Related Content
Search Google Scholar for:
More Information
Related Jobs from ScienceCareers
|
|
Science 6 March 1998: Vol. 279. no. 5356, pp. 1514 - 1517 DOI: 10.1126/science.279.5356.1514
|
|
Reports
Origin of Mountains on Io by Thrust Faulting and Large-Scale Mass Movements
Paul M. Schenk,
*
Mark H. Bulmer
Voyager stereoimages of Euboea Montes, Io, indicate that this
mountain formed when a large crustal block was uplifted 10.5 kilometers
and tilted by approximately 6 degrees. Uplift triggered a massive slope
failure on the northwest flank, forming one of the largest debris
aprons in the solar system. This slope failure probably involved
relatively unconsolidated layers totaling approximately 2 kilometers in
thickness, overlying a rigid crust (or lithosphere) at least 11 kilometers thick. Mountain formation on Io may involve localized
deep-rooted thrust faulting and block rotation, due to compression at
depth induced during vertical recycling of Io's crust.
P. M. Schenk, Lunar and Planetary Institute, Houston,
TX 77058, USA.
M. H. Bulmer, Center for Earth and Planetary Science, National Air
and Space Museum, Washington, DC 20560, USA.
*
To whom correspondence should be addressed. E-mail:
schenk{at}lpi3.jsc.nasa.gov
Read the Full Text
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
- Structural analysis and analogue modeling of the kinematics and dynamics of rockslide avalanches.
- T. Shea and B. van Wyk de Vries (2008)
Geosphere
4, 657-686
| Abstract »
| Full Text »
| PDF »
- Chaos on Io: A model for formation of mountain blocks by crustal heating, melting, and tilting.
- W. B. McKinnon, P. M. Schenk, and A. J. Dombard (2001)
Geology
29, 103-106
| Abstract »
| Full Text »
| PDF »
- Galileo at Io: Results from High-Resolution Imaging.
- A. S. McEwen, M. J. Belton, H. H. Breneman, S. A. Fagents, P. Geissler, R. Greeley, J. W. Head, G. Hoppa, W. L. Jaeger, T. V. Johnson, et al. (2000)
Science
288, 1193-1198
| Abstract »
| Full Text »
- The Galilean Satellites.
- A. P. Showman and a. R. Malhotra (1999)
Science
286, 77-84
| Abstract »
| Full Text »
|
|