The surfaces of Larissa and Proteus

@article{Stooke1994TheSO,
  title={The surfaces of Larissa and Proteus},
  author={P. Stooke},
  journal={Earth, Moon, and Planets},
  year={1994},
  volume={65},
  pages={31-54}
}
  • P. Stooke
  • Published 1994
  • Geology
  • Earth, Moon, and Planets
Topographic models of Neptune's small inner satellites Larissa and Proteus were derived from the shapes of limbs and terminators in Voyager images, modified locally to accomodate large craters and ridges. The models are presented here in tabular and graphic form, including the first map of Larissa and the first detailed relief map of Proteus. The shape of Larissa is approximated by a triaxial ellipsoid with axes of 208, 192 and 178 km, but is only weakly constrained by the single available view… Expand
Topography and geology of Hyperion
Solar System Physics for Exoplanet Research
MAPPING WORLDS WITH IRREGULAR SHAPES

References

SHOWING 1-8 OF 8 REFERENCES