Galilean satellite observation plans for the near‐infrared mapping spectrometer experiment on the Galileo spacecraft
- 21 September 1995
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 100 (E9) , 18957-18972
- https://doi.org/10.1029/95je01766
Abstract
On December 7, 1995, the Galileo spacecraft will begin observations of the Jovian system with orbit insertion and a satellite tour of 10 orbits. The Galilean satellites will be observed with four remote sensing instruments spanning the ultraviolet, visible, near infrared, and thermal infrared regions of the spectrum. The Galileo near‐infrared mapping spectrometer will observe the satellites in the wavelength range 0.7–5.2 μm, a region particularly well suited for analyzing volatile components. Planned observations include mapping most available longitudes at about 100‐km resolution per pixel at full wavelength resolution, together with observing limited regions at high spatial resolution. The opportunity to affect the choice and design of observations for the Galileo tour extends until June 1996.Keywords
This publication has 45 references indexed in Scilit:
- Charge‐coupled device spectra of the Galilean satellites: Molecular oxygen on GanymedeJournal of Geophysical Research, 1995
- Spectra of the icy Galilean satellites from 0.2 to 5μm: A compilation, new observations, and a recent summaryJournal of Geophysical Research, 1995
- The albedo spectrum of Europa from 2200 Å to 3300 ÅJournal of Geophysical Research, 1995
- Ground-based observations of IoReviews of Geophysics, 1995
- Io's heat flow from infrared radiometry: 1983–1993Journal of Geophysical Research, 1994
- The 2.5–5.0 μm spectra of Io: Evidence for H2S and H2O frozen in SO2Icarus, 1990
- Sulfur flows of Ra Patera, IoIcarus, 1984
- Spectral evidence for SO2 frost or adsorbate on Io's surfaceNature, 1979
- Significance of absorption features in Io's IR reflectance spectrumNature, 1979
- Identification of gaseous SO2 and new upper limits for other gases on IoNature, 1979