Infrared radiometry of Uranus and Neptune at 21 and 32 microns

Physics

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Brightness Temperature, Emission Spectra, Infrared Radiometers, Neptune Atmosphere, Uranus Atmosphere, Infrared Filters, Infrared Telescopes, Space Infrared Telescope Facility, Planets, Giant Planets, Infrared, Wavelengths, Radiometry, Temperature, Uranus, Neptune, Earth-Based Observations, Telescope Methods, Brightness, Equipment, Procedure, Transmissions, Spectra, Structure, Jupiter, Satellites, Callisto, Ganymede

Scientific paper

Radiometric measurements of Uranus and Neptune near 21 and 32 μm have been made with filters with widths of 8 and 5 μm, respectively. The observations at 21 μm, made on 1985 June 19 at the NASA Infrared telescope facility at Mauna Kea, Hawaii, corresponded to brightness temperatures of 54.1±0.3K for Uranus and 58.1±0.3K for Neptune. The observations at 32 μm were made on three nights: 1983 May 1 and 1984 May 30 and 31, also at the NASA IRTF. These measurements corresponded to brightness temperatures of 51.8±1.5K for Uranus and 55.6±1.2K for Neptune. The observations are consistent with higher-resolution studies and confirm the general decrease of brightness temperatures going from about 20 to 30 μm.

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