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  2. Rings of Saturn - Wikipedia

    en.wikipedia.org/wiki/Rings_of_Saturn

    The full set of rings, imaged on 19 July 2013 as Saturn eclipses the Sun from the vantage of the Cassini orbiter, 1.2 million kilometres (3 ⁄ 4 million miles) distant. . Earth appears as a dot at 4 o'clock, between the G and E rings – with its brightness artificially exaggerated in this photog

  3. Saturn - Wikipedia

    en.wikipedia.org/wiki/Saturn

    However, measurements of Saturn's rings suggest a much more diffuse core, with a mass equal to about 17 Earths and a radius equal to about 60% of Saturn's entire radius. [47] This is surrounded by a thicker, liquid metallic hydrogen layer, followed by a liquid layer of helium-saturated molecular hydrogen , which gradually transitions to a gas ...

  4. Saturn's rings will disappear from view of ground-based ... - AOL

    www.aol.com/saturns-rings-disappear-view-ground...

    Saturn’s rings are seen as viewed by NASA’s Cassini spacecraft, which obtained the images that comprise this mosaic at a distance of approximately 450,000 miles from Saturn April 25, 2007.

  5. The rings of Saturn are going to disappear in a few months ...

    www.aol.com/rings-saturn-going-disappear-few...

    That doesn’t include Saturn’s rings. Saturn is the sixth planet from our sun and orbits at a distance of about 886 million miles from it. Saturn takes about 10.7 hours (no one knows precisely ...

  6. Phoebe (moon) - Wikipedia

    en.wikipedia.org/wiki/Phoebe_(moon)

    The Phoebe ring is one of the rings of Saturn. This ring is tilted 27 degrees from Saturn's equatorial plane (and the other rings). It extends from at least 128 to 207 [20] times the radius of Saturn; Phoebe orbits the planet at an average distance of 215 Saturn radii. The ring is about 40 times as thick as the diameter of the planet. [21]

  7. Roche limit - Wikipedia

    en.wikipedia.org/wiki/Roche_limit

    Indeed, almost all known planetary rings are located within their Roche limit. (Notable exceptions are Saturn's E-Ring and Phoebe ring. These two rings could possibly be remnants from the planet's proto-planetary accretion disc that failed to coalesce into moonlets, or conversely have formed when a moon passed within its Roche limit and broke ...

  8. Great mystery of Saturn’s Rings May Have Been Solved: New Study

    www.aol.com/news/great-mystery-saturn-rings-may...

    A study published in the journal Science suggests a hypothetical moon (called Chrysalis) came too close to Saturn's gravitational pull and was torn apart, forming the planet's iconic rings.

  9. Pallene (moon) - Wikipedia

    en.wikipedia.org/wiki/Pallene_(moon)

    The faint Pallene ring is visible at the bottom left as indicated. In 2006, images taken in forward-scattered light by the Cassini spacecraft enabled the Cassini Imaging Team to discover a faint dust ring around Saturn that shares Pallene's orbit, now named the Pallene Ring. [11] [12] The ring has a radial extent of about 2,500 km. Its source ...