Isostasy in Geology and Basin Analysis This exercise is drawn from Angevine, Heller and Paola (1990), with inspiration and essential planning by R. Dorsey.

Slides:



Advertisements
Similar presentations
Prepared by Betsy Conklin for Dr. Isiorho
Advertisements

Liquids and Gasses Matter that “Flows”
Metamorphic core complexEarth *Geological context: syn to post-orogenic extension -interpreted as MCC for the first time in 1980 in the « Basin.
Movement of the Earth’s Crust
Lecture 1-2 continued Material balance and properties Uplift and subsidence. Topography, crustal and lithospheric thicknesses, 1)LATERAL TRANSPORT OF MATERIAL.
Isostatic Equilibrium Lab
Chapter 17 Earth’s interior. Earth’s interior structure Earth is composed of three shells; –Crust –Mantle –Core.
Large Scale Gravity and Isostasy
GEO 5/6690 Geodynamics 05 Nov 2014 © A.R. Lowry 2014 Read for Fri 7 Nov: T&S Last Time: Flexural Isostasy Tharsis example Is the Tharsis province.
Geology of the Lithosphere 2. Evidence for the Structure of the Crust & Upper Mantle What is the lithosphere and what is the structure of the lithosphere?
Physics 102 Part II Thermal Physics Moza M. Al-Rabban Professor of Physics Fluids (2)
Chapter 12 Earth’s Interior
Friday, November 6, 1998 Chapter 9: shear modulus pressure Pascal’s Principle Archimedes’ Principle.
Iceberg off Newfoundland Density,PressureAndBuoyancy.
GEO 5/6690 Geodynamics 24 Oct 2014 © A.R. Lowry 2014 Read for Fri 31 Oct: T&S Last Time: Flexural Isostasy Isostasy is a stress balance resulting.
Integrated 2-D and 3-D Structural, Thermal, Rheological and Isostatic Modelling of Lithosphere Deformation: Application to Deep Intra- Continental Basins.
How to show what you know Solve problems or answer questions related to: - Fourier’s Law of heat conduction - Lithostatic pressure gradients - Isostasy.
Section 1: Earth: A Unique Planet
Force on Floating bodies:
Monday, Nov. 22, 2004PHYS , Fall 2004 Dr. Jaehoon Yu 1 1.Density and Specific Gravity 2.Fluid and Pressure 3.Absolute and Relative Pressure 4.Pascal’s.
Chapter 11 Fluids. Density and Specific Gravity The density ρ of an object is its mass per unit volume: The SI unit for density is kg/m 3. Density is.
Dr. Jeff Amato Geological Sciences 8/26/08 GEOL 470 Structural Geology OUTLINE Why structure is important An example of structural analysis Earth Structure.
Tom.h.wilson Department of Geology and Geography West Virginia University Morgantown, WV.
1 Rocks and the Earth’s Interior GLY Summer 2015 Lecture 6.
Section 1: Earth: A Unique Planet
Environmental Science
Chapter 3: Equations and how to manipulate them
CE 1501 CE 150 Fluid Mechanics G.A. Kallio Dept. of Mechanical Engineering, Mechatronic Engineering & Manufacturing Technology California State University,
1 The Earth’s Shells Quantitative Concepts and Skills Weighted average The nature of a constraint Volume of spherical shells Concept that an integral is.
GEO 5/6690 Geodynamics 10 Sep 2014 © A.R. Lowry 2014 Read for Wed 10 Sep: T&S Last Time: Radiogenic Heating; Topography Radioactive decay of crustal.
Fault Mechanics and Strain Partitioning Session Axen, Umhoefer, Stock, Contreras, Tucholke, Grove, Janecke.
The Lithosphere There term lithosphere is in a variety of ways. The most general use is as: The lithosphere is the upper region of the crust and mantle.
Earth’s Interior. The Earth’s Core Much of the information scientists have about the Earth’s interior has come not only from complex instruments but also.
Monday, November 9, 1998 Chapter 9: Archimedes’ principle compressibility bulk modulus fluids & Bernoulli’s equation.
Physics. Fluid Mechanics - 1 Session Session Objectives.
Fluids 101 Chapter 10. Fluids Any material that flows and offers little resistance to changing its shape. –Liquids –Gases –Plasma?
Chapter 19 Liquids.
Hydrostatics Lesson 6 © nitatravels. Fluids are Everywhere  Liquids or Gasses  Air is a fluid!!!  Typically take the shape of their container.
Tom.h.wilson Department of Geology and Geography West Virginia University Morgantown, WV Equation Manipulation illustrated around.
Chapter 3: Equations and how to manipulate them Factorization Multiplying out Rearranging quadratics Chapter 4: More advanced equation manipulation More.
Section 1: Earth: A Unique Planet
Tom Wilson, Department of Geology and Geography tom.h.wilson tom. Department of Geology and Geography West Virginia University Morgantown,
Tom.h.wilson Department of Geology and Geography West Virginia University Morgantown, WV.
Tom Wilson, Department of Geology and Geography tom.h.wilson Department of Geology and Geography West Virginia University Morgantown,
Plate Boundaries colllisional.
Tom Wilson, Department of Geology and Geography tom.h.wilson Department of Geology and Geography West Virginia University Morgantown,
GEO 5/6690 Geodynamics 24 Oct 2014 © A.R. Lowry 2014 Read for Wed 29 Oct: T&S Last Time: Brittle-field rheology The “Seismogenic Zone” is observed.
Introduction To Fluids. Density ρ = m/V ρ = m/V  ρ: density (kg/m 3 )  m: mass (kg)  V: volume (m 3 )
The Structure of the Earth
Ying Yi PhD Chapter 11 Fluids 1 PHYS HCC. Outline PHYS HCC 2 Density and Pressure Pressure and Depth in a Static fluid Buoyant Forces and Archimedes’
Tom.h.wilson tom. Department of Geology and Geography West Virginia University Morgantown, WV More about Isostacy.
Geology 6600/7600 Signal Analysis 18 Nov 2015 Last time: Deconvolution in Flexural Isostasy Tharsis loading controversy: Surface loading by volcanic extrusives?
Unit 10.
Rocks and the Earth’s Interior
Earth’s Interior EQ: Describe the different layers of the earth. Explain how scientist learned about these layers.
But, classic Plate Tectonics do not explain everything…
Section 1: Earth: A Unique Planet
Nils Holzrichter, Jörg Ebbing
What is the earth like inside?
To understand pressure
Earth’s Interior EQ: Describe the different layers of the earth. Explain how scientist learned about these layers.
Investigation: Isostasy and Global Elevation Patterns
Chapter 8 Objectives Define a fluid. Distinguish a gas from a liquid.
Chapter 7: Solid and Fluids
DO NOW Turn in Review #8. Pick up notes sheet..
Section 1: Earth: A Unique Planet
Earth’s Layers.
Fluid Mechanics – Buoyancy
Geol Geomath Isostacy II - Wrap up isostacy and begin working on the settling velocity lab tom.h.wilson tom. Department of Geology.
Presentation transcript:

Isostasy in Geology and Basin Analysis This exercise is drawn from Angevine, Heller and Paola (1990), with inspiration and essential planning by R. Dorsey. A. Martin-Barajas generously provided material used in this exercise.

Archimedes Principle: When a body is immersed in a fluid, the fluid exerts an upward force on the body that is equal to the weight of the fluid that is displaced by the body.”

This rule applies to all mountain belts and basins under conditions of local (Airy) isostatic compensation: the lithosphere has no lateral strength, and thus each lithospheric column is independent of neighboring columns (e.g. rift basins).

To work isostasy problems, we assume that the lithosphere (crust + upper mantle) is “floating” in the fluid asthenosphere. A simple, nongeologic example looks like this - Solid ss 1 2 h2h2 h1h1 Fluid (  f ) depth of equal compensation

Because fluid has no shear strength (yield stress =0), it cannot maintain lateral pressure differences. It will flow to eliminate the pressure gradient. Solid ss 1 2 h2h2 h1h1 Fluid (  f ) depth of equal compensation

Solid ss 1 2 h2h2 h1h1 Fluid (  f ) depth of equal compensation To calculate equilibrium forces, set forces of two columns equal to each other: F 1 = F 2 (f=ma) m 1 x a = m 2 x a m 1 = m 2 (gravitational acceleration cancels out)

Because m=  x v (density x volume), convert to m=  h, and:  f h 1 =  s h 2 Solid ss 1 2 h2h2 h1h1 Fluid (  f ) depth of equal compensation This equation correctly describes equilibrium isostatic balance in the diagram.

Onward to geology – Courtesy Sue Cashman

EXAMPLE 1Estimate thickness of lithosphere: In this example, we’ve measured the depth to the moho (hc) using seismic refraction. Elevation (e) is known, and standard densities for the crust, mantle, and asthenosphere are used:  c =2800 kg/m 3  m =3400 kg/m 3  a =3300 kg/m 3 cc cc elevation=3km mm mm hc=35km hm=? asthenosphere (  c ) Z=?

How deep to the base of the lithosphere? Solve for Z:  a (Z) =  c (hc+e) +  m (Z-hc)  a (Z) -  m Z =  c (hc+e) -  m hc  c (hc+e) -  m hc (  a -  m ) cc cc elevation=3km mm mm hc=35km hm=? asthenosphere (  a ) Z=? Z=Z=

How deep to the base of the lithosphere? Solve for Z:  a (Z) =  c (hc+e) +  m (Z-hc)  a (Z) -  m Z =  m (Z-hc) -  m hc  c (hc+e) -  m hc (  a -  m ) 2800(35+3) – 3400(35) ( ) -12, cc cc elevation=3km mm mm hc=35km hm=? asthenosphere (  c ) Z=? Z=Z= = = Z = 126 km

EXAMPLE 2 What is the effect of filling a basin with sediment? Courtesy Scott Bennett

Consider a basin 1km deep that is filled only with water. How much sediment would it take to fill the basin up to sea level?  C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation Let  w = 1000 kg/m 3 Let  s = 2200 kg/m 3 ho= 1km hc hm hs=?  C = 2800  C = 2800  m = 3400  m =

 C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation ho= 1km hc hm hs=?  C = 2800  C = 2800  m = 3400  m = 3400 Remember, force balance must be calculated for entire column down to depth of compensation (=depth below which there is no density difference between columns). Also, thickness of crust and mantle lithosphere does not change, so they cancel out on both sides of the equation. 1 2

 C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation ho= 1km hc hm (hs-ho) hs=?  C = 2800  C = 2800  m = 3400  m = 3400  w ho +  c hc +  m hm +  a (hs-ho) =  s hs +  c hc +  m hm  w ho +  a (hs-ho) =  s hs  w ho +  a hs –  a ho =  s hs hs(  a -  s ) =  a ho –  w ho hs = ho(  a -  w )  a -  s )

 C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation ho= 1km hc hm (hs-ho) hs=?  C = 2800  C = 2800  m = 3400  m = 3400 hs = ho(  a -  w )  a -  s ) = 1.0 ( ) ( ) = 2.1 km

 C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation ho= 1km hc hm (hs-ho) hs=?  C = 2800  C = 2800  m = 3400  m = 3400 How much sediment would it take to fill a water- filled basin up to sea level? “rule of thumb”: the thickness of sediment needed to fill a basin is ~ 2.1 times the depth of water that the sediment replaces

EXAMPLE 2BSediment filling – Alarcon Basin example Determine the maximum water depth in the Alarcon Basin from your profile or spreadsheet. Calculate how much sediment would be needed to fill the Alarcon Basin up to sea level. (Kluesner, 2011)

 C = 2800  C = 2800  m = 3400  m = 3400  a = 3300 water crust mantle lithosphere  s = 2200 sediment crust mantle lithosphere depth of equal compensation ho= 1km hc hm (hs-ho) hs=?  C = 2800  C = 2800  m = 3400  m = 3400 hs = ho(  a -  w )  a -  s ) = 3 ( ) ( ) = 6.3 km

Calculate how much sediment would be needed to fill the Alarcon Basin up to sea level: Maximum water depth in the Alarcon Basin = 3km. Our calculation shows that ~6.3 km of sediment would be needed to fill the basin up to sea level.

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere EXAMPLE 3 How does crustal thinning affect the depth of sedimentary basins? 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Newly-formed basin Thin crust and mantle lithosphere to half of original. How deep a basin forms in response to thinning? Solve for Z. Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z  c (hc1) +  m (hm1) =  s (Z) +  c (hc2) +  m (hm2) +  a (ha) 30  c + 90  m =  w (Z) + 15  c + 45  m +  a ( Z) 30  c + 90  m = Z  w + 15  c + 45  m + 60  a - Z  a Z(  a -  w ) = 60  a -45  m -15  c

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Z Z(  a -  w ) = 60  a -45  m -15  c If the new basin is filled by water, what is its depth (Z)? - A: Fill with water (  w = 1.01 g/cm 2 ) Z= 60  a -45  m -15  c (  a –  w )

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Z Z(  a -  w ) = 60  a -45  m -15  c If the new basin is filled by water - A: Fill with water (  w = 1.01 g/cm 2 ) Z= 60  a -45  m -15  c (  a –  w ) 60(3.3)- 45(3.4)-15(2.8) ( ) = = = 1.31 km for water

If crust and mantle lithosphere are thinned to half of original thickness, how deep a basin would form in response to thinning? Our calculation shows that the newly-formed basin would be ~1.3 km deep if it was filled by water.

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Z Z(  a -  w ) = 60  a -45  m -15  c If the new basin is filled by sediment, how deep will it be? - B: Fill with sediment (  s = 2.2 g/cm 2 ) Z= 60  a -45  m -15  c (  a –  s )

crust mantle litho- sphere mantle litho- sphere crust mantle litho- sphere mantle litho- sphere 1 2 hc1= 30km hc2 hm1= 90km hm2 ha Z Z(  a -  w ) = 60  a -45  m -15  c Basin is formed: A: fill with water B: fill with sediment B: Fill with sediment (  s = 2.2 g/cm 2 ) Z= 60  a -45  m -15  c (  a –  s ) 60(3.3)- 45(3.4)-15(2.8) ( ) = = = 2.7 km for sediment

If crust and mantle lithosphere are thinned to half of original thickness, how deep a basin would form in response to thinning? Our calculation shows that the newly-formed basin would be ~2.7 km deep if it was filled by sediment.

(Martin-Barajas et al., 2013) EXAMPLE 3B What rifting parameters can produce the crustal structure observed in the Upper Delfin basin? Experiment with different sediment densities and different crust and mantle lithosphere initial thicknesses to find values that could produce the thicknesses shown on this cross-section.

This cross-section spans the Delfin and Tiburon basins. The core of the Baja California peninsula (NW end of cross-section) is un-rifted crust, and its thickness (35-40 km) is a reasonable approximation of pre-rift crustal thickness. (Martin-Barajas et al., 2013)

Delfin Basin Location map, Northern Gulf of California (Martin-Barajas et al., 2013)

From the cross-section, measure and record: hc1, initial crustal thickness (use crustal thickness at the NW end of the cross-section as an estimate) hc2, crustal thickness under Delfin basin after extension (0!) hs, thickness of sediments (and intrusions at base of sediments) in Delfin basin (Martin-Barajas et al., 2013)

crust mantle litho- sphere mantle litho- sphere 1 2 hc1= __km hc2=0 hm1= 90km hm2=0 ha Delfin basin Solve for Z. Then see how well your answer matches sediment thick- ness Z on the cross-section Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z(=hs) Experiment #1 Use 90 km for a starting thickness of mantle lithosphere, and hc1 and hc2 values measured from the cross-section.

crust mantle litho- sphere mantle litho- sphere 1 2 hc1= __km hc2=0 hm1= 50km hm2=0 ha Delfin basin Solve for Z. Then see how well your answer matches sediment thick- ness Z on the cross-section Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z(=hs) Experiment #2 Use 50 km for a starting thickness of mantle lithosphere, and hc1 and hc2 values measured from the cross-section.

crust mantle litho- sphere mantle litho- sphere 1 2 hc1= __km hc2=0 hm1= 20km hm2=0 ha Delfin basin Solve for Z. Then see how well your answer matches sediment thick- ness Z on the cross-section Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z(=hs) Experiment #3 Use 20 km for a starting thickness of mantle lithosphere, and hc1 and hc2 values measured from the cross-section.

crust mantle litho- sphere mantle litho- sphere 1 2 hc1= __km hc2=0 hm1= 20km hm2=0 ha Delfin basin Solve for Z. Then see how well your answer matches sediment thick- ness Z on the cross-section Note: ha = hc1 + hm1 - hc2 - hm2 - Z Z(=hs) Experiment #4 Use same thickness values you used in experiment #1, but change  s to  s varies with total sediment thickness….

Experiment #1  c (hc1) +  m (hm1) =  s (Z) +  c (hc2) +  m (hm2) +  a (ha) and ha = hc1 + hm1 - hc2 - hm2 - Z Solve for Z. Plug in thickness values: hc1=35km, hm1=90km, hc2=0, hm2=0 and density values:  c =2800 kg/m 3,  m =3400 kg/m 3,  a =3300 kg/m 3,  s =2200 kg/m 3 Solution: Z = 7.7 km (too small, does not match cross- section)

Experiment #2  c (hc1) +  m (hm1) =  s (Z) +  c (hc2) +  m (hm2) +  a (ha) and ha = hc1 + hm1 - hc2 - hm2 - Z Solve for Z. Plug in thickness values: hc1=35km, hm1=50km, hc2=0, hm2=0 and density values:  c =2800 kg/m 3,  m =3400 kg/m 3,  a =3300 kg/m 3,  s =2200 kg/m 3 Solution: Z = 11.4 km (about right, matches cross-section)

Experiment #3  c (hc1) +  m (hm1) =  s (Z) +  c (hc2) +  m (hm2) +  a (ha) and ha = hc1 + hm1 - hc2 - hm2 - Z Solve for Z. Plug in thickness values: hc1=35km, hm1=20km, hc2=0, hm2=0 and density values:  c =2800 kg/m 3,  m =3400 kg/m 3,  a =3300 kg/m 3,  s =2200 kg/m 3 Solution: Z = 14.1 km (too large, does not match cross- section)

Experiment #4  c (hc1) +  m (hm1) =  s (Z) +  c (hc2) +  m (hm2) +  a (ha) and ha = hc1 + hm1 - hc2 - hm2 - Z Solve for Z. Plug in thickness values: hc1=35km, hm1=90km, hc2=0, hm2=0 and density values:  c =2800 kg/m 3,  m =3400 kg/m 3,  a =3300 kg/m 3,  s =2400 kg/m 3 Solution: Z = 9.4 km (about right)

Delfin Basin Location map, Northern Gulf of California Note: These solutions assume sufficient sediment supply to keep the basin filled. That’s a good assumption here because of the very high sediment input from the Colorado River. (Martin-Barajas et al., 2013)

Our assumption that there is sufficient sediment supply to keep the basin filled would not be a good assumption further south in the Gulf of California where basins are sediment starved. Delfin Basin Google Earth