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Farallon plate (oceanic) America (cont.)

30 Ma

10 Ma

0 Ma

Rio Grande Rift Basin and range

Rio Grande Rift Basin and range

0 km

1020 km

Rio Grande Rift Basin and range

G eosph ysic al c onstr ain ts Setup

References

"one suture model"

"Two suture model"

No strong effect on the rising of the astenosphere

No strong effect Suture

Sutures

106 108 110

0 250 500 750 1000

x (km)

Tplume=550o Tplume=750o Tplume=950o 106

108 110

0 250 500 750 1000

x (km)

Δx=25km Δx=50km Δx=100km

106 107 108 109

0 250 500 750 1000

x (km)

Δx=25km Δx=50km Δx=100km

?

Enhancing astenosphere rising/lithospheric mantle breaking/Decreasing localisation in the crust/ Enlarging the rift’s size

114 116 118 120

0 250 500 750 1000

x(km)

t=0Myr t=2.2Myr t=3.7Myr t=5.1Myr t=6.7Myr t=9.9Myr

Lithospher e thick ness (Km)

Control of initial heterogeneities and boundary conditions on the deformation partitioning of continental rift: a comparison between Rio Grande Rift and Main Ethiopian Rift.

CédricThieulot1,2, Melody Philippon1, Dimitrios Sokoutis1,3, Jolante van Wijk4, Enrst Willingshofer1 & Sierd A.P.L. Cloetingh1

Introduction Contientntal rifting leads to break up, and is therefore a key process in plate tectonics. Understanding the proces- ses of strain localization and partitioning in such tectonic context appears to be essential. Earth dynamic processes such as subduction, continental collision and continental rifting affect the whole lithosphere. This results in introdu- cing heterogeneities at lithosphere scale in terms of com- position, temperature, structure enhancing regional

strength variations. These heterogeneities strongly

control the deformation pattern as they act either as weak or strong zone within the lithosphere. Rifts development is controlled by such heterogeneities. A deep investiga- tion of the controls of initial heterogeneities and the in- fluence of boundary conditions on rifting is required to understand the mechanics of continental rifting and its evolution toward drifting or its abortion. We propose here to investigates two natural examples by the means of nu- merical modelling, carried out with ELEFANT (http://www.

cedricthieulot.net/elefant.html), an improved version of FANTOM (Thieulot, 2011). We present here a preliminary study of the main controls affecting continental rifting in various regions. The final and non acheived yet goal of this study is to investigate theses problems in 3D.

-10898 0

8271 Main continental rifts

Extensional collapse (after Dewey, 1988)

1. Faculty of Geosciences, Departement of Earth Sciences. Budapestlaan 4. 3584 CD Utrecht (m.m.b.philippon@uu.nl 2. PGP, Sem Selands vei 24 NO-0316 Oslo NORWAY

3. Department of Geosciences, University of Oslo, PO Box 1047 Blindern, N-0316 Oslo, Norway

4. University of Houston. Department of Earth and Atmospheric Sciences312 Science & Research 1 Rm #312Houston, TX 77204-5007

Amante, C. and Eakins, B.W. 2009. ETOPO1 1 Arc-Minute Global Relief Model: Procedures, Data Sources and Analysis. NOAA Technical Memorandum NESDIS NGDC-24, 19 pp. // Baker, B.H., 1987. Outline of the petrology of the Kenya rift alkaline province, in Fitton, J.G., and Upton, B.G.J., eds., 1987, Alkaline igneous rocks: Geological Society London Special Publication 30, p. 293–311.//Bagherbandia M. and Sjöberga, L.E. Modelling the density contrast and depth of the Moho discontinuity by seismic and gravimetric–isostatic methods with an application to Africa//Buehler J.S. and Shearer, P.M. 2010. Pn tomography of the western United States using USArray. JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115, B09315.//Ebinger, C. J., 1989. Tectonic development of the western branch of the East African Rift system, Geol. Soc. Am. Bull., 101, 885 – 903.//Ebinger, C.J., Poudjom, Y., Mbede, E., Foster, F., and Dawson, J.B., 1997. Rifting Archean lithosphere: The Eyasi-Manyara-Natron rifts, East Africa: Geological Society [London] Journal, v. 154, p. 947–960.//Golombek, M.P., MCGill, G.E. and Brown, L.1983.Tectonic and geologic evolution of the Espanola basin, Rio Grande Rift: structure, rate of extension and relation to the state of the stress in the western united states. Tectonophysics, 94, 483-507.//Korrnel, T., Acocella, V., and Abebel, B. 2004. The Role of Pre-existing Structures in the Origin, Propagation and Architecture of Faults in the Main Ethiopian Rift. Gondwana Research, 7 ( 2), pp. 467-479.//Liu L. and Stegman D.R. 2011. Segmentation of the Farallon slab. Earth and Planetary Science Letters. 311,(1–2),1–10.//Manley, K.. 1979. Stratigraphy and structure of the Espaiiola basin, Rio Grande rift, New Mexico, In: R.E. Riecker (E!.ditor), Rio Grande Rift: Tectonics and Magmatism. American Geophysical Union. Washington, D.C.. pp. 71-86.//Pérez-Gussinyé, M., Metois, M., Fernández, M., Vergés, J., Fullea, J., Lowry, A.R. 2009. Effective elastic thickness of Africa and its relationship to other proxies for lithospheric struc- ture and surface tectonics. Earth and Planetary Science Letters 287, 152–167.//Priestley K., Tilmann, F..Relationship between the upper mantle high velocity seismic lid and the continental lithosphere. Lithos 109 (2009) 112–124//Pulliam J., S. P. Grand, Y. Xia, C. Rockett, and T. Barrington. Edge-Driven Convection Beneath the Rio Grande Rift .inSights the EarthScope newsletter Summer 2010//Seager, W.R. and Morgan, P.. 1979. Rio Grande rift in southern New Mexico, west Texas, and northern Chihuahua. In: R.E. Riecker (Editor), Rio Grande Rift: Tectonics and Magmatism. Am. Geophysical Union, Washington, D.C., pp. 87-106.//Shen W. and Ritzwoller M. H. . A 3-D Shear Ve- locity Model of the Crust and Uppermost Mantle Beneath the Western US from Bayesian Monte Carlo Inversion of Surface Wave Dispersion and Receiver Functions. 2012 IRIS Workshop//Shen, W., Ritzwoller, M.H., Schulte-Pelkum, V. and Lin, F.C. Joint inversion of surface wave dispersion and receiver functions: A Bayesian Monte-Carlo approach. Submitted.//Tedla, G.E., van der Meijde, M.,Nyblade, A.A. and van der Meer, F. D.A. 2011. Crustal thickness map of Africa derived from a global gravity field model using Euler deconvolution. Geophys. J. Int. Geodynamics and tectonics, 187, 1–9//Thieulot, C., 2011. Two- and three-dimensional numerical modelling of creeping flows for the solution of geological problems. Physics of the Earth and Planetary Interiors, doi:10.1016/j.pepi.2011.06.011.

235˚ 240˚ 245˚ 250˚ 255˚ 260˚

30˚

35˚

40˚

45˚

50˚

3.4 3.5 3.6 3.7 3.8

3.2 3.4 3.6 3.8

Crustal Velocity (km/s)

−8

−6

−4

−2 0 2 4 6 8

Velocity Perturbation (%)

0 20 40 60 80 100 120 140

238 240 242 244 246 248 250 252 254 256 258 260 262

0 2000 4000

0 2000

Great 4000

Valley Sierra Nevada

Basin and Range Colorado

Plateau Great Plains

Rio Grande Rift Cascade

Volcanic Arc

Snake River

Plain Big Horns

Black Hills

Great Plains

0 20 40 60 80 100 120 140

236 238 240 242 244 246 248 250 252 254 256 258 260 262

0 2000 4000

0 2000

A A’ 4000

B B’

High Lava Plains

Vsv, at 17.5 km depth (Shen and Ritzwoller 2012)

Te

(Pérez-Gussinyé et al., 2009) Crustal Thickness

(Telda et al., 2010)

235˚ 240˚ 245˚ 250˚ 255˚ 260˚

30˚

35˚

40˚

45˚

50˚

4.

0 4.

1 4.

2 4.

3 4.

4 4.

5 4.

6 4.

7 4.

8

Vsv, at 120 km depth (Shen and Ritzwoller 2012) A

B

A’

B’

East African rift

Rio Grande Rift

G eosph ysic al c onstr ain ts In order to have an in-depth control, we gathered available geophysical

data from Eastern Africa. The initial crustal thickness is approached by looking at surrounding non-rifted area on a model based on gravity data (Tedla et al. 2010) and is estimated to be at 45km.

Lithospheric thickness is also available and as been obtained from a combination of surface-wave and body-wave tomographies (Priesltey and Tillman 2009). To begin with a classical thickness of 120 km for the whole lithosphere has been chosen.

The rheological behavior of the whole lithosphere can be approached looking at its elastic thickness Te (obtained by the mean of topography and Bouguer anomaly data)(Perez-Gussinyé et al., 2009). The Te of the East african lithosphere shows basically two areas: 1/ north of the rift, in the Afar area, where the rift is itself a zone of low Te compare to the sur- roundings, and 2/ the central part of the rift that show the Tanzania

craton and its surrounding in blue shade showing a high Te whereas the boundaries of the cratons have a low Te.

The setup of our reference model is 2D and consist of a 120km lithosphere containing one suture zone (modeling the North of the East African rift) and two suture zone (for the South of the rift). The suture is implemented in the model thanks to zone of least strength that affects the whole lithosphere (Green line on the srength profile).

The model of the South-Western America crust and upper most mantle has been obtained from receiver function (Shen and

Rotzwoller and Shen et al., in progress) and the Moho depth is deduced from Pn arrival times on USArray (Julliam et al., 2000). The initial state of the lithosphere before rifting can be approach by looking at the northern cross section AA', where the Rio Grande Rift did not developped. The Rio Grande Rift developped at the interface between a Western hot delaminated lithosphere and cold cratonic lithosphere to the East. The setup of our reference model is 2D and consists of a 120km lithosphere. The East-West profile of our lithosphere is closely inspired by the cross section AA'. The first western part of the model consist of a delaminated

"hot" lithosphere (red line on the strength profile) whereas the eastern part of the model consist of a cratonic "cold lithosphere"

(green line on the strength profile).

Moho Depth

(Buehler and Shearer 2010)

Setup

N

NUBIA

SOMALIA

From North to South, the East African rift is composed from north to south: the Main Ethiopian Rift (MER), the Kenya Rift, the eastern and western of the bran- ches that surrounds the Tanzania craton (Map after Krome et al 1983).

In east Africa horn, continental breakup that leads to the individualization of Nubia, Arabia and Somalia plates occurred along the Mozambic Ocean Suture Zone (MOSZ) that trends NNW-SSE (Kazmin et al., 1978, Stern 1994).

During Eocene, the evolution from collision to active subduction of the boun- dary conditions at the northern convergent margin of the African plate

(Bellahsen et al., 2003) , coupled with the presence of the Afar plume, helped strain localization along the MOSZ and lead to the Red Sea sea opening (Gass, 1977).

During Miocene, a second episode of "pre-rift" basaltic flood emplaced (Zanettin et al.,1978; Ebinger et al., 1993) and predates the opening of the Main Etiopian Rift (MER), south of the Afar region, that separates the Nubia and Somalia plates.

The western and eastern branch of the East African Rift starts to open at the same time and (12–10 Ma) (Baker, 1987, Ebinger, 1989, Ebinger et al., 1997),

and is still in its early stage of development contrary to the MER that is close to beakup is its northern part.

ARABIA

East African rift Rio Grande Rift

The Rio Grande Rift is an active zone of extension separating the Colorado plateau from the Great Plains from the Southern Rocky Mountains (North) to the Basin & Range (south) (Map after Golombek et al., 1983, USGS GIS data- base).

The area consist of the upper plate of the Farallon subduction zone (cross sections modilied after Liu and Stegman 2011). Dynamic of subduction and deformation of the upper plate are closely linked. Since Eocene, the subduc- tion started to retreat and the upper plate is first affected by wide type rif- ting: the basin and range developped till Mid Oligocene (30 Ma).

Then, extension switch from wide to narrow rift in the Rio Grande Area. The early rifting stage started in mid-Oligocene (30 Ma). Opening continued during late Miocene (10 Ma). The rift is still active these days (Seager and Morgan, 1979, Manley 1979).

Cross sections (Shen and Ritzwoller 2012)

UPPER CRUST MOHO DEPTH LITHOSPHERIC MANTLE

Utrecht University

500 km

TANZANIA

M AD AGASC AR

0 5.107 108 1,5.108

Strength (Pa)

brittle upper crust

upper mantle ductile Lower crust

lower mantle

0

40 20

60

80

100

120

"Normal lithosphere"

"Suture zone"

D epth (k m)

Plate boundaries extension compression

T53F-2732

∆x

One suture zone/North of the EAR

Two suture zones/South of the EAR

1000 km

120 k m

1000 km 120 k m w et Qz dr y O livine

∆x

T °C plume

Reference

Reference

550

T Ma

0 5 10

T Ma

0 5 10

T Ma

0 5 10

Eastern Branch

Western Branch MER

Kenya Rift

Craton

Neo-Proterozoic Suture zones Cenozoic lava flows

Rift valley

Basement+Cenoizoic sediments strike slip (Inherited strucures) Normal fault

Afar

High : 4385 Low : 421 Cretaceous

Trias to Jurassic

Pr ot er oz oic Paleo zoic M eso zoic Paleogene Neogene

Sediments Volcanic rocks Granite

Sediments Volcanic rocks Granite

Sediments Volcanic rocks Granite

Sediments Volcanic rocks Sediments Volcanic rocks Sediments Volcanic rocks

Granite Q

200 km

Colorado plateau

Great plains Basin &

range

N

0 km

1020 km

0 km

1020 km

v=6mm.y-1 v=6mm.y-1

v=6mm.y-1

25

950 750

50 100

∆x

25 50 100

∆x=50km,

T = 750°C plume

116 118 120

0 250 500 750 1000

t=0Myr t=5Myr t=10Myr

Eastward migration

x (km)

Lithospher e thick ness (Km)

117 118 119 120

0 200 400 600 800 1000

t=0Myr t=5Myr t=10Myr

x (km)

Lithospher e thick ness (Km)

At the initiation of the experiment, the strain is strongly located in the brittle crust at the place of the suture zone. The lower crust and lithospheric mante are affected by large-scale localised shear zones. At 5 Ma, the thinning concentrates mainly in the lithospheric mantle and at 10 Ma the astenosphere reaches the base of the crust. The time evolution of the topography shows that the rift is asymetric with an eastern margin is

smoother and displaced toward the East. The western margin topography stays steep and steady during the experiment.

At the initiation of the experiment, the strain is strongly located in the brittle crust at the place of the suture zone. This situation is comparable to the previous experiment containing one suture. However, he following of the experiment differs greatly. As there are two zones of weaknesses in the lithosphere, deformation is equaly accommodated by both of these zones. The final result is different in terms of astenosphere exhuma- tion, that is in this case simply not happening. The thinning affect the whole lithosphere and the litho-

spheric mantle is least thinned than in the one suture zone experiment.

20 40 60 80 100 120

0 2e+08 4e+08

depth K m

strength (Pa)

Western part Eastern part

Lithospher e thick ness (Km)

2e+08 4e+08

Depth (Km)

Strength (Pa)

steep initial T. gradient

102 104 106 108 110 112 114

0 250 500 750 1000

x (km)

steep initial T. gradient medium initial T. gradient low initial T gradient

Lithospher e thick ness (Km)

final

0 20 40

60 80 100 120

2e+08 4e+08

Depth (Km)

Strength (Pa)

medium initial T. gradient

0 20 40

60 80 100 120

2e+08 4e+08

Depth (Km)

Strength (Pa)

low initial T. gradient

0 20 40

60 80 100 120

At the onset of the experiment, the temperature gradient between the western delaminated lithosphere

and the eastern cold lithosphere is steep. After 5 Ma of extension, deformation is localized to the west of the boundary between the two lithospheres (in the hot lithosphere). The structural inheritance is controlling the development of a rift, analogue to the Rio Grande Rift.

Next step will be to test the 3D behavior of such systems using ELEPHANT including:

- Surface deformation pattern

- Strain partitioning at the surface but also at the interface of the different layers within our lithosphere - Vertical stress transmission accross the materials

Parameters such as the initial temperature at the base of the model, the amount of stretching and the strain rate will be investigated.

Initial T gradient

Steep Medium Low

Southern Rocky Mountains

East African Rift Rio Grande

Rift

temperature

temperature Interpretation

Interpretation

materials + strain rate

crust

lithos. mantle Asteno.

materials + strain rate

materials at t

initial

temperature at t

Influence of the suture width

Influence of the suture width

Influence of the initial temperature gradient

Influence of the Temperature at the base of the lithosphere

Partly delaminated lithosphere

Lithospher e thick ness (Km) Lithospher e thick ness (Km)

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