Cascading parallel fractures on Enceladus
Douglas J. Hemingway, Maxwell L. Rudolph, Michael Manga

TL;DR
This paper presents a model explaining the formation and spacing of the tiger stripe fractures on Enceladus, attributing their origin to global tensile stresses from ice shell cooling and subsequent cascading failure.
Contribution
It introduces a comprehensive explanation for the location, parallel arrangement, and spacing of fractures on Enceladus based on thermal and mechanical processes.
Findings
Fractures originate at the pole where ice is thinnest due to tidal heating.
Sequential failure leads to regularly spaced parallel fissures.
The model explains the observed ~35 km spacing of fractures.
Abstract
Active eruptions from the south polar region of Saturn's small (~500 km diameter) moon Enceladus are concentrated along a series of lineaments known as the `tiger stripes', thought to be partially open fissures that connect to the liquid water ocean beneath the ice shell. Whereas aspects of the tiger stripes have been addressed in previous work, no study to date simultaneously explains why they should be located only at the south pole, why there are multiple approximately parallel and regularly spaced fractures, and what accounts for their spacing of ~35 km. Here we propose that secular cooling and the resulting ice shell thickening and global tensile stresses cause the first fracture to form at one of the poles, where the ice shell is thinnest due to tidal heating. The tensile stresses are thereby partially relieved, preventing a similar failure at the opposite pole. We propose that…
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