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| Failure Modes of the Lineaments on Jupiter's Moon, Europa |
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Personnel: Atilla Aydin |
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Support: This is Atilla's hobby and any coins you can throw in his way will be appreciated!
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Description:
Lineaments referred to as ridges, troughs, bands, and faults on the icy surface of Jupiter's moon, Europa, have long been
interpreted as extensional structures due to brittle fracturing of ice and intrusion of the mobile materials from the interior
of the satellite. This project explores the possibility that the kinematics and failure mechanisms of these structures are
variable and more complex than previously thought. A dense network of structures of multiple generations, forming the background
on the surface of the planet, is here interpreted as localized zones of volumetric strain, likely compaction and/or dilation
bands. The next class of linear failure structures is shear bands with significant offset of the pre-existing markers. The mode
of youngest features can be characterized as sharp, dilational, brittle fracturing and subsequent shearing, thereby producing
fragmentation in various sizes, leading to a series of younger faults with detectable vertical, as well as lateral, offset. This
rich variability in the nature of localization, kinematics, and formation mechanisms, if true, suggests that the conditions
prevailing within the crust of Europa must have changed dramatically over time. The implication of this conclusion is that
structures interpreted to be compaction/dilation bands and shear bands are localized zones of strain and are composed of
deformed materials similar to the surrounding ice, whereas the youngest faults developed by brittle fracturing and
fragmentation, and may be conduits for mobile substrate to reach the surface, and thus, offer the highest potential for
recovering evidence for life on the satellite.
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| Publication:
Aydin, A., Failure modes of the lineaments on Jupiter's moon, Europa: Implications for the evolution of its icy crust (in
review). Journal of Structural Geology. |
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