Observations of Ganymede, Callisto, Ceres, Uranus, and Neptune at 3.33 MM wavelength

Details Observations of Ganymede, Callisto, Ceres, Uranus, and Neptune at 3.33 MM wavelength Observations of Ganymede, Callisto, Ceres, Uranus, and Neptune at 3.33 MM wavelength

Feb 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976icar...27..183u&link_type=abstract

Icarus, vol. 27, Feb. 1976, p. 183-189.

Physics

9

Brightness Temperature, Callisto, Ceres Asteroid, Microwave Spectra, Neptune (Planet), Uranus (Planet), Black Body Radiation, Extremely High Frequencies, Planetary Radiation, Planetary Rotation, Polarized Electromagnetic Radiation, Radiant Flux Density

Scientific paper

The paper reports measurements of the 3.33-mm disk brightness temperatures of Ganymede (136 plus or minus 21 K), Callisto (95 plus or minus 17 K), Ceres (137 plus or minus 25 K), Uranus (125 plus or minus 9 K), and Neptune (126 plus or minus 9 K). The observations of Ganymede are consistent with the radiation from a blackbody in solar equilibrium, whereas Callisto's microwave spectrum indicates a surface similar to that of the moon. The disk temperature for Ceres agrees with that expected from a rapidly leading rotating blackbody. The millimeter temperatures of Uranus and Neptune greatly exceed solar equilibrium values, implying atmospheres with large temperature gradients.

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