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Saturn's clouds appear in bands of yellow, beige, and off-white. Its rings appear white and relatively thin. Four moons are visible: Titan on the upper-right of Saturn's disk as an orange circle, and three small white dots, two on the left and one at the very edge of Saturn on the right. The two moons on the left are casting shadows onto Saturn's clouds, slightly above and to the right of them.

Quadruple Saturn Moon Transit

Saturn's comparatively paper-thin rings are tilted edge on to Earth every 15 years. Because the orbits of Saturn's major satellites are in the ring plane, too, this alignment gives astronomers a rare opportunity to capture a truly spectacular parade of celestial bodies crossing the face of Saturn. At the upper right is Saturn's giant moon Titan, which is larger than the planet Mercury. The frigid moon's thick nitrogen atmosphere is tinted orange with the smoggy byproducts of sunlight interacting with methane and nitrogen. The smaller, white moons are much closer to Saturn, hence much closer to the ring plane in this view. They are (from left to right) Enceladus, Dione, and Mimas. The Hubble Space Telescope's exquisite sharpness also reveals Saturn's banded cloud structure in this image.

Image Credit: NASA, ESA, and the Hubble Heritage Team (STScI/AURA); Acknowledgment: M.H. Wong (STScI/UC Berkeley) and C. Go (Philippines)
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