Thermally induced brittle deformation in oceanic ... · RITTLE deformation of oceanic lithosphere...
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T33B-1367
Thermally induced brittle deformation in oceanic lithosphere and the spacing of fracture zonesEun-seo Choi and Michael Gurnis
Seismological Laboratory, California Institute of Technology, Pasadena, CA 91125, U.S.A.
T33B-1367
Abstract
BRITTLE deformation of oceanic lithosphere due to thermal stress is explored with
a numerical model, with an emphasis on the spacing of fracture zones. Brittle
deformation is represented by localized plastic strain within a material having an
elasto-visco-plastic rheology with strain softening. We show that crustal thickness, creep
strength, and the rule governing plastic flow control the formation of cracks. The spacing
of primary crack decreases with crustal thickness as long as it is smaller than a threshold
value. Creep strength shifts the threshold such that crust with strong creep strength de-
velops primary cracks regardless of crustal thicknesses, while only a thin crust can have
primary cracks if its creep strength is low. For a thin crust, the spacing of primary cracks
is inversely proportional to creep strength, suggesting that creep strength might indepen-
dently contribute to the degree of brittle deformation. Through finite versus zero dilatation
in plastic strain, associated and non-associated flow rule results in nearly vertical and V-
shaped cracks, respectively. Changes in the tectonic environment of a ridge system can be
reflected in variation in crustal thickness, and thus related to brittle deformation. The frac-
ture zone-free Reykjanes ridge is known to have a uniformly thick crust. The Australian-
Antarctic Discordance has multiple fracture zones and thin crust. These syntheses are
consistent with enhanced brittle deformation of oceanic lithosphere when the crust is thin
and vice versa.
Introduction
SPACING of fracture zones exhibit correlations with regional variations in crustal
thickness, creep strength, and mantle temperature. For instance, the Reykjanes
ridge above the Iceland hot spot is known to have a uniform and much thicker crust
for its spreading rate (Bunch and Kennett, 1980; Murton and Parson, 1993; Smallwood
and White, 1998). This hot spot-affected ridge has been shown to exhibit signatures of wet
mantle source for basaltic melt (Nichols et al., 2002). The water in crustal and mantle min-
erals has a strong weakening effect on creep strength although the preferential partitioning
of water into melt phases complicates this straightforward relation (e.g., Karato, 1986;
Hirth and Kohlstedt, 1996). In contrast, the Australian-Antarctic Discordance (AAD)
has a highly rugged seafloor indicating increased fracturing (Hayes and Conolly, 1972;
Weissel and Hayes, 1974) as well as anomalously thinner crust in comparison with other
parts of the Southeast Indian Ridge (SEIR) (Tolstoy et al., 1995; Okino et al., 2004). Such
regional features were attributed to colder mantle beneath the AAD (Weissel and Hayes,
1974), a hypothesis that was later supported by the systematics of major elements of basalt
along the SEIR (Klein et al., 1991). These two regions, the Reykjanes ridge and the AAD,
respectively exhibit reduced and enhanced segmentations at both the 1st and 2nd order
compared with the other parts of the same ridge systems.
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-80 -40 0 40 80Gravity Anomaly (mGal)
Iceland
Reyk
jane
s Ri
dge
A
A’
105˚ 110˚ 115˚ 120˚ 125˚ 130˚ 135˚ 140˚
-60˚
-55˚
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-45˚
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Antarctic plate
Australian plateAAD }
BB’
-40-20
02040
A A’
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02040
B B’
05
10
0 400 800km
05
10
0 400 800 1200 1600km
FIGURE 1: Gravity anomaly maps derived from satellite altimetry of theReykjanes ridge and the Australian-Antarctic Discordance (Sandwell andSmith, 1997). Thick white lines track the plate boundary (Bird, 2003). Free-airgravity (in mGal) with mean removed (bottom panels) show the profiles (A-A’and B-B’) with simplified variation of crustal thickness in km (lower plots). Seetext for crustal thickness references.
Although originally applied to crack spacing in permafrost, the theory of thermal cracks
(Lachenbruch, 1962) provides an explanation to the variations in the fracture zone spacing.
FIGURE 2: Coordinateaxes for the discussion oflong straight cracks.
FIGURE 3: Theoretical values of elasticstress relief to a vertical tension crack ex-tending from the surface of a semi-infinitemedium in which tension increases linearlywith depth.
However, the theory leads to an apparent paradox. The model predicts a shorter spacing of
cracks when the ambient level of stress is higher or the depth extent of cracks is shallower
(Lachenbruch, 1962). Consequently, for fast and hot spreading centers, the Lachenbruch
model implies a smaller fracture zone spacing because the amount of thermal stress is
larger and brittle layers thinner compared to slow cooler spreading centers. In fact, the
opposite trend is observed.
Numerical Models
WE use SNAC (StGermaiN Analysis of Continua), which is an energy-based fi-
nite difference code solving equations of momentum balance and heat energy
conservation. SNAC can descritize a fully 3-D model domain into a structured
tetrahedral mesh. Lagrangian description of motion is adopted.
• Constitutive Model:
Total strain is assumed to be the sum of ealstic, viscous, and plastic strain. This consiti-
tutive model assumes Maxwell viscoelasticity as a base rheology. When stress increases
faster than the relaxation rate, material can yield according to a given criterion: e.g., the
Mohr-Coulomb model. Viscosity can be Newtonian or a power-law type.
• Thermal stress due to cooling.
• Control parameters
– Crustal thcikness: Thin (4 km), normal (7 km), thick (10 km).
– Creep strength of crust : Strong (dry) vs. weak (wet) diabse.
– Plastic flow rule: associated vs. non-associated.
FIGURE 4: Model geometry and boundary conditions. (a) The model do-main is a vertical 2-D plane parallel to the ridge axis. The hypothetical ridgesegment is assumed to be straight. The oceanic lithosphere has two layers.Temperature change by cooling within the domain is equivalent to tracking anewly formed slice of lithosphere (shaded plane) with time. (b) The domainis 500 km and 50 km deep. Crust and mantle are assumed to be com-posed of diabase and dunite, respectively. Kinematic boundary conditionsare free-slip for all the surfaces except the top one, which can deform freely.Temperature is fixed at 0◦ on top and at 1350◦C on the bottom. The ini-tial temperature field is given by the analytic solution for half-space coolingmodel with the age of 0.3 My.
Model parameters
Symbol Description Model value Symbol Description Model value
ρc Density of crust 2900 kg/m3 Cp Isobaric heat capacity 1100 J kg
−1 K−1
ρm Density of mantle 3300 kg/m3 αV Volumetric thermal expansion co-
efficient
3.2×10−5 K−1
λ Lame’s constant Crust: 30 GPa R Gas constant 8.3145 Jmoli−1K−1
Mantle: 60 GPa φ Friction angle 30◦
µ Shear modulus Crust: 30 GPa ψ Dilation angle 30◦ or 0◦
Mantle: 60 GPa C0 Initial cohesion Crust: 44 MPa
A Pre-exponential coefficient Crust::100 (100)∗ Mantle: 150 MPa
Mantle: 1000 (28840)∗ ǫps,1 Parameters for piecewise linear
strain softening
0.01
H Activation enthalpy (kJ/mol) Crust: 260 (485)∗ kJ/mol C1 0.22 MPa
Mantle: 520 (535)∗ kJ/mol C2 4.4 kPa
n Stress exponent Crut: 3.4 (4.7)∗ ǫps,2 0.05
Mantle: 3.0 (3.6)∗ C3 0 kPa
ǫref Reference strain rate 10−16 s−1 ǫps,3 1000
k0 Enhanced thermal conductivity 7.5 Wm−1K−1 k1 Normal thermal conductivity 3.0 Wm
−1K−1
τ Decay time for thermal conductiv-
ity
1 My
∗Values for the weak rheology; values within the parentheses for the strong rheology.
Results
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0 100 200 300 400 500Distance (km)
0 MyTopography (m)
-50
0
Accumulated plastic strain
(km)
0.000 0.005 0.010 0.015
-50
0
Temperature (oC)0 250 500 750 1000 1250
-50
0
Viscosity (log10(η))20 22 24 26 28 30
1 My
2 My 4 My
7 My 10 My
FIGURE 5: Evolution of topography, temperature, viscosity, and brittle de-formation (plastic strain) for the model with weak and normal thickness crust.Viscosity fields directly reflect temperature change, but low-viscosity lowercrust highlights the two-layer structure. Brittle zones (with a 10 km spacing)start to emerge by 7 My, and some brittle zones continue deforming as coolingproceeds. These later brittle zones create valleys on surface with a relief ofabout 20 m by 10 My.
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0 20 40 60 80 100
Accumulated plastic strain(a) 4 My
Dep
th (
km)
Distance (km)
0.000 0.005 0.010
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0 20 40 60 80 100
σII (MPa)(b) 4 My 0 20 40 60 80 100
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0
0 20 40 60 80 100
Primay crackSecondary crack
7 My (c)
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0 20 40 60 80 100
7 My (d)
FIGURE 6: The upper left part of the model shown in Fig. 5 is magnified tocompare the brittle zones at 4 and 7 My. Each panel covers 0-100 km in theridge-parallel direction and 0-25 km in depth. The accumulated plastic strainand the second invariant of deviatoric stress (σII) at 4 My are shown in (a)and (b), respectively; those at 7 My in (c) and (d).
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(a) Weak crust
Thin (4 km)
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0 100 200 300 400 500
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200Normal (7 km)
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0 100 200 300 400 500
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200Thick (10 km)
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0 100 200 300 400 500Accumulated plastic strain
0.00 0.01 0.02 0.03 0.04 0.05
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(b) Strong crust
Thin (4 km)
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0
0 100 200 300 400 500
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200Normal (7 km)
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0
0 100 200 300 400 500
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200Thick (10 km)
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0
0 100 200 300 400 500
FIGURE 7: Topography (in m) andaccumulated plastic strain for themodels with associated plasticity at10 My. (a) Weak crust models withvaried crustal thicknesses. (b) Mod-els with the strong crustal rheology.
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(a) Weak crust
Thin (4 km)
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0
0 100 200 300 400 500
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200Normal (7 km)
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0
0 100 200 300 400 500
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200Thick (10 km)
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0 100 200 300 400 500Accumulated plastic strain
0.00 0.01 0.02 0.03 0.04 0.05
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(b) Strong crust
Thin (4 km)
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0
0 100 200 300 400 500
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200Normal (7 km)
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0
0 100 200 300 400 500
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200Thick (10 km)
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0
0 100 200 300 400 500
FIGURE 8: Same as Fig. 7, but forthe models with zero dilation angle.(a) Weak crust models with variedcrustal thicknesses. (b) Models withthe strong crustal rheology.
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(a) Weak crust
Thin (4 km)
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0
0 100 200 300 400 500
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200Normal (7 km)
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0
0 100 200 300 400 500Accumulated plastic strain
0.00 0.01 0.02 0.03 0.04 0.05
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(b) Strong crust
Thin (4 km)
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0
0 100 200 300 400 500
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200Normal (7 km)
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0
0 100 200 300 400 500
FIGURE 9: Same as Fig. 7, butthe mantle temperature is loweredto 1250 ◦C from 1350 ◦C.
Associated Non-associated
Strong Thin 73±23 km∗ 47±13 km
Normal 76±28 km 62±17 km
Thick 71±22 km 105±50 km
Weak Thin 125±34 km 100±14 km
Normal N/A N/A
Thick N/A N/A
∗mean ± standard deviation.
25
50
75
100
125
150
175
4 6 8 10Crustal thickness (km)
Pri
may
cra
ck s
pac
ing
(km
)
(a)
Strong Associated
Non-associated
Weak Associated
Non-associated
25
26
27
28
29
30
31
4 6 8 10Crustal thickness (km)
Cre
ep s
tren
gth
(lo
g10
(η))
(b)
47 km
62 km
99 km100 km
FIGURE 10: (a) Plot of the primary crack spacing at 10 My versus crustalthickness for different combinations of crustal rheology and the plastic flowrule. (b) Plot of the primary crack spacing with respect to crustal thickness andcreep strength of lower crust. Only the cases with non-associated plasticityare plotted. The crack spacing is denoted by labels and also represented bythe sizes of symbols. The creep strength is represented by the logarithm ofviscosity (log10(η)) taken from the bottom layer of crust in each model at 10My and the values of the other parameters are listed in Table 3.
Conclusions
WE show that crustal thickness, crustal creep strength, and the rule for plastic flow can
substantially influence the brittle deformation of oceanic lithosphere. The larger
spacing of thermally-induced brittle deformation in a thicker crust provides a qualitative
explanation for the correlation between anomalously thick crust and the lack of fracture
zone in the Reykjanes ridge. By the same token, the connection between thin crust and
increased number of fracture zones within the AAD appears parallel to the small spacing
of primary cracks in a thin crust.
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