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Southern Basins Geology

IntroductionStructure & StratigraphySource RockReservoirsHydrocarbon IndicationsPlay TypesData

Introduction

Three connected basins surround the southern Falklands:

  • the Falkland Plateau Basin lies to the east;
  • the South Falkland Basin lies to the south;
  • the Malvinas Basin lies to the west.

Although all connected, each of the three basins exhibits its own unique structural style.

These three basins are isolated from the North Falkland Basin, and have a completely different infill.

All three of the Southern Basins probably share a similar stratigraphic infill, which is more marine than the predominantly continental North Falkland Basin.

None of the three southern basins has been drilled in Falklands waters.

Seventeen or so wells have been drilled in the Argentine part of the Malvinas Basin, with some limited success.

Boreholes drilled by the DSDP on the Maurice Ewing Bank at the easternmost extremity of the Falkland Plateau Basin tested rich marine source rocks that probably extend throughout much of the Southern Basin area, probably pinching out just into Argentine waters.

The Southern Basins are at the very earliest stage of exploration.

Only regional reconnaissance seismic data covers the area.

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Structure & Stratigraphy

Structure

Three separate basins with distinct structural styles are recognised in the southern basins area:

  • The Falkland Plateau Basin is an essentially passive margin basin, with Jurassic and Cretaceous marine rocks both gently onlapping, and prograding off, a Palaeozoic plateau
  • The South Falkland Basin is a narrow basin zone of ?Jurassic extensional fault blocks with an overthrust sequence of Cenozoic rocks developed along the boundary between the Scotia and South American plates: this basin forms a connection between the Falkland Plateau Basin and the Malvinas Basin
  • The Malvinas Basin is a ?Jurassic failed rift that deepens towards the south, where it is bounded by the transform plate margin of the Scotia and South American Plates: the basin runs eastwards into the South Falkland Basin.

Falklands Plateau Basin

This basin lies beneath 200 m to 2500 m of water to the east of the Falkland Islands.

It is bounded to the west by the Falklands Platform, to the north by a steeply sloping feature termed the Falkland Escarpment, to the east by the Maurice Ewing Bank and to the south by the Scotia/South American plate boundary, which has a sinistral and northwards over-thrust movement: this plate boundary produces a topographic feature known as the Scotia Ridge, which includes shallow water areas such as the Burdwood Bank (immediately south of the Falklands), as well as the islands of South Georgia and the South Sandwich Islands.

To the south-west, along the deep water trough known as the Falkland Chasm, the basin merges with the South Falkland Basin.

The central parts of the Falkland Plateau Basin may be underlain by thinned continental crust (about 16 km thick) or by oceanic crust, although the northern margin of the basin (the Falkland Escarpment) is underlain by a prolongation of probably gneissic continental crust that joins the Falklands Plateau with the Maurice Ewing Bank. To the west of the basin the Falklands Plateau itself is underlain by continental crust about 30 km thick.

The western boundary of the basin is in relatively shallow water (c.750–1000 m).

It is defined by a north-east – south-west oriented series of normal, down to the east faults in a linear trend approximately 650 km long.

This fault zone appears to comprise numerous shears offset along transfer zones, rather than a single fault.

The amount of throw along the fault zone varies from a few hundred metres to perhaps a kilometre or so.

There is a zone of high magnetic and gravity anomalies oriented along and (spread across) the western basin margin fault zone.

This gravity high is located over an area of apparent isostatic equilibrium, and can be explained partially as an edge effect due to crustal thinning beneath the sedimentary basin. However, the steep western slope of the observed anomaly and its sharp apex preclude a wholly deep crustal explanation; one explanation for these other features of the anomaly are pre- and syn-rift basaltic rocks, possibly sheet basalts, together with a deep-seated, dense magnetic body near the basin margin fault.

Along the western margin significant faulting is observed at possible Permo-Triassic to Jurassic level.

The apparent gentle westwards onlap of Cretaceous and Cenozoic reflectors near the basin margin suggests that the main phase of extension was in the Permo-Triassic or Jurassic.

Gentle onlap of the basin margin replaced active wedging some time in the Late Jurassic or Early Cretaceous.

The early extension was probably followed by post-rift sag through the Cretaceous and Cenozoic.

South Falkland Basin

This basin lies beneath 500 m to 2500 m of water to the immediate south of the Falkland Islands.

The basin can be defined bathymetrically, since it corresponds, more or less, with the deeper water zone of the Falklands Chasm, the foredeep that runs adjacent to the northern edge of the Scotia plate.

It is bounded to the south by the Scotia/South American plate boundary, which is a combined sinistral strike-slip and north-east-directed thrust fault.

It is contiguous with the Malvinas Basin to the west and the Falkland Plateau Basin to the east, but has a somewhat different structural style.

In terms of preserved structural style the basin is most similar to the southern part of the Malvinas Basin.

It exhibits numerous major normal faults downthrowing to the north that display reactivation into recent times, and a number of thrust faults of probable Cenozoic age, some of which splay off the southern bounding fault/plate boundary.

Most faults within the basin trend generally east to west and may have a major strike-slip component but look superficially like true normal faults.

They are orientated parallel to the boundary between the South American and Scotia plates, and are probably reactivated older, possibly basement-controlled faults that have been rejuvenated by the continued north-east- directed thrusting and sinistral strike-slip motion along the plate boundary.

Wedging of reflectors above the Permo-Triassic section (Fig. 6) suggests that much of the normal faulting in the basin was probably of Jurassic through Early Cretaceous age, contemporaneous with the deposition of sediments in the actively rifting trough.

Syn-depositional movement related to active extension may have ceased in the Valanginian or Hauterivian, as in other South American and offshore Southern African basins.

However, some wedging of reflectors is observed above this level, possibly as high as top Lower Cretaceous.

Normal fault movement may have continued throughout the Cretaceous as the basin sagged in a thermal relaxation phase following earlier extension, but most faults die out upwards before the top Cretaceous level.

Many of the faults have apparently been reactivated in the late Cenozoic, and some penetrate to the sea bed.

Much of this fault reactivation, probably with a strike-slip component, may have occurred in the Oligocene through mid Miocene as a result of uplift and lateral displacement of the Scotia arc along the Falkland Thrust as the West Scotia Basin to the south opened.

The plate boundary fault appears to have a more or less normal fault geometry in many places, with deep basins to the north and shallower basins or basement (Burdwood Bank) to the south.

However, it is complicated in places by a number of Cenozoic thrusts.

These thrusts affect only the higher stratigraphic levels in a zone within about 5–20 km of the basin margin.

The onset of thrusting marks a change from transtension to transpression along the plate boundary and has a significant effect on stratal geometries within the South Falkland Basin.

The lower part of the succession transected by thrust sheets appears, if the effects of thrusting are palinspastically reconstructed, to thicken southwards into the plate boundary. Thickening of the succession northwards, away from the basin margin as a result of syndepositional thrusting occurs near the mid-Cenozoic interval, possibly some time in the late Paleogene or Neogene. The thrusting may be genetically related to the Oligocene through Miocene opening of the Scotia Sea to the south of the Falkland Islands.

The South Falkland Basin plunges eastwards.

Malvinas Basin

This basin lies beneath 150 m to 250 m of water to the west of the Falkland Islands.

The basin extends westwards to the Rio Chico High in Argentine waters, and then further westwards to the onshore area of Tierra Del Fuego and southern Argentina, where it is termed the Austral or Magallanes Basin.

To the east it terminates by onlap onto Palaeozoic rocks of the Falklands Platform.

To the south it is constrained by the South American–Scotia plate boundary.

To the south-east it passes laterally into the South Falkland Basin, which essentially underlies the deeper water area adjacent to Burdwood Bank.

There are several distinct structural provinces in the basin, each possibly related to different elements in the formation and post-extensional modification of the basin:

  • the axial part of the basin trends north-west - south-east and is essentially a zone of widely-spaced tilted blocks
  • the eastern margin of the basin, within Falkland waters, is a sloping terrace area;
  • the southern part of the basin, running along the foredeep in front of the Scotia/South American plate boundary, is an overthrust zone.
  • The basin plunges southwards, and has a steers-head shape in cross section.

    Its structural configuration probably results from a combination of Triassic or Early to Mid Jurassic extension in a generally east–west direction, coupled with Cenozoic strike-slip related pull-apart during the sinistral movement of the southern bounding fault that separates the South American and Scotia plates. 

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Source Rock

No wells have been drilled in South Falklands waters, and therefore the presence and maturity of source rocks in the Falklands area is somewhat conjectural.

However, good quality source rocks have been drilled on the Maurice Ewing Bank to the east, and some source rock systems are also present in the Argentine parts of the Malvinas Basin to the west.

  • Oxfordian to Aptian claystones encountered in DSDP boreholes 330 and 511 on the Maurice Ewing Bank to the east of the Falklands contain terrestrial and aquatic organic matter, with up to 6% TOC, and a potential hydrocarbon yield of around 25 kg/ton of rock from Type II kerogens.
  • Thermal subsidence modelling suggests that the source rocks are possibly mature for oil generation at about 3000m below sea bed, over a wide area of the Falkland Plateau Basin and Malvinas Basin.
  • Generation of oil here may have started in the Campanian, about 81 million years ago.
  • Within the South Falkland Basin the same source rocks may be oil mature at a depth of either 11 100 ft below sea bed or 8500 ft below sea bed depending on whether a low or high heat flow is computed during the main rift phase of the basin.
  • Maturity levels of the main Upper Jurassic to Lower Cretaceous source interval within the South Falkland Basin may have increased gradually during the Cretaceous, with oil generation starting at around 98 to 102 million years ago.
  • Similarly aged source rocks within the Malvinas Basin may be mature for oil at a depth of around 11 000 ft below sea bed, with oil generation possibly starting at 40 million years ago (i.e. in the mid Eocene).
  • Drilling in the Argentine sector near the axis of the Malvinas Basin has been only partly successful, due largely to the unpredictable nature of the reservoir target in the area. However, some of the wells, particularly the more northerly, may have been dry because of their distance from the site of mature source rocks to the south and east.

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Reservoirs

Permo-Triassic, Mesozoic and Cenozoic sediments occur beneath or within all three of the Southern Basins, and each interval could contain potential reservoir rocks.

  • The only Mesozoic clastics of possible reservoir quality proven so far in the Falkland Plateau Basin are of probable Oxfordian age, and were penetrated in DSDP borehole 330, where the Oxfordian succession commences with a clean, beach sand deposit marking the Late Jurassic marine transgression over a swampy terrestrial environment.
  • The Lower Cretaceous Springhill Formation forms the main reservoir interval in the Argentine part of the Malvinas Basin, and may extend eastwards into the South Falkland Basin. It is a fluvial and transgressive sandstone that was deposited over the eroded basement topography.
  • Proximal sediments derived from the Devonian-Carboniferous Falklands Platform area may substantially improve reservoir quality locally at the Lower Cretaceous level in Falklands waters, in all of the Southern Basins.
  • Albian to Cenomanian sandstones are present in the western part of the Malvinas Basin, and isolated developments of these sandstones draped over basement highs or Jurassic tilted fault blocks may be found in the Falklands Designated Area.
  • The Palaeocene glauconitic sandstones recorded in the Argentine Ciclon No.1 well in the southern Malvinas Basin were probably deposited during a shallow marine transgression, and may therefore occur over large parts of the basin.
  • Transgressive sandstone may have developed at several horizons throughout the Mesozoic and Cenozoic.
  • Reservoir intervals may also be found in lowstand systems-tract wedges, similar to those which form reservoir intervals in the offshore southern Africa basins.
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Hydrocarbon Indications

Hydrocarbon indicators for the Falkland Plateau Basin are confined to data from the only borehole penetrations of the basin – the DSDP holes on the Maurice Ewing Bank some 750 km to the east of the Islands.

  • A 225 m thick fetid claystone, representing the deposits of an oxygen minimum zone were deposited in an enclosed basin from the Late Jurassic until the mid Cretaceous.
  • These claystones exude a strong petroliferous odour.
  • The Oxfordian to Aptian claystones encountered in DSDP boreholes 330 and 511 on the Maurice Ewing Bank contain terrestrial and aquatic organic matter, with up to 6% TOC, and a potential hydrocarbon yield of around 25 kg/ton of rock from dominantly Type II kerogens.
  • The kerogens found in the DSDP boreholes are somewhat immature with respect to oil generation, although appear to be overmature with respect to their present depth of burial. They were either once more deeply buried, or the geothermal gradient here was previously higher than at present.
  • The geothermal gradient at the DSDP sites has been measured at 70 ° C/km, indicating that oil-rich sediments could have reached oil maturation thresholds here at a depth of only 700 m.
  • The Argentine part of the Malvinas Basin has been partly explored, and there is some production from fields very close to the Argentine coast. However, a handful of wells have also found sub-commercial hydrocarbons in the central parts of the Malvinas Basin.
  • Calamar x-1, Salmon x-2 and Ciclon 1, all drilled by Exxon, had some hydrocarbon indicators:
    • Production test summary (Salmon x-2)
      2 production test were run in January 1982 for total of 7 days.
      Test 1:   2662–2667m Zone A, Basal Springhill sst. Produced 35deg API oil at average flow of 372 bopd.
      Test 2:   2648–2656.6m Zone B, Upper Springhill sst. Produced gas and condensate at av rates of 21 MMCF/D and 609 bopd. Condensate:/gas ratio was 29 STB/MMCF.
      There appears to be no communication between the two tested zones.

No hydrocarbon shows have been established for the South Falkland Basin due to the lack of drilling.

However, there are some high amplitude events on seismic sections, especially above tilted fault blocks, that might be considered as direct hydrocarbon indicators.

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Play Types

Note that play types and prospects/leads developed for the Southern Basins so far are made on the basis of widely spaced reconnaissance seismic data only. Parts of this dataset were reprocessed in 2003 by Falkland Oil and Gas Ltd (FOGL) , but the data were acquired in 1993.


Potential 'play' types for these basins include:

  • large-scale wedges of low stand fan deposits–Falkland Plateau Basin
  • localised sandstone wedges associated with the basin margin faults–Falkland Plateau Basin
  • rollovers associated with basin margin faulting–Falkland Plateau Basin
  • tilted fault-block traps at Jurassic level–South Falkland Basin
  • intra-basinal mounds of low-stand fan origin at Cretaceous level–Falkland Plateau Basin
  • sub-thrust sheet structures along the southern basin margin–South Falkland Basin
  • folded Cretaceous sandstones deformed by, or draped over, east–west orientated strike-slip faults and associated flower structures–South Falkland Basin
  • the pinchout of Lower Cretaceous Springhill Formation equivalent sandstones – Malvinas Basin
  • stratigraphic wedge-outs or lateral facies change of Albian to Cenomanian sandstones developed over intra-basinal structural highs or palaeoslope breaks–Malvinas Basin
  • fractured Jurassic volcanic rocks overlain and sealed by Cretaceous or Cenozoic mudstones around the basin margin–Malvinas Basin
  • probable Permo-Triassic rocks in structural traps beneath a seal of either Jurassic volcanic rocks or Cretaceous-Cenozoic mudstones–all of the basins.

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Data

Seismic data

There are three sets of 2D seismic data over the Southern Basins:

  • In 1977–78, two speculative, regional seismic surveys were shot by Western Geophysical and GSI, totalling some 21 652 km of data. Parts of this dataset were reprocessed in 1992.
  • These data are now part of Western-Geco’s data holdings, and can be purchased from them.
  • Western-Geco also acquired 4 339 km of regional reconnaissance spec data across all of the Southern Basins in 1993. A partial subset of these data were reprocessed in 2003 by Falkland Oil and Gas Ltd (FOGL).
  • The original 1993 processed versions of this survey are available, free of charge, to bona-fide exploration companies, from BGS in Seg-Y or Landmark project format.
  • The 2003 reprocessed versions can be obtained directly from Falkland Oil and Gas Ltd (FOGL) as part of their farm-in activity.
  • Spectrum Energy acquired an infill grid of data across the Special Co-operation Area (at the eastern margin of the Malvinas Basin) in 1997, and reprocessed these data in 2000.
  • The original 1998 processed versions of this survey will be released by BGS, to bona-fide exploration companies, in September 2008.
  • Until data release, the data can be obtained directly from Spectrum Energy at the appropriate commercial rate.
  • The 2000 reprocessed versions can be obtained directly from Spectrum Energy at the appropriate commercial rate (they will not be released until 2011).
  • GSI have aquired a large amount of spec data across the region since December 2004. These data are available from GSI.

Other spec data

  • Marine grav-mag surveys were conducted at the same time as the spec seismic surveys. These data are available from the same sources as provided in the links above.
  • Other data, such as surface seep studies from radar, are available directly from the companies that conducted these studies. For example, Infoterra has a comprehensive suite of satellite seep study data over the region.

All released data are supplied free of charge to bona-fide exploration companies and supplied on the following basis: Data are provided by the British Geological Survey on behalf of the Falkland Islands Government, and should not be distributed to third parties without the consent of the Falkland Islands Government.

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Images

Basins
Fig.1: Regional basins map

Basin stratigraphy correlation
Fig.2: Southern Basin Strat correlation

Source rock distribution
Fig.3: Source rock distribution in Southern Basins

Basin names and location
Fig.4: The basins, with some structural nomeclature

Falklands Basin Plateau
Fig.5: Detailed nomeclature/ structure of FPB

FPB Cross section
Fig.6: Cross section of FPB

Structural lineaments superimposed on grav map
Fig.7: Structural lineaments superimposed on grav map

South Falkland Basin
Fig.8: Detailed nomeclature/ structure of SFB

Seismic section across thrusts
Fig.9: Seismic section across thrusts

SFB cross section
Fig.10: SFB cross section

Mature source rock in SFB
Fig.11: Mature source area

position of Argentine wells
Fig. 12: Position of Argentine wells relative to mature source

Malvinas Basin seismic
Fig.13: Seismic showing progrades into the south-west

cretaceous progrades
Fig.14: Seismic showing progrades to east

DPSP core logs
Fig.15: DPSP core logs

Gas indicators on SFB seismic
Fig.16: Piece of seismic with DHIs above fault blocks

Data across SFB
Fig.17: Data across Southern Basins

Spec data in SFB
Fig.18: Pre 2004 Spec data across the area