TY - JOUR
T1 - Strike-slip faults on Europa
T2 - Global shear patterns driven by tidal stress
AU - Hoppa, Gregory
AU - Tufts, B. Randall
AU - Greenberg, Richard
AU - Geissler, Paul
N1 - Funding Information:
We thank the technical staff of the Galileo project for making this study possible, D. Durda and the members of the Galileo imaging team, led by Mike Belton, and their associates for their comments and suggestions; and C. Phillips and M. Milazzo for the mosaics used to identify the features discussed here. Robert Pappalardo and Anthony Dobrovolskis provided careful reviews of the manuscript. Theoretical aspects of this work were supported by NASA’s Planetary Geology and Geophysics program. The mapping section of this work was supported by NASA’s Jupiter Science Data Analysis program.
PY - 1999/10
Y1 - 1999/10
N2 - Diurnal tides due to orbital eccentricity may drive strike-slip motion on Europa through a process of "walking" in which faults open and close out of phase with alternate right- and left-lateral shear. Mapping of five different regions on Europa has revealed 121 strike-slip faults, including Astypalaea Linea, a 800-km-long fault with 42 km of right-lateral offset. At high southern latitudes near Astypalaea Linea all of the strike slip faults identified were right-lateral. Europa appears to preferentially form right-lateral faults in the southern hemisphere and left-lateral faults in the northern hemisphere, consistent with tidal walking. At the five locations, nonsynchronous rotation explains the azimuthal orientations and distribution of sense of shear, which fit formation ∼60° to 90° west of their current positions. Alternatively, stress due to differential rotation might also explain the observed shear patterns. Nearly all identified strike-slip faults were associated with double ridges or bands, but few were detected along ridgeless cracks (even older ones). Thus, cracks without ridges may not have penetrated to a decoupling layer, consistent with the models for ridge formation that require cracks to penetrate to a liquid water ocean.
AB - Diurnal tides due to orbital eccentricity may drive strike-slip motion on Europa through a process of "walking" in which faults open and close out of phase with alternate right- and left-lateral shear. Mapping of five different regions on Europa has revealed 121 strike-slip faults, including Astypalaea Linea, a 800-km-long fault with 42 km of right-lateral offset. At high southern latitudes near Astypalaea Linea all of the strike slip faults identified were right-lateral. Europa appears to preferentially form right-lateral faults in the southern hemisphere and left-lateral faults in the northern hemisphere, consistent with tidal walking. At the five locations, nonsynchronous rotation explains the azimuthal orientations and distribution of sense of shear, which fit formation ∼60° to 90° west of their current positions. Alternatively, stress due to differential rotation might also explain the observed shear patterns. Nearly all identified strike-slip faults were associated with double ridges or bands, but few were detected along ridgeless cracks (even older ones). Thus, cracks without ridges may not have penetrated to a decoupling layer, consistent with the models for ridge formation that require cracks to penetrate to a liquid water ocean.
KW - Europa
KW - Satellites of Jupiter
KW - Tectonics
KW - Tides
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U2 - 10.1006/icar.1999.6185
DO - 10.1006/icar.1999.6185
M3 - Article
AN - SCOPUS:0033210467
SN - 0019-1035
VL - 141
SP - 287
EP - 298
JO - Icarus
JF - Icarus
IS - 2
ER -