Feedbacks between mountain building, erosion and climate

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Presentation transcript:

Feedbacks between mountain building, erosion and climate Eroding landscapes: fluvial processes Feedbacks between mountain building, erosion and climate Mikaël ATTAL Acknowledgements: Jérôme Lavé, Peter van der Beek and other scientists from LGCA (Grenoble) and CRPG (Nancy) Marsyandi valley, Himalayas, Nepal

Lecture overview I. Introduction: mountain building and the critical taper theory. II. Erosion controls the geometry of mountains? III. Erosion controls the structure of mountains? 1) Orographic effect. 2) The curious case of the Himalayas. IV. To which extent does erosion affect deformation in mountains? “Revisiting river anticlines”.

I. Introduction: mountain building and the critical taper theory.

Convergence friction accretion 1. Subduction

Example : Barbados accretionary prism The Atlantic plate plunges under the Caribbean plate Source: C. Beck, Chambery

Example : Barbados accretionary prism Structure of the prism (seismic imagery + bathymetry) Folds + thrusts Source: C. Beck, Chambery

Convergence friction accretion 2. Collision Building of the Alps (schematic representation): Structural map of the Alps The “piémontaise” units (dark green) correspond to the relicts of the Alpine ocean: to the west, units are European; to the east, they are African Source: "GEOL-ALP" (http://www.geol-alpes.com), Maurice GIDON, 1998-2003

Geological cross-section of the Alps (Schmid, 2000) New tectonic interpretation of the ECORS-CROP profile NW SE Flexural basin African Units European Units Suture zone

Geological cross-sections across the Himalayas Indus-Tsangpo suture is what remains of the ocean which has been closed due to the convergence and collision of the Asia and India plates. To the south, Indian units; to the north, Asian units. Zhao, 1993 Lavé & Avouac, 2001

The critical taper theory Characteristics of the accretionary wedge: “Mechanics of Fold-and-Thrust Belts and Accretionary Wedges” Davis, Suppe & Dahlen, JGR, 1983 Characteristics of the accretionary wedge: - basal decollement, - important compressive deformation above decollement, minor deformation below, - taper shaped.

Mechanical model

Mechanical model Coulomb failure criterion : τ = shear traction at failure, S0 = cohesive strength, μ = coefficient of friction, σn = normal traction, pf = pore fluid pressure. Tau : shear traction at failure, S0 = cohesive strength, mu = coefficient of friction, sigma_n = normal traction and pf = pore fluid pressure.

The critical taper The Mohr diagram is used to solve the equation and describe the shape of the taper

Linear relationship between α and β where and μ = coefficient of friction (μb = basal coef.) α mu_b = basal coefficient of friction Linear relationship between α and β β

Application to natural objects: Taiwan

Topographic profiles (Western Range of Taiwan): values of α β α

Determination of the parameters producing the best fit between model and field data β α

Other examples: values of α and β β α

Linear relationship between α and β Constraining the parameters Linear relationship between α and β β α

Modification of the equilibrium Example: mountain building A: subcritical / “stable”  α can increase. X C B: critical taper. α cannot increase anymore. If α > critical value, the taper becomes supercritical / unstable and collapses. B A C: to carry on growing, the taper cannot steepen anymore so it has to “expand” horizontally as well as vertically. β α A β B α β C α

II. Erosion controls the geometry of mountains? D Steady-state: FE = FA C B A A: no topography, FE = 0. B: mountain grows  FE increases. C: critical taper stage, slope α cannot increase anymore. D: FA = FE  steady-state. The topography does not evolve anymore. Flux D FA Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time Willett & Brandon, Geology, 2002 C B FA = flux of material accreted, FE = flux of material eroded. FE A Time

II. Erosion controls the geometry of mountains? D D-E Steady-state: FE = FA A D: FA = FE  steady-state. E: drop in FE (e.g., climate change with less rain)  erosion rate decreases  the topography is not at steady-state anymore. F: mountain grows again  FE increases until a new steady-state is reached (FA = FE) Flux D F FA Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time Willett & Brandon, Geology, 2002 C B E FA = flux of material accreted, FE = flux of material eroded. FE A Time

II. Erosion controls the geometry of mountains? Steady-state: FE = FA  Erosion controls the GEOMETRY of the mountain range Remark: “real” mountains are more complex: - presence of discontinuities (e.g. faults), - different lithologies (more resistant in the core of the range), - change in crust rheology (e.g. lower crust partially molten under Tibet  no basal friction). Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time Willett & Brandon, Geology, 2002 FA = flux of material accreted, FE = flux of material eroded.

II. Erosion controls the geometry of mountains? Evolution of the Alps (Schlunegger et al., 2001, 2002) Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time Schlunegger et al., 2001

II. Erosion controls the geometry of mountains? Evolution of the Alps (Schlunegger et al., 2001, 2002) Schlunegger et al., 2001 Crystalline rocks exhumed ~20 Ma ago  decrease in erosion rate  range grows and widens. Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time

II. Erosion controls the geometry of mountains? D D-E Steady-state: FE = FA A D: FA = FE  steady-state. E: drop in FE (e.g., more resistant rocks exposed)  erosion rate decreases  the topography is not at steady-state anymore. F: mountain grows again  FE increases until a new steady-state is reached (FA = FE) Flux D F FA Critical taper theory: taper growth is self similar, slopes on both sides are invariant through time Willett & Brandon, Geology, 2002 C B E FA = flux of material accreted, FE = flux of material eroded. FE A Time

III. Erosion controls the structure of mountains? 1) Orographic effect. Willett et al., 1993

III. Erosion controls the structure of mountains? 1) Orographic effect. Dominant wind/rain on retro - side Dominant wind/rain on pro - side Willett, JGR, 1999

III. Erosion controls the structure of mountains? 1) Orographic effect. Field data: Southern Alps, New Zealand Metamorphism grade Rainfall Willett, JGR, 1999

III. Erosion controls the structure of mountains? 1) Orographic effect. Field data: Olympic Mts, NW USA Metamorphism grade Rainfall Laumontite (L), prehnite-pumpellyite (Pr+Pu), pumpellyite (Pu), and chlorite-epidote (Cl+Ep). Willett, JGR, 1999

III. Erosion controls the structure of mountains? 1) Orographic effect. Southern Alps, New Zealand: erosion on the retro side Willett, JGR, 1999

III. Erosion controls the structure of mountains? 1) Orographic effect. Olympic Mts, NW USA: erosion on the pro side Willett, JGR, 1999

NOTE: deadlines for essays = Monday 23rd March, 16:00 III. Erosion controls the structure of mountains? 2) The curious case of the Himalayas Break NOTE: deadlines for essays = Monday 23rd March, 16:00

III. Erosion controls the structure of mountains? 2) The curious case of the Himalayas (Patriat & Achache, 81)

III. Erosion controls the structure of mountains? 2) The curious case of the Himalayas India – Asia collision mm/yr ~50 mm/yr at the moment Convergence rate India / Asia (Patriat & Achache, 81)

 The highest mountain range + the largest high-altitude plateau on Earth (Tapponnier et al., 2001)