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Mueller, Steve

Publications and source records attributed to Mueller, Steve.

On the initiation of subduction

Estimates of shear resistance associated with lithospheric thrusting and convergence represent lower bounds on the force necessary to promote trench formation. Three environments proposed as preferential sites of incipient subduction are investigated: passive continental margins, transform faults/fracture zones, and extinct ridges. None of these are predicted to convert into subduction zones simply by the accumulation of local gravitational stresses. Subduction cannot initiate through the foundering of dense oceanic lithosphere immediately adjacent to passive continental margins. The attempted subduction of buoyant material at a mature trench can result in large compressional forces in both subducting and overriding plates. This is the only tectonic force sufficient to trigger the nucleation of a new subduction zone. The ubiquitous distribution of transform faults and fracture zones, combined with the common proximity of these features to mature subduction complexes, suggests that they may represent the most likely sites of trench formation if they are even marginally weaker than normal oceanic lithosphere.

Mueller, Steve↗

The density of Triton - A prediction

The density of Triton is predicted as a function of radius, based on the assumptions that it was captured from solar orbit and has a rock/ice ratio similar to that of the Pluto-Charon system. The best present estimates for Triton's radius are 1000-2000 km, and if the present origin hypothesis is correct, its density should be greater than 2.0 g/cu cm, increasing slowly wih radius. On the other hahd, if Triton is an original regular satellite whose orbit has been perturbed, its density will be lower and more consistent with the derived rock fractions of other icy satellites.

Mckinnon, William B.↗

Three-layered models of Ganymede and Callisto - Compositions, structures, and aspects of evolution

The structural models presently defined for Ganymede and Callisto, which encompass a pure-ice upper layer, a mixed ice/rock lower mantle, and a rock core, incorporate three alternative rock component candidates representing various degrees of silicate hydration and oxidation. The three-layered model facilitates close study of the radius increase required for the internal differentiation of an ice-rock satellite; such expansion is determined to be most significant early in the process, and less so as differentiation approaches completion. The probability of postaccretional melting due to radiogenic heating is calculated.

Mueller, Steve↗

Pluto's structure and composition suggest origin in the solar, not a planetary, nebula

The four explanations for Pluto's large rock/ice ratio, (1) formation in the inner solar system, (2) volatile loss during accretion, (3) volatile loss during the large-body impact that created Charon, and (4) formation as a large, ice-poor outer solar system planetesimal, are considered. It is shown that only the last two explanations are feasible, and that the depletion of water ice in Pluto is so severe that both explanations may be necessary.

Mckinnon, William B.↗

Lunar composition - A geophysical and petrological synthesis

Lunar compositional constraints are derived on the basis of geophysical data (in particular, the lunar seismic model as revised by Nakamura) and petrological arguments. Only in the case of extreme assumptions can critical aspects of bulk lunar composition be demonstrated to be equivalent to the present-day terrestrial mantle; specifically, the moon has an Mg number that is too low and an alumina abundance that is too high. Over a broad range of crustal densities the presence of a metallic core at least 150 km in radius is necessary to reconcile the upper mantle lunar seismic model with mass and moment of inertia constraints. A significant seismic discontinuity at 500 km depth may mark the lowest extent of early lunar differentiation, possibly representing a transition between highly fractionated upper mantle and less fractionated, perhaps even primordial, middle/lower mantle.

Mueller, Steve↗