Near infrared imaging of Uranus and Neptune

Details Near infrared imaging of Uranus and Neptune Near infrared imaging of Uranus and Neptune

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2330..213s&link_type=abstract

In JPL Uranus and Neptune p 213-223 (SEE N85-11927 02-91)

Astronomy and Astrophysics

Astronomy

2

Imaging Techniques, Infrared Astronomy, Infrared Imagery, Neptune Atmosphere, Uranus Atmosphere, Albedo, Brightness, Clouds, Image Resolution, Methane

Scientific paper

Imaging of Uranus and Neptune in the deep methane absorption band at 890 nm has been used to detect high-altitude atmospheric hazes and to search for possible undiscovered close-in satellites. The appearances of Uranus and Neptune are very different from one another and Uranus seems to be changing with time. The Neptune images show rotation in the direct sense. No new satellites have been found to date.

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