EOS - Volume 83, n.1 January 2002
Anatomy of a continental transform fault in Tierra
del Fuego
Authors
E. Lodolo, R. Geletti, P. Sterzai, Istituto Nazionale di Oceanografia
e di Geofisica Sperimentale (OGS), Trieste, Italy; M. Menichetti, Istituto
di Geodinamica e Sedimentologia, Università di Urbino, Italy;
A. Tassone, H. Lippai, Instituto de Geofisica “Daniel Valencio”, Universidad
de Buenos Aires, Argentina; J.-L. Hormaechea, Estación Astronómica
Rio Grande, Argentina.
For additional information, contact E. Lodolo, Istituto Nazionale di
Oceanografia e di Geofisica Sperimentale (OGS). E-mail: elodolo@ogs.trieste.it
A comprehensive suite of field surveys was carried
out by a team of Italian and Argentinean scientists in the Tierra del
Fuego region, the southern tip of South America, to investigate the
600-km-long Magallanes-Fagnano fault system (MFS), a transform-type
margin developed on continental crust (Figure 1). The identification
and analysis of the morphological and structural elements related to
the MFS, and the understanding of mechanisms of slip along the fault,
are the principal objectives of an ongoing project called TESAC (Tectonic
Evolution of the South America-Scotia plate boundary during the Cenozoic),
jointly managed by the Istituto Nazionale di Oceanografia e di Geofisica
Sperimentale (OGS) of Trieste, and the Dpto. de Geologia, Universidad
de Buenos Aires.
The MFS, which represents one of the major segments of the South
America-Scotia plate boundary, runs from the western arm of the
Magallanes Strait to the Atlantic offshore, and substantially splits
the Isla Grande, the main island of Tierra del Fuego, in two continental
blocks. An integral part of the project is focused on the pull-apart
basins, the elongated depocenters which generally form in correspondence
of the principal displacement zone of the fault system. The three-dimensional
architecture of the pull-apart basins is strongly controlled by
the magnitude and type of motion along the principal displacement
zone, and by the geometry of the underlying basement-fault systems.
The identification of the deep crustal features within a fault zone
and the analyses of the sedimentary settings associated with strike-slip
motion are thus key elements to reconstruct the geometry and the
kinematic development of the transcurrent system.
Data gathered during the TESAC project off the Atlantic coast of
the Tierra del Fuego, along Lago Fagnano - a major depression which
hides a significant part of the MFS - and the central-eastern part
of Isla Grande, have imaged the surface and sub-surface structure
of the transform fault and its associated basins. |
|
The MFS is composed of distinct tectonic lineaments
that are segments of the transform system and are represented by mostly
near-vertical faults, with polarities that change along the strike of
the fault. The sedimentary architecture of the asymmetric basins formed
within the principal displacement zone, in which the thick end of the
depositional wedge abuts the transform fault, suggest simultaneous strike-slip
motion and transform-normal extension, a common feature found in other
continental transtensional environments.
The Tierra del Fuego is one of the few places on Earth which offers
the opportunity to observe the surface and subsurface geological features
related to a continental transform plate boundary, but it is one of
the least known because its remoteness and the difficulties of access
in most of its territory. The presence of large peat zones, widespread
lagoons, forestry covers and the absence of paths, have always impeded
the collection of geophysical and geological data on a regular basis
along the strike of the transform segment.
TESAC logistics
Four separate campaigns, spanning the period February 1998 - December
2000, were realized both onshore and offshore in the Tierra del Fuego
region. The group of geologists and geophysicists were logistically
supported during the overall field operations by technicians of the
Estación Astronómica Rio Grande, that realized the D-GPS
data network, and supported the researchers for the acquisition of the
380 gravity and magnetic data points. The main effort was dedicated
to reach some the outcrops of the central and eastern part of the Isla
Grande to conduct the field structural and geological reconnaissance.
The bathymetric survey of the Lago Fagnano was for the first time realized
in collaboration with the Prefectura Naval - Dpto. Lago Fagnano, which
made available a Zodiac boat during the measurements. The offshore seismic
survey was carried out off the Atlantic coast of Isla Grande aboard
the A.R.A. Puerto Deseado, an oceanographic vessel owned by the Argentinean
Navy. During the two weeks preceding the cruise, which took place on
October 1999, a portable multichannel seismic reflection equipment was
installed onboard. It consisted of a 96-channels, 1.2-km-long solid-state
analogue streamer, and two GI-guns (total volume 4 liters) for the acoustic
energization. A total of about 900 km of high-resolution seismic profiles
have been collected across the eastward projection of the MFS, and on
the southern continental margin of the Isla Grande. This survey implemented
previous seismic studies conducted by the research vessel OGS-Explora
in the Magallanes Strait with the purpose to image the along-strike
seismic structure of the MFS. In addition to the collected data, multi-spectral
SPOT images, Synthetic Aperture Radar (SAR) frames and aerial photographs
have helped in identifying on a regional scale the main morphostructural
lineaments of the study area.
Wrench tectonics in the Tierra del Fuego region
The field geological mapping of the Isla Grande was preceded by a careful
analysis of the remote-sensing images, and in particular of the aerial
photos, in order to select those accessible areas where the majority
of outcrops occur along the principal deformation zone of the MFS. The
study was conducted in three key areas: Along the Ruta Nacionál
N. 3, the only N-S arterial road of the Isla Grande, which connects
Rio Grande and Ushuaia; along the northern shore of the Lago Fagnano
and its surroundings; and, in some sectors of the Atlantic coast of
the island, characterized by noticeable, sub-vertical cliffs.
Along the Ruta Nacionál N. 3 it is possible to analyze, from
north to the south, the progressive deformation affecting the Palaeocene-Eocene
rocks pertaining to the Magallanes basin, from sub-horizontal packages
of sandstone-dominated beds, to a series of ESE-WNW-oriented folds and
associated N-verging thrusts (i.e., the Magallanes fold and thrust belt).
This system developed adjacent to the northern flank of the southernmost
Andes in response to a mid-Cretaceous to Tertiary compressional phase,
and involved also the Jurassic-Cretaceous assemblages of the Rocas Verdes
marginal basin (Dalziel, 1989). Several wrenching shear zones have been
identified along the northern shore of the Lago Fagnano, where the most
active deformation occurs. The field evidence include shear bands, sigmoidal
en-echelon tension gashes, and in some cases composite fluid inclusions
in the deforming sedimentary beds. To the east of Lago Fagnano, there
are morphological evidences of fault-related Quaternary activity, with
linear truncation of river meanders, deflection of stream directions,
and talus slopes. Some of these features are very recent, and include:
A cross-stratified glacio-fluvial sand outcrop in a small quarry located
just to the east of the eastern shore of Lago Fagnano, where several
sets of sub-vertical, S-dipping normal faults are present; a W-E scarp
of about 1 m, associated with a gravel barrier; and, a sag pond of the
Rio Turbio, the eastern tributary of the Lago Fagnano. They were probably
created during the 1949, December 17 earthquake, described by Lomnitz
(1970) in these terms: “Landslides occurred along the west coast of
Tierra del Fuego…and along the banks of Lago Fagnano…The epicenter was
located presumably on the fault structure which includes Lago Fagnano
and the western arm of the Magallanes Straits...The magnitude was 7.5”.
Important strike-slip activity were recognized also in many of the steep
outcrops which characterize part of the Atlantic coast of Isla Grande,
from Cabo San Pablo to Cabo Leticia. In this area, the logistic effort
was particularly remarkable, because the absence of paths and the difficulty
of access. The Dirección Provincial de Aeronáutica – Tierra
del Fuego, got available a helicopter during part of the field survey
along the coast to reach the most remote areas, and transport all the
camp equipment. The field geological reconnaissance was mainly conducted
during the low-standing tide intervals, that allow impressive exposition
of the structures of the deformed sedimentary strata.
Lago Fagnano: a large pull-apart basin
The bathymetric map of the 105-km-long, E-W-trending Lago Fagnano, was
realized utilizing seventeen echo-sounder profiles acquired, often under
prohibitive meteorological conditions, aboard a Zodiac boat. The map
(Figure 2) delineates the main submerged morphological expressions of
the South America-Scotia plate boundary in this sector of the Isla Grande,
and most probably reflects its sub-bottom structure. The basin profile
presents an highly asymmetric shape, and the sense of asymmetry changes
along its length. Lago Fagnano is probably the surface expression of
a large pull-apart basin, formed by strands of the MFS. Its length is
comparable to some of the largest strike-slip basins along continental
transforms, which are mostly asymmetric in shape (Ben-Avraham and Zoback,
1992). Onshore, the strands of the MFS are well recognizable from the
SPOT and Digital Elevation Model (DEM) maps, that show the presence
of an ESE-WNW major lineament which traverses the central-eastern Isla
Grande from the eastern shore of Lago Fagnano to the Atlantic coast.
It is constituted by at least two sub-parallel, unconnected segments
in an en-echelon arrangement. The western segment is characterized by
a narrow depression, occupied by the Rio Turbio valley (Figure 3); the
other, morphologically less evident, reaches the coast to the east in
correspondence of Cabo Colorado, where a complex deformational system
include multilayer folds, thrust cleavage, and strike-slip faulting.
The complete Bouguer anomaly map shows distinct relative minima along
the trace of the MFS in the central-eastern part of the Isla Grande.
These gravity features may be interpreted as localized depocenters (the
pull-apart basins) generated in correspondence of the unconnected ends
of the master segments of the MFS. Offshore, these gravity minima may
be linked to the east with the major negative gravity anomaly that regionally
extends E-W within the Falkland Trough, as seen from satellite-derived
data.
The cross-section geometry of the MFS and associated basins, has been
imaged by the seismic lines acquired by the TESAC project off the Atlantic
coast of the Isla Grande, and those gathered during precedent R/V OGS-Explora
Antarctic Campaigns in the central and western Magallanes Strait. The
profile presented in Figure 4 shows a 8-km-wide asymmetric basin – comparable
to the depression occupied by Lago Fagnano - which is bounded by a near-vertical
discontinuity on one side reaching the sea floor (the transform segment),
and a set of subsidiary normal faults on the other side. The complex
sedimentary architecture of the basin may reflect different tectonic
mechanisms, in which periods of oblique extension can alternate with
transform-normal extension (Ben Avraham and Zoback, 1992). Comparable
features are known for other transform environments, like as the Dead
Sea rift, San Andreas fault, Polochic fault (Guatemala), El Pilar fault
(off Venezuela), Lupa fault (Rukwa Lake, Tanzania).
Transtension along the Magallanes-Fagnano fault system
The data gathered both onshore and offshore support the interpretation
that the MFS is remarkably transtensive in nature, and is structurally
and temporally superposed on the older tectonic style of the Tierra
del Fuego region (i.e., the Cretaceous-Tertiary contractional system
of the Magallanes fold and thrust belt). It is constituted by diverse
segments in a en-echelon arrangement, along which pull-apart depocenters
have formed. The stress style that characterizes the MFS contrasts however
with those of the North Scotia Ridge at the central-eastern part of
the South America-Scotia plate boundary, where seismic profiles have
documented N-S-directed convergence (Ludwig and Rabinowitz, 1982).

The evolution of the MFS is intimately related to the complex tectonic
events responsible of the late-Oligocene development of the oceanic
floor of the western Scotia Sea, which definitively led to the separation
of Antarctica from the South America continent. The role of the MFS
in accommodating the South America-Scotia relative motion system may
have been predominant after cessation of seafloor spreading in the western
Scotia Sea (~9 Ma), but some displacements may have occurred a long
time before (Cunningham et al., 1995). Analyses of fault populations
conducted in the Chilean side of Isla Grande (Klepeis, 1994b), indicate
that these fault zones have accommodated left-lateral strike-slip motion
which may have been present since Cretaceous time (Grunow et al., 1992).
In a larger scale, the regional deformation mechanism has generated
impressive topographic lineaments associated to strike-slip displacements
in the central region of the Magallanes Strait, with abundant evidence
of present activity (Winslow, 1982). These fault trends, that partly
exploit early Tertiary and Cretaceous structural trends, represent the
diverse segments constituting the MFS.

The present-day seismicity along the transform boundary is very low
(<3.5 in magnitude) and shallow, as monitored in the period 1997-1999
by an array of portable broad-band seismic stations located in the Chilean
territory, and by a permanent broad-band station installed near Ushuaia
in 1996 (Vuan et al., 1999). Historical seismicity is however significant,
as demonstrated by the 1949 event, and by a preceding, magnitude 7 earthquake,
occurred in the western Magallanes Strait in 1879 (Lomnitz, 1970). The
low seismicity can be explained by the slow relative motion between
the South America and Scotia plates along the boundary, which is less
than 0.5 cm/yr, as documented by re-occupation of D-GPS stations located
in both the South America and Scotia sides of the fault system in the
Isla Grande (Del Cogliano et al., 2000). The relative motion is partitioned
along the diverse segments which make up the fault array, where the
linkage and step-over geometry play an important role in the pull-apart
system development.
Acknowledgments
Funds for this study were provided by the Italian Programma Nazionale
di Ricerche in Antartide (PNRA), and partly by the Dirección
Nacional del Antártico (DNA). L. Barbero, G. Connon and C. Ferrer
(EARG) greatly contributed during the field operations. F. Coren, R.
Vidmar and P. Vascotto (OGS) aided with processing of satellite-derived
maps. Thanks are due to the Argentinean Navy, and particularly to Captain
J.A. Gopcevich Canevari and crew of the research vessel A.R.A. Puerto
Deseado (CONICET-SHIN) for their support during data acquisition at
sea. We are also grateful to C. Maidana, D. Bravo, S. Prieto and C.
Silva for the invaluable help offered during the bathymetric survey.
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EOS – Tierra del Fuego