Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
Europlanet Science Congress 2020
Virtual meeting
21 September – 9 October 2020
EPSC Abstracts
Vol.14, EPSC2020-95, 2020
https://doi.org/10.5194/epsc2020-95
Europlanet Science Congress 2020
© Author(s) 2020. This work is distributed under
the Creative Commons Attribution 4.0 License.

Tiger stripes revisited - effect of fault zone rheology

Ondřej Souček1, Kateřina Sládková2, Marie Běhounková2, and Ondřej Čadek2
Ondřej Souček et al.
  • 1Charles University, Faculty of Mathematics and Physics, Mathematical Institute, Prague, Czechia (soucek@karel.troja.mff.cuni.cz)
  • 2Charles University, Faculty of Mathematics and Physics, Department of Geophysics, Prague, Czechia

Abstract

We present preliminary results of a numerical study of tidally induced deformation of Enceladus’s ice shell containing fissures (Tiger Stripes) in the south polar region (SPR). It is a follow-up study of Souček et al. (2016), which brings in a more realistic description of the faults' behavior. In particular, the fault zone is described by a model of effectively visco-elasto-plastic material with yield stress depending on the stress state. Such a model mimics the Coulomb-type friction contact at idealized fault surfaces. We show the basic features of the model and discuss the importance of fault description on the predicted tidal deformation and stress field within Enceladus's ice shell.

Introduction

In Souček et al. (2016), we have numerically demonstrated a profound effect of faults (Tiger Stripes) on the tidally induced deformation and stress fields in the south polar region of Enceladus. In Běhounková et al. (2017), we showed how this effect can be further enhanced in a synergetic way, when combined with a realistic thinning of the ice shell in the SPR for a shell thickness model based on inversion of gravity and libration data (Čadek et al., 2016). In both these studies, the faults were modelled as zones with significantly reduced elastic moduli. Effectively, such description corresponds to faults being described as narrow slots partially filled with water (compensating the overburden pressure within the layer). Such description of the faults is oversimplified since it does not take into account any friction at the faults. We attempt to circumvent this deficiency in the new study.

Model

We solve equations of deformation of a 3D Maxwell visco-elastic planetary shell containing faults in the SPR. The shell's deformation is driven by the incremental tidal potential and at the fault, Coulomb, type response is considered. The Coulomb-type friction is mimicked by a continuum model of a fault zone of finite thickness with stress limiting viscosity. The stress limiter is given by the yield stress, composed of (hydro)static contribution due to overburden pressure and a dynamic contribution due to normal stress variations during the tidal period.

Results

We present preliminary results with one active fault in the SPR, corresponding to the Baghdad Sulcus. In Figure 1, we plot the displacement in SPR for four instants during the tidal period, colors indicate the amplitude of normal displacement, vectors show the horizontal displacement. Compared to the case with frictionless faults, the model with Coulomb-type friction exhibits asymmetry - the lateral motion is facilitated during the opening phase and suppressed during the closing (compressional) phase of the period.

 

Acknowledgements

The research leading to these results received funding from the Czech Science Foundation through project No. 19-10809S. The computations were carried out in IT4Innovations National Supercomputing Center (project no. LM2015070). The study was supported by the Charles University, project GA UK No. 304217, SVV-2019-260447 and SVV 115-09/260581 (K.S.), and by Charles University Research program No. UNCE/SCI/023 (O.S.).

References

Běhounková, M., Souček, O., Hron, J.and O. Čadek (2017), Plume activity and tidal deformation of Enceladus influenced by faults and variable ice shell thickness, Astrobiology, 17(9), 941-954, https://doi.org/10.1089/ast.2016.1629.

Čadek, O., Tobie, G., van Hoolst, T., Massé, M., Choblet, G., Lefèvre, A., Mitri, G., Baland, R.-M., Běhounková, M., Bourgeois, O., and Trinh, A. (2016) Enceladus’s internal ocean and ice shell constrained from Cassini gravity, shape, and libration data. Geophys Res Lett 43:5653–5660.

Souček, O., Hron, J., Běhounková, M., and O. Čadek (2016), Effect of the tiger stripes on the deformation of Saturn's moon Enceladus, Geophysical Research Letters, 43(14), 7417–7423, https://doi.org/10.1002/2016GL069415.



 

How to cite: Souček, O., Sládková, K., Běhounková, M., and Čadek, O.: Tiger stripes revisited - effect of fault zone rheology, Europlanet Science Congress 2020, online, 21 September–9 Oct 2020, EPSC2020-95, https://doi.org/10.5194/epsc2020-95, 2020

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