Abstract
In 1848 the eighth moon of Saturn was discovered. Named Hyperion, it was a dim object, so dim that it could be no larger than a few hundred miles across—perhaps 300—making it only about one-tenth the size of Earth’s moon. It orbited well outside Saturn’s rings at a distance of 980,000 miles from the planet, and its orbit, although eccentric compared to planetary orbits, was considerably less eccentric than many of the asteroid orbits.
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References
Binzel, Richard, Green, Jacklyn, and Opal, Chet, “Chaotic Rotation of Hyperion?” Nature 320 (April 10, 1985 ) 511.
Klavetter, James, “Rotation of Hyperion” The Astronomical Journal 97 (February 1989) 570.
Murray, Carl, “Chaotic Spinning of Hyperion” Nature 311 (October 25, 1984 ) 705.
Wisdom, Jack, Peale, Stanton, and Mignard, Francois, “The Chaotic Rotation of Hyperion” Icarus 58 (May 1984) 137.
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© 1996 Barry Parker
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Parker, B. (1996). The Strange Case of Hyperion, and Other Mysteries. In: Chaos in the Cosmos. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-3370-6_10
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DOI: https://doi.org/10.1007/978-1-4899-3370-6_10
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