Ganymede, Europa, Callisto, and Saturn's rings: Compositional analysis from reflectance spectroscopy

Icarus

Volumn 44, Issue 2, 1980, Pages 388-409

  Clark, Roger N ^a,b  

^a UNIVERSITY OF HAWAII   (United States)

^b MASSACHUSETTS INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000920140     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/0019-1035(80)90033-0     Document Type: Article

References (35)

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2. The spectral reflectance of water-mineral mixtures at low temperatures
3. A large scale one-dimensional array processing system
4. The Galilean satellites: New near-infrared spectral reflectance measurements (0.65–2.5 μm) and a 0.325–5 μm summary
5. The rings of Saturn: New near-infrared reflectance measurements and a 0.326–4.08 μm summary
6. Structural and thermal models of icy Galilean satellites
7. Significance of absorption features in Io's infrared reflectance spectrum
8. Infrared spectra of the satellites of Saturn: Identification of water ice on Iapetus, Rhea, Dione, and Tethys
9. Spectral reflectance characteristics of the Meteorite Classes
10. A laboratory determination of the geometric albedo of water frost, 0.2 μm to 2.0 μm
11. Visible and near-infrared spectra of minerals and rocks: I. Silicate minerals
12. Visible and near-infrared spectra of minerals and rocks: III. Oxides and hydroxides
13. Photometric properties of Saturn's rings
14. Optical properties of carbonaceous chondrites and their relationship to asteroids
15. Spectral geometric albedo of the Galilean satellites, 0.3 to 2.5 microns
16. Chemical Composition of Saturn's Rings and Icy Satellites
17. Identification of water frost on Callisto
18. Laboratory reflection spectra for the determination of chemical composition of icy bodies
19. Saturn's rings: Spectral reflectivity and compositional implications
20. Visible spectral reflectance measurements (0.3–1.1 μm) of the Galilean satellites at many orbital phase angles
21. Io's surface composition based on reflectance spectra of sulfur/salt mixtures and protonirradiation experiments
22. Spectral reflectivities of the Galilean satellites and Titan, 0.32 to 0.86 micrometers
23. Radar observations of Saturn's rings at intermediate tilt angles
24. Saturn's rings: Identification of water frost
25. Galilean satellites: Identification of water frost
26. Evidence about hydrate and solid water in the Martian surface from the 1969 Mariner infrared spectrometer
27. The rings of Saturn
28. Near-infrared spectra of the Galilean satellites: Observation and compositional implications
29. The 2–4 μm spectrum of Saturn's rings
30. Visible and near-infrared spectral photometry of the rings of Saturn from silicon diode vidicon images
31. The Jupiter system through the eyes of Voyager I
32. 2 frost or absorbate on Io's surface
33. 2O liquid-ice interfaces in the martian crust
34. Photometry of the surface features of Ganymede: First Voyager results