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Updated: Jul 7, 2026

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Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
Ultraviolet imaging spectroscopy shows an active saturnian system
Larry W Esposito1, Joshua E Colwell, Kristopher Larsen
1University of Colorado, Laboratory for Atmospheric and Space Physics, 234 Innovation Drive, Boulder, CO 80303-7814, USA. larry.esposito@lasp.colorado.edu
Summary
Saturn
Area of Science:
- Planetary Science
- Space Physics
- Astrochemistry
Background:
- The Saturnian system exhibits dynamic processes affecting its atmospheric composition and ring structure.
- Understanding these processes is key to deciphering the evolution of gas giants and their environments.
Purpose of the Study:
- To investigate the variability of neutral oxygen, auroral activity, and water-ice distribution within the Saturnian system.
- To determine the origin of Phoebe and the evolutionary history of Saturn's rings.
Main Methods:
- Analysis of observational data pertaining to neutral oxygen abundance.
- Spectroscopic comparison of Saturn's aurora with Jupiter's.
- Assessment of water-ice content variations on Phoebe and within Saturn's rings.
Main Results:
- Neutral oxygen in the Saturnian system shows variability, with a peak abundance of 4 x 10(34) atoms.
- Saturn's aurora responds to solar-wind forcing and shares spectral similarities with Jupiter's.
- Phoebe's surface exhibits variable water-ice content, suggesting an outer solar system origin.
- Saturn's rings display radial variations in water abundance, with the purest ice in the A ring.
Conclusions:
- The observed radial variation in Saturn's rings supports a model of initial purity followed by meteoritic bombardment.
- Smaller radial structures suggest recent renewal events in Saturn's rings within the last 10(7) to 10(8) years.
- Phoebe's composition points to a formation in the outer solar system, contributing to our understanding of planetary body origins.
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