2.7- to 4.1-μm spectrophotometry of icy satellites of Saturn and Jupiter
- 31 August 1985
- Vol. 63 (2), 237-242
- https://doi.org/10.1016/0019-1035(85)90008-9
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
- The composition and origin of the Iapetus dark materialIcarus, 1985
- Saturn's satellites: Nuar-infrared spectrophotometry (0.6–2.5 μm) of the leading and trailing sides and compositional implicationsIcarus, 1984
- Frost grain size metamorphism: Implications for remote sensing of planetary surfacesIcarus, 1983
- The dark side of IapetusIcarus, 1983
- Infrared observations of the dark side of IapetusIcarus, 1982
- Ganymede, Europa, Callisto, and Saturn's rings: Compositional analysis from reflectance spectroscopyIcarus, 1980
- Near-infrared spectra of the Galilean satellites: Observations and compositional implicationsIcarus, 1978
- The 2–4-μm spectrum of Saturn's ringsIcarus, 1977