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Updated: Jun 18, 2026

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Preparation of Monodomain Liquid Crystal Elastomers and Liquid Crystal Elastomer Nanocomposites
Published on: February 6, 2016
Composition and physical properties of Enceladus' surface
Robert H Brown1, Roger N Clark, Bonnie J Buratti
1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
Summary
Cassini
Area of Science:
- Planetary Science
- Astrobiology
- Spectroscopy
Background:
- Saturn's moon Enceladus exhibits unique surface compositions and thermal anomalies.
- The south polar region, known as the "tiger stripes," is of particular interest.
Purpose of the Study:
- To analyze the surface composition and thermal properties of Enceladus using Cassini's Visual and Infrared Mapping Spectrometer (VIMS).
- To investigate the presence of key molecules and determine temperature limits in specific regions.
Main Methods:
- Utilized data from three Cassini flybys of Enceladus in 2005.
- Employed the Visual and Infrared Mapping Spectrometer (VIMS) for spectral analysis.
Main Results:
- Enceladus' surface is predominantly water ice, with light organics and CO2 near the south pole.
- Upper limits were established for atmospheric carbon monoxide (CO) at 5 precipitable nanometers and ammonia (NH3) in surface deposits at 2%.
- Temperatures in the tiger stripe regions were constrained to an upper limit of 140 Kelvin.
Conclusions:
- The composition of Enceladus' surface, especially the tiger stripes, provides insights into its geological activity.
- The derived limits for CO and NH3 offer constraints for atmospheric and surface models of Enceladus.
- Thermal data from the tiger stripes suggest localized energy sources or processes.
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