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



Historical perspective on overthrusts:

Fold and thrust belts - typically found in orogenic forelands or in rear-arc position. There are exceptions.

Some examples:

Fold and thrust belts versus accretionary wedges - what are the differences and similarities.?


Thrust fault geometries and map patterns:

klippe and windows:

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:

Fold duplexes:

Cleavage duplexes: likely a lower strain rate type of duplex.

Animation of duplex formation from Allmendinger.


Thrust kinematics:

foreland propagating sequence:

out-of-sequence faults:

migration of foreland basins:

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?

Analysis of gravity sliding versus tectonic push:


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.

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:


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