A shear heating origin for ridges on Triton

@inproceedings{Prockter2005ASH,
  title={A shear heating origin for ridges on Triton},
  author={Louise M. Prockter and Francis Nimmo and Robert T. Pappalardo},
  year={2005}
}
[1] Triton and Europa each display a variety of distinctive curvilinear ridges and associated troughs. Here we propose that ridges on Triton may have formed by diurnal tidal stresses, in a manner similar to that proposed for ridge formation on Europa. The greater width of ridges on Triton is likely a consequence of the lower surface temperature and greater brittle-ductile transition depth on this body compared to Europa. The magnitudes of the stresses and heat fluxes required to generate ridges… CONTINUE READING

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References

Publications referenced by this paper.
Showing 1-10 of 30 references

The coupled orbital and thermal evolution of Triton

  • M. N. Ross, G. Schubert
  • Res . Lett .
  • 1990
Highly Influential
1 Excerpt

Ages and interiors: The cratering record of the Galilean satellites, in Jupiter: The Planet, Satellites and Magnetosphere, edited by F. Bagenal

  • Schenk, M P.
  • 2004

Combined effects of diurnal and nonsynchronous surface stresses on Europa

  • M Stempel
  • Proc. Lunar. Planet. Sci. Conf., [CD-ROM],
  • 2004

Ridges and tidal stress on Io, Icarus

  • Bart, D G.
  • 2004

On the origins of band topography

  • F. Nimmo, R. T. Pappalardo, B. Giese
  • Europa, Icarus,
  • 2003
2 Excerpts

Polar wander on Triton and Pluto due to volatile migration, Icarus

  • D. P. Rubincam
  • 2003
1 Excerpt

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