Strike-slip motion and double ridge formation on Europa
نویسندگان
چکیده
[1] There is abundant observational evidence for strike-slip displacement on the surface of Europa. Strike-slip motion between crustal blocks produces shear heating and an increase in temperature. We model the shear heating within the ice crust using a two-dimensional, finite difference formulation, with a near-surface brittle layer of constant specified thickness and a Newtonian ductile layer beneath. We obtain a maximum temperature anomaly of 66 K for a brittle layer thickness of 2 km and shear velocity of 6 10 7 m s . Such a velocity is appropriate for diurnal (85 hour) tidal motion. The local increase in temperature may cause 100 m uplift around the shear zone through thermal buoyancy. The stresses required to produce velocities of order 10 7 m s 1 are similar to estimates for present-day tidal stresses on Europa (10–10 Pa). Brittle layer thicknesses >2 km are unlikely to persist at active shear zones because of the effect of shear heating. Shear velocities greater than or equal to 10 6 m s 1 will give rise to melting at shallow depths. The removal of material by downwards percolation of meltwater may cause surface collapse along the shear zone; inward motion, leading to compression, may also result. The combination of thermally or compression-induced uplift and melt-related collapse may be responsible for the pervasive double ridges seen on Europa’s surface.
منابع مشابه
Comparison of Ridges on Triton and Europa
Introduction: Triton and Europa each display a variety of ridges and associated troughs. The resemblance of double ridges on these two satellites has been previously noted [R. Kirk, pers. comm.], but as yet, the similarities and differences between these feature types have not been examined in any detail. Triton's ridges, and Europa's, exhibit an evolutionary sequence ranging from isolated trou...
متن کاملFormation mechanisms of Europan ridges with apparent lateral offsets
Introduction: Ridges are the most common linear and tectonic surface features on Europa [1,2,3,4] and apparent lateral offsets are often observed along them [4,5]. Ridges have formed throughout Europa’s geologic history, creating identifiable crosscutting relationships [3,4]. These crosscutting relationships offer us an opportunity to determine the mechanisms responsible for ridge formation [6,...
متن کاملStrike-slip motion of a mega-splay fault system in the Nankai oblique subduction zone
We evaluated the influence of the trench-parallel component of plate motion on the active fault system within the Nankai accretionary wedge from reflection seismic profiles, high-resolution seafloor bathymetry, and deep-towed sub-bottom profiles. Our study demonstrated that a large portion of the trench-parallel component of oblique plate subduction is released by strike-slip motion along a fau...
متن کاملImplications of shear heating and fracture zones for ridge formation on Europa
[1] We present 2D and 3D numerical simulations of convection to test the role of shear heating and fracture zones on Europan ridge formation. Our simulations show that a pre-existing fracture zone promotes upwelling and lithospheric thinning, leading to topographic uplift of 50 m. Shear heating also promotes lithospheric thinning and buoyant ascent, producing a ridge-like feature with topograph...
متن کاملStrike-slip fault patterns on Europa: Obliquity or polar wander?
Variations in diurnal tidal stress due to Europa’s eccentric orbit have been considered as the driver of strike-slip motion along pre-existing faults, but obliquity and physical libration have not been taken into account. The first objective of this work is to examine the effects of obliquity on the predicted global pattern of fault slip directions based on a tidal-tectonic formation model. Our...
متن کامل