Abstract
AbstractThe radar properties of icy satellites of Jupiter and Saturn commonly differ by more than an order of magnitude from those of rocky planets because of the lower absorptivity of water ice than that of rock. However, the specific mechanisms behind these differences are not confidently known yet. Here we show that the global radar albedos and the circular polarization ratios of icy satellites are correlated and vary together along a continuum, which is not satisfactorily explained by existing models. We modified a backscatter model that includes the coherent backscatter opposition effect (CBOE) and found that it fits successfully the observed continuum, indicative of CBOE’s primary role in driving the circular polarization ratios of icy satellites. We predict that the linear polarization ratios and the incidence angle variation properties also vary along the observed continuum, and that, globally, Europa and Enceladus have very heterogeneous surfaces/subsurfaces with very little microwave absorption. The modified CBOE model suggests that some worlds beyond Saturn’s orbit that are rich in non-water ices may have even more extreme radar properties.
Funder
NASA Europa Lander Pre-project
Publisher
Springer Science and Business Media LLC
Subject
Astronomy and Astrophysics
Reference38 articles.
1. Ostro, S. J. Planetary radar astronomy. Rev. Mod. Phys. 65, 1235–1279 (1993).
2. Black, G. J., Campbell, D. B. & Carter, L. M. Arecibo radar observations of Rhea, Dione, Tethys, and Enceladus. Icarus 191, 702–711 (2007).
3. Hagfors, T. Relationship of geometric optics and autocorrelation approaches to the analysis of lunar and planetary radar. J. Geophys. Res. 71, 379 (1966).
4. Fung, A. K. Microwave Scattering and Emission Models and Their Applications (Artech House, 1994).
5. Wye, L. C. Radar Scattering from Titan and Saturn’s Icy Satellites Using the Cassini Spacecraft. PhD thesis, Stanford Univ. (2011).
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