East-west faults due to planetary contraction
Mikael Beuthe

TL;DR
This paper demonstrates how variations in lithospheric thickness influence fault patterns on planetary bodies, explaining observed fault orientations and features like Iapetus's equatorial ridge and Mercury's lobate scarps.
Contribution
It introduces a model of elastic shells with variable thickness to predict fault patterns resulting from planetary contraction, expansion, and despinning.
Findings
Equatorial lithospheric thinning leads to east-west faults.
Lithospheric thickness variations weakly affect despinning fault patterns.
Contraction combined with despinning can produce diverse fault orientations.
Abstract
Contraction, expansion and despinning have been common in the past evolution of Solar System bodies. These processes deform the lithosphere until it breaks along faults. The type and orientation of faults are usually determined under the assumption of a constant lithospheric thickness, but lithospheric thinning can occur at the equator or at the poles due either to latitudinal variation in solar insolation or to localized tidal dissipation. Using thin elastic shells with variable thickness, I show that the equatorial thinning of the lithosphere transforms the homogeneous and isotropic fault pattern caused by contraction/expansion into a pattern of faults striking east-west, preferably formed in the equatorial region. By contrast, lithospheric thickness variations only weakly affect the despinning faulting pattern consisting of equatorial strike-slip faults and polar normal faults. If…
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