit 3. It shows considerablevariation in thickness, can be subdivided into several parts, and ischaracterised by slumping. Unit 4 is interpreted to representslumping of Unit 3 (and possibly parts of Unit 2) northwards intothe basin as the Sumba Ridge was elevated with several phases ofslumping (Fig. 4) separated by minor unconformities. Slumpedpackages were derived from the south and backstep southwards asthe basin was filled, facilitated by extensional faulting at the top ofthe slope, preserved in Unit 3.

The slumps have many features similar to deep water debrisflows, from cohesive slumps to large mass transport complexes,described byMcGilvery and Cook (2003) and Bull et al. (2009). Theyare characterised by a chaotic and transparent internal seismiccharacter and include headwall scarps, internal thrusts, folds andramps, and small pop-up structures. Local cohesive slumps, formedby downslope creep, have well defined toe thrusts and associatedfolding at their distal end. Large blocks are often present withinlarger mass transport complexes which in places retain somebedded character. Disturbed units are separated in places by wellbedded units suggesting episodes of major slope failure alternatingwith smaller slumps or turbidite flows.

There are a number of ramp features in the upper part of Unit 4(Fig. 8) with an average height of about 0.5 s TWT. These are slumpswith a well defined base, which detached at a bedding plane, inwhich the basal thrust ramped up against underlying sediment atthe distal end. The front walls of these features are often steep,

Figure 7. At the western edge of the Savu Basin slumped packages within well bedded sediments of Unit 3 record downslope movements at the basin edge. Individual slumppackages occur at various levels within Unit 3, and are localised features, none of which can be correlated between lines. There is considerable variation in internal structure. Theupper slumped section in A has very well defined toe thrusts associated with folding at its distal end.

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ramping up against, and truncating strata already in place. Tilting ofstrata has facilitated the downcutting associated with the ramps.The generation of such ramp structures has been discussed by Bullet al. (2009) based on 3D seismic data, and their development isthought to reflect localised variations in stress conditions for shearfailure. Downcutting may also reflect a component of gougingduring transport and deposition (Posamentier and Kolla, 2003).

The thickness of Units 3 and 4 varies significantly from east towest. Unit 3 is thin in the SE close to Timor and Roti (up to 0.25 sTWT) and Unit 4 is thick (about 1 s TWT). In the SW, close to Sumba,the thicknesses of Units 3 and 4 are reversed. The number andthickness of slumps associated with Unit 4 increase in importancetowards the east. In the northern part of the basin, Unit 4 is betterbedded with flat, parallel and bright reflectors which are lessprominent at greater depths. These interfinger with the slumps.The well bedded sequences could represent turbidite deposits atthe distal ends of debris flows or material transported from thevolcanic arc to the north. Interfingering of bedded deposits withslumps of Unit 4 favours a Flores origin. There are also someslumped horizons at the very top of the seismic sections closest toFlores suggesting deposition downslope from the volcanic arc.

Features similar to those of Unit 4 have been described fromSumba and seismic lines crossing the Savu Basin (van Weeringet al., 1989a,b; Fortuin et al., 1992; van der Werff et al., 1994;Roep and Fortuin, 1996) and were suggested to indicate simulta-neous uplift and downslope transport of debris into the northern

part of the Savu Basin during the Early Pliocene. Unit 3 largelyrepresents the depositional phase of development of the fan andthinning to the east in the Savu Basin reflects a greater distancefrom the sediment source to the SW. Unit 4 represents the nextstage of development involving uplift. Its distribution can beassessed from the isochron map (Fig. 9) and the three lines whichcross the basin from east to west. Our new data show that the areaaffected by slumping is at least 18,000 km2 and is much greaterthan previously estimated. We suggest that the fan had two sour-ces. Initially, material was derived from Timor and spread outtowards the northwest. In the western part of the basin, Unit 4 wasderived from the western Sumba Ridge and the southern end ofSumba, and carried eastwards. There was little material carriednorth from Sumba.

4. Deformation history

The principal structures mapped from our seismic dataset areshown on Figure 10. In the major part of the basin sediments areflat-lying with normal faulting in the deeper parts of the section.There are some differences from earlier studies. Thrusts shown inthe Savu Basin by van der Werff (1995a) are probably slumps, andhe shows a different orientation of structures SE of Sumba that weattribute to the much wider spacing and poorer quality of the olderseismic data. On regional maps major thrust zones are often tracedoffshore across the Savu Basin, typically from Timor. For example,

Figure 8. Ramp features in Units 3 and 4 are associated with the transport of material from uplifted areas into the Savu Basin. A and B show variation in size. They cut both up anddown, truncate surrounding reflectors, and are characterised by a chaotic internal structure with steep front walls.

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the Savu Thrust is exposed on land at the northern margin of SavuIsland (Harris et al., 2009) and is sometimes shown as majorcontinuous feature crossing the south side of the Savu Basin (e.g.Audley-Charles, 1985, 2004; Harris, 2006; Shulgin et al., 2009). Infact, there is no continuous thrust zone crossing it and most of theSavu Basin is little deformed apart from tilting and slumping,except close to the islands of Savu and Roti where there are zones ofthrusting which can be broadly described as the Savu Thrust andthe Roti Thrust.

4.1. Sea floor features

The irregular topography of the sea floor is an indication of localactive deformation. On the slopes descending from the Savu Ridge,close to the basin floor, this is probably due to recent downslopemovements of material. This is clear on lines perpendicular to theslope but is more difficult to prove on lines sub-parallel to strike.These show small scarps with heights up to 100 m and abrupttermination of bedding at these features on the seabed, but slumpsor mass transport complexes are difficult to identify.

Narrow canyons are seen on seismic lines that run across the topof the slope at the southwestern edge of the Savu Basin close toSumba (Fig. 11). McGilvery and Cook (2003) suggest that suchcanyons, the majority of which are steep walled, developed byexcavation through gravity mass wasting and can act as localsediment conduits. They are clearly very young as they incise wellbedded horizontal strata at the top of Unit 4. It is probable that thecanyons are erosional products of material carried from Sumbawhere in the western part of the island there are deeply incisedsteep-sided valleys, running mainly northeast, from the highestmountains of the island, implying young uplift on land.

Two areas of similar prominent sea floor topography are presentin the northern part of the basin (Fig. 12). One shown on Figure 12Brises approximately 300 m from the sea floor in the deepest part ofthe basin south of Flores. It has a low gradient profile, is roughly

13 km across, and has a small 100 m deep crater-like centre.Internally, the uppermost 0.3 s is well stratified feature abovea section of poor quality seismic suggesting movement of materialfrom beneath. The feature resembles mud volcanoes found in areasof rapid sedimentation where there is active hydrocarbon genera-tion (Dimitrov, 2002). However, since the feature is cut by only oneline its shape is uncertain. It could be part of a submarine turbiditecanyon system with levees which is consistent with the wellstratified upper part of the feature.

4.2. Normal faults in the Savu Basin

Many large extensional faults cut the bright reflectors at the topof Unit 1 and created a series of full and half graben, which weinterpret to have formed in the Middle Miocene based on correla-tion with limestones on Sumba. Faults at the northern edge of theSumba Ridge, are typically 15 km apart, and although the extensiondirection cannot be precisely determined because of the widespacing of seismic lines, it is broadly north-south. There arenumerous normal faults further north in the Savu Basin (Fig. 10).Extension on these faults contributed to the initial subsidence ofUnit 1 which is now at depths of 2 s on the Sumba Ridge to 7 s TWTin the deepest parts of the Savu Basin. The faults have not beeninverted, with the exception of some close to the Savu and RotiThrusts. The main Savu Thrust does appear to have reactivated atthe position of a previous normal fault (Fig. 13). The relatively smallnumber of shallow depth (<50 km) earthquake solutions (Das,2004; GCMT, 2011) within the basin show normal and strike-slipfaulting in the basin but no indication of thrusting.

4.3. Savu Thrust

The Savu Thrust is not a single thrust but a zone of thrusting(Figs. 10 and 13), as shown by Harris et al. (2009) on land andoffshore of northern Savu. We have not attempted to map the

Figure 9. Isochron map of Unit 4 shows thickening towards the north suggesting that most of the material, including many slumped packages, is derived from the northern marginof Sumba and Savu, with material flowing towards the northeast. Unit 4 thickens away from the base of slope at the southern edge of the basin.

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thrusts in detail as we have only a few widely spaced lines thatcross the closely spaced grid of 1975 seismic profiles in the smallarea mapped by Harris et al. (2009). The older seismic profilesimage the upper part of the section (<1 s TWT), with one well thatpenetrates to 1227 m TD, from which Harris et al. (2009) interpretsouth-dipping and north-dipping thrusts to a depth of 5 km.

The new seismic lines allow interpretation to about 1.5 s TWTbelow the sea floor in the structurally complex area close to thethrusts. They show that the thrust zone dies out to the east andwest within about 50 km of Savu. It can be traced from the westthrough north Savu and further east is offset to the south byroughly 5 km. The total displacement diminishes to the east andwest. We could not identify any north-dipping thrusts near Savu,although they are present much further south on the south side ofthe SavueRoti Ridge (Figs. 2 and 10). All the thrusts dip south andthe largest has a displacement of between 0.4 and 1.3 s TWT.Immediately in front of the largest thrust (Fig.13) there is a footwallsyncline in Unit 3 and behind the main thrust, faults and associatedfold limbs are progressively steepened. Some thrusts reach theseabed whereas others are blind but their geometry is obscured bypoor seismic quality in the uplifted areas. There are numerous smallinverted normal faults, both behind and in front of the main thrust,which also dip south.

There are several episodes of deformation associated with thethrust zone, marked by prominent unconformities in deformedUnit 3. The first major phase of movement folded deeper parts ofUnit 3 and folds are onlapped by younger reflectors. There arenumerous subsequent subtle onlaps of reflectors near the top ofUnit 3, associated with syn-deformation thickening away from themain fault.

4.4. Roti Thrust

The Roti Thrust (Figs. 10 and 14) is about 25 km south of theeastern strand of the Savu Thrust and is located offshore 20 kmnorth of Roti with a NNE-SSW orientation parallel to the coast foralmost the entire 70 km length of the island. It has a similar char-acter to the Savu Thrust, being a zone of thrusting, with thrusts thatdip southwards and die out to the east and west. The thrust zone iswider but the maximum displacement on the most importantthrusts is less than in the Savu thrust zone. The largest thrust hasa displacement of about 0.5 s TWT. There are some inverted normalfaults in front of themain thrust. The net displacement is greatest inthe centre of the thrust zone and appears comparable to the Savuthrust zone. Like the Savu Thrust, several phases of deformation canbe identified by mapping of minor unconformities in the deformedzone with onlap and thickening of packages in front of the mainthrust. As noted above, the Roti and Savu thrust zones do not linktogether.

4.5. SE-directed thrusting SE of Sumba

In the area southeast of Sumba, on the south side of the SumbaRidge, there is a zone of thrusting roughly 60 km across that widenstowards the Lombok Basin to the west. There are a number ofanticlines (Fig. 15) well imaged on the seismic lines which are1000e1400m across associatedwith numerous NW-dipping thrustfaults (Fig. 10). The orientation of faults and fold axes is difficult todetermine because of the wide spacing of seismic lines in this areabut they are clearly oblique to the Sumba Ridge and we estimatea trend of about 030�. We interpret these to be structures formed in

Figure 10. Summary structure map with the principal features identified in the area of study. The coloured shaded area north of the Java Trench and Timor Trough is, fromwest toeast, the transition from the Sunda forearc, which passes east into a deformed zone including forearc and Australian sedimentary cover forming the SavueRoti Ridge, into thearcecontinent collision zone of Timor. The fine dotted black line north of Timor is the inferred northern limit of Australian continental basement. The dashed red line below Sumbais the inferred northern and western limits of the underthrust Scott Plateau. Most of the Savu Basin is undeformed, except by slumping, and major structures in the basin are normalfaults. Thrusts are observed only close to Savu and Roti. The heavy dashed line along the north side of the Savu Basin is suggested to mark a steep structure with a large verticaloffset which could be a thrust or normal fault and is named the Alor-Flores Fault. (For interpretation of the references to colour in this figure legend, the reader is referred to the webversion of this article.)

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the former accretionary complex north of, but close to, the formerBanda Trench.

The thrusts and folds are overlain unconformably by almost 1 sTWT of sediments which dip very gently northwards. It is notpossible to correlate these with units in the Savu Basin as there areno lines that cross from SW to NE of the Sumba Ridge but theyresemble Unit 3 and were probably derived from the NW, thin tothe southeast, and have been tilted by the rise of the SavueRotiRidge.

4.6. SE-directed thrusting of the SavueRoti Ridge

The SavueRoti Ridge is a broad zone of largely seismicallyopaque, apparently highly deformed material. Within the ridgeare narrow zones in the upper 1 s TWTof the seismic sections withNEeSW striking thrusts that dip northwards and reach theseabed. There are two particularly clear zones of deformation(Fig. 10). The majority of faults within the northern, slightlybroader, zone dip north, although some smaller antithetic faultscan also be seen. The southern zone is characterised by smallnorthward-dipping thrusts (Fig. 16), which become progressivelyrotated and steepened towards the north. Between these twozones some faults and reflectors can be seen in places. Deforma-tion in the SavueRoti Ridge may be active today and thrusts areevidently younger than those close to Sumba since they are notoverlain by sediment.

4.7. Alor-Flores Fault

The northernmost part of the Savu Basin is not crossed byany of the seismic lines of this study. There are also no seismiclines by previous surveys that approach the coast of Flores,undoubtedly because of the rapid change in water depth at thenorthern edge of the Savu Basin. Here (Fig. 2) there is a spec-tacular slope with gradients of 15e20� that descends from theFlores coast over a distance of 10e15 km to water depths ofmore than 3 km (Hamilton, 1979; Karig et al., 1987) which isalso evident in global bathymetry data (Gebco, 2003; Sandwelland Smith, 2009). The gradient is even greater if the landmorphology is included as volcanoes very close to the coast onthe south side of Flores have elevations of more than 1 km. Notonly is this slope very steep, it is quite unlike any feature inany volcanic arc elsewhere in Indonesia in being so close to theactive arc itself.

Rutherford et al. (2001) speculated that there was a dextralstrike-slip fault parallel to the southern coastline of Flores definingthe edge of a former west-moving Sumba block, but inactive sinceabout 7 Ma. We did not find most of the structures postulated bythem (e.g. Rutherford et al., 2001, their Fig. 5) in the basin andsurrounding region and our interpretation of timing of events isvery different. However, they are undoubtedly correct in identi-fying a fault along the north side of the basin but we suggest this isan active fault with an important dip-slip component which wename the Alor-Flores Fault (Fig. 10). No seismic lines cross the fault

Figure 11. Canyons on the seabed east of Sumba are suggested to be a result of erosion by turbidity currents from the direction of Sumba. The tilted fault blocks at the base of Unit 2,present throughout the basin, are particularly well imaged. In this area there is less contrast between Units 3 and 4 than elsewhere.

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but the steep slope and free air gravity gradient are illustrated byRutherford et al. (2001) and there is a concentration of earthquakeepicentres (Engdahl et al., 1998) close to the postulated fault. Thereare only three earthquake solutions on the line of the fault (GCMT,2011); assuming an ENE fault trend the easternmost is sinistral, thesecond is a normal fault with a sinistral component, and thewesternmost is normal.

On the north side of the volcanic arc are the two active north-directed Flores and Wetar Thrusts (Fig. 2). These do not link toform a single thrust zone and are separated by a zone of strike-slipfaulting on the north side of Flores (McCaffrey, 1988; Das, 2004;GCMT, 2011) in the sector north of our interpreted Alor-FloresFault. It is not coincidental that the Flores and Wetar Thrusts arenorth of the two rectilinear continental promontories of East Timorand the Scott Plateau (see below), and in the sectors where volcanicactivity has ceased (Wheller et al., 1987). The Alor-Flores Fault couldbe an extensional response to loading and tilting of the forearcbetween the promontories where collision has caused volcanicactivity to terminate. It could alternatively be a steep thrust butwith the opposite vergence to the Flores and Wetar Thrusts, andvan derWerff (1995a) shows south-directed thrusts at the northernend of two seismic lines close to Flores. If this is correct, the Floresand Wetar Thrusts are unlikely to represent the early stages ofsubduction polarity reversal, and the thrusts simply represent

shallow crustal features accommodating contraction across theentire arc.

5. Discussion: Cenozoic evolution

The shape of the Savu Basin and the unusual way in whichSumba crosses the forearc have been the cause of controversy andspeculation over many years (e.g. Hamilton, 1977, 1979; Audley-Charles, 1985; van der Werff, 1995a,b; Rutherford et al., 2001;Fleury et al., 2009). It is nowaccepted that Sumbawas part of the SEAsian continental margin since the Cretaceous, and the Savu Basinwas part of the SundaeBanda forearc. Many authors have recog-nised the importance of trench retreat or rollback as an importantfeature of Banda Arc development (e.g. Hamilton, 1976, 1979;Harris, 1992, 2003, 2006; Hall, 1996, 2002; Charlton, 2000;Milsom, 2001; Hinschberger et al., 2005). However, when theSavu Basin reached its present depth, the nature of the underlyingbasement, and how these relate to Banda rollback remain uncer-tain. We have proposed elsewhere (Rigg and Hall, 2011) a tectonicinterpretation of the Savu Basin that builds on previous studies ofthe region and incorporates our new observations in the context ofa subduction rollback model which includes detailed reconstruc-tions of the whole Banda Arc (Spakman and Hall, 2010). We do notrepeat the interpretation here but discuss below key points based

Figure 12. A. Basin floor structure close to Flores. There is some bedding, which suggests the end of a channel with levees sourced from the volcanic arc or a relatively low viscositymud volcano suggested by deeper disturbed section. B and C. Zones of disrupted bedding in the upper part of Unit 4 are suggested to be due to gas escape linked to minor faults.Small offset faults are not uncommon at this depth but are normally sharp, as seen on the left of C, and not associated with such disruption.

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on the new seismic data that are important in the late Cenozoicdevelopment of the Savu Basin.

5.1. Basement

The Sumba margin was the site of arc volcanism during thelatest Cretaceous, Paleocene and Eocene (Abdullah et al., 2000;Lytwyn et al., 2001). A continental basement for the Sumbaregion was favoured by many early workers (e.g. Hamilton, 1977;Bowin et al., 1980; von der Borch et al., 1983; van der Werff et al.,1994) although it was uncertain if this had come from SE Asia orAustralia. Palaeomagnetic evidence indicates Sumbawas part of theSundamargin by the Late Cretaceous (Wensink,1994,1997) and hasnot moved significantly relative to SE Asia since the Early Miocene(Wensink & van Bergen, 1995). Rutherford et al. (2001) suggestedthe Cretaceous arc was built on oceanic crust and Harris (2006)described it as a continent-fringing arc mounted on oceanic base-ment. In contrast, van der Werff (1995a) interpreted a strong SavuBasin to be underlain by rigid crust of continental origin. Wesuggest that the region from SW Sulawesi to West Timor includingSumba and the Savu Basin is underlain by Australian continentalcrust that was accreted to SE Asia in the mid Cretaceous (Wakitaet al., 1996; Parkinson et al., 1998; Hall et al., 2009; Hall, 2011) on

which later arcs were constructed. This suggestion is supported bycrustal thicknesses and densities (Shulgin et al., 2009) and byJurassic ammonites and bivalves reported from South Sulawesi(Sukamto and Westermann, 1993) and Sumba (Roggeveen, 1929).

Whatever the nature of the deep crust it is generally agreed thatvolcanic activity ceased in the Eocene when the region must havebeen close to sea level or emergent. There have been a number ofdifferent suggestions for the development of the southeastern partof the Sundamargin since the Eocene. Fleury et al. (2009) suggestedthat the “intact internal structure of the Savu Basin” is due to therigidity of its oceanic basement. Harris (2006) interpreted Sumbaand the Sumba Ridge as remnants of a “continental arc terrane”fragmented and dispersed by Oligocene extension, and Harris(2003) showed the Savu Basin as a marginal basin formed at25e35 Ma, appearing to imply that it is underlain by oceanic crust,and certainly that it subsided in the Oligocene. In an earlier paper,Harris (1992) suggested the eastern Savu Basin was underlain bya supra-subduction zone ophiolite formed since about 6 Ma duringtrench retreat whichwould suggest it subsided in the Late Miocene.

Although the present active volcanic arc is north of Sumba,Fortuin et al. (1994) suggested that Sumba and the Savu Basin werein a backarc position in the Middle Miocene and moved to a forearclocation since the Late Miocene. They did not identify a mechanism

Figure 13. Seismic line crossing the centre of the Savu Thrust north of Savu, where there is themaximum amount of displacement and folding in front of the thrust. Deformedmaterialsouth of the thrust includes Australian margin rocks and sediments from the southern margin of the Savu Basin and is separated from less deformed Units 1 to 3 in the basin.

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but this could be explained by oceanic spreading in the Savu Basinassociated with a movement of the arc, or by a jump of the arc fromsouth to north forming an interarc basin (Charlton, 2000) withcrust of an uncertain nature. This would imply the basin subsidedfrom the Middle Miocene.

We interpret Unit 1 in the Savu Basin to represent the LateCretaceous to Early Miocene interval and correlate the distinctivereflectors at the top of Unit 1 with Upper Oligocene-Lower Mioceneshallow marine limestones described on Sumba and Timor. Thishorizon can be traced across the whole of the area covered by ourdata implying that it was close to sea level in the Early Miocene.This, and the structure of Unit 1, rules out suggestions that thebasement is oceanic crust. It also conflicts with the suggestion ofHarris (2003, 2006) that there was major extension and formationof marginal basins within the SE Asian forearc during the Oligocenefollowing collapse of the Sulawesi orogen. There may have beenoceanic crust further east in the Banda forearc, now preserved inthe Banda Terrane on Timor, but the area between West Timor andSumba including most of the Savu Basin did not subside before theMiddle Miocene and does not include oceanic crust.

5.2. Subsidence and volcanism

Subsidence on Sumba began in the Middle Miocene withbreakup of a carbonate platform leading to rapid subsidence fromabout 16 Ma (Fortuin et al., 1994). This was an effect of the begin-ning of hinge rollback into the Banda embayment that led to theformation of the Banda Arc (Spakman and Hall, 2010). There wasa significant influx of volcaniclastic turbidites that we correlatewith Unit 2 deposited in deep water on Sumba and in the Savu

Basin (Fortuin et al., 1992,1994). Fortuin et al. (1997) suggested thatthese deposits were derived from a volcanic arc south of Sumba andform part of a fan that prograded northwards. This arc should besomewhere beneath the Sumba-Roti Ridge before it moved to itspresent position in Flores north of the Savu Basin and Sumba.However, volcanic activity is known on Flores from 16 Ma(Hendaryono, 1998; Fleury et al., 2009) and there is no indication inour seismic data of coarsening or thickening of beds to the southconsistent with another arc south of Sumba. We propose that thearc was always in its present position north of the Savu Basin andvolcaniclastic debris fromwest Flores and Lombok was transportedESE through the Lombok Basin and then turned northward into theSavu Basin. Sediment movement was broadly parallel to theWNW-trending Sumba Ridge that followed a deep basement trend in theunderlying Australian continental basement that had been accretedin the mid Cretaceous (Hall et al., 2009). The top of the ridge inWest Sumba was at very shallow depths through the Neogene butbecame much deeper to the eastat which point sediment was ableto turn northwards. NE-SW orientated faults in Sumba, whichallowed East Sumba to subside to depths of 4e5 km (Fortuin et al.,1994, 1997) would have opened a passage into the Savu Basin fromthe SW.

In the Savu Basin extensional faults have a broadly E-W trend,curving fromWNW in thewest to ENE in the east.We suggest theseextensional faults in the basin formed in response to subductionand rollback into the Banda embayment which began after 16 Ma(Hall, 2002, 2009, 2011; Spakman and Hall, 2010). Offshore to thenorth of Sumba, faults that can be correlated between seismic linesappear to be oriented NeS, which we interpret to be due to along-arc extension.

Figure 14. The Roti Thrust resembles the Savu Thrust but the zone of deformation extends further north than in the Savu area. Prominent unconformities within deformed materialare evident. It is not possible to correlate strata at this location with those further to the west near the Savu Thrust.

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5.3. Strike-slip faulting and thrusting

There is no obvious evidence for the large strike-slip faultsshown to cross or bound the basin by some authors (e.g. Soeria-Atmadja et al., 1998; Rutherford et al., 2001) and surmised tohave produced thrusting SWof Sumba. Previously, in the absence ofoffshore data, several authors suggested that north-directedthrusting north of Timor could be connected to surmised offshorestructures that cross the Savu Basin or join the Roti and SavuThrusts (e.g. Audley-Charles, 1985; Roosmawati and Harris, 2009;Shulgin et al., 2009). Our seismic data show that the Roti andSavu Thrusts are discontinuous and there are no major thrusts in

the deeper part of the basin. In the central Savu Basin the only signsof contractional deformation are slumps in Unit 4, and the seabed isflat or gently sloping.

The oldest thrusts found in this study are SE of Sumba and northof the SavueRoti Ridge (Figs. 10 and 15). They have an ENEeWSWtrend and are now covered by up to 1 s TWT of sediment resem-bling Unit 3. We interpret them to have formed in the accretionarycomplex close to the former Banda Trench (Breen et al., 1986).

The Sumba Ridge was elevated during the collision process(Figs. 6 and 13) after the first arrival of Australian continentalmargin at the Banda Trench south of Sumba (Harris, 1991; van derWerff, 1995a,b). Bedding of Unit 3 dips at up to 5e6� as a result of

Figure 15. SE-vergent folds and thrusts SE of Sumba. The deformation in this area is suggested to be related to subduction at the former Banda Trench and predate arcecontinentcollision. Folds and thrusts are locally overlain by 1 s TWT of sediment. Anticlines contain some flat spots which cut across stratigraphy and may indicate the presence of previous, orin place, hydrocarbons.

Figure 16. The southern side of the deformed complex south of the SavueRoti Ridge shows SE-directed thrusting and folding. The thrust faults are well imaged at the southern endof the uplifted area, and become progressively steeper towards the NW. As thrusts become steeper, internal deformation also increases, which results in a poorly imaged section.

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uplift of the ridge and rotation of beds and there is an increasingabundance of slumps up section. Slumps in Unit 4 are directedbasinward from Sumba and Timor. Deformation of Unit 3 wouldhave begun after 4 Ma based on correlation with Sumba wherethere was uplift from depths of more than 5 km since then (Fortuinet al., 1997). The present elevation of more than 1 km on Sumbawith carbonate reefs up to 500m above sea level record uplift in thelast 1 million years (Pirazzoli et al., 1993). There is no observableinversion of normal faults or thrusting associated with the uplift ofSumba Island which appears to have risen as a broad upwarp.

The Savu and Roti Thrusts (Figs. 13 and 14) are much youngerthan all other structures and are currently active zones of defor-mation that include multiple thrusts. The seismic lines show thatthey are not lithosphere-scale features, nor major through-goingregional structures, as they die out rapidly to the east and westand do not link up. Both zones include thrusts that emerge at thesea floor, blind thrusts associated with deformation of the sequenceabove, and folding of the seabed.

The accretionary complex that presumably formed north of theBanda Trench during oceanic subduction has been overridden and/orincorporated in thewedge of deformedmaterial south of the Savu andRoti Thrusts, except in the extreme SE where it is seen beneath flatlying sediments SE of Sumba. Unit 4 records slumping associatedwithuplift of the SavueRoti Ridge andRoosmawati andHarris (2009) showthat significant and rapid uplift fromwater depths of more than 2 kmto emergence of the islands of Savu and Roti began at about 2Ma. Thebroad zone of seismically opaque material with narrow thrust zoneswould therefore have been deformed since then. Most of the ridgemust includematerial from both the Banda forearc and the Australiancontinental margin, as also suggested by observations on land in Rotiand Savu (Harris et al., 2009; Roosmawati and Harris, 2009).

Thrusting south of Sumba and the Savu Basin has two causes:deformation associated with subduction at the Java and former

Banda Trench, and collision of the Banda forearc with the Australianmargin which began at around 4 Ma (e.g. Audley-Charles, 1986a,2011; Harris, 1991; Hall, 1996, 2002; Spakman & Hall, 2010). Thecollision was also influenced by the shape of the Australian marginwhich had rectilinear offsets north of East Timor and the ScottPlateau similar to those seen today at the Exmouth Plateau of theNWAustralian shelf. This is the major cause of the unusual shape ofthe Savu Basin. Fortuin et al. (1994) noted that the Sumba regiondeparted from timeespace equivalence predictions for the westernBanda orogen of Harris (1991). Harris explained this as the result ofcollision of the Scott Plateau whereas Fortuin et al. (1997) postu-lated a role for their surmised southern volcanic arc. We agree withHarris (1991). The first volcanic arcecontinent collision was northof East Timor and deformation propagated west with time in Timor(Harris, 1991). It then began independently in Sumba as the ScottPlateau came into contact with the forearc. The shape of the marginmeans that beneath Savu and Roti Australian continental crust hasonly recently underthrust the leading edge of the Banda forearc(Rigg and Hall, 2011).

6. Implications for hydrocarbon exploration

Forearc regions are generally not considered attractive targetsfor hydrocarbons. Because there has been little exploration andalmost no drilling in the region around the Savu Basin the age andnature of the basement and overlying units was not known. Toothilland Lamb (2009) suggested possible hydrocarbon sources based oncomparison with Seram and Timor, and the pre-collisional riftedmargin of northern Australia. They interpreted the age of rifting atthe top of Unit 1 as Mesozoic whereas we suggest it is MiddleMiocene, and we therefore differ in suggestions of possible sourcerocks for a petroleum system. We agree that the deep basement islikely to be Australian continental crust with a structure inherited

Figure 17. Localised discontinuous high amplitude reflectors (outlined) in the upper part of Unit 4. Many, but not all, are close to faults, and there is an unusual abundance of themin this area. They may indicate the presence of shallow gas.

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from the pre-rifted Australian margin but suggest that thisAustralian basement arrived in the Cretaceous. Regional deepseismic lines have indicated a thick pre-Cenozoic section (Emmetet al., 2009; Granath et al., 2011) in the East Java Sea possiblyanalogous to the Canning Basin based on tectonic reconstructions(Hall et al., 2009; Hall, 2011) which could be present beneathSumba. This could provide a possible petroleum source althoughmuch deeper than anything interpreted from seismic lines of thisstudy.

Unit 1 may include source rocks. Based on correlation withSumba the upper part is likely to include shales, mudstones, silt-stones and tuffaceous sandstones (van Bemmelen, 1949; Burolletand Salle, 1981, 1982; von der Borch et al., 1983; Effendi andApandi, 1993; Fortuin et al., 1994; van der Werff, 1995a) withsmall Paleogene intrusions. Hamilton (1979) mentions lignites.There is limited evidence for hydrocarbon generation in the basinfrom these sources, or others. Toothill and Lamb (2009) drewattention to satellite mapping of oil slicks on the surface of the SavuSea and the position of some of them above structures identified onseismic lines. Steeply dipping beds at the sea floor or faults whichpenetrate to the seabed can be directly linked to slicks on thesurface of the Savu Sea. The correlation of these potential conduitswith the slicks on the sea surface would further suggest thegeneration of hydrocarbons at some level within the subsurface(Toothill and Lamb, 2009).

Near the northern edge of the Savu Basin there are fluid-escapestructures that could be gas chimneys (Figs. 12 and 17). They aredifferent from faults well imaged elsewhere at the same depth inthe section, and there is a change in seismic character in thesurrounding subsurface, not seen in faulted areas, which originatesand widens in a triangular fashion from a point at depth. They maybe associated with leakage from deeper gas accumulations ratherthan breaching of shallow hydrate layers. If so, they would indicatethe presence of a generating source rock within the basin. Possiblemud volcanoes (Fig. 12) suggest overpressured zones which couldbe associated with hydrocarbons although these also suggest therisk of damage to seals.

In some areas just north of the northern coast of Sumba (Fig. 17)numerous short (up to 500 m) localised, high amplitude reflectorsare visible at depths of 2e3 s TWT. They could be microbial gasdeposits formed at shallow depths and buried due to high sedi-mentation rates (Floodgate and Judd, 1992). It is also possible thatthese could have a thermogenic origin and have migrated fromdepth. The small bright spots suggest trapping against the exten-sional faults that are present in Unit 3. The small and localisednature of the accumulations may relate to the lack of a laterallycontinuous sealing horizon, the lack of a suitable reservoir or thesignificant deformation experienced by Unit 3.

The relative lack of deformation throughout most of the SavuBasin suggests that the integrity of a traps is not a major concern.Possible reservoirs are carbonates at the top of Unit 1 and possibly,but much less attractive, the volcaniclastic sandstones in Units 2 to4. There may be stratigraphic traps formed by the numerousonlapping surfaces. Rotated domino-style fault blocks could alsoserve as potential hydrocarbon traps at depth. Inversion anticlineshave been identified as possible traps in Banda area by Charlton(2004) and well imaged anticlines are located 35 km to the southof Sumba (Fig. 15) within the Sumba Basin. Associated with theseare prominent flat spots, which are between 600 and 700 m inlength. These features appear to be within a layer 0.15 s thick,bounded on either side by bright horizons. These could be hydro-carbons or may represent a palaeo oil-water-contact, markingdiagenetic effects of previously in-place hydrocarbons. Overall,there are possibilities for both hydrocarbon sources and reservoirs,but on the basis of information available at present this is clearly

a high risk area. Much of the basin is undeformed but water depthsare greater than 3 km. The relatively shallow areas close to Sumba,and the Sumba Ridge are the most accessible.

7. Conclusions

The Savu Basin is probably underlain by Australian continentalcrust accreted to the SE Asian margin in the Cretaceous and was thesite of volcanic activity in the Late Cretaceous and Early Cenozoic.From the Late Eocene to Early Miocene it was close to sea level andcarbonates were deposited over a widespread area, includingSumba and the Savu Basin. It subsided rapidly to depths of severalkilometres in the late Middle Miocene in response to extensioninduced by rollback at the Banda Trench as subduction propagatedeast into the Banda Embayment. The extension was marked bywidespread normal faulting.

From the Middle Miocene a thick succession of volcaniclasticturbidites was deposited in the basin. They entered the basin fromthe SW but were probably derived from the volcanic arc to thenorth of Sumba. Transport was influenced by the Sumba Ridge inthe forearc which caused turbidity currents to flow first ESE parallelto the ridge, and then NE into the Savu Basin. The ridge is suggestedto be a feature that reflects the deep structure of the Sunda margin.The western part of the ridge remained a shallow bathymetricfeature during the Neogene although the eastern part subsided todepths of several kilometres.

Apart from tilting and slumping the Savu Basin is little deformedand there are no thrusts within it but its southern margin recordsPliocene to Recent collision of the Australian continent and theforearc. Thick Middle Miocene to Pliocene sediments of the SavuBasin thin northwards into the basin, whereas Pliocene to Recentsediments thicken northwards due to slumping into the basin fromthe south. Sumba and the Sumba Ridge was elevated as continentalcrust of the Australian margin arrived at the Banda Trench and wasflexed into a broad upwarp that tilted the volcaniclastic turbiditesequence and later caused debris flows and turbidites to flownorthwards into the basin. Slumps came from both Sumba andTimor.

Collision began earliest in the east in East Timor where thecollision complex is nowalmost in contact with the former volcanicarc. Rectilinear offsets in the former Australian continent-oceanboundary meant that forearc-continent contact occurred later inthe SavueRoti area at the south side of the basin. This is the reasonfor NE-narrowing of the Savu Basin. In the west the northern edgeof the Scott Plateau is now beneath the Sumba Ridge, contributingto the elevation of Sumba and extensional collapse seen on theisland.

SE of Sumba a small part of the original forearc accretionarycomplex is preserved, now buried beneath almost 1 s of sediment.The SavueRoti Ridge is composed partly of Banda forearc sedi-ments and partly of Australian margin sedimentary cover. Most ofthe pre-collisional accretionary complex has been incorporated inthe ridge south of the Savu and Roti Thrusts including the islands ofSavu and Roti which rose from depths of more than 2 km since 2Maand emerged very recently. The deformed complex is partlybounded to the north and south by north- and south-vergentthrusts; the former trench is now deep beneath this complex andthe lithospheric faults do not emerge at the surface. To the souththe surface of this wedge dips south and is underlain by Australianmargin sedimentary cover.

On the north side of the Savu Basin is the volcanic arc and northof the arc are the active north-directed Flores and Wetar Thrusts.These are located north of the two rectilinear continental prom-ontories of East Timor and the Scott Plateau in sectors wherevolcanic activity has ceased. Between them on the south side of

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Flores is a major fault, very close to the volcanic arc, which issuggested to be a normal fault downthrown to the south formed bynorthward tilting of the forearc, or a steep southward-vergentthrust. The Flores and Wetar Thrusts are unlikely to represent theearly stages of subduction polarity reversal, and the faults simplyrepresent shallow crustal features accommodating contraction inthe region between the Banda backarc and Australian continent.

Acknowledgements

We thank the consortium of oil companies who support the SEAsia Research Group, Steve Toothill and CGGVeritas for data and forhelpful discussion, and Chris Elders, Gordon Lister and WimSpakman for advice and discussion.We are grateful toMike Audley-Charles and Ron Harris for review comments that helped improvethe paper.

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