EXTENSIONAL BOUDINAGE OF COOLING LITHOSPHERE
Following the discovery of 150-250-km-wavelength cross-grain gravity lineations in the Pacific Plate [Haxby, 1986], some attempted to explain these as extensional instabilities under plate driving forces [Winterer and Sandwell, 1987], while others proposed small-scale convection as the underlying mechanism [e.g., Buck and Parmentier, 1986]. Plate motions, mantle rheology, stress, and thermal state in the past are poorly constrained. Whether diffuse extension or small-scale convection or some other mechanism is the prime source of the short wavelength undulations remains an open question [Wessel and Bercovici, 1996; Sandwell and Fialko, 2004; Forsyth et al., 2006].
In any case, finite-amplitude deformation of a cooling, extending lithosphere does not lend itself to simple analytic models, and is complicated by the coupling of thermal and density anomalies to finite strain with Coulomb strength envelopes under gravitational loads. Such a regime may exist not only at mid-ocean ridges but in transient spreading centers of the terrestrial planets and icy moons.
This paper will show that a multi-layer approximation to young oceanic lithosphere tends to have the highest growth rates of instabilities at wavelengths 4x lithospheric thickness, casting doubt on the extensional boudinage mechanism for wavelengths in excess of 150 km. Model strength envelopes that achieve the observed Pacific Plate wavelength have low growth rates. We also review the results of finite-element models for a case applicable to the oceanic problem.