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Convective instability in Europa's floating ice shell
- W. McKinnon
- Environmental Science, Physics
- 1 July 1997
Models of the tidally heated, floating ice shell proposed for the jovian satellite Europa generally find shell thicknesses less than 30 km. Past parameterized convection models indicated that such…
The tectonics of Mercury
- H. Melosh, W. McKinnon
- Geology
- 1988
The probable tectonic history of Mercury and the relative sequence of events are discussed on the basis of data collected by the Mariner-10 spacecraft. Results indicate that Mercury's tectonic…
Interior composition, structure and dynamics of the Galilean satellites
- G. Schubert, J. Anderson, T. Spohn, W. McKinnon
- Physics
- 2004
Gravitational fiels of the satellites: flyby determination of C22, gravity results; Io, Europa, Ganymede, Callisto - interior models; Thermal considerations in the maintenance of intra-ice oceans on…
The Pluto system: Initial results from its exploration by New Horizons
- S. Stern, F. Bagenal, E. Zirnstein
- Geology, PhysicsScience
- 16 October 2015
TLDR
Liquid water on Enceladus from observations of ammonia and 40Ar in the plume
This corrects the article DOI: 10.1038/nature08153
On convection in ice I shells of outer Solar System bodies, with detailed application to Callisto
- W. McKinnon
- Geology, Physics
- 1 August 2006
Cratering of planetary satellites.
- C. Chapman, W. McKinnon
- Physics, Geology
- 1986
Recent findings concerning craters and cratering populations on the satellites of Jupiter and Saturn are discussed. Current understanding of cratering mechanics is reviewed with emphasis placed on…
Liquid water on Enceladus from observations of ammonia and 40Ar in the plume
Jets of water ice from surface fractures near the south pole of Saturn’s icy moon Enceladus produce a plume of gas and particles. The source of the jets may be a liquid water region under the ice…
The small satellites of Pluto as observed by New Horizons
- H. Weaver, M. Buie, A. Zangari
- Geology, PhysicsScience
- 18 March 2016
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