On the State of Water Ice on Saturn's Moon Titan and Implications to Icy Bodies in the Outer Solar System
Weijun Zheng, David Jewitt, and Ralf I. Kaiser

TL;DR
This study investigates how water ice on icy bodies like Titan changes between amorphous and crystalline states due to temperature and radiation, revealing a balance influenced by thermal recrystallization and irradiation effects.
Contribution
It provides systematic experimental data on the effects of ionizing radiation and temperature on water ice's crystalline state relevant to outer Solar System bodies.
Findings
Crystalline water ice can only be partially amorphized by electron irradiation.
Thermal recrystallization dominates at temperatures above 50 K.
Most icy bodies in the Solar System have crystalline water ice due to their temperature conditions.
Abstract
The crystalline state of water ice in the Solar System depends on the temperature history of the ice and the influence of energetic particles to which it has been exposed. We measured the infrared absorption spectra of amorphous and crystalline water ice in the 10-50 K and 10-140 K temperature range, respectively, and conducted a systematic experimental study to investigate the amorphization of crystalline water ice via ionizing radiation irradiation at doses of up to 160 \pm 30 eV per molecule. We found that crystalline water ice can be converted only partially to amorphous ice by electron irradiation. The experiments showed that a fraction of the 1.65 \mum band, which is characteristic for crystalline water ice, survived the irradiation, to a degree that strongly depends on the temperature. Quantitative kinetic fits of the temporal evolution of the 1.65 \mum band clearly demonstrate…
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