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| Rhea moon of Saturn |
category : satellites of planets |
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Rhea is the second moon of Saturn by the size after Titan. It was discovered in 1672 by Giovanni Domenico Cassini. Rhea was glanced through for the first time to Travel 1 in November, 1980. The Cassini probe is crossed in November 26th, 2005, in 500 km above its surface. Rhea is an ice-cold body of weak density (1240 kg / m3), indicating that the moon consists of a rocky nucleus counting only for a third of the mass of Rhea, the rest being mainly some ice-cold water. The temperature on the surface of Rhea is of-174°C in the sun, and of-200°C in-220°C in the shadow. In orbit synchronous around Saturn, Rhea always presents the same hemisphere to Saturn. The space probe Cassini presents us here the "back" face of Rhea. The hemisphere before is strongly craterised and uniformly clearly. As Callisto, craters lack structures in the marked relief presents on the Moon and the Mercury. The back hemisphere presents a network of clear trails on a dark bottom, and few craters. These trails could be the matter ejected by volcanoes of ice while Rhea was still liquid under the surface. |
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The universe of Rhea |
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In the Greek mythology, Rhea, Rheia or Rhee was
Titanide, a girl of Ouranos ( the Sky) and Gaia the Earth), sister and
woman of the Titan Cronos, and the mother of the gods Hestia, Demeter,
Hera, Hades, Poseidon and Zeus. |
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Related subjects |
category : satellites of saturn |
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Astronomy - october 15th 2007 |