Regular ArticleKeck Infrared Observations of Jupiter's Ring System near Earth's 1997 Ring Plane Crossing☆
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Near-IR photometry of the small Uranian satellites with Keck at phase angles 0–2°
2023, IcarusCitation Excerpt :The other moons, overall, are either neutral or slightly reddish in color. Such colors have been seen for other small moonlets in the jovian system (e.g., Thomas et al., 1998; de Pater et al., 1999; Takato et al., 2004), and for Galatea in the neptunian system (de Pater et al., 2005). In the present paper, we show that the phase curves in the near-infrared are very similar to those at the visible wavelengths reported by Karkoschka (2001b).
Electrostatic lofting of dust grains from the surfaces of Thebe and Amalthea
2020, Planetary and Space ScienceInstrumentation for Planetary Exploration Missions
2015, Treatise on Geophysics: Second EditionThe lunar dust environment
2011, Planetary and Space ScienceCitation Excerpt :This ring system was investigated with remote imaging from the Earth and by the Voyager, Galileo, Cassini, and New Horizons spacecrafts, revealing a significant structure in the ring. By now, at least four components have been identified (Ockert-Bell et al., 1999; Burns et al., 1999; de Pater et al., 1999): the main ring, interior halo and two gossamer rings. The faint gossamer rings appear to extend primarily inward from the orbits of Amalthea and Thebe.
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R. GreenbergA. Brahic