Proteus: Geology, shape, and catastrophic destruction☆
References (55)
- et al.
The shape and internal structure of Mimas
Icarus
(1988) - et al.
Saturn's icy satellites: Thermal and structural models
Icarus
(1983) Compaction and internal structure of Mimas
Icarus
(1990)- et al.
Compression effects in rock-ice mixtures: An application to the study of satellites
Phys. Earth Planet. Inter.
(1989) - et al.
Experimental study on the velocity of fragments in collisional breakup
Icarus
(1980) - et al.
Correlation of mechanical and thermal properties of the lunar surface
Icarus
(1969) - et al.
On the fragmentation of asteroids and planetary satellites
Icarus
(1990) - et al.
Topography on satellite surfaces and the shape of asteroids
Icarus
(1973) - et al.
Rheological properties of ammonia-water liquids and crystal-liquid slurries: Planetological applications
Icarus
(1991) Tectonic patterns on a tidally distorted planet
Icarus
(1980)
A semiempirical model of catastrophic breakup processes
Icarus
Some recent advances in the scaling of impact and explosion cratering
Intl. J. Impact Eng.
Neptune's small inner satellites
J. Geophys. Res.
Neptune's small inner satellites
J. Geophys. Res.
Neptune's small inner satellites
J. Geophys. Res.
Small satellites
The Martian hemispheric dichotomy may be due to a giant impact
Nature
Cratering of planetary satellites
Impact Craters from Centimeters to Megameters
Ripple ring basins on Ganymede and Callisto
Rep. Planet. Geol. Geophys. Prog.—1984
The scaling of complex craters
Crater morphology and morphometry on the Uranian satellites
Rep. Planet. Geol. Geophys. Prog.—1986
Mechanical and thermal properties of planetologically important ices
Rep. Planet. Geol. Geophys. Prog.—1986
Crater depth/diameter/morphology relations on the icy satellites: Implications for ice rheology
Iapetus: Tectonic structure and geologic history
Rep. Planet. Geol. Geophys. Prog.—1990
Mimas: Tectonic structure and geologic history
Rep. Planet. Geol. Geophys. Prog.—1990
Aspects of tectonics on icy satellites
Proteus: Satellite on the brink?
Geology of the uranian satellites
Cited by (45)
Craters and ejecta on Pluto and Charon: Anticipated results from the New Horizons flyby
2015, IcarusCitation Excerpt :Because of Triton’s probable origin and perplexing cratering record (Schenk and Zahnle, 2007; McKinnon and Singer, 2010), we consider Triton as a poor constraint on the heliocentric impactor flux at Neptune. Proteus is an inner moon of Neptune on which large craters were seen, but imaging is limited because the moon was only discovered during Voyager’s approach to Neptune, and exposures were short to reduce smear (Croft, 1992; Stooke, 1994). Thus a crater SFD cannot be determined for Proteus.
Rate-dependent strength of porous ice-silica mixtures and its implications for the shape of small to middle-sized icy satellites
2010, IcarusCitation Excerpt :However, small icy satellites very close to planets, such as Pan and Prometheus, have an ellipsoidal figure due to tidal stress. Croft (1992) proposed that the dominant mechanism driving topographic relaxation was viscous flow: the transition radius between relaxed and non-hydrostatic shapes could be determined from the ratio of gravitational stress to planetary material viscoelasticity. He suggested that internal temperature strongly affects viscous creep, which drives the relaxation to a spherical shape.
Which are the dwarfs in the Solar System?
2008, Icarus
- ☆
Presented at Neptune/Triton Conference in Tucson, Arizona, during January 6–10, 1992.