Ganymede: Observations by Radar
- 20 June 1975
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 188 (4194) , 1211-1212
- https://doi.org/10.1126/science.188.4194.1211
Abstract
Radar cross-section measurements indicate that Ganymede scatters to Earth 12 percent of the power expected from a conducting sphere of the same size and distance. This compares with 8 percent for Mars, 12 percent for Venus, 6 percent for Mercury, and about 8 percent for the asteroid Toro. Furthermore, Ganymede is considerably rougher (to the scale of the wavelength used, 12.6 centimeters) than Mars, Venus, or Mercury. Roughness is made evident in this experiment by the presence of echoes away from the center of the disk. A perfectly smooth target would reflect only a glint from the center, whereas a very rough target would reflect power from over the entire disk.Keywords
This publication has 7 references indexed in Scilit:
- Four-color photometry of the Galilean satellitesIcarus, 1974
- An Atmosphere on Ganymede from Its Occultation of SAO 186800 on 7 June 1972Science, 1973
- Infrared Spectra of the Galilean Satellites of JupiterThe Astrophysical Journal, 1973
- Galilean Satellites: Identification of Water FrostScience, 1972
- Low temperature condensation from the solar nebulaIcarus, 1972
- Spectral Geometric Albedo of the Galilean Satellites, 0.3 to 2.5 MicronsThe Astrophysical Journal, 1971
- Polarization measurements of the Galilean satellites of JupiterIcarus, 1971