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Closing the gap on Mesozoic extensional tectonics: the Torre
Poglina Lias carbonate system, western Sardinia
CHARLES R. SINGER1
1Department of Earth Science and Engineering, Imperial College London
ABSTRACT
In western Sardinia, a Lower Jurassic carbonate tempestite section exhibits a series of NE
dipping listric faults. Identification of lateral thickness variations within the rotated hanging
wall blocks coupled with erosional intersections of marker horizons provides new evidence for
syn-sedimentary faulting in the Lower Jurassic. A SE stereographic tensional regime supports
the magnitude and direction of extensional tectonics in this chronostratigraphic interval
following restoration attributed to the counter clockwise rotation of the Sardinian-Corsican
block. A comparison with stratigraphic sections and structural orientations of eastern Sardinia
and the French Maritime Alps is made, attempting to improve the continuity in reconstruction
of the Western Tethyan margin with implications for an extensional regime on hydrocarbon
bearing Lower Jurassic source rocks.
INTRODUCTION
In Western Sardinia, a sequence of Jurassic to
Cretaceous carbonates overlies post-Hercynian
Permian and Triassic siliciclastics and
transgressive marine evaporites associated with
localised basin subsidence. This cover represents
the first (Early Jurassic) Mesozoic sedimentary
cycle in western Sardinia.
Prior to Early Miocene anticlockwise rotation
of the Corsican-Sardinian block, attachment of
Sardinia to mainland Europe during the
Mesozoic provides constraints with the
geodynamic evolution of the French Maritime
Alps (Stanley & Mutti, 1968). Palaeogeographic
evidence of the Jurassic and Cretaceous periods
highlights a large and spatially continuous
carbonate megabank which occupied vast areas
of the west-Mediterranean, as well as significant
portions of Adria (Cherchi & Schroeder, 1985).
However, closer reconstructions of restorations
reveal the gradual westward propagation of the
Neo-Tethys sea-floor spreading axis during the
Late Triassic to early Jurassic. This is proposed
to pre-date opening of the central Atlantic and
the Piedmont segment of the oceanic Tethys
(Ricou, 1994). Submergence produced isolated
shallow water carbonate shelves sheltered from
terrigenous clastics by deeper troughs and
plateaus sharing affinities to the modern
Bahamas archipelago (Bernoulli & Jenkins, 1974;
Ziegler, 1988).
The aim of this paper is to provide evidence
for improved temporal and spatial resolution of
Lower Jurassic extensional tectonics associated
with the coeval opening with the Alpine Tethys.
The results of direct field observations in
western Sardinia attempt improve the accuracy
of geographic restorations of past tectonic
regimes across the French Maritime Alps and
eastern Sardinia and provide further support
against general consensus of tectonic stability in
the Jurassic (Costamagna, 2015; Dardeau, 1988).
The implications of sediment accumulation and
extensional faulting on potential Liassic
hydrocarbon deposits in the proximity of the
central Mediterranean are discussed (Di Cuia &
Riva, 2016). Focus is placed on a proximal
marine carbonate succession composed of
argillaceous limestones belonging to the Torre
Poglina Lias located 7 km south of the town of
Alghero (Fig. 1). This is where the formation is
best developed both spatially and temporally.
METHODS
Geological mapping in comparison to
surrounding Jurassic and Cretaceous carbonate
2
deposits is undertaken with close examination on
sedimentological characterisation, facies
interpretation, and structural analysis. Adjacent
to the small town of Torre Poglina, an
abandoned quarry provides a well-exposed
succession of carbonate lithologies with evidence
for alpine compressive tectonics and extensional
faulting; the latter providing the basis for
detailed assessment of syn-sedimentary
structures. Interaction between sedimentary
facies and normal faulting has allowed a localised
palaeoenvironmental reconstruction to be
developed.
Fault measurements are collected using a
Suunto Compass Clinometer MC2 along a SW-
NE transect along the quarry face with
examination of slickenside orientations and slip
directions. Strike errors are likely to have arisen
when the compass datum line was not aligned
horizontally coupled with misalignment due to
their indistinction. Repeated observations and
averaging aids to overcome this problem
allowing stereographic projection. Woodcock
(1976) concluded that high errors (>5‫ﹾ‬) could
arise from trend measurements on steeply
plunging lineation’s.
Scaled photographs of sedimentary structures
and fault interaction are collated to assess their
relationships within the depositional system.
Images collected of sedimentary structures are
on the centimetre scale and hence the scaling
factor associated with parallax error is minimal
between the top and bottom of investigated
sequences. Annotated digitised field sketches of
the quarry face pose higher degrees of scaling
errors of approximately 2 calculated between the
top and bottom of the quarry face in accordance
to the rules of triangulation. Sections of interest
are predominantly towards the base of the
outcrop minimising scaling errors associated.
RESULTS
The quarry exposure forms a 70 m by 13 m
high outcrop of massive sub-horizontal
carbonate beds with distinctly faulted marker
horizons 0.4 to 1.4 m thick interbedded with a
series of variably grey laminated micrites. The
latter lithofacies is represented at its base by dark
grey bioclastic grainstones up to 5 cm thick
composed of laterally aligned fragmented
bivalves 3 – 4 mm in length. These allochems
typically concave downwards with occasional
locking with adjacent non-inverted shells (60%
vol.) set in a depleted mud matrix (Fig. 2a). In its
lower part, a basal erosional surface marks a
contact with beige micrites belonging to the
underlying sequence. The basal part passes up
sharply into gradationally fining carbonate silts
with indistinct sedimentary structures.
Laminations become increasingly defined and
closely spaced with traces of hummocky cross
stratification existing in the upper parts of each
sequence up to 4 cm in amplitude (Fig. 2b).
Compilation of fault plane measurements and
slickenside orientations are denoted in figure 3a.
Figure 1. Regional and local study map. General formation ages and spatial relationships mapped with investigated sections
highlighted.
3
Fault planes are plotted and an average plane
calculated to correlate slickenside data. The
directions of present fault planes are closely
clustered towards the NE with an outlier
orientated towards the ENE aligning with the
slickenside orientations. Through accounting for
the 95‫ﹾ‬ counter clockwise rotation of the
Sardinian block defined using palaeomagnetic
evidence of Advokaat et al. (2014), a restored
stereonet is constructed with principal vector
directions displayed using data concentration on
a restored rose diagram plot (Fig. 3b; Fig. 3c). A
mean displacement towards the SE is shown.
A digitised field sketch is presented using
computer overlay of scaled photographs (Fig. 4).
Distinct marker horizons and fault intersections
are highlighted to provide direct observation of
potential sediment thickening within fault
hanging walls. A series of NE verging synthetic
listric faults dominate the quarry face varying
significantly in length from sub-metre up to 10
m with conjugate antithetic faults steeply dipping
towards the SW producing uplifted horst blocks.
Maximum fault dips reach up to 70‫ﹾ‬. The
majority of faults are concentrated within the
bottom half of the quarry exposure with several
protruding to intersect an upper brown bed used
Figure 2. Torre Poglina Lias deposits. (a) Succession composed of bioclastic grainstones in the lower part fining upwards into
laminated micrites. (b) Hummocky cross stratification.
4
Figure 3. (a) Stereographic projections of present day fault and slickenside orientations and (b) restored projection corresponding to
~95‫ﹾ‬ counter clockwise rotation (Avokaat, 2014). (c) Restored rose plot representing mean trends of fault planes and slickensides.
a
b
c
5
Figure 4. Scaled photograph of quarry exposure and overlain digitised field sketch along studied transect. A prominent central grey
marker horizon has been used to assess syn-sedimentary thickening.
6
as a further marker horizon beneath alluvium
cover. The listric nature of faults is noted with
increasing angle between the vertical with depth
and appear to flatten to a lower detachment
horizon comprised of a poorly sorted 20 cm
thick fault breccia composed of angular micrite
clasts up to 25 cm. An internal duplex structure
detaching on the lower breccia sequence
consists of NNW-NW verging fault striations,
perpendicular to those associated with synthetic
listric normal faults. The presence of bedding
parallel styolites with amplitudes up to 2 mm
support lithological discontinuity.
The magnitude of dip of the beds is strongly
rotated within the hanging walls of successive
normal faults in comparison to sub-horizontal
laminae preserved towards the top of the
exposure. Beds are recorded to dip as much as
25‫ﹾ‬ towards the SW with the inclination of strata
reducing towards the southern end of the
outcrop associated with decreased fault
concentration.
Associated displacements are also variable,
but range only to several tens’ of centimetres. A
positive correlation of the magnitude of
displacement to fault distance is presented in
figure 5. These offsets produce lateral thickness
variations along a central grey marker bed. Over
the region studied, the unit reaches a maximum
thickness difference of approximately 0.93 m
with evidence for 0.35 m of thickening across a
single normal fault (Fig. 4). Thickness variations
of marker horizons beyond the transect become
too indistinct to accurately measure.
Underlying laminae exhibit evidence for oblique
intersection with greater degrees of rotation
than the truncating marker horizon (Fig. 4).
DISCUSSION
The data presented here provides improved
constraint on the temporal extent of Jurassic
rifting episodes, with evidence from direct
observations to supplement compiled
palaeogeographic reconstructions.
Lithofacies
The sedimentological characteristics of the
Torre Poglina Lias reflect deposition within
shallow, near-shore carbonate producing seas.
The presence of an erosive basal bioclastic
grainstone passing upwards to normally graded
argillaceous silts and laminated micrites is
analogous to turbidite deposits formed by
density driven flows on shallow continental
shelves. The repeated truncations of upper
planar laminae with successive cycles represent
episodic sedimentation phases triggered by
pulses of sediment instability (Meiburg &
Kneller, 2009). However, identification of
hummocky cross stratification is believed to be
diagnostic of storm-dominated shallow marine
environments forming above the storm wave
base, typically around 30 m in modern
carbonate settings (Cheel & Leckie, 2009).
Recent published data from Yang et al. (2006)
has provided further evidence that HCS
wavelength is controlled by the bottom orbital
diameter (d0) of oscillatory wave motion,
implying the maximum size of HCS sets should
increase with decreasing water depth; according
to the relationship:
λ ≈ 0.75 d0
The centimetre scale magnitude of hummocks
observed within the Torre Poglina Lias suggests
deposition offshore of the surf zone. The
absence of overlying ripple cross laminations
and underlying fragmented shell beds support
an interpreted proximal to intermediate
carbonate tempestite sequence (Fig. 6; Fig 7).
Figure 5. Graph constructed of the magnitude of
displacement in comparison to the perpendicular distance
between fault segments along the length of the studied
transect (Fig. 3).
7
Figure 6. General sketch of interpreted stratigraphic sequence
of the Torre Poglina Lias, western Sardinia.
Extensional Structure
Collaboration of structural features and
quantifiable bed thickening variations support
the presence of syn-sedimentary deposition.
Analysis of a grey marker horizon exhibits
significant thickness variations along a lateral
transect with nearly a metre scale variation in
vertical accumulation. The rotation and
thickening of beds into the hanging wall of
listric faults coupled with discrete erosional
truncations provides unequivocal evidence for
syn-rift facies (Fig. 4). Calcite filled fractures up
to 5 cm in length orientated parallel to
macroscopic faults highlights the influence of a
tensile regime even on small scale sedimentary
deposition. Presence of a detachment horizon
comprised of interpreted basal slump deposits
also displays an internal horse structure.
Slickenside striations suggest a WNW transport
direction, approximately perpendicular to the
vergence of the extensional regime. Hence, this
could represent an inverted extensional duplex
structure associated with Alpine orogenic events
further supported by a gently folded antiformal
structure to the north of the section. Interaction
between these tectonic episodes lies beyond the
scope of this paper.
Analyses of restored stereographic and rose
diagram projections strongly support a NW-SE
tensional regime producing a series of
extensional listric faults presently dipping
towards the NE. A component of oblique slip is
noted through mean vector offsets between the
average planes and slickenside orientations
approximately equal to 50‫ﹾ‬. The variability in
fault displacement direction with a dominant
oblique nature is likely related to the localised
linkage of previously unconnected fault
segments (Dawers & Anders, 1995). Cartwright
et al. (1996) emphasised the displacement
decrease on one fault segment is balanced by a
sympathetic increase on another. Figure 5
denotes a correlation between lateral fault
distance and offset magnitude. Within the
studied section, closely spaced faults exhibit
reduced displacements suggesting these may
have experienced progressive linkage and strain
uptake during formation. Fault concentrated
regions further exhibit the thickening of
sediments which could suggest implications of
strain distribution maintaining accommodation
space for sediment build-up prior to migrations
in the loci of strain accumulation.
The interaction between structural
development and sediment deposition is
proposed through bed morphology and
sedimentary structures. Erosional intersections
may suggest the structural involvement in
localised subsidence and uplift to subaerial
exposure. Constraints on data collection means
subsidence rates and magnitudes are difficult to
ascertain solely from a 2D transect. Myrow &
Southard (1996) discussed the catastrophic
introduction of sediments as a result of
earthquake activity. The non-uniformity in the
thickness of tempestite deposits throughout
geological history coupled with changes in the
fluctuations of storm intensity corresponding to
global environmental supercycles, means fault
movement within the syn-sedimentary
succession should not be ruled out as a
triggering mechanism (Ito et al. 2001).
However, the low subsidence suggested by the
sedimentary record and small degrees of
thickening, absence of large scale tectonic
disturbances and presence of shallow marine
HCS suggests influence of storm-induced waves
as a more likely scenario (Durmas & Arnott,
2006).
IMPLICATIONS
The prospect of active extensional tectonics
in the Lower Jurassic period aids understanding
of continental assemblage and restorations of
palaeogeographies. In SE France and Western
8
Figure 7. Palaeoenvironmental sketch of the western Sardinian carbonate ramp during the Liassic. Structural features and their
influence on sediment accumulation are annotated.
Sardinia, Cherchi & Montadert (1982) provided
models to support the close proximity of these
domains prior to Oligo-Miocene Sardinia-
Corsica block drift. However, it has been
proposed tectonic uplift was spatially and
temporally limited resulting in the ephemeral
replacement of Middle Jurassic carbonate
shallow platform deposits (Cherchi &
Schroeder, 1985). The results from this study
argue for the role of active extensional tectonics
within epeiric basins and interaction with
carbonate platform sedimentation. Stereonet
projections of faults and associated striation
orientations strongly indicate a NW-SE
extensional regime prior to combined Eocene
and Miocene block rotation. According to
Monleau (1986), the Jurassic Provençal facies of
the Maritime Alps and those of eastern Sardinia
can be correlated. Palaeogeographic
reconstructions compiled by Dardeau (1988)
indicate a NNW-SSE tectonic regime producing
SE verging extensional faults on the eastern
Sardinian margin. The absence of significant
rotation of the Argentiera massif means the
comparable trends of half-graben structures are
today preserved on the North-Provence edge
(Fig. 8).
The Tacchi area, eastern Sardinia
Evidence for extensional tectonics in the
early Middle Jurassic sedimentary cycle of
eastern Sardinia is linked to the coeval opening
of the Alpine Tethys (Bernoulli & Jenkins,
1974). The impact of active tensional tectonics
on sedimentation is highlighted with the uplift
of a temporary tectonic high with rapid collapse
forming initial continental to transitional and
finally shallow marine deposits comprising the
Genna Selole Fm. Features including neptunian
dykes and indications of sudden immersion
provide further support of syn-sedimentary
9
tectonics within the Middle Jurassic
(Costamagna, 2015). Structural trends
orientated towards the NE strongly correlate
with those observed within the Torre Poglina
Lias. Absence of Mesozoic sediments across
present day central Sardinia makes basin
analysis difficult but the comparison of
structural trends from the province platform of
the Maritime Alps to Eastern Sardinia supports
an underlying extensional regime operating
from the Liassic to Middle Jurassic periods
across a subsiding NW Alpine Tethys passive
margin (Dardeau, 1988). This suggests eastern
Sardinian horst-and-graben structures
developing during the Bajocian do not
represent initiation of opening of the Alpine
Tethys (Costamagna et al. 2007).
Triassic rifting
Stratigraphic relationships of sediments
deposited during the Upper Triassic and Lower
Jurassic on the western Tethys Iberian platform
may suggest correlation of Jurassic extension
with Late Triassic palaeogeographies. Seismic
data has highlighted a series of depocentres
controlled by syn-depositional faults (Gómez &
Goy, 2005). The consenus of back-arc
spreading associated with the Palaeo-Tethyan
subduction zone operating until the Late
Triassic may have provided pre-existing
structures inherited by Jurassic extensional
episodes (Stampfli et al. 2002). Further research
of this chronostratigraphic relationship could
suggest a more continual extensional regime
operating within the Mesozoic rather than
individual tensional episodes.
Hydrocarbon exploration
The direct evidence for rifting in Lower Jurassic
sediments has further reaching implications
beyond structural and palaeogeographic
reconstructions, highlighting the geodynamic
evolution of epicontinental basins. Jurassic
carbonates and siliciclastic sediments are
common source rocks for hydrocarbon
exploration in areas including the
Kimmeridgian-Brent system in the Northwest
European shelf. Fourteen petroleum systems
with Upper Jurassic source rocks contain one
quarter of the world’s currently discovered oil
and natural gas with eleven other smaller
systems with Liassic carbonate source
lithologies. It is estimated that one third of the
Lower and Middle Jurassic source rocks lack an
overlying Upper Jurassic source rock with two
thirds of these hydrocarbon occurrences related
to regional or local uplift (Klemme, 1993).
Modelling of Triassic and Jurassic rifting in
central north Bulgaria has emphasised the
impact of significant subsidence during the
Early-Middle Jurassic on the degree of source
rock maturity (Botoucharov, 2014). Hence,
understanding of syn-rift sediments deposited
during the Liassic improves the application to
proximal to distal basinal carbonate plays. This
form of play is expected to consist of traps
which could be pinch-outs of turbidite flows in
distal marine environments or against structural
highs that stop the flows associated with a fault-
controlled platform margin; comparative to the
previous Barbagia tectonic high in eastern
Sardinia. Recent exploration studies have
highlighted this play type could be present on
the western Sardinian margin in addition to
basinal deposits within the Gulf of Lion (Di
Cuia & Riva, 2016). Improved constraints on
rifting initiation aids the collaboration of
continental reconstructions and hence the start
of marine sedimentation during the Rhaetian
time. The formation of widespread organic-rich
(type II, marine) intervals could promote
further interest in Liassic deposits with evidence
for syntectonic deposition controlling the
creation of accommodation space in rift basins
Figure 8. Schematic palaeogeographic reconstruction of the
Tethyan margin during Middle Callovian times (modified from
Costamagna et al. (2007), Middle Collovian).
10
(Mascle & Vially, 1999; Gawthorpe et al. 1994).
The potential of fault linkage within the Torre
Poglina Lias may pose wider implications of
fault interaction in controlling synrift
stratigraphic sequences.
CONCLUSIONS
The lithofacies of the Torre Poglina Lias
represents a shallow marine carbonate
tempestite sequence deposited during an
extensional tectonic regime associated with the
development of the Alpine Tethys passive
margin. The series of present day NE verging
listric normal faults have controlled block
rotation and wedge-shaped accumulation of
sediments likely deposited from storm induced
flows. Restoration of structural planes and
lineation’s following the counter clock-wise
rotation of the Sardinian-Corsican block during
the Miocene to early Oligocene correlate
strongly with palaegeographic reconstructions
and the NW-SE trending extensional regime
operating between the Provençal margin of the
Maritime Alps and offshore eastern Sardinia.
Hence, the evidence for syn-tectonic
deformation of Liassic sediments bridges the
gap between Upper Triassic and Middle Jurassic
rifting episodes both spatially and temporally.
This serves for future implications aiding to
dismiss the stability of carbonate platforms
during the Jurassic. Evidence for interaction
between extensional tectonics and
sedimentation within this chronostratigraphic
interval provides further importance in
understanding source rock maturity and the
potential of hydrocarbon deposits within
Jurassic source rocks within the central
Mediterranean.
ACKNOWLEDGEMENTS
Many thanks to Dr. Matthew Genge and Dr.
Mark Sutton for organisation of fieldwork in
Western Sardinia. The assistance in data
collection from Jennifer Reeves, and
collaboration of structural measurements from
Katherine Siuda, Qaitong Ren, Madeleine
Hann, Sophie Munson and Bethany Mitchell-
Bunce has greatly improved the quality of
interpretations made.
REFERENCES
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Charles R. Singer - Syn-rifting in the Lower Jurassic

  • 1. 1 Closing the gap on Mesozoic extensional tectonics: the Torre Poglina Lias carbonate system, western Sardinia CHARLES R. SINGER1 1Department of Earth Science and Engineering, Imperial College London ABSTRACT In western Sardinia, a Lower Jurassic carbonate tempestite section exhibits a series of NE dipping listric faults. Identification of lateral thickness variations within the rotated hanging wall blocks coupled with erosional intersections of marker horizons provides new evidence for syn-sedimentary faulting in the Lower Jurassic. A SE stereographic tensional regime supports the magnitude and direction of extensional tectonics in this chronostratigraphic interval following restoration attributed to the counter clockwise rotation of the Sardinian-Corsican block. A comparison with stratigraphic sections and structural orientations of eastern Sardinia and the French Maritime Alps is made, attempting to improve the continuity in reconstruction of the Western Tethyan margin with implications for an extensional regime on hydrocarbon bearing Lower Jurassic source rocks. INTRODUCTION In Western Sardinia, a sequence of Jurassic to Cretaceous carbonates overlies post-Hercynian Permian and Triassic siliciclastics and transgressive marine evaporites associated with localised basin subsidence. This cover represents the first (Early Jurassic) Mesozoic sedimentary cycle in western Sardinia. Prior to Early Miocene anticlockwise rotation of the Corsican-Sardinian block, attachment of Sardinia to mainland Europe during the Mesozoic provides constraints with the geodynamic evolution of the French Maritime Alps (Stanley & Mutti, 1968). Palaeogeographic evidence of the Jurassic and Cretaceous periods highlights a large and spatially continuous carbonate megabank which occupied vast areas of the west-Mediterranean, as well as significant portions of Adria (Cherchi & Schroeder, 1985). However, closer reconstructions of restorations reveal the gradual westward propagation of the Neo-Tethys sea-floor spreading axis during the Late Triassic to early Jurassic. This is proposed to pre-date opening of the central Atlantic and the Piedmont segment of the oceanic Tethys (Ricou, 1994). Submergence produced isolated shallow water carbonate shelves sheltered from terrigenous clastics by deeper troughs and plateaus sharing affinities to the modern Bahamas archipelago (Bernoulli & Jenkins, 1974; Ziegler, 1988). The aim of this paper is to provide evidence for improved temporal and spatial resolution of Lower Jurassic extensional tectonics associated with the coeval opening with the Alpine Tethys. The results of direct field observations in western Sardinia attempt improve the accuracy of geographic restorations of past tectonic regimes across the French Maritime Alps and eastern Sardinia and provide further support against general consensus of tectonic stability in the Jurassic (Costamagna, 2015; Dardeau, 1988). The implications of sediment accumulation and extensional faulting on potential Liassic hydrocarbon deposits in the proximity of the central Mediterranean are discussed (Di Cuia & Riva, 2016). Focus is placed on a proximal marine carbonate succession composed of argillaceous limestones belonging to the Torre Poglina Lias located 7 km south of the town of Alghero (Fig. 1). This is where the formation is best developed both spatially and temporally. METHODS Geological mapping in comparison to surrounding Jurassic and Cretaceous carbonate
  • 2. 2 deposits is undertaken with close examination on sedimentological characterisation, facies interpretation, and structural analysis. Adjacent to the small town of Torre Poglina, an abandoned quarry provides a well-exposed succession of carbonate lithologies with evidence for alpine compressive tectonics and extensional faulting; the latter providing the basis for detailed assessment of syn-sedimentary structures. Interaction between sedimentary facies and normal faulting has allowed a localised palaeoenvironmental reconstruction to be developed. Fault measurements are collected using a Suunto Compass Clinometer MC2 along a SW- NE transect along the quarry face with examination of slickenside orientations and slip directions. Strike errors are likely to have arisen when the compass datum line was not aligned horizontally coupled with misalignment due to their indistinction. Repeated observations and averaging aids to overcome this problem allowing stereographic projection. Woodcock (1976) concluded that high errors (>5‫ﹾ‬) could arise from trend measurements on steeply plunging lineation’s. Scaled photographs of sedimentary structures and fault interaction are collated to assess their relationships within the depositional system. Images collected of sedimentary structures are on the centimetre scale and hence the scaling factor associated with parallax error is minimal between the top and bottom of investigated sequences. Annotated digitised field sketches of the quarry face pose higher degrees of scaling errors of approximately 2 calculated between the top and bottom of the quarry face in accordance to the rules of triangulation. Sections of interest are predominantly towards the base of the outcrop minimising scaling errors associated. RESULTS The quarry exposure forms a 70 m by 13 m high outcrop of massive sub-horizontal carbonate beds with distinctly faulted marker horizons 0.4 to 1.4 m thick interbedded with a series of variably grey laminated micrites. The latter lithofacies is represented at its base by dark grey bioclastic grainstones up to 5 cm thick composed of laterally aligned fragmented bivalves 3 – 4 mm in length. These allochems typically concave downwards with occasional locking with adjacent non-inverted shells (60% vol.) set in a depleted mud matrix (Fig. 2a). In its lower part, a basal erosional surface marks a contact with beige micrites belonging to the underlying sequence. The basal part passes up sharply into gradationally fining carbonate silts with indistinct sedimentary structures. Laminations become increasingly defined and closely spaced with traces of hummocky cross stratification existing in the upper parts of each sequence up to 4 cm in amplitude (Fig. 2b). Compilation of fault plane measurements and slickenside orientations are denoted in figure 3a. Figure 1. Regional and local study map. General formation ages and spatial relationships mapped with investigated sections highlighted.
  • 3. 3 Fault planes are plotted and an average plane calculated to correlate slickenside data. The directions of present fault planes are closely clustered towards the NE with an outlier orientated towards the ENE aligning with the slickenside orientations. Through accounting for the 95‫ﹾ‬ counter clockwise rotation of the Sardinian block defined using palaeomagnetic evidence of Advokaat et al. (2014), a restored stereonet is constructed with principal vector directions displayed using data concentration on a restored rose diagram plot (Fig. 3b; Fig. 3c). A mean displacement towards the SE is shown. A digitised field sketch is presented using computer overlay of scaled photographs (Fig. 4). Distinct marker horizons and fault intersections are highlighted to provide direct observation of potential sediment thickening within fault hanging walls. A series of NE verging synthetic listric faults dominate the quarry face varying significantly in length from sub-metre up to 10 m with conjugate antithetic faults steeply dipping towards the SW producing uplifted horst blocks. Maximum fault dips reach up to 70‫ﹾ‬. The majority of faults are concentrated within the bottom half of the quarry exposure with several protruding to intersect an upper brown bed used Figure 2. Torre Poglina Lias deposits. (a) Succession composed of bioclastic grainstones in the lower part fining upwards into laminated micrites. (b) Hummocky cross stratification.
  • 4. 4 Figure 3. (a) Stereographic projections of present day fault and slickenside orientations and (b) restored projection corresponding to ~95‫ﹾ‬ counter clockwise rotation (Avokaat, 2014). (c) Restored rose plot representing mean trends of fault planes and slickensides. a b c
  • 5. 5 Figure 4. Scaled photograph of quarry exposure and overlain digitised field sketch along studied transect. A prominent central grey marker horizon has been used to assess syn-sedimentary thickening.
  • 6. 6 as a further marker horizon beneath alluvium cover. The listric nature of faults is noted with increasing angle between the vertical with depth and appear to flatten to a lower detachment horizon comprised of a poorly sorted 20 cm thick fault breccia composed of angular micrite clasts up to 25 cm. An internal duplex structure detaching on the lower breccia sequence consists of NNW-NW verging fault striations, perpendicular to those associated with synthetic listric normal faults. The presence of bedding parallel styolites with amplitudes up to 2 mm support lithological discontinuity. The magnitude of dip of the beds is strongly rotated within the hanging walls of successive normal faults in comparison to sub-horizontal laminae preserved towards the top of the exposure. Beds are recorded to dip as much as 25‫ﹾ‬ towards the SW with the inclination of strata reducing towards the southern end of the outcrop associated with decreased fault concentration. Associated displacements are also variable, but range only to several tens’ of centimetres. A positive correlation of the magnitude of displacement to fault distance is presented in figure 5. These offsets produce lateral thickness variations along a central grey marker bed. Over the region studied, the unit reaches a maximum thickness difference of approximately 0.93 m with evidence for 0.35 m of thickening across a single normal fault (Fig. 4). Thickness variations of marker horizons beyond the transect become too indistinct to accurately measure. Underlying laminae exhibit evidence for oblique intersection with greater degrees of rotation than the truncating marker horizon (Fig. 4). DISCUSSION The data presented here provides improved constraint on the temporal extent of Jurassic rifting episodes, with evidence from direct observations to supplement compiled palaeogeographic reconstructions. Lithofacies The sedimentological characteristics of the Torre Poglina Lias reflect deposition within shallow, near-shore carbonate producing seas. The presence of an erosive basal bioclastic grainstone passing upwards to normally graded argillaceous silts and laminated micrites is analogous to turbidite deposits formed by density driven flows on shallow continental shelves. The repeated truncations of upper planar laminae with successive cycles represent episodic sedimentation phases triggered by pulses of sediment instability (Meiburg & Kneller, 2009). However, identification of hummocky cross stratification is believed to be diagnostic of storm-dominated shallow marine environments forming above the storm wave base, typically around 30 m in modern carbonate settings (Cheel & Leckie, 2009). Recent published data from Yang et al. (2006) has provided further evidence that HCS wavelength is controlled by the bottom orbital diameter (d0) of oscillatory wave motion, implying the maximum size of HCS sets should increase with decreasing water depth; according to the relationship: λ ≈ 0.75 d0 The centimetre scale magnitude of hummocks observed within the Torre Poglina Lias suggests deposition offshore of the surf zone. The absence of overlying ripple cross laminations and underlying fragmented shell beds support an interpreted proximal to intermediate carbonate tempestite sequence (Fig. 6; Fig 7). Figure 5. Graph constructed of the magnitude of displacement in comparison to the perpendicular distance between fault segments along the length of the studied transect (Fig. 3).
  • 7. 7 Figure 6. General sketch of interpreted stratigraphic sequence of the Torre Poglina Lias, western Sardinia. Extensional Structure Collaboration of structural features and quantifiable bed thickening variations support the presence of syn-sedimentary deposition. Analysis of a grey marker horizon exhibits significant thickness variations along a lateral transect with nearly a metre scale variation in vertical accumulation. The rotation and thickening of beds into the hanging wall of listric faults coupled with discrete erosional truncations provides unequivocal evidence for syn-rift facies (Fig. 4). Calcite filled fractures up to 5 cm in length orientated parallel to macroscopic faults highlights the influence of a tensile regime even on small scale sedimentary deposition. Presence of a detachment horizon comprised of interpreted basal slump deposits also displays an internal horse structure. Slickenside striations suggest a WNW transport direction, approximately perpendicular to the vergence of the extensional regime. Hence, this could represent an inverted extensional duplex structure associated with Alpine orogenic events further supported by a gently folded antiformal structure to the north of the section. Interaction between these tectonic episodes lies beyond the scope of this paper. Analyses of restored stereographic and rose diagram projections strongly support a NW-SE tensional regime producing a series of extensional listric faults presently dipping towards the NE. A component of oblique slip is noted through mean vector offsets between the average planes and slickenside orientations approximately equal to 50‫ﹾ‬. The variability in fault displacement direction with a dominant oblique nature is likely related to the localised linkage of previously unconnected fault segments (Dawers & Anders, 1995). Cartwright et al. (1996) emphasised the displacement decrease on one fault segment is balanced by a sympathetic increase on another. Figure 5 denotes a correlation between lateral fault distance and offset magnitude. Within the studied section, closely spaced faults exhibit reduced displacements suggesting these may have experienced progressive linkage and strain uptake during formation. Fault concentrated regions further exhibit the thickening of sediments which could suggest implications of strain distribution maintaining accommodation space for sediment build-up prior to migrations in the loci of strain accumulation. The interaction between structural development and sediment deposition is proposed through bed morphology and sedimentary structures. Erosional intersections may suggest the structural involvement in localised subsidence and uplift to subaerial exposure. Constraints on data collection means subsidence rates and magnitudes are difficult to ascertain solely from a 2D transect. Myrow & Southard (1996) discussed the catastrophic introduction of sediments as a result of earthquake activity. The non-uniformity in the thickness of tempestite deposits throughout geological history coupled with changes in the fluctuations of storm intensity corresponding to global environmental supercycles, means fault movement within the syn-sedimentary succession should not be ruled out as a triggering mechanism (Ito et al. 2001). However, the low subsidence suggested by the sedimentary record and small degrees of thickening, absence of large scale tectonic disturbances and presence of shallow marine HCS suggests influence of storm-induced waves as a more likely scenario (Durmas & Arnott, 2006). IMPLICATIONS The prospect of active extensional tectonics in the Lower Jurassic period aids understanding of continental assemblage and restorations of palaeogeographies. In SE France and Western
  • 8. 8 Figure 7. Palaeoenvironmental sketch of the western Sardinian carbonate ramp during the Liassic. Structural features and their influence on sediment accumulation are annotated. Sardinia, Cherchi & Montadert (1982) provided models to support the close proximity of these domains prior to Oligo-Miocene Sardinia- Corsica block drift. However, it has been proposed tectonic uplift was spatially and temporally limited resulting in the ephemeral replacement of Middle Jurassic carbonate shallow platform deposits (Cherchi & Schroeder, 1985). The results from this study argue for the role of active extensional tectonics within epeiric basins and interaction with carbonate platform sedimentation. Stereonet projections of faults and associated striation orientations strongly indicate a NW-SE extensional regime prior to combined Eocene and Miocene block rotation. According to Monleau (1986), the Jurassic Provençal facies of the Maritime Alps and those of eastern Sardinia can be correlated. Palaeogeographic reconstructions compiled by Dardeau (1988) indicate a NNW-SSE tectonic regime producing SE verging extensional faults on the eastern Sardinian margin. The absence of significant rotation of the Argentiera massif means the comparable trends of half-graben structures are today preserved on the North-Provence edge (Fig. 8). The Tacchi area, eastern Sardinia Evidence for extensional tectonics in the early Middle Jurassic sedimentary cycle of eastern Sardinia is linked to the coeval opening of the Alpine Tethys (Bernoulli & Jenkins, 1974). The impact of active tensional tectonics on sedimentation is highlighted with the uplift of a temporary tectonic high with rapid collapse forming initial continental to transitional and finally shallow marine deposits comprising the Genna Selole Fm. Features including neptunian dykes and indications of sudden immersion provide further support of syn-sedimentary
  • 9. 9 tectonics within the Middle Jurassic (Costamagna, 2015). Structural trends orientated towards the NE strongly correlate with those observed within the Torre Poglina Lias. Absence of Mesozoic sediments across present day central Sardinia makes basin analysis difficult but the comparison of structural trends from the province platform of the Maritime Alps to Eastern Sardinia supports an underlying extensional regime operating from the Liassic to Middle Jurassic periods across a subsiding NW Alpine Tethys passive margin (Dardeau, 1988). This suggests eastern Sardinian horst-and-graben structures developing during the Bajocian do not represent initiation of opening of the Alpine Tethys (Costamagna et al. 2007). Triassic rifting Stratigraphic relationships of sediments deposited during the Upper Triassic and Lower Jurassic on the western Tethys Iberian platform may suggest correlation of Jurassic extension with Late Triassic palaeogeographies. Seismic data has highlighted a series of depocentres controlled by syn-depositional faults (Gómez & Goy, 2005). The consenus of back-arc spreading associated with the Palaeo-Tethyan subduction zone operating until the Late Triassic may have provided pre-existing structures inherited by Jurassic extensional episodes (Stampfli et al. 2002). Further research of this chronostratigraphic relationship could suggest a more continual extensional regime operating within the Mesozoic rather than individual tensional episodes. Hydrocarbon exploration The direct evidence for rifting in Lower Jurassic sediments has further reaching implications beyond structural and palaeogeographic reconstructions, highlighting the geodynamic evolution of epicontinental basins. Jurassic carbonates and siliciclastic sediments are common source rocks for hydrocarbon exploration in areas including the Kimmeridgian-Brent system in the Northwest European shelf. Fourteen petroleum systems with Upper Jurassic source rocks contain one quarter of the world’s currently discovered oil and natural gas with eleven other smaller systems with Liassic carbonate source lithologies. It is estimated that one third of the Lower and Middle Jurassic source rocks lack an overlying Upper Jurassic source rock with two thirds of these hydrocarbon occurrences related to regional or local uplift (Klemme, 1993). Modelling of Triassic and Jurassic rifting in central north Bulgaria has emphasised the impact of significant subsidence during the Early-Middle Jurassic on the degree of source rock maturity (Botoucharov, 2014). Hence, understanding of syn-rift sediments deposited during the Liassic improves the application to proximal to distal basinal carbonate plays. This form of play is expected to consist of traps which could be pinch-outs of turbidite flows in distal marine environments or against structural highs that stop the flows associated with a fault- controlled platform margin; comparative to the previous Barbagia tectonic high in eastern Sardinia. Recent exploration studies have highlighted this play type could be present on the western Sardinian margin in addition to basinal deposits within the Gulf of Lion (Di Cuia & Riva, 2016). Improved constraints on rifting initiation aids the collaboration of continental reconstructions and hence the start of marine sedimentation during the Rhaetian time. The formation of widespread organic-rich (type II, marine) intervals could promote further interest in Liassic deposits with evidence for syntectonic deposition controlling the creation of accommodation space in rift basins Figure 8. Schematic palaeogeographic reconstruction of the Tethyan margin during Middle Callovian times (modified from Costamagna et al. (2007), Middle Collovian).
  • 10. 10 (Mascle & Vially, 1999; Gawthorpe et al. 1994). The potential of fault linkage within the Torre Poglina Lias may pose wider implications of fault interaction in controlling synrift stratigraphic sequences. CONCLUSIONS The lithofacies of the Torre Poglina Lias represents a shallow marine carbonate tempestite sequence deposited during an extensional tectonic regime associated with the development of the Alpine Tethys passive margin. The series of present day NE verging listric normal faults have controlled block rotation and wedge-shaped accumulation of sediments likely deposited from storm induced flows. Restoration of structural planes and lineation’s following the counter clock-wise rotation of the Sardinian-Corsican block during the Miocene to early Oligocene correlate strongly with palaegeographic reconstructions and the NW-SE trending extensional regime operating between the Provençal margin of the Maritime Alps and offshore eastern Sardinia. Hence, the evidence for syn-tectonic deformation of Liassic sediments bridges the gap between Upper Triassic and Middle Jurassic rifting episodes both spatially and temporally. This serves for future implications aiding to dismiss the stability of carbonate platforms during the Jurassic. Evidence for interaction between extensional tectonics and sedimentation within this chronostratigraphic interval provides further importance in understanding source rock maturity and the potential of hydrocarbon deposits within Jurassic source rocks within the central Mediterranean. ACKNOWLEDGEMENTS Many thanks to Dr. Matthew Genge and Dr. Mark Sutton for organisation of fieldwork in Western Sardinia. The assistance in data collection from Jennifer Reeves, and collaboration of structural measurements from Katherine Siuda, Qaitong Ren, Madeleine Hann, Sophie Munson and Bethany Mitchell- Bunce has greatly improved the quality of interpretations made. REFERENCES Advokaat, E. L., van Hinsbergen, D. J.J., Maffione, M., Langereis, C. G., Vissers, R. L.M., Cherchi, A., Schroeder, R., Madani, H. & Columbu, S. 2014. Eocene rotation of Sardinia, and the palaeogeography of the western Mediterranean region. Earth and Planetary Science Letters, 401, 183-195. Bernoulli, D. & Jenkins, H. C. 1974 Alpine, Mediterranean, and Central Atlantic Mesozoic facies in relation to the early evolution of the Tethys. In: Dott, R. H & Shaver, R. H. (eds) Modern and Ancient Geosynclinal Sedimentation. Society of Economic Palaeontologists and Mineralogists, Special Publication, 19, 129- 160. Botoucharov, N. 2014. Modelling of the Triassic and Jurassic Rifting in the Southern Part of Central North Bulgaria – Implications for the Source Rock Maturity. In: 14th International Multidisciplinary Scientific GeoConference SGEM, 1, 735-742. Cartwright, J. A., Manfield, C. & Trudgill, B. 1996. The growth of normal faults by segment linkage. Geological Society, London, Special Publications, 99, 163-177. Cheel, R. J. & Leckie, D. A. 1993. Hummocky Cross-Stratification, In: Wright, V. P. Sedimentology Review. (ed), Blackwell Publishing Ltd., Oxford, UK. Cherchi, A. & Montadert, L. 1982. The Oligo- Miocene rift of Sardinia: a model for the early history of the Western Mediterranean Basin. Nature, 298, 736-739. Cherchi, A. A. & Schroeder, R. 1985. Vidalina radoicicae n. sp/ and Pseudorhapydionina (?) anglonensis n. sp. (Foram.) form the Upper Cenomanian of Angola region (NW Sardinia). Bolletino della Società Paleontologica Italiana, 24, 185-188. Costamagna, L. G. 2015. Middle Jurassic continental to marine transition in an extensional tectonics context: the Genna Selole Fm depositional system in the Tacchi area (central Sardinia, Italy). Geological Journal, http://doi: 10.1002/gj.26080.
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