Thermally induced stresses in boulders on airless body surfaces, and implications for rock breakdown
Jamie L. Molaro, Shane Byrne, Jia-Liang Le

TL;DR
This study models the thermomechanical stresses in lunar boulders caused by diurnal temperature changes, revealing size-dependent stress patterns that influence rock breakdown and longevity on airless planetary surfaces.
Contribution
It introduces a detailed modeling approach to understand how thermal stresses vary with boulder size and surface conditions, impacting their breakdown and survival times.
Findings
Larger boulders experience higher stresses, leading to faster breakdown.
Boulders smaller than 30 cm are less affected by thermal stresses.
Buried boulders are protected from thermal breakdown.
Abstract
This work investigates the macroscopic thermomechanical behavior of lunar boulders by modeling their response to diurnal thermal forcing. Our results reveal a bimodal, spatiotemporally-complex stress response. During sunrise, stresses occur in the boulders' interiors that are associated with large-scale temperature gradients developed due to overnight cooling. During sunset, stresses occur at the boulders' exteriors due to the cooling and contraction of the surface. Both kinds of stresses are on the order of 10 MPa in 1 m boulders and decrease for smaller diameters, suggesting that larger boulders break down more quickly. Boulders <30 cm exhibit a weak response to thermal forcing, suggesting a threshold below which crack propagation may not occur. Boulders of any size buried by regolith are shielded from thermal breakdown. As boulders increase in size (>1 m), stresses increase to…
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