STIS spectroscopy of Jupiter, Saturn, Titan and the Moon in the UV

Details STIS spectroscopy of Jupiter, Saturn, Titan and the Moon in the UV STIS spectroscopy of Jupiter, Saturn, Titan and the Moon in the UV

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7717c&link_type=abstract

HST Proposal ID #7717

Physics

Hst Proposal Id #7717 Solar System

Scientific paper

This program will use the STIS to observe the Moon, Jupiter, Saturn and
Titan in the UV. The goal is to determine weak absorption features, due
to atmospheric gases, as well as Raman scattering features in the
spectra of Jupiter, Saturn and Titan. The Moon will be used as a solar
analog to reduce planetary fluxes to reflectivities.

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