Evidence for spreading-rate dependence in the displacement-length ratios of abyssal hill faults at mid-ocean ridges DelWayne R. Bohnenstiehl* Department of Earth and Environmental Sciences and Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York 10964, USA Martin C. Kleinrock Department of Geology, Vanderbilt University, Nashville, Tennessee 37235, USA ABSTRACT New data from the eastern flank of the Mid-Atlantic Ridge (~25–27°N) show that slow-spreading abyssal hill faults maintain maximum displacement-length ratios that are systematically greater than those reported on the fast-spreading East Pacific Rise. Lower displacement-length ratios in the fast-spreading environment may reflect the importance of fault linkage (rather than lateral propagation) in determining the lengths of abyssal hill faults and the limited ability of fault systems that evolve within an extremely thin lithosphere to acquire additional displacement during or following linkage. strain necessary for propagation (i.e., a critical d/L ratio). Field observations suggest, however, that the self-similar scaling of individual faults also may be preserved by systems or arrays of nonphysically linked, but mechanically interacting, fault segments (e.g., Dawers and Anders, 1995; Contreras et al., 2000). Hence, substantial readjustment may occur prior to, or in the absence of, physical linkage, the displacement-distance profile of a linkage fault system adjusting gradually to maintain a shape resembling that expected for a more isolated fault (e.g., Anders and Schlische, 1994; Dawers and Anders, 1995; Cowie, 1998; Contreras et al., 2000). This is facilitated by the positive feedback between optimally oriented fault segments within the array (i.e., those parallel and coplanar for normal faulting) (cf. Cowie, 1998). Keywords: mid-ocean ridges, faults, faulting, fault scarps, abyssal hills. INTRODUCTION Quantifying the relationship between maximum fault displacement and fault length has provided significant insight into our understanding of fault growth and evolution (e.g., Cowie and Scholz, 1992; Dawers and Anders, 1995; Cartwright et al., 1995). Previous studies characterizing the relationship between maximum scarp height (d) and fault length (L) within the abyssal hills of the fast-spreading East Pacific Rise have suggested maximum throw (the displacement parameter typically reported for normal faults) versus length ratios that are consistently at the low end of the range exhibited by terrestrial fault data sets (e.g., Cowie et al., 1993, 1994; Carbotte and Macdonald, 1994). Here we present the first data quantifying the d/L scaling of faults in the slow-spreading abyssal hill environment. We show that faults on the flanks of the Mid-Atlantic Ridge maintain d/L ratios that are systematically larger than those reported for faults of similar scale (L = 5–50 km) on the East Pacific Rise, with values approaching both the terrestrial mean (e.g., Schlische et al., 1996) and those exhibited by much smaller (L = 0.15–2 km) more isolated faults on the median valley floor of the Mid-Atlantic Ridge (e.g., Bohnenstiehl and Kleinrock, 1999). These results imply some variability in the mechanics of fault growth as a function of spreading rate, which we suggest may reflect the relative ability of slowand fast-spreading faults to acquire additional displacement either during or following the along-strike growth of faults through linkage. FAULT GROWTH MODELS Post-yield fracture mechanics models for the growth of an isolated fault predict a linear relationship between maximum displacement and length of the form d = γL, where γ represents a critical shear strain necessary for fault propagation that depends on the shear strength of the rock normalized by its shear modulus, as well as the ratio of shear strength to remote loading stress (e.g., Cowie and Scholz, 1992). In the terrestrial environment, a global compilation of data indicates that a roughly linear d/L relationship is maintained over ~8 orders of magnitude in fault length, with a mean d/L ratio 0.03 and a range of ~0.001–0.1 (Schlische et al., 1996). Because lengthening results from segment linkage, as well as simple lateral propagation, this scale-independent linearity implies that the d/L ratio of a fault that grows by linkage may evolve toward that expected for a more isolated fault. Cartwright et al. (1995) suggested that fault growth might be thought of as a step-like process, in which following linkage the resulting fault preferentially acquires displacement until regaining some critical level of shear *E-mail: [email protected]. Geology; May 2000; v. 28; no. 5; p. 395–398; 3 figures; 1 table. METHODS A 1996 survey aboard the R/V Ewing collected hull-mounted Hydrosweep bathymetry (16 kHz) data and surface-towed HMR1 sidescan data (11–12 kHz) over an ~75 000 km2 region extending from the ridge axis out to ~340 km (26 Ma) off axis on the eastern flank of the Mid-Atlantic Ridge between ~25 and 27°N (Tucholke et al., 1998). A small subset of these data is shown in Figure 1. Tracklines were run at ~50° oblique to the ridge axis, with spacings sufficient to provide ~200% sidescan coverage (i.e., ~100% in both look directions) and nearly 100% Hydrosweep bathymetric coverage. We utilize a predominantly northeast- or outward-facing sidescan mosaic gridded at 70 m and coregistered with the bathymetric data. The HMR1 sonar system can consistently image portions of a fault trace having >~30 m throw and is capable of resolving fault traces separated by >~200 m (Cowie et al., 1994). At this scale, mapped faults may represent arrays of both physically linked and nonphysically linked fault segments that interact mechanically, rather than simple isolated faults. Our analysis is restricted to the larger scale faulting (L = 5–50 km) within the upper bounding walls of the median valley and inactive ridge flanks (beginning ~10 km off axis). The resolution of these data is comparable to that available on the East Pacific Rise, where d/L data have been derived from a combination of equivalent resolution SeaMARC II and GLORIA sonar imagery and high-resolution bathymetric profiles (e.g., Cowie et al., 1993, 1994; Carbotte and Macdonald, 1994). Hence, we can investigate the mechanics of fault growth by quantifying the relationship between displacement and length at different spreading rates (Table 1). We defined fault length as the straight line distance between fault tips within the sidescan imagery. Fault traces were considered linked if separated by <200 m, although offsets to 1 km were allowed between swaths to account for inaccuracies in instrument heading and navigation. Maximum throw was determined by extracting from the gridded data a series of bathymetric profiles perpendicular to the fault (Fig. 1); it was not presumed to occur at the center of the fault trace, although it generally was found to be within the center third. Maximum scarp height measurements are estimated to be accurate within 50 m, accounting for bathymetric resolution (~20 m) and some ambiguity in defining the top and bottom of the fault scarp (Fig. 1). Sediment thickness is ~10–40 m and volcanism appears to be restricted to the inner valley floor in this area (Jaroslow, 1996). DISPLACEMENT-LENGTH DATA AT MID-OCEAN RIDGES Mid-Atlantic Ridge abyssal hill faults exhibit a positive linear correlation (R2 = 0.65) between maximum scarp height and length, with a mean of d/L ratio of 0.016 and a range of ~0.009–0.04 (Fig. 2). The d/L ratios of 395 C C a A b a Scarp Height (m) b′ low/shallow C′ BB 43°15′W Bathymetric Depth 43°25′W C –3800 –3900 D –4000 50 0 a 400 b 300 200 100 E0 0 Scarp Height (m) Backscatter Intensity 43°15′W 43°25′W 250 200 150 100 25°00′N 25°00′N A C′ b′ high/deep Backscatter Intensity A' A ~ 5 km a′ a′ Bathymetric Depth 25°10′N 25°10′N b a′ –4100 a′ a b′ 10 5 Distance Along Fault b-b' (km) 500 c 400 300 200 100 0 F 0 15 20 c′ 10 Such extensive and systematic overprinting is not supported by the most complete studies of the active plate boundary zone, which indicate that synchronous volcanism and faulting are restricted to a narrow 1–2-km-wide zone near the ridge axis (e.g., Carbotte et al., 1997) and that fault throw increases significantly to distances ~10–30 km off axis (e.g., Lee and Solomon, 1995; Alexander and Macdonald, 1996). Table 1 summarizes available d/L data for mid-ocean ridge fault populations at all scales. Previous d/L scaling work on the Mid-Atlantic Ridge has been restricted to a population of much smaller faults on the median valley floor of the TAG segment (~26°N), where analysis of high-resolution DSL-120 sidescan imagery and coregistered bathymetric data indicates a d/L ratio of ~0.03 (Bohnenstiehl and Kleinrock, 1999). The higher resolution of that data set imposes an inherent bias; however, a first-order comparison of the on-axis TAG and off-axis abyssal hill data sets is reasonable in this instance because the change in data resolution between the two studies is met by a proportional change in fault size between the two populations (Table 1) (cf. Bohnenstiehl and Kleinrock, 1999). Near-axis studies at an equivalent scale and resolution have not been conducted on the East Pacific Rise; however, estimates of scarp width and length made from SeaMARC I sonar data (without bathymetric data) collected on the ridge flanks suggest a d/L ratio of ~0.015 for faults having lengths of 2–10 km (Cowie et al., 1994). This is similar to that observed at the larger 5–50 km scale on the Mid-Atlantic Ridge, but it is unclear if these SeaMARC I data can be compared directly, due to the lack of bathymetric control on fault displacement and the inclusion of fault segments, which may have d/L ratios strongly influenced by neighboring fault interactions. 30 20 Distance Along Fault c-c′ (km) Figure 1. A: Example of HMR1 sonar imagery used in this study (insonified from west-southwest). High-amplitude backscatter returns are dark. White circles mark tips of four west-dipping fault arrays used in study, as defined using criteria outlined in text. B: Gray scale image of Hydrosweep bathymetric data used in study. Faults can be identified by their characteristic high-amplitude backscatter (C) and steep slopes (D). Displacement-distance profiles extracted from gridded bathymetry are shown along faults b-b′ (E) and c-c′ (F). these faults are therefore systematically greater than those reported within the abyssal hills of the East Pacific Rise (Fig. 2). The resolution and scale of both abyssal hill fault data sets, as well as the criteria used to define a fault in these studies, are quite similar (Table 1), indicating that the observed spreading-rate dependent variability cannot be attributed to a simple sampling bias. While volcanic overprinting has been shown to obscure some faulting locally along the East Pacific Rise (e.g., Alexander and Macdonald, 1996; Carbotte et al., 1997), >50%–75% of each fault’s total throw would need to be consistently obscured to account for the observed variation in the d/L ratio. FAULT GROWTH MECHANICS AND SPREADING RATE Changes in the d/L ratio of terrestrial faults have been attributed largely to variations in the shear strength of the brittle lithosphere, associated with either changing lithology (e.g., Dawers et al., 1993) or an increase in shear strength at depth (e.g., Cowie and Scholz, 1992; Schlische et al., 1996). In the mid-ocean ridge environment the mechanical properties of the lithosphere are controlled largely by thermal structure and composition, with rheologic models predicting a brittle thickness of ~4 –10 km along a slow-spreading ridge and ~1–3 km along a fast-spreading ridge (within the zone active fault growth) (e.g., Shaw and Lin, 1996). We argue that the lower d/L ratios observed on the flanks of the East Pacific Rise can be explained by considering the limits imposed on maximum fault displacement by the presence of a thin lithosphere together with the importance of fault linkage in the lateral growth of abyssal hill faults. Lateral Fault Growth Scaled physical models of extensional fault systems illustrate the increasingly important role of fault linkage as the population evolves, with a more rapid lengthening per unit displacement observed with increasing strain (Spyropoulos et al., 1999; Ackermann and Schlische, 1999). These models suggest that the lengthening of faults within populations accommodating >~10%–15% strain is accomplished primarily by linkage, with a gradual transition from a lower (<~2.5%) strain regime in which individual faults nucleate and propagate laterally (Spyropoulos et al., 1999). Strain estimates TABLE 1. DISPLACEMENT VERSUS LENGTH DATA SETS IN THE MID-OCEAN RIDGE SETTING Scale range Setting Spreading On/off d/L ∗ (km) rate (mm/yr) axis mean 9o N EPR 120 Off 150 Off 5-50 3o S EPR 26o N MAR 25 Off 2-10 12o N EPR 110 0.15-2 26o 3-35 3-55 N MAR d/L range N 0.006 0.003-0.02 35 0.004 0.002-0.008 35 0.016 0.009-0.04 65 Mixed 0.015 0.007-0.03 35 OC Sidescan/bathyemtric instrument used (m) Strain (%) Characterization Reference 1 200 SeaMARC II/ Deep-Tow 5-15 Segmented fault arrays 150 GLORIA/ Deep-Tow 5-15 Segmented fault arrays 200 HMR1/ Hydrosweep 5-20# ? SeaMARC I / none 5-15 2,3 This study Segmented fault arrays Includes some fault segmets 3 0.5-2.5 Dominantly isolated faults 25 0.03 0.015-0.08 30 15 DSL-120/ DSL-120 On Note: N, number of faults in each environment; OC, offset criteria used to define a fault; MAR, Mid-Atlanric Ridge; EPR, East Pacific Rise; d/L, maximum scarp height versus length ratio; ∗, determined from least-squares regression constrained at the origin; 1, Carbotte and Macdonald (1994); 2, Cowie et al. (1993); 3, Cowie et al. (1994); 4, Bohnenstiehl and Kleinrock (1999); #, Jaroslow (1996). 396 4 GEOLOGY, May 2000 Figure 2. Relationship between maximum throw and length for abyssal hill fault arrays on flank of Mid-Atlantic Ridge (MAR). Vertical error bars ±50 m, horizontal error bars +2.5 km (accounting for portions of fault tip that may not be properly imaged). Data for abyssal hill fault arrays at 9°N (triangles) and 3°S (squares) on East Pacific Rise (EPR) are also shown (Cowie et al., 1993, 1994; Carbotte and Macdonald, 1994). Vertical errors for EPR data were given as 10% of maximum throw by Cowie et al. (1994). Horizontal errors +2.5 km. Dashed line is projection of mean displacement-length (d/L) ratio reported for much smaller (L < 2 km) faults on TAG valley floor (Bohnenstiehl and Kleinrock, 1999). Regression lines shown above were determined by least-squares fit constrained at origin. MAR Abyssal Hill Fault Arrays d/L=0.016 (R2=0.65) 700 Projection of data from TAG median valley floor: d/L=0.03 for faults 0.15-2 km in length 500 400 EPR 9o N d/L=0.006 (R2=0.45) 300 McAllister and Cann, 1996; Searle et al., 1998; Bohnenstiehl and Kleinrock, 1999). These morphologic data confirm that the abyssal hill faults examined here were formed by the coalescence of numerous smaller segments, as evidenced by observations of anastomosing fault traces in map view, fault scarps of variable width, and relay-ramp structures accommodating the deformation between overlapping segments. Linkage-dominated patterns of growth also have been suggested within the boundary faults of the East African rift system (reasonable analogs to abyssal hills faults) (e.g., Morley, 1999; Contreras et al., 2000). Seismic stratigraphy indicates that these fault systems extend to their near final lengths early in their development, with displacement then increasing with little further lengthening (Morley, 1999). 200 3.5o S EPR d/L=0.004 (R2=0.40) 100 0 0 10 20 30 Fault Length L (km) 40 50 Throw within the abyssal hills indicate strains of ~10% (see Table 1), suggesting that fault linkage, rather than propagation, has been the dominant contributor in their lateral growth. Within the resolution of our data, most faults appear as a single scarp (Fig. 1F), with some first-order segmentation (Fig. 1E). A finer scale segmentation (segment lengths ~2–10 km) is apparent, however, within higher resolution sonar and bathymetric data sets (e.g., Cowie et al., 1994; Limits Imposed on Maximum Fault Displacement The thinness of the lithosphere within the fast-spreading environment will (1) suppress interactions between large faults that penetrate the brittle d/L= X (all faults) Maximum throw locked for MAR abyssal hill fault array (Time 4S in A) Maximum throw slow-spreading environment Distance along strike Map View C B A D d/L= X d/L< X Distance along strike Map View Time 2 Fault Throw Throw Time 1 L d/ Maximum throw fast-spreading environment Throw C Distance along strike D Map View B Throw Time 3 Predicted maximum throw fast-spreading environment d/L< X (entire fault array) Distance along strike Map View Throw Time 4F: Fast-Spreading Evironment Throw necessary to maintain a linear d/L relationship Predicted maximum throw slow-spreading environment d/L=X (entire fault array) Distance along strike X Maximum throw locked on EPR (Time 4F in A) d/L< X (entire fault array) Throw necessary to maintain a linear d/L relationship = Incre a as th sing ma ximu e fau m lt arr ay ev throw olves Maximum Scarp Height d (m) 600 B kage Growth by lin A Resulting fault array (Time 3 in A) Fault Segments (Time 1 in A) Fault Length Figure 3. A: Fault evolution in mid-ocean ridge environment. Small faults (time 1, cf. Bohnenstiehl and Kleinrock, 1999) link together forming abyssal hill fault arrays mapped off axis (times 2–3, cf. McAllister and Cann, 1996; Searle et al., 1998; Bohnenstiehl and Kleinrock, 1999). Slow-spreading fault arrays (time 4S, see Fig. 1E) can acquire larger displacements during or following linkage, relative to fastspreading fault arrays (time 4F, cf. Cowie et al., 1994; Alexander and Macdonald, 1996), and consequently are more likely to maintain or regain displacement-length (d/L) ratios consistent with those exhibited at time 1. B: Displacement-length plot showing evolution of fault array and potential limits imposed by maximum fault displacement on d/L ratio of evolving mid-ocean fault system. Map View Time 4S: Slow-Spreading Environment A GEOLOGY, May 2000 Figure 10: Bohnenstiehl and Kleinrock: "Fault scaling at TAG" 397 layer (e.g., Ackermann and Schlische, 1997), and (2) limit the maximum displacement that faults can obtain (e.g., Shaw and Lin, 1996; Ackermann and Schlische, 1999). The latter effect has been shown to limit the scale over which a linear d/L ratio can be preserved in scaled physical models (Ackermann and Schlische, 1999). We summarize the potential consequences of variable lithospheric thickness on the d/L scaling of mid-ocean ridge fault populations in Figure 3. Consider a simple model of fault growth in which a fault’s maximum displacement will continue to increase provided the sum of the stresses resisting fault growth (i.e., friction, σf , and the stress associated with plate flexure, σe ) does not exceed the stress necessary to initiate a new fault near the ridge axis (σf + cohesion, σc ) (e.g., Shaw and Lin, 1993, 1996). In this formulation, the stresses resisting fault growth are dependent on both the fault dip and the effective elastic thickness of the lithosphere, with a thicker lithosphere and shallower fault dip resulting in larger allowable displacements (Shaw and Lin, 1993, 1996). The maximum allowable throw on an East Pacific Rise abyssal hill fault was investigated using the formulation by Shaw and Lin (1996). Their results, which account for lithospheric thickening off axis, show that for fault dips of 45° a fault growing in fast-spreading oceanic lithosphere should obtain a maximum throw of no more than ~100–200 m. Assuming a d/L ratio of 0.015– 0.030 (Cowie et al., 1994; Bohnenstiehl and Kleinrock, 1999), this implies that any linking system of faults along the East Pacific Rise that extends to a length >3–14 km will be incapable of gaining the displacement needed to preserve linearity in the d/L relationship (Fig. 3). This includes many, if not most, of the faults previously used to constrain the d/L ratio within the fast-spreading environment. East Pacific Rise d/L data sets, therefore, exhibit only a weak linear correlation, with maximum throws that appear to level off between ~50 and 150 m and d/L ratios that are systematically less than those reported on the Mid-Atlantic Ridge (Fig. 2). The presence of a significantly thicker lithosphere within the slow-spreading environment results in larger predicted maximum throws (~0.4–1 km) (e.g., Shaw and Lin, 1993). Thus, synlinkage or postlinkage increases in displacement may allow Mid-Atlantic Ridge abyssal hill faults to maintain d/L ratios similar to those exhibited by more isolated faults near the axis and consistent with those exhibited across a range of scales in the terrestrial environment (Figs. 2 and 3). SUMMARY Faults on the eastern flank of the Mid-Atlantic Ridge (25–27°N) maintain d/L ratios that are systematically greater than those reported for structures of similar length on the East Pacific Rise (Fig. 2). High-resolution sonar imagery (e.g., McAllister and Cann, 1996; Searle et al., 1998), scaled physical modeling (e.g., Spyropoulos et al., 1999; Ackermann and Schlische, 1999), and terrestrial observations (e.g., Morley, 1999) all indicate that the lengthening of mid-ocean ridge faults may be accommodated largely by linkage at the abyssal hill scale. We suggest that the low d/L ratios observed on the East Pacific Rise reflect the inability of fault systems that evolve within the thin lithosphere of the fast-spreading environment to acquire additional displacement during or following linkage. Within the slowspreading environment, larger synlinkage or postlinkage increases in displacement allow abyssal hill faults to maintain systematically larger d/L ratios that are more consistent with those observed elsewhere. ACKNOWLEDGMENTS We thank the crew and scientific party of cruise EW9606, especially Chief Scientist B. Tucholke and Co-Chief Scientist J. Lin; M. Edwards, B. Appelgate, and R. Davis for assistance with HMR1 processing; S. Carbotte, C. Scholz, and M. Tolstoy for discussion; and P. Vogt and an anonymous reader for very constructive reviews. This work was supported by National Science Foundation grants OCE-9503561 and OCE-9712230. This is Lamont-Doherty Earth Observatory publication 6044. REFERENCES CITED Ackermann, R.V., and Schlische, R.W., 1997, Systematics of an evolving population of normal faults in scaled physical models: Geological Society of America Abstracts with Programs, v. 29, no. 6, p. 198. Ackermann, R.V., and Schlische, R.W., 1999, Uh-Oh! 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