Is H 2O Present on Io? The Detection of a New Strong Band Near 3590 cm -1 (2.79 μm)
Abstract
A strong absorption band at 3590 ± 20 cm -1 (2.790 ± 0.015 μm) has been discovered in the spectrum of Io using the Kuiper Airborne Observatory (KAO). The 2 v1 + v3 combination mode of solid SO 2 falls at this position. Since SO 2 is abundant on Io it must contribute to the new band. However, a band due to H 2O was predicted near this frequency in Io's spectrum based on laboratory experiments of H 2O: SO 2 mixed Io ice analogs which were used to assign the two weak, variable features at 3370 and 3170 cm -1 (2.97 and 3.15 μm) to trace amounts of H 2O frozen in solid SO 2 on Io. The new band probably originates from both SO 2 and H 2O. Unfortunately, the spectral resolution of the data is insufficient to settle the issue of whether there are two resolvable components.
- Publication:
-
Icarus
- Pub Date:
- February 1994
- DOI:
- 10.1006/icar.1994.1033
- Bibcode:
- 1994Icar..107..413S
- Keywords:
-
- Absorption Spectra;
- Abundance;
- Ice;
- Io;
- Sulfur Dioxides;
- Water;
- Chemical Composition;
- Kuiper Airborne Observatory;
- Spectrum Analysis;
- JUPITER;
- SATELLITES;
- IO;
- WATER;
- AIRCRAFT OBSERVATIONS;
- KAO AIRCRAFT;
- OPTICAL PROPERTIES;
- SPECTROSCOPY;
- SPECTRA;
- ABSORPTION;
- COMPOSITION;
- REFLECTIVITY;
- SULFUR DIOXIDE;
- MIXING;
- ICE;
- HYDROXYL;
- COMPARISON;
- Astrophysics; Satellites of Jupiter