Overthrusts, and fold and thrust
belt structures
Reading:
Chapt. 18 - Fold-thrust belts in Earth Structure,
2nd edition, van der Pluijm and Marshak, p. 444-470.
Term list
- thin-skinned overthrust style
- klippe and windows
- Heart Mntn. thrust in Wyoming
- examples of fold-thrust belts
- mechanical enigma and solution to large overthrusts
- ramps and flats
- detachments and decollements
- ramp antiforms (fault bend folds)
- oblique ramps and tear faults
- wedge geometry and dynamics (critical taper
angle)
- foreland and hinterland
- foreland propagation
- duplexes
- out-of sequence thrusts
- backthrusts
- fault propagation folds
- balanced cross sections
Historical perspective on overthrusts:
- 1841 - Arnold Escher Van der Linth desribed
Glarus thrust in Switzerland and gave it double fold interpretation,
in order to minimize required movement - still required 15 km
of transport on a subhorizontal surface.
- Marcel Bertrand - reinterpretation as on
N directed thrust with a minimum of 30 km of movement.
- Many other similar structures soon documented.
- Overthrusts: sheets emplaced on subhorizontal
surfaces.
- Gretner (reference on handout) gives vital
statistics:
- 3-6 km thick, up to 150 km wide, 10s of km
of transport.
- this does not included hinterland crystalline
thrust sheets which are often larger (e.g. the Appalachians Piedmont
thrust sheet which is > 10 km thick
Fold and thrust belts
- typically found in orogenic forelands or in rear-arc position.
There are exceptions.
Some examples:
- Valley and Ridge, Appalachians and Ouachitas
- formed ca. 320-275 Ma.
- southern Canadian Rockies - formed ca. 80
Ma.
- Spitsbergen fold-thrust belt - formed 60-40
Ma.
- western Taiwan, actively forming.
Fold and thrust belts versus accretionary wedges
- what are the differences and similarities.?
Thrust
fault geometries and map patterns:
klippe and windows:
- erosional: Heart Mountain a classic example
- structural: due to antiformal stacks and
folding of thrusts by underlying foreland propagation.
tear faults:
strike-slip faults that link thrusts.
oblique and lateral ramps: strike of ramp is at a significant angle to the transport
direction
backthrusts and
wedge insertion.
large scale wedge geometry. Taper angle of the wedge is a critical descriptor.
basement involved thrusts vs. thin-skinned
detachments.
duplexes - all
sorts of duplexes.
Cross section showing earthquake
activity and thrust-fold development in the Seattle area. Note
the compartmentalization depicted associated with the fault bends.
Image source: http://geomaps.wr.usgs.gov/pacnw/psv1/index.html
.
Duplexes
Duplexes are mechanisms by which slip is transferred
from one detachment horizon to another.
Fault duplexes:
- parts: flats, ramps, roof thrust, floor thrust,
horses.
- hinterland dipping duplex.
- antiformal stack: characterized by folded
thrusts.
- foreland dipping duplex.
- horse transport (ht) versus horse width (hw):
- if ht < hw then get hinterland dipping
duplex.
- if ht = get antiformal stack.
- if ht >> hw then get hinterland dipping
duplex.
Fold duplexes:
- note decreasing displacement gradient towards
tip lines.
- with either fault propagation folds or with
detachment folds.
Cleavage duplexes:
likely a lower strain rate type of duplex.
Animation of duplex formation from Allmendinger.
Thrust kinematics:
foreland propagating sequence:
- seen in laboratory models and in active fold
and thrust belts.
- basically a history of footwall plucking.
- most common type of history.
out-of-sequence faults:
- suggest change in dynamics of fold-thrust
belt.
- recognized by decapitated structures.
migration of foreland basins:
- foreland basins form due to flexural loading
and isostatic depression of the foreland.
- as wedge tip propoagates basin depocentre
migrates.
cross section balancing: already addressed.
Mechanical paradox of overthrusts:
An introduction to the paradox - Heart
Mountain, Wyoming:
To start out with it is important to realize
that this is not typical, but a highly unusual situation.

In the view above of Heart Mountain above the
unit forming the steeper slops is Paleozoic carbonate and underneath
are Eocence basin fill sediments. the overthrust contact is semi-horizontal.
Two simple models for emplacing
overthrusts, tectonic push and gravity sliding.
1) tectonic
push - simple model of boundary force applied to rear of rectangular
thrust sheet.

For a given h the normal stress is constant and independent of
Ft, but the greater the block length the greater Ft needed to
produce a high enough shear stress for slip to occur. The higher
Ft the higher internal stresses in the block produced by Ft. Critical
limit: stress within block > rocks internal strength, block
will break up internally, i.e. there is a maximum size of block
you can push from behind. Computed reasonable values - 1 km thick
by 8 km wide (in transport direction) or 5 km thick by 18.4 km.
Actual thrust sheets exceed notably the restrictions imposed by
this model.
2) gravitational sliding - must be overall downslope dip to detachment. Thrusting
might then be a response to vertical uplift. Question - what slope
is necessary for gravitational sliding?
S will be symbol for
stress traction.
Sn
= p g h' cos (ø), where ø
is slope angle, and p is rock density and h' is vertical thickness
of thrust slab.
h' = h/cosø so Sn = pgh, where h is vertical
thickness of slab.
St
= p g h' sin ø = p g h tan ø,
where St is the critical shear stress needed fro slip.
St = K + Sn tan µ , where µ
is failure envelope slope angle and K is internal strength
if K close to 0 then we have p g h tan ø = p g h tan µ
µ = 10-45°, so these are appropriate
slope angles also.
If overthrust transport has been 30 km then
a 5.3 km high source is needed - preposterous. Not only that,
but need to produce uplift, gravity sliding, and then tilting
to remove the original dip of the slide surface. No evidence for
such uplifts.
Possible resolution of paradox - Hubbert and Rubey (1959):
Key is the role of internal fluid, effective
stress. Pore pressure will negate normal stress and will not effect
shear stresses
pr g hr
tan ø = (pr
g hr - pw g hw) tan µ
tan ø = (1 - (pw hw/ pr
hr))tan µ
= (1-lambda) tan m
where lambda is the ratio of pore pressure
to lithostatic pressure.
Implication is that by reducing the normal
stress on the shear plane, the shear stress necessary for failure
is reduced. In turn the tectonic push or the slope required is
also reduced.
Lambda can approach one. Mechanisms for producing
overpressures?
- need subhorizontal permeability barrier.
- compaction and dewatering associated with
burial and diagenesis
- tectonic loading
Analysis of gravity
sliding versus tectonic push:
- mechanism for providing uplift? - batholithic
intrusion, utilized for Wyoming fold and thrust belt with the
Idaho batholith as the cause.
- major difficulty - most thrust systems have
a major detachment that roots at depth and not into the ground.
- tectonic push provided by plate convergence:
some thought needed on actually what are the pushing or buttressing
elements, but plate tectonics , with its dominance of horizontal
motions, naturally incorporated the tectonic push model.
Wedge model and orogenic topography.
On a large scale accretionary wedges within
subduction zones, and fold-and-thrust belts in collision zones
can be viewed as having a wedge geometry.
The basis of a theoretical model: Mohr-Coloumb
failure criteria with pore pressure considered applied to a wedge
in front of a bulldozing element.
- Critical taper angle
-"wedge is on the verge of failure under horizontal compression
everywhere, including the basal decollement." Davis, Suppe,
and Dahlen.
- 3 possible states:
- a) taper angle less than critical angle =
(too thin) internal failure of wedge material and increase in
taper angle. Likely associated with out-of-sequence thrusting.
- b) taper angle equal to critical angle, constant
taper. Underplating along the length of the decollement adds
material, or wedge slides stably (bending underlying platform)
without accretion. May be characteristic of some submarine wedges
associated with subduction. Do wedges spend any appreciable time
in equilibirum.
- c) taper angle greater than critical angle
= internal extension within the wedge (Platt), a form of gravitational
spreading, or, if basal decollement configuration can change,
foreland propogation. In case of accretionary wedge, oceanic
crust-sediment boundary controls the level of the basal decollement.
Super critical state would be expected to produce foreland propagation.
- What is bulldozing element? thickened crust, arc terrane, accreted terrane,
crystalline basement
- Applicability extent
? once decollement greater than 15 km depth no longer obeys Mohr-Coloumb
failure criteria.
- Actual taper angles - plots in Suppe, range
from 4-10 degrees.
- What pertubates the system?
- erosion and sedimentation: redistribution
of load and change in taper angle.
- change in strength: evolving fluid pressures,
development of deformation fabrics (strain weakening), change
of material becoming involved.
- change in convergence rate.
- magmatic activity.
- Along strike changes in taper angle?
This model has been widely applied.
Spreading wedges - the Absoraka volcanic pile
and the Heart Mountain detachment. Other examples of gravitational
collapse.

USGS seismic cection with interpretation
from the Gulfo of Penas, along the Andean trench showing the accretionary
wedge associated with subduction. Image source: http://walrus.wr.usgs.gov/research/sopac.html
.
Laboratory demonstration:
Copyright Harmon D. Maher Jr., This may be
used for non-profit educational purposes as long as proper attribution
is given. Otherwise, please contact me. Thank you.