Elsevier

Tectonophysics

Volume 348, Issues 1–3, 15 April 2002, Pages 5-24
Tectonophysics

Compartmentalisation of fluid migration pathways in the sub-Andean Zone, Bolivia

https://doi.org/10.1016/S0040-1951(01)00246-3Get rights and content

Abstract

Numerous observations indicate that faults play a major role on the migration pathways of fluids in the Bolivian sub-Andean Zone. Most oil seeps in the foothills are located on faults, but oil fields in the foredeep are closed by faults. In the foothills, analysis of cements in fractures inside and around fault zones indicates that the faults act as barriers for transversal migration but can be preferential lateral migration pathways for both hydrocarbons and water. A detailed study of these apparent contradictions suggests that the hydraulic behaviour of faults changes with depth in relation with sandstone diagenesis, but it is strain-independent. From microstructural analyses of fault zones, we suggest that the main controlling factor is temperature, which facilitates or inhibits quartz precipitation. This result implies that the same fault is a barrier for lateral and transversal migration at depths >3 km, due to sealing of fractures by authigenic quartz at T>80 °C, and is a lateral drain in its shallower parts. As a result, the various thrust sheets are isolated from a hydraulic point of view, whereas migration in the foreland may take place over long distances (>100 km).

Introduction

The role of faults and fractures along the migration pathways of fluids has been mainly studied at the reservoir scale and after fault activity. On a basin scale, however, the number of studies is much more limited. Some papers suggest that normal faults act as drains, especially when they are seismically active, and that reverse faults act as barriers (Muir Wood and King, 1993). Seismic studies in fault zones have proven the existence of overpressures which facilitate displacement (Evans, 1992; and many others) and imply, at least temporarily, impermeable fault zones. On the other hand, geological data show evidence for paleo-fluid circulation both in normal (Travé et al., 1998) and thrust fault zones Larroque et al., 1996, Labaume et al., 1997. In the Barbados accretionary prism, direct monitoring of the décollement level also demonstrated current fluid circulation along the fault plane (Moller et al., 1995) and seismic parameters have been interpreted as the mark of overpressure in another part of the fault (Shipley et al., 1997). All these examples strongly suggest that the hydraulic behaviour of faults may change with time. In the case of sand/shale intercalations, some predictive models have been proposed based on the clay smearing approach Weber et al., 1978, Lehner and Pilaar, 1997. Following this theory, shaly beds undergo plastic deformation when sandstones undergo brittle faulting. The shale smears the fault plane which becomes impermeable if the offset is small enough to permit the continuity of the clay smearing. When the offset increases, the hydraulic behaviour changes when the clay smear is disrupted along the fault plane. This model has been developed in deltaic series (e.g. Niger delta) for small-scale normal faults (offsets of a few meters to hundreds of meters). In this work on sandstone series, we propose another predictive model for the behaviour of fluids based on a multidisciplinary study of the Andean thrust front in southeastern Bolivia.

In petroleum-rich compressional provinces such as the Bolivian Andean foothills, oil seeps are numerous along reverse fault planes. However, in the Bolivian foredeep, various fields are closed by reverse faults. Working from the regional to thin-section scales, we have tried to understand this apparent discrepancy between fault behaviour in the foreland, below the syntectonic deposits, and that of the outcropping faults in the foothills. The structure of fault zones in the foothills and their paleo-hydraulic behaviour are deduced from the distribution of cements and carbon and oxygen isotope geochemistry of carbonate cements that are presented in detail in Labaume and Moretti (2001) and Labaume et al. (2001). In this paper, we summarise these results obtained on paleo-fluids, then we describe the present fluid flow systems (hydrocarbons and water) and focus the discussion on the resulting large-scale fluid flow pattern and its implication for exploration in the foothills.

Section snippets

Geological setting

The sub-Andean Zone of Bolivia is a Neogene east-verging thrust system Roeder, 1988, Sheffels, 1990, Baby et al., 1992, Baby et al., 1993 that constitutes the eastern border of the Andes (Fig. 1). The thrust sheets comprise an approximately 10-km-thick, mainly siliciclastic succession with Palaeozoic–Mesozoic platform sediments at the base overlain by up to 3-km-thick Neogene continental foreland deposits, which mainly consist of fluvial sandstones. The present paper concerns the southern

Source rocks

The shale source rocks are rather homogeneous and relatively well known, at least for the Middle Devonian and younger formations in the southern sub-Andean Zone. The Yacimientos Petroliferos Fiscales Bolivianos (YPFB) compiled a major database in 1995 that was published by Moretti et al., 1994, Moretti et al., 1995 and numerous more recent wells have allowed us to predict more precisely the potential of the deepest part, i.e. the Lower Devonian and Silurian. In the summary below, we outline the

Fault zone structure and paleo-fluid flow

This aspect has been described and discussed in detail in separate papers Labaume and Moretti, 2001, Labaume et al., 2001 and only the main features pertinent to the discussion of the thrust system-scale fluid flow are summarised here.

Twelve faults were studied at outcrops and one (Honduras fault) on well cores recovered at about 2500 m depth Fig. 1, Fig. 3, Fig. 4. Nine faults are large thrusts (offset up to 20 km: Rio Azero, Cuevo, Carohuaicho, Piedra Larga, Canaletas, Honduras well, Pajonal,

Oil seeps

More than 200 oil seeps have been reported in the Bolivian sub-Andean Zone, which we have classified relative to their structural position: 60% leak from large thrust faults, 30% from anticline hinges and only 10% from monoclines (Fig. 8). This classification emphasises the capacity of faults to focus oil migration. However, it may be noted that most oil seeps are located in the Upper Devonian, i.e. very close to the source rock, and hence the required migration distance along faults never

Synthesis of results

Integration of data on present and past fluid flows give important clues to the organisation of the fluid flow pattern and its relationships with the thrust system in the sub-Andean Zone.

(a) In the current petroleum system, which is characterised by structural traps in thrust ramp anticlines, faults play different and important roles in hydrocarbon migration and accumulation. In the foredeep, faults seal traps at depth, whereas migration can occur over long distances in the absence of faults,

Acknowledgements

This study has been made possible thanks to FAM (Fault and Hydrocarbon Migration), a consortium created in 1996 between various oil companies involved in exploration in the Bolivian foothills, and the IFP and French universities. The goal was to study fault hydraulic behaviour in the specific Bolivian context. This consortium was funded by Elf, Maxus and Pluspetrol, and partially by Repsol, Mobil and Exxon. We are grateful to Yacimientos Petroliferos Fiscales Bolivianos for access to data and

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