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Sunday, August 14, 2022
Home This false-color image to the right shows an infrared spectral map of Saturn’s A, B and C rings, captured by Cassini’s VIMS. (Infrared image credit: NASA/JPL-Caltech/University of Arizona/CNRS/LPG-Nantes); (Saturn image credit: NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic) This false-color image to the right shows an infrared spectral map of Saturn's A, B and C rings, captured by Cassini's VIMS. (Infrared image credit: NASA/JPL-Caltech/University of Arizona/CNRS/LPG-Nantes); (Saturn image credit: NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic)

This false-color image to the right shows an infrared spectral map of Saturn’s A, B and C rings, captured by Cassini’s VIMS. (Infrared image credit: NASA/JPL-Caltech/University of Arizona/CNRS/LPG-Nantes); (Saturn image credit: NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic)

This false-color image to the right shows an infrared spectral map of Saturn's A, B and C rings, captured by Cassini's VIMS. (Infrared image credit: NASA/JPL-Caltech/University of Arizona/CNRS/LPG-Nantes); (Saturn image credit: NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic)

This false-color image to the right shows an infrared spectral map of Saturn’s A, B and C rings, captured by Cassini’s VIMS. (Infrared image credit: NASA/JPL-Caltech/University of Arizona/CNRS/LPG-Nantes); (Saturn image credit: NASA/JPL-Caltech/Space Science Institute/G. Ugarkovic)

A false-color image mosaic shows Daphnis, one of Saturn’s ring-embedded moons, and the waves it kicks up in the Keeler gap. Images collected by Cassini’s close orbits in 2017 are offering new insight into the complex workings of the rings. (NASA/JPL-Caltech/Space Science Institute)