Neptune and Rings (WF/PC-30) Cycle 1

Details Neptune and Rings (WF/PC-30) Cycle 1 Neptune and Rings (WF/PC-30) Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3186w&link_type=abstract

HST Proposal ID #3186

Physics

Hst Proposal Id #3186

Scientific paper

Observations will provide high-resolution images of Neptune and its rings in spectral regions not covered by Voyager spacecraft cameras and/or not possible from the Earth-based observations. At short wavelengths, the global reflectivity of Neptune is less than that of a pure Rayleigh atmosphere; thus structure may be visible. Observations will be made in four sequences, distributed over 18 hours. The tenuous ring system and the associated satellites will be observed with the Planetary Camera.

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