thesaotome´ deep-seaturbidite authors system …research interests focus on marine sedimentation,...
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AUTHORS
A. Viana � Petrobras, E&P, UN-EXP, 500, GeneralCanabarro St., Rio de Janeiro, 20271-200, Brazil;[email protected]
Adriano Viana is an advisor for sedimentology atPetrobras E&P, which he joined in 1986. He receivedhis bachelor’s degree in geology from the Uni-versidade Federal do Rio Grande do Sul in Brazilin 1982, and his Ph.D. in marine geology from theUniversite Bordeaux 1 in France in 1998. From 1988to 2001, he studied deep-water sedimentation in theBrazilian Atlantic margin, including the character-ization of modern deep-water depositional systems,turbidite and contour-current-controlled depositionalsystems, and geohazards assessment. In 2001, hejoined the Petrobras Santos Basin Exploration Group.He also coordinates several industry-academy jointprojects.
A. Figueiredo � Laboratorio de Geologia Marinha,Instituto de Geociencias, Universidade Federal Flu-minense, Avenida Litoranea, 24210-340, Niteroi, RJ,Brazil
Alberto G. Figueiredo, Jr. was born in Mococa, Brazil,in 1947. He is a full professor at Fluminense FederalUniversity, Niteroi, Brazil; he is also researcher ofthe Brazilian National Research Council. Albertoobtained a Ph.D. at the University of Miami in 1984and undertook postdoctoral work at the State Uni-versity of New York at Stony Brook in 1991. His majorresearch interests focus on marine sedimentation,processes and products, and shelf and deep-seaenvironments.
J.-C. Faugeres � Departement de Geologie etOceanographie, UMR 5805 ‘‘EPOC,’’ UniversiteBordeaux I, Talence 33405, France;[email protected]
Jean-Claude Faugeres graduated from Paris Univer-sity (France) where he received a third-cycle degreein sedimentology. After a seven-year stay as lecturerat Rabat University (Maroco), where he subsequentlyundertook sedimentological research on the SouthRifan series, he moved back to France at BordeauxUniversity where he obtained a Doctorat d’EtatEs Sciences in 1978. Since that time, his researchinvolved the modern deep-sea sedimentation inpassive and active continental margins with a majorinterest on the contour-current-controlled deposits.He was professor of geology since 1991 and is nowjust retired.
A. Lima � Instituto Oceanografico, USP, Praca doOceanografico, 191, 05508-900 Sao Paulo, SP, Brazil
Andrea Franca Lima is a Ph.D. student in theInstitute of Oceanography of the University of SaoPaulo, Brazil. She graduated in geology and has an
The Sao Tome deep-sea turbiditesystem (southern Brazil Basin):Cenozoic seismic stratigraphyand sedimentary processesA. Viana, A. Figueiredo, J.-C. Faugeres, A. Lima,E. Gonthier, I. Brehme, and S. Zaragosi
ABSTRACT
The Sao Tome deep-sea turbidite system, elongated parallel to the
rise of the south Brazilian continental margin, was first interpreted
as a channel-levee system resulting from contour-current activity.
Study of new seismic data permits the proposal of a stratigraphy for
the system and a new interpretation of depositional processes. Three
major depositional units have been recognized that are separated
by major erosive discontinuities. The basal unit seems to be Paleo-
cene to lower or middle Eocene, and the second one, subdivided
into two subunits, is probably upper Oligocene to middle Miocene.
Both units show superimposed north-to-south–channelized turbi-
dite systems, with supply provided directly from a channel network
that crosses the upper margin in the north. The third unit is upper
Miocene(?) to Pliocene or Quaternary and is still under predomi-
nantly gravity processes: turbidite processes in the lower and upper
subunits, and major mass-flow processes in the median subunit. The
sediment sources are located either in the north or in the south, with
sediment provided by major deep-sea channels. The base of the upper
subunit is well marked by an erosive discontinuity (late Pliocene or
Pliocene–Quaternary boundary). Impact of the contour currents is
mainly recorded as widespread erosive surfaces (seismic discontinui-
ties) correlated to global hydrological events and transparent or wavy
deposits. Because this system contains a significant amount of upper
Quaternary sands, it suggests the occurrence of petroleum reservoirs
along the rise and the Sao Paulo Plateau in the lower continental slope.
INTRODUCTION
Giant sedimentary levees are commonly observed on the world’s
deep ocean sea floor. Various processes may be involved in their
Copyright #2003. The American Association of Petroleum Geologists. All rights reserved.
Manuscript received November 15, 2001; provisional acceptance May 20, 2002; revised manuscriptreceived August 22, 2002; final acceptance December 10, 2002.
AAPG Bulletin, v. 87, no. 5 (May 2003), pp. 873–894 873
874 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
formation such as gravity flows (turbidity currents, mass flows) and
bottom geostrophic currents, with processes acting either individ-
ually or simultaneously. Giant levees occur generally in turbidite
systems or contourite drifts (bibliography in Faugeres et al., 1998,
1999; Migeon et al., 2000; Zaragosi et al., 2000) and are commonly
associated with major channels along which they are located, forming
very large channel-levee systems.
Numerous turbidite channel-levee systems have been described
since the 1970s (e.g., Normark, 1978; Normark et al., 1980; Cremer
et al., 1985; Kolla and Coumes, 1987; Hesse, 1989; Pirmez and Flood,
1995; Piper and Normark, 2001). These systems are deposited down-
slope from a canyon mouth. They commonly show a trend directed
perpendicular to the continental margin because of gravity flows
but may be more or less parallel because of the Coriolis force.
Channel-overflow processes are responsible for the lateral growth
of levees. The levee deposits may sometimes contain a significant
amount of sand interfingered in muddy deposits and may form a
good-quality reservoir for hydrocarbons (Migeon et al., 2000).
Contour-current-derived channel-levee systems are less common,
yet more examples have become available in the literature during
the last decade. Various types of contourite levees have been identi-
fied in a variety of morphological and hydrological contexts (McCave
and Tucholke, 1986; Faugeres and Stow, 1993; Faugeres et al.,
1993, 1999). In many cases, the system is elongated parallel to the
margin, as the drift levees tend to be built along the current path-
way. In such systems, the levee consists of major muddy material
and minor sands. These systems are characterized as poor oil-bearing
reservoirs, but can develop large accumulations of gas hydrates (Tu-
cholke and Moutain, 1986; Dillon et al., 1996; Drury et al., 1996).
Sandy drift levees or sheets are deposited only in a certain hydrologi-
cal and morphological setting (Viana et al., 1998), such as along the
upper slope of the Brazilian margin (Viana and Faugeres, 1998) or
in the Gulf of Cadiz (Faugeres et al., 1985; Nelson et al., 1993;
Habgoad et al., 2000).
As a consequence, the levee patterns (trends, bedforms, deposit
geometry, and lithology) vary according to the predominant process
involved. However, overlapping features commonly make the rec-
ognition of the levee-building processes difficult (Masse et al., 1998;
Faugeres et al., 1998, 1999). Such recognition is still more difficult
when both processes are interactive in an area. That is why recog-
nition of deep-sea levee-building processes remains a challenge, es-
pecially for petroleum research.
This paper is a study of an example of such deep-sea levees, the
Sao Tome channel-levee system located on the rise in the southern
Brazil Basin (Viana, 1998).
REGIONAL SETTING OF THE STUDY AREA
The Sao Tome channel-levee system is located in the southern
Brazil Basin, which lies between the Vitoria Trindade volcanic
M.S. degree on shallow seismic in coastal region.Presently, she works on the recognition of contouriteand turbidite-current processes in the Braziliancontinental margin.
E. Gonthier � Departement de Geologie et Ocea-nographie, UMR 5805 ‘‘EPOC,’’ Universite BordeauxI, Talence 33405, France
Eliane Gonthier is researcher in a Centre Nationalde Recherche Scientifique laboratory of Bordeaux IUniversity (France). Eliane obtained a Ph.D. in 1972.Since that time, she has worked on modern deep-sea sediments with a major interest on sedimentaryfacies characteristics and deposit origin and dis-tribution in turbidite and contourite systems.
I. Brehme � Laboratorio de Geologia Marinha,Instituto de Geociencias, Universidade FederalFluminense, Avenida Litoranea, 24210-340, Niteroi,RJ, Brazil
Isa Brehme is a geology professor at FluminenseFederal University, Niteroi, Brazil. She received herPh.D. at the University of Bremen in 1991. Since thattime, her major research interest focus on glacio-marine and marine deep-sea sedimentation, espe-cially in the Antarctic and the south Brazilian margins.
S. Zaragosi � Departement de Geologie et Oceano-graphie, UMR 5805 ‘‘EPOC,’’ Universite Bordeaux I,Talence 33405, France
Sebastien Zaragosi received a Ph.D. in 2001 fromBordeaux I University (France). He investigates thephysiography and Quaternary sediment distribution andprocesses of deposition of the deep-sea fans in the Bayof Biscay in response to sea level and global climaticvariations. He is now a lecturer in Bordeaux andfocuses his interest on deep-sea sand accumulationand paleoenvironments.
ACKNOWLEDGEMENTS
The research presented in this paper was conductedunder a program of cooperation between the Uni-versite Bordeaux I (France) and the UniversidadeFederal Fluminense (Laboratorio de Geologia Ma-rinha), Niteroı, Brasil. Lowrie and Kumar are grate-fully acknowledged for their reviews that helped tosignificantly improve the paper. The job done by theeditor to improve the final copy and the Englishwriting is highly appreciated. This is an UMR/EPOCCNRS 5805 contribution no. 1475.
seamounts to the north and the Rio Grande Rise to the
south (Figure 1).
The continental margin of this basin (Leyden et al.,
1976; Asmus and Guazelli, 1981; Gorini and Carvalho,
1984; Cande et al., 1988; Alves et al., 1997; Aguiar, 1997)
is a large plateau, the Sao Paulo Plateau, located on the
slope at a depth ranging from 2000 to 3400 m (Figures
2, 3). This plateau is affected by numerous halokinetic
structures related to the Aptian salt deposits and sepa-
rates the steep uppermost part of the slope from the
rise. The downslope boundary of the plateau is marked
by the Sao Paulo Plateau escarpment, about 200 m
high, that shows a north-south trend more or less par-
allel to the trend of the margin in the study area. The
escarpment corresponds to the external limit of the
thick salt sequence (Castro, 1992) and is located where
the continental and oceanic crust transition occurs. Be-
yond the escarpment, the continental rise is a more reg-
ular surface that gently dips toward the abyssal plain
and is locally disturbed by volcanic seamounts such
as Almirante Saldanha. A complex network of channels
crosses the plateau where the channel courses are con-
trolled by active diapiric structures. Beyond the escarp-
ment, these channels converge into a small number of
major channels that run across the rise (Brehme, 1984;
Mello, 1988; Castro, 1992; Miller et al., 1996; Alves,
1999). They are active channels transporting sands dur-
ing the late Quaternary (Machado et al., 1998; Viana,
1998). Locally, the escarpment is strongly eroded by
secondary channels.
Between about 22j and 24jS, a gentle accumula-
tion zone (Figures 3, 4), about 100 km long and 60 km
wide, is located at the foot of the northern part of the
escarpment. It is separated from the escarpment by a
channel-like depression. This system was originally iden-
tified in seismic profiles collected as part of the Bra-
zilian REMAC Project (Reconhecimento global da
Margem Continental Brasileira) (Asmus and Guazelli,
1981) and more recently in maps and data published
by Cherkis (1983), Mello (1988), and Castro (1992).
Viana et al. 875
Figure 1. Localizationof the study area in thesouthern Brazil Basin.
Sediment distribution on the rise was interpreted as
mainly controlled by the Antarctic bottom-water cur-
rents (Damuth and Hayes, 1977; Kumar and Gamboa,
1979; Barker et al., 1983a,b; Gamboa and Rabinovitz,
1981, 1983; Johnson and Rasmussen, 1984; Brehme,
1984; Mello et al., 1992; Mezerais et al., 1993; Masse
et al, 1994, 1996; Petchick et al., 1996; Faugeres et al.,
2002). Likewise, the system was interpreted as de-
rived from contour-current activity and was named the
Guanabara Channel and Drift (Mello et al., 1992).
This system, 3500–4000 m deep, corresponds to
the transitional zone between the North Atlantic deep
water and the Antarctic bottom water (Reid et al.,
1977; Reid, 1996; Hogg et al., 1982). The North At-
lantic deep water flows southward with a very low ve-
locity (less than 5 cm/s) at a depth of 1200–4000 m,
and the Antarctic bottom water flows northward at a
depth greater than 4000 m at a velocity not exceeding
10 cm/s in the open basin. However, recent data (Reid,
1989, 1996; DeMadron and Weatherly, 1994; Siedler
et al., 1996; Hogg et al., 1996) have shown a more
complex circulation with rapid and temporary velocity
and trend changes. Uncertainty in the paleocirculation
patterns since their initiation during the late Eocene
to early Oligocene (Kennett, 1982) makes the inter-
pretation of sediment patterns difficult. Several Ceno-
zoic hydrological events are responsible for major dis-
continuities in the deep-sea deposits, as observed at a
876 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
Figure 2. Physiography of the South Brazilian continental margin: (a) the channel network (after Castro, 1992) and the location ofthe Sao Tome channel-levee sytem; (b) 3-D view of the sea-floor morphology along the Brazilian margin off Cape Sao Tome. Note in theupper slope the Almirante Camara canyon (1) and the Sao Tome canyon (2) that provide sediments to the modern Sao Tome deep-seaturbidite system (ST-DSTS), the complexity of the submarine morphology and drainage complex over the Sao Paulo Plateau as a resultof the Aptian salt halokynesis, and, in the first plan, the Sao Paulo Plateau outer escarpment, the Guanabara Channel, and the SaoTome levee (ST-DSTS).
global scale. The Quaternary has also seen a variety of
current variations (Johnson et al., 1977; Ledbetter, 1986;
Masse et al., 1994, 1996).
DATA AND METHODS
During the BYBLOS cruise (Faugeres et al., 1998), 470
km of air-gun seismic lines and echo-sounder lines and
seven Kullenberg cores were collected in the study area
(Figure 3). These new data were used to prepare a de-
tailed bathymetric map and to determine the distribu-
tion of depositional environments in the area (Figure
4). However, the available seismic data are not suffi-
cient to map any of the facies over large areas. Corre-
lation with data from Deep-Sea Drilling Program site
515, located south of the study area, and more recent
studies in the southern Brazil Basin (Mezerais et al.,
1993; Castro,1992; Alves, 1998; see Table 1) suggest
that the sediment deposition in the study area took
place mostly during the Oligocene and Neogene, and
the basal sediments were deposited during the Paleogene
or possibly later (see age discussion in Stratigraphy).
Sao Tome Channel-Levee System Morphology
The Guanabara Channel is about 70 km long. Its width
ranges from 2 km in the north to 10 km in its central
part and 4 km in the south. It is approximately 200 m
deep with respect to the top of the escarpment and
as much as 75 m deep with respect to the levee in its
middle part. The relative depth decreases northward
and southward. The sediment accumulation area shows
a sector of maximum deposition along the channel, here
called the levee (s.s.), and a transitional area between
the levee and the rise (Figure 4).
The north-south–elongated levee (s.s.) is 70 km
long to 30 km wide. It is separated into northern and
southern parts by an east-west depression. This de-
pression is about 40 m deep and opens downslope. In
the north, the levee deepens southward, and has a short
western flank toward the channel and a wide eastern
flank gently sloping basinward. The sea floor displays
large flat areas with a few small sediment mounds scat-
tered throughout. In the south, the levee has a more
symmetric shape and regular sea floor molded by sed-
iment waves and uncommon small mounds. Here, the
Viana et al. 877
Figure 2. Continued.
top of the accumulation reaches the shallowest depth
(3500 m) and gently deepens northward.
The transitional area presents a far more chaotic
sea floor, with gullies, sediment wavelike and hum-
mocklike bedforms in the north and the middle part of
the system, and more regular wavy bedforms and west-
east–directed gullies in the south (Figure 4).
Two major deep-sea channels (about 15–20 km
wide and 40–60 m deep) supply sediments to the area.
The Macae Channel to the north (Figures 2, 4) is part
of a continuous feature (Figure 2) that connects the
continental shelf and upper slope (Almirante Camara
canyon, Machado et al., 1998; Gorini et al., 1998) to
the deep rise and the Columbia Channel (Brehme,
1984). It plays a major role in feeding the northern part
of the system. Farther south, secondary channels may
feed this area directly across the escarpment (Figure
2). The Carioca Channel (Brehme, 1984; Mello, 1988;
Castro, 1992; Alves, 1999) in the southernmost part
of the study area cross the rise close to the southern end
of the system, where our profiles cross this channel only
once (Figures 2–4). However, we suspect that such a
major channel plays a significant role on the deposit
geometry in this area. The linkage between the Carioca
Channel and the upper margin channel network re-
mains unclear. It may be linked to the Sao Tome canyon
system and/or to southern Campos basin canyons.
Neogene Deposit Geometry
Three depositional units, units I, II, and III, respec-
tively, from the base to the top of the sedimentary se-
quence (Figures 5–10) have been defined. However,
neither an acoustic basement nor a clear basal boundary
for unit I is recorded by most of the BYBLOS seis-
mic lines except for the southernmost one (Figure 7),
where a volcanic basement might be present. The total
878 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
Figure 3. Detailed bathymetric map of the Sao Tome channel-levee system and location of the seismic lines and cores (11,12,. . . 17).
Figure 4. The Sao Tome channel-levee system and the differ-ent modern depositional areas and associated channels; arrowssuggest turbidity-current pathways.
thickness of the deposits ranges from about 1 to 1.7 s
(two-way traveltime) and represents about 900–1500 m
of sediments, assuming a mean velocity of wave prop-
agation of 1800 m/s. Each of these units are bounded
by major discontinuities that are spread all over the en-
tire accumulation area.
Unit I
The basal unit I is observed in all the profiles, and it
has a mean thickness of 0.5–0.6 s. Nearly transparent
reflections form the deepest layers. In the upper part,
unit I shows high-amplitude, continuous to semicontin-
uous, parallel reflections with locally wavy geometry.
It is bounded upward by a gently erosive discontinuity
(R1) that deepens slightly southward.
In the north, there are some shallow channels and
mounded geometry (Figures 9, 10b) that seems to con-
verge southward into a major mounded depositional
system (Figure 5). This system could be elongated north
to south, as it seems to extend up to the southern end of
the study area where unit I shows a slightly mounded,
lobelike geometry (Figures 7, 11). The system axis (Fig-
ure 5) corresponds to a fairly high relief with high-
amplitude reflectors and some channel features. East-
ward and westward from the sediment high, downlapping
and offlaping reflections suggest the occurrence of lat-
eral levees that gently deepen toward lower relatively
flat areas. This geometry suggests a turbidite-perched
channel-levee system (in Bouma et al., 1985; Pirmez
and Flood, 1995). At the foot of the escarpment, evi-
dence of shallow channels is observed (Figures 5, 6c, 9).
In the southernmost part of the system (Figure 7), the
distal lobelike deposit overlays layered deposits filling
up the relief irregularities of what could be the oceanic
crust. The unit total thickness here is about 1 s, in-
cluding about 0.5 s for the lobelike upper part. In the
north, near Almirante Saldanha Seamount (Figures 4,
10a), shallow channels, probably directed southwest-
northeast, develop during the last stage of unit I.
All these patterns point out a predominantly
turbidite-depositional process, with a northern source
and a major north-south–directed system (Figure 11).
Unit II
Unit II is the thickest unit (0.5–0.95 s, 400–800 m),
and the maximum thickness is developed in a western
Viana et al. 879
*Dce = discontinuity; see text for further explanations.
Table 1. Tentative Correlations of the Seismic Major Sequences and Unconformities in the Southern Brazil Basin from PreviousPublished Works and Correlations with the Proposed Stratigraphical Interpretation for the Sao Tome Deep-Sea Turbidite System*
880 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
Figu
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depression inherited from R1 erosive surface (Figures
5, 9). This unit’s reflections are predominantly trans-
parent to chaotic. The unit is divided into two subunits
by a semicontinuous, irregular, high-amplitude reflec-
tor (discontinuity R1a) that shows erosive features in
the west and becomes more regular and undulated east-
ward (Figure 5). However, in the south, this disconti-
nuity has disappeared (Figure 7), and no subunits can be
distinguished.
Subunit IIa
The basal subunit IIa is the thickest (0.4 s, 360–400
m) in the west, close to the Sao Paulo Plateau (Figure
5). There, it shows semicontinuous reflections that,
eastward, onlap onto the channel-levee relief inherited
from unit I. That supports the occurrence of a new
north-south–feeding channel system (Guanabara Pa-
leochannels), located between the Sao Paulo Plateau
escarpment and the unit I channel system (Figure 11).
Farther east, the deposit thickness decreases (0.25 s,
230 m) and the facies becomes more or less transparent
with some tiny wavy reflections of either turbidity or
contour-current origin.
Subunit IIb
The overlying subunit IIb is thicker than subunit IIa
(as much as 0.6 s, 550 m) with a more predominant
transparent facies (Figures 5–10b). This facies is asso-
ciated with discontinuous high-amplitude reflections
scattered throughout, most of them stacked in a column-
like shape (Figure 5). Some more continuous reflections
show a divergent geometry (Figure 5) that suggests a
possible mounded deposit center similar to the unit I
system. However, such a feature is not visible farther
north (Figure 9) and south (Figure 7).
At the foot of the escarpment (Figures 5, 6c), well-
stratified, more or less discontinuous, high-amplitude
reflections form a thick lens of deposits that are inter-
digitated eastward into the transparent deposits. West-
ward, they show small-scale moats and minor channels
and levees that present no drift geometry. Such depos-
it patterns suggest the presence of active Guanabara
Paleochannels at that time, with dominant turbidity cur-
rents and little or no activity of contour currents. Far-
ther north (Figure 9), these deposits show more irregular
discontinuous reflections and lenses of transparent fa-
cies. They could be caused by either depositional-gravity
Viana et al. 881
Figure 6. Details of the BC profile (location in Figure 5): (a) active diapirlike structures associated with subunit IIIb, and subunit IIIcdeposits trapped and deformed between these structures, (b) slumped deposits. AB profile crossing Guanabara Channel (location inFigure 3); (c) seismic line and interpretation. Twt = two-way traveltime.
882 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
Figu
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processes (e.g., debris flows or turbidity currents) or post-
depositional sediment deformation (e.g., slide or tec-
tonic). Such deposits would correspond to a north-south
system trapped at the foot of a probably already existing
escarpment (Figure 11).
The upper part of the subunit is characterized by
transparent facies that are very thick toward the west,
where they fill the depression between the lenticular
system in the west and the mounded system in the east
(Figure 5). At the top, wavy reflections are widespread
(Figures 5–7, 9), which suggests sediment waves con-
trolled by contour currents.
In the southern end of the system (Figure 7), no
subunits can be defined. Most of unit II consists of trans-
parent facies associated with high-amplitude discontin-
uous reflections showing chaotic dips (hummocklike
reflections) that suggest deposit deformations induced
by argilokinetic processes or by overpressured water ex-
pulsion (Cartwright, 1994). At the base of the unit, a
lens of more continuous well-stratified reflections with
an erosive top surface is visible to the west. It could be
intrepreted as lobelike deposits linked to the unit IIa tur-
bidite system (Figure 11). Laterally to the east, the trans-
parent facies merges into high-amplitude reflections
suggesting a channel-levee geometry (Carioca Paleochan-
nel, Figure 8). That supports the activity of a southern
sediment source, during the base of unit II deposition.
In the northern end of the system, there is no clear
evidence of the occurrence of an active Macae Paleo-
channel at the foot of Almirante Saldanha Seamount.
The unit II tentative reconstruction (Figure 11) sug-
gests depositional conditions in some way similar to
those of unit I as we infer stacked north-south–elongated
systems. These systems could be fed by a major turbi-
dite supply coming from the north and by minor slides
and debris flows coming probably from the escarpment
directly. A southern minor source was active at least
at the time of lower unit II. The transparent chaotic
deposits interbedded in the turbidite systems could
have been deposited by contour currents similar to the
Columbia channel-levee system farther north (Fau-
geres et al., 2002). However, postdepositional distur-
bance by fluid overpressure might also be responsible
for this seismic facies.
A major discontinuity (R2) strongly marks the units
II and III boundary (Figures 5, 7, 9). It is underlined by
a very irregular surface showing erosive depressions (as
much as 3–4 km large, 50 m deep) and a seismofacies
change. The modern erosive Guanabara Channel is al-
ready well developed, and was probably initiated slightly
earlier (Figures 5, 6c).
Unit III
Unit III shows far more complex deposit geometry
and variations in thickness that do not exceed 0.4 s
(350 m). According to the geometry, three subunits
can be recognized.
Subunit IIIa (0–205 m)
This subunit corresponds to a major change in the sed-
iment distribution compared to unit II. It is well de-
veloped in the northeastern part of the system (Figures
9, 10b) but has not been deposited (or preserved) in the
south (Figures 5, 7). In the northernmost part of the
system (Figure 10a), these deposits are clearly related to
the Macae Channel, now an erosional-depositional chan-
nel (Clark and Pickering, 1996). They consist of high-
amplitude continuous reflections that are parallel or
divergent and downlap southward, suggesting turbidite-
overflowing processes for most subunit IIIa deposits. No
deposits in the south suggest no active southern source
of sediments (Figure 11).
Subunit IIIb (0–200 m)
This subunit is a distorted layer well developed in the
central part of the system (Figures 5, 9, 11). In this area,
Viana et al. 883
Figure 8. Details of the LA profile (see location Figure 7).Detailed deposit geometry is associated with the Carioca Chan-nel and Paleochannel. Twt = two-way traveltime.
884 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
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eltim
e.
Viana et al. 885
Figure 10. Profiles crossing the north-ern Sao Tome system. (a) IJ1 strike pro-file crossing the northernmost part ofthe Sao Tome system and the MacaeChannel and profile interpretation. (b)J1J2 dip profile crossing the midpart ofthe Sao Tome system and profile inter-pretation. Twt = two-way traveltime.
its top surface is very irregular with reliefs as much as
40 m. Transparent facies with some chaotic reflections
are predominant. Diapirlike structures, rotational blocks,
minor faults, and compressional ridges or wavy bed-
forms may occur (Figures 5, 6, 9). Locally, the struc-
tures suggest slumped deposits (Figures 5, 6a). In some
other places, the deposits may have nearly completely
disappeared (Figure 9). Most of these features may be
caused by active argilokinetic or halokinetic deforma-
tions. In case of halokinetic processes, the subunit could
correspond to a giant mass flow of salt coming from the
Sao Paulo Plateau. The diapiric processes, whatever the
886 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
Figure 11. Diagrams showing the major stages of the Sao Tome system evolution. SPPl = Sao Paulo Plateau; SPPlE = Sao PauloPlateau Escarpment; aAS = active volcanic Almirante Saldanha Seamount; AS = nonactive seamount; a = Antarctic bottom water; b =North Atlantic deep water; numbers 5–13 refer to the figure that illustrates the seismic facies and deposit geometry associated withthe environments mapped for each unit.
origin, have been active recently, as the overlying deposits
(subunit IIIc) are deformed between active diapirs (Figure
6b). Subunit IIIb could then correspond to a major
slope failure with a mass flow directed eastward (Figure
11). That could explain the central depression observed
today in the system.
Westward, at the foot of the Sao Paulo Plateau es-
carpment, the Guanabara Channel is well developed,
with deposits showing both high-amplitude, continuous
reflections (probably turbidites) and chaotic to transpar-
ent reflections (slide, debris flows[?]) (Figures 5, 6c, 9).
In the southern end of the system (Figure 7), subunit
IIIb presents no evidence of postdepositional deforma-
tion or sliding, and the thickness drastically decreases.
The deposits show discontinuous to chaotic reflections
in the west and merge eastward into more continuous
and undulated reflections. Farther down, the deposits
are bounded by the Carioca Channel that erodes the
Sao Tome levee deposits down to unit II (Figure 8).
Most of the channel erosion is synchronous of subunit
IIIc basal erosive event (R3). However, the channel was
probably active during subunit IIIb deposition and could
have provided sediment to the system.
In the northern end of the system, the deposits pinch
out westward (Figure 10b) close to Guanabara Channel
and extend eastward (0.2–0.3 s in thickness). Stratified
reflections similar to that of subunit IIIa are associated
with minor lenses of transparent facies similar to that
of the mass flow in the central depression (Figure 10).
They probably correspond to mass-flow sediments inter-
digitated into turbidites overflowing the Macae Chan-
nel (Figure 10a).
Subunit IIIb sediments seem then to have been sup-
plied, for one part, by the very active Macae Channel
in the north and, for another part, probably by the
Carioca Channel in the south (Figure 11). The origin
of the sediments that form the slide deposits, however,
remains speculative.
Subunit IIIc
The major discontinuity (R3) at the base of subunit IIIc
shows reliefs both inherited from the subunit IIIb top
surface and from erosion at that time. A drastic erosion
affects the southern part of the Guanabara Channel (Fig-
ures 5, 6c), which cuts down throughout subunits IIIb
and IIb. Farther north, the channel erosion decreases pro-
gressively (Figures 9, 10b), suggesting processes caused
by northward-directed turbidity currents. That fits with
the eastward minichannel migration observed in the chan-
nel infill (Figure 5). In the south, active erosion by the
Carioca Channel also occurs (Figures 7, 8) as mentioned
previously. Only gentle erosion takes place in the Macae
Channel at that time (Figure 10a).
The southern Guanabara Channel infill shows a
maximum thickness (0.25 s; as much as 250 m), and the
adjacent levee, only thin deposits (0.05 s); the chan-
nel plays as a sediment trap for the turbidite supply.
Northward, the deposit thickness decreases along the
channel (0.15 s), but increases relatively on the levee
(0.09 s). That suggests deposition by turbidites over-
flowing the levee (Figures 5, 9). In the north (Figure
10b), the channel deposits increase again slightly (0.12
s). Such sediment distribution is consistent with a ma-
jor source in the south (Carioca Channel) and a minor
source in the north (Macae Channel) (Figure 11).
The deposits consist mainly of well-stratified re-
flections interpreted as turbidites. They form locally a
continuous cover on the levee (Figures 5, 9) or pounded
turbidites that fill in small troughs between mounded
(diapiric?) structures (Figure 6b). Wavy bedforms north
and south of the Carioca Channel (Figure 7) could be
turbidity or contour-current sediment waves.
During the deposition of subunit IIIc, west- to east-
directed turbidite systems have controlled the sedi-
mentation, and the overflowing processes are far more
active in the south than in the north.
The predominance of turbidite processes is well
demonstrated for the Quaternary sediment deposition
by the Kullenberg core data (Viana, 1998; Gonthier et al.,
personal communication). The Guanabara Channel de-
posits consist of thick (as much as 30 cm) sandy turbi-
dites (median diameter as much as 140 mm) and debris
flows interbedded in hemipelagites (Figure 3, core 11).
On the levee (cores 12, 15, and 13), the deposits are com-
posed of frequent (5 sequences/m), thin (centimeter-
scale), sandy-silty (mean diameter as much as 74 mm) to
silty-clayey turbidites (as much as 25 mm). The turbi-
dites are interbedded in hemipelagic and pelagic de-
posits. The ratio of sandy silt to mud ranges from 0.10
to 0.22. These deposits result from turbidity currents
overflowing the Guanabara Channel and come from
both southern and northern sources. Similar deposits are
present in the transitional zone (cores 13, 14, 16, and 17).
However, in this area, the turbidite frequency may be
slightly higher (as much as 6 sequences/m), and the ratio
of sandy silt to mud is as much as 0.29. These features
suggest that the turbidites in the transitional zone did
not overflow directly from the Guanabara Channel but
from other channels (Carioca and Macae channels). No
striking evidences of contour-current–controlled deposits
are observed in these cores. The deposits that indicate
the impact of contour current are yellowish, brownish,
Viana et al. 887
silty-clayey beds associated with erosional surfaces and
black laminations with manganese oxides.
DISCUSSION
Sedimentary Processes
The predominant sedimentary processes involved in
the building of the Sao Tome system are downslope
processes, including major turbidity currents. They form
(Figure 11) (1) north-south channel-levee systems and
lobes (units I and II), (2) overbank deposits associated
with major west-east channels (subunits IIIa and IIIc),
(3) major mass flow (giant sliding) (subunit IIIb), and
(4) small-scale slides or debris flows (units II and III)
originating probably from the Sao Paulo Plateau escarp-
ment. The seismic data show little reliable evidence of
contour-current control on the deposit distribution; only
some wavy reflections observed at the top of subunits
IIa, IIb, and IIIb, as well as IIIc southeastward, could
have been formed by such currents.
However, we know that the study area has been
swept by the active Antarctic bottom-water and North
Atlantic deep-water circulation during the Paleogene to
Neogene. Then, the question is What is the real impact
of contour-current processes in such an area that has
suffered such active turbidite processes, and how was
it recorded?
The widespread discontinuities appear to be ero-
sive surfaces that represent time lines. In a turbidite
system, major discontinuities are commonly discon-
tinuous and diachronous surfaces, as they are mainly
formed through channel migration. That is why the dis-
continuities observed here seem to have been formed
by contour currents (Faugeres et al., 1999) instead of
turbidity currents. Consequently, we have tentatively
correlated them with the major hydrological events
known at the global scale.
The transparent facies of unit II has been inter-
preted elsewhere in the southern Brazil Basin as con-
tourite deposits (Castro, 1992; Alves, 1999; Faugeres
et al., 2002). Why not a similar interpretation for the
Sao Tome levee? In our study area, as these deposits are
clearly associated with turbidite systems, the role of the
contour current could have mainly concerned the re-
distribution of the fine-grained sediment pirated from
turbidite plumes. However, no seismic evidences sim-
ilar to those in the Antarctic margin (Rebesco et al.,
1997) are present here.
Stratigraphy
We know that during the Paleogene–Neogene, events
of very intense Antarctic bottom-water and North At-
lantic deep-water circulation occurred several times:
Paleocene–Eocene boundary (50–55 Ma), early to mid-
dle Oligocene (40–34 Ma), end of the Oligocene (25
Ma), during the late Miocene (12–8 Ma) and late
Pliocene (3–2.5 Ma) (e.g., Kennett, 1982; Johnson,
1983; Mountain and Tucholke, 1985; Tucholke and
Mountain, 1986; McMaster et al., 1989; Locker and
Laine, 1992; Berger and Wefer, 1996). These episodes
have been recorded all over the world’s oceans in the
form of major erosive surfaces and a large hiatus in the
sediment record. We have collected the available data
concerning the records of these events in the southern
Brazil Basin (DSDP site 515, Figure 1; Barker et al.,
1983a,b; Gamboa et al., 1983; Viana et al., 1990;
Castro, 1992; Alves, 1999; Mezerais et al., 1993). All
of these data have been summarized and correlated
with the Sao Tome system data (Table 1).
The most reliable correlation that clearly arises
is between the R2 discontinuity and unconformity
IV of site 515, DVI of Castro, R4 of Mezerais, and D4
of Alves, corresponding to the middle to late Miocene.
This event is marked by a high-amplitude reflector
all along the east Brazilian margin dated at 10.8 Ma
(reflector Cinza of Viana et al.,1990). The age of the
underlying and overlying discontinuities is more spec-
ulative. However, as shown in Table 1, we propose the
following assumed stratigraphic frame for the Sao Tome
system: unit I = Cretaceous(?)–Paleogene; unit IIa =
upper Oligocene; unit IIb = lower to middle Miocene;
subunits IIIa and b = upper Miocene(?)–lower Plio-
cene; subunit IIIc = upper Pliocene(?)–Quaternary.
Sao Tome System Evolution
A six-stage scenario may be proposed for the system
growth since the Paleogene.
Stage 1 (unit I, 450-m-thick deposits, Paleocene[?]–
Eocene) deposits seem to correspond to a major turbi-
dite depocenter directed north to south (about 40 km)
along the middle part of the study area. It merges south-
ward into a lobelike accumulation. Sediments were sup-
plied from the northern plateau. Such a deep turbidite
system fits with the abundant terrigenous supply, tur-
bidite complexes (Barracuda/Caratinga of Assis et al.,
1998), and large-scale debris flows (pebbly sandstone
of Guardado et al., 1990) present at that time in the
888 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
upper slope. This stage stopped with the R1 erosive
event (late Eocene to Oligocene).
Stage 2 (subunit IIa, 400-m-thick deposits, late
Oligocene) deposition was still controlled by a north-to-
south–directed turbidite system, but the system shifted
westward. A minor source was probably active in the
south. This stage corresponds to a global sea level fall
during the late Oligocene (Chatian–Rupelian, 35 Ma)
and the huge amount of sediment delivered into the
deep sea (Vail et al., 1977; Haq, 1991). Eastward, trans-
parent reflections could correspond to sediment redis-
tributed by contour currents. A second major event (R1a)
(Oligocene–Miocene boundary) is responsible for local
erosion and wavy bedforms.
Stage 3 (subunit IIb, 550-m-thick deposits, early to
middle Miocene) deposits seem to have been controlled
by contour currents and have transparent reflections.
They are associated with a well-stratified turbidite sys-
tem, restricted at the foot of the escarpment, and still
directed north to south. A Sao Tome paleosystem would
have been initiated at that time. This stage is synchro-
nous with an episode of low sea level and abundant
sediment supply on the upper slope (Castro, 1992; Car-
minatti and Scarton, 1991; Souza Cruz, 1995). A third
erosive event (R2) marks the end of the stage (middle/
upper Miocene boundary).
Stage 4 (subunit IIIa, late Miocene[?] to early Pli-
ocene) shows a new sediment-distribution pattern with
a maximum thickness of 250 m in the north and no
sediment in the south. The sediment still came from
the northern plateau but converged into a west-east
major Macae Channel that had just been formed on
the northern boundary of the system. Only turbidity
currents overflowing from this channel fed the system.
There is no evidence of a significant southern source of
sediments.
Stage 5 (subunit IIIb, [?] late Neogene) is marked
by a major slope failure and a giant mass flow in the
central part of the system. However, the northern
source is still active, with turbidite overflowing from
the Macae Channel. The southern source becomes active
again, with turbidites overflowing the southeastern end
of the system from the erosive Carioca Channel. The
R3 event at the top (Pliocene/Pleistocene boundary)
is responsible for drastic erosion caused by turbidity
currents and possibly contour currents. It induces the
modern system morphology and fits with active ero-
sion on the upper slope (Viana et al., 1999).
During Stage 6 (subunit IIIc, late Pliocene(?) to
Quaternary) deposition, the major source of sediment
was in the south. The sediments were first transported
into the deeply eroded southern end of the Guanabara
Channel where ponded turbidites were deposited. Tur-
bidity currents flowed northward along the channel and
overflowed onto the top of the levee. Probably, another
major part of the available supply flowed downward
along the Carioca Channel from where it may have
overflowed onto the southern system. Some sediments
were also provided by the Macae Channel.
Sediment Origin and the Sea Level and Tectonic Control ofSedimentary Processes and Deposits
Most of the sediments that were deposited in the Sao
Tome system came from the upper part of the margin
after crossing the Sao Paulo Plateau. There were at least
two major drainages: one in the north, with sediments
transported by the Almirante–Itapemirin canyon net-
work (Figure 2b) and connected farther down with
Macae Channel, and one in the south, with sediments
transported through Sao Tome or Campos basin south-
ern canyons beyond the plateau to the Carioca Chan-
nel. Variations in the impact of these sources upon
sedimentation may be explained by variations of sea
level and the location of the major river mouths, the
channel network on the plateau caused by sedimentary
processes or salt-diapiric activity, and the continental
margin trend and trend of the dip caused by tectonic
and volcanic activity.
Unit I (Paleogene(?)–Eocene) corresponds to a pe-
riod of high volcanic activity in the southern Brazil
Basin (Cordani and Blazekovich, 1970; Fodor and Hanan,
2000), which could have controlled the deep-sea to-
pography and favored the triggering of sediment de-
livery. The rise of the Almirante Saldanha Seamount
and Vitoria Trindade chain (40–50 Ma) north of the
study area may have induced a southward dip of the
sea floor and generated north-south turbidite systems
during unit I and II deposition. Later during unit III
deposition, the decrease of the volcanic activity may
have caused the sea floor to die to the east, which is the
dip of the present margin. At that time, the downslope
currents that crossed the rise were directed eastward,
excavating the Macae Channel. The high-amplitude
to transparent reflectors and prolonged sea-floor echo
observed inside that channel suggest coarse-grained
sediment transport. Sand supply by the northern chan-
nel network upslope was previously demonstrated by
Machado et al. (1998).
Modifications of Sao Paulo Plateau morphology
may have occurred throughout the Cenozoic because
of salt diapirism. Diapirism would have induced shifts
Viana et al. 889
in the course of the channels as they crossed the es-
carpment. These processes may explain the variations
of the sediment volume delivered to the north and to
the south of the study area and the variation of the pre-
dominant source during deposition of unit IIIa (Macae
Channel northern source) and unit IIIc (Carioca Chan-
nel southern source).
A direct relationship between sea level fluctua-
tions and the volume of deposits is difficult to address,
because of the low resolution of the available seismic
lines and probable interaction between the relative sea
level and bottom-current activity. Based only on the
upper Quaternary data, major periods of sediment
input to the deep sea via turbidity currents seem to be
related to sea level falls (Gonthier et al., personal com-
munication). During unit IIb deposition (early to mid-
dle Miocene), the widespread transparent seismic facies
could be associated with bottom-current activity. At this
period, huge sedimentary drifts developed at the upper
margin (Souza Cruz, 1995). That also corresponds to a
major sea level fall, which provided the basin with a
large quantity of sediment (Carminatti and Scarton,
1991; Souza Cruz, 1995; Appi, 1995).
Hydrocarbon Implications
Extremely deep-water prospects (i.e., depths greater
than 3000 m) have not yet been targeted in hydrocar-
bon exploration along the southeastern Brazilian mar-
gin and the Santos, Campos, and Espırito Santo basins.
According to Mello et al. (2001), the origin of the hy-
drocarbons in those sedimentary basins is related to
Barremian anoxic lakes that ranged from freshwater to
saline, Late Cretaceous anoxic global events, and a Ter-
tiary marine delta complex, the occurrence of which is
presently seen only in the Espırito Santo Basin. Most of
the oil discoveries are related to turbidite reservoirs
formed after deposition of the Aptian salt. These res-
ervoirs were charged with hydrocarbons formed in la-
custrine source rocks that were deposited before salt
deposition.
As stated previously, the seismic-stratigraphic anal-
ysis indicated that an Albian to Quaternary sequence
was deposited on the outer southeastern Brazilian mar-
gin, including the continental rise off the Sao Paulo
Plateau. The continental rise in the study area develops
basinward from the foot of the plateau escarpment,
above an oceanic crust formed after the continental
breakup at the Neocomian. Sedimentation processes
that followed the breakup phase included the trans-
gression of the basin margins by thick marine carbonate
successions (Armentrout, 1999). That phase is followed
by the Late Cretaceous and Tertiary reactivation of
older crustal structures, resulting in strong onshore up-
lift and exhumation, an increase in sediment supply to
deep-water settings, and offshore subsidence, increasing
the sea-floor gradient and accelerating the sediment-
rich gravity flows. Thus, thick terrigenous clastic wedges
prograded into the basin from the middle to Late Cre-
taceous, forming the Namorado turbidites in Campos
Basin and the Ilhabela turbidites in Santos Basin. The
extensive Late Cretaceous progradation (Pereira, 1990;
Cobbold et al., 2001) suggests that a large quantity of
gravity-flow sediments could have reached a very dis-
tal setting.
Meisling et al. (2001) suggested that the deep-water
plays in the southern Brazilian margin are influenced by
the presence of the widely distributed lacustrine, rift-
related source rocks. However, we think that the devel-
opment of a thick column of marine sediments above
an oceanic crust can also provide a complete petroleum
system, as it does in other world-class oil-prone basins
such as the Gulf of Mexico (Roberts and Reilly, 2001)
and the western margin of Africa (Costa et al., 2001).
This system would include (1) the Albian or Cenoma-
nian to Turonian marine source rocks related to anoxic
events, (2) thermal efficiency of the oceanic crust pro-
viding heat to mature the source rocks, as observed in
the Red Sea where geothermal gradients range from
3 to more than 12jF/100 ft (�16 to �11jC/30.5 m)
(Clifford, 1986), (3) the potential for vertical and lat-
eral migration pathways through accommodation faults,
oceanic crust faults, and porous, coarse-grained turbidite-
carrier beds, (4) the presence of turbidite reservoirs,
mainly those related to the Late Cretaceous and lower
Tertiary, similar to the Holocene examples in the study,
and (5) efficient hydrocarbon-charging mechanism in
a thick, mud-rich, deep-marine system.
Following the above statements, we can expect the
development of such a sand-rich turbidite petroleum
system in the study area. In turbidite systems, channels
and lobes are the features most rich in sand and com-
monly form oil reservoirs. Roncador field, recently dis-
covered in Campos Basin, is located at a depth ranging
from 1700 to 200 m and is about 130 km upslope of our
study area. Its reservoir rocks are Campanian to Mio-
cene (Guimaraes et al., 2001). The lower reservoirs
include coarse-grained turbidites with channel-fill con-
glomerates and coarse sandstones (30% porosity and
one- to three-dimensional permeability). Upper reser-
voirs consists of confined and unconfined lobes and
890 The Sao Tome Deep-Sea Turbidite System (southern Brazil Basin)
have porosities ranging between 29 and 33% and per-
meabilities between 400 and 700 md (Guimaraes et al.,
2001; Barroso et al., 2000). Those reservoir features
indicate the high energy of the feeding system and con-
firm the possibility of delivering sand into deeper water
in the direction of our study system, as demonstrated
previously in this study.
In the study area, we mainly expect reservoirs of
the turbidite-levee type in addition to possible lobe and
channel reservoirs. Turbidite levees commonly consist
of thin-bedded deposits and are developed over a large
area. They are known to be gas-prone reservoirs (Pea-
kall et al., 2000) and have a net sand percentage ranging
from 30 to 55% (Kendrick, 1999; Field et al., 2000).
The existence of good lateral reservoir continuity in levee-
hosted sheet sands has also been noted by Kolla et al.
(1998). The presence of such widespread, thin, silty-
sand layers is expected in the studied system. These
layers would have formed mostly in the periods that
followed huge margin sediment delivery, as suggested
by our interpretation of the available cores and seis-
mic lines.
Because of the great water depths involved, such
a geologic setting still remains unexplored along open
oceanic margins. Major geologic uncertainties remain,
including the thermal state of potential source rocks
and the preservation of original fabric-supported po-
rosity as stated by Roberts and Reilly (2001) for the
deep-water plays of the Gulf of Mexico. Besides those
uncertainties, engineering and economic challenges in-
volving exploring and producing in water depths greater
than 2500 m still remain to be overcome.
CONCLUSION
The Sao Tome channel-levee system is located on the
rise of the South Brazilian margin. It is composed of the
elongated north-south Guanabara Channel, parallel to
the margin trend, at the foot of the Sao Paulo Plateau
escarpment, and a fairly flat levee adjacent to the chan-
nel that deepens eastward. It was first interpreted as a
system built by contour currents derived from the Ant-
arctic bottom-water circulation. Study of new seismic
data allowed us to reconstruct the system stratigraphy
and to propose a new interpretation of the predomi-
nant depositional processes.
1. Three major depositional units, which were divided
in subunits, have been recognized. They are separated
by major erosive discontinuities.
2. Gravity processes are predominant in the system
sedimentation. Unit I (Cretaceous[?]–Paleocene) is
characterized by a north-to-south–channelized tur-
bidite system. The overlying unit II is composed of
two subunits: lower to middle Miocene subunit IIb
with basal discontinuity R1a and upper Oligocene
subunit IIa with basal discontinuity R1. It shows
several superimposed turbidite channel-levee sys-
tems still elongated north to south that shift west-
ward compared to unit I. Most of the supply seems
to be brought along by a channel network that
crosses the upper part of the margin in the north of
the system. A minor southern source of sediment
may have been active at least during deposition of
lower unit II. Unit III (upper Miocene(?)–Pliocene–
Quaternary) at the top of the series has a complex
geometry with three subunits stacked on a basal
erosive discontinuity (R2). Turbidite processes are
still predominant during subunits IIIa and IIIc, with
supply coming either from the north (Macae Chan-
nel, subunit IIIa) or from the south (Carioca Chan-
nel, subunit IIIc). In between, subunit IIIb corre-
sponds to a major mass flow that affects the central
part of the system. The base of subunit IIIc corre-
sponds to a major erosive discontinuity (R3).
3. Impact of the contour currents linked to the Ant-
arctic bottom water or the North Atlantic deep water
has been recorded in the form of widespread ero-
sive surfaces (discontinuities R1 to R3) correlated to
major hydrological events known at the scale of the
Brazil Basin and the world ocean, such as the middle
to upper Miocene event (R2) and the upperEocene(?)–
lower Oligocene event (R1). Transparent facies of
unit II and some wavy bedforms of unit III are thought
to partly correspond to contouritic deposits.
4. The Guanabara Channel levee morphology and pro-
cess of deposition seems to have been initiated dur-
ing the early to middle Miocene (unit IIb), where
evidences of channelized deposits have been observ-
ed at the foot of an already existing plateau escarp-
ment. However, the modern system seems to have
been definitely established above the R3 discontinui-
ty (upper Pliocene or Pliocene–Quaternary boundary).
5. An along-slope trend of the channel-levee system is
here associated with gravity processes. Such a trend
might be controlled by faults involved in the south-
ern Brazil Basin oceanic expansion and by the plateau
escarpment caused by the Aptian salt diapirism.
6. Presence of fine-grained, sand-silt turbidites in Quater-
nary sediments suggests the deposition of signifi-
cant sand bodies at the scale of the whole Sao Tome
Viana et al. 891
turbidite system and potential hydrocarbon reser-
voirs in the deep, south Brazilian margin, especially
in the Sao Paulo Plateau.
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