Impact of Coherent Backscattering on the Spectra of Icy Satellites of Saturn and the Implications of Its Effects for Remote Sensing

Details Impact of Coherent Backscattering on the Spectra of Icy Satellites of Saturn and the Implications of Its Effects for Remote Sensing Impact of Coherent Backscattering on the Spectra of Icy Satellites of Saturn and the Implications of Its Effects for Remote Sensing

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...711l..71k&link_type=abstract

The Astrophysical Journal Letters, Volume 711, Issue 2, pp. L71-L74 (2010).

Astronomy and Astrophysics

Astronomy

1

Methods: Data Analysis, Methods: Numerical, Planets And Satellites: General, Planets And Satellites: Individual: Rhea Iapetus, Techniques: Spectroscopic

Scientific paper

We have found systematic variations in the spectra of Saturn's icy satellites Rhea and Iapetus obtained by the Cassini Visual and Infrared Mapping Spectrometer (VIMS). The main attribute of these variations is a significantly different depth of the absorption bands at different phase angles. We show that these variations likely result from the coherent backscattering effect (CBE). This effect has been mainly known as the probable reason for a steep opposition spike in brightness observed for some asteroids, moons, and Kuiper Belt Objects at phase angles smaller than 3°. The opposition spike has different steepness at different albedos due to the strong dependence of the CBE on the absorption of the material. As a result of this dependence, the impact of the CBE should be different within and outside of the absorption spectral bands. This produces a systematic change in the depth of the absorption bands at different phase angles, as we see in the VIMS spectra of Rhea and Iapetus. Neglecting this effect may result in misinterpretation of the spectra and misleading conclusions about compositional and particle size differences of icy bodies studied at different phase angles. Our computer modeling of the CBE reproduces the observed spectral variations and also shows that they are strongly affected by the size and packing of particles. Thus, the variations in the absorption bands produced by the CBE not only allow us to improve interpretation of the spectra, but also provide a promising approach to study size and packing of the regolith and dust particles.

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