Enceladus

Enceladus (ĕnsĕl`ədəs), in astronomy, one of the named moons, or natural satellites, of Saturn. Also known as Saturn II (or S2), Enceladus is 310 mi (500 km) in diameter, orbits Saturn at a mean distance of 147,900 mi (238,020 km), and has equal orbital and rotational periods of 1.37 earth days. It was discovered in 1789 by the English astronomer Sir William Herschel. Enceladus has the highest reflectivity (almost 100%) of any body in the solar system. Its surface, believed to be dominated by fresh, clean ice, is marked by few craters, smooth plains, and extensive fissures and ridges. Observations indicate that Enceladus has had five distinct geologic periods. The fresh surface suggests relatively recent volcanism, caused perhaps by tidal forces exerted by Saturn and the moon Dione, with which Enceladus forms a satellite pair (that is, they interact gravitationally). In 2005 the space probe Cassini discovered Enceladus has an atmosphere, albeit one that must be replenished by a source on the moon, because its gravity is too weak to permanently retain an atmosphere. The probe also discovered (2006) geyserlike eruptions on the moon.

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Enceladus [‚en·se′lä·du̇s]

(astronomy)

A satellite of Saturn orbiting at a mean distance of 153,600 miles (238,000 kilometers).

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Enceladus

powerful giant whose hisses cause volcanic eruptions. [Gk. Myth.: Kravitz, 88]

See : Giantism

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Enceladus

a satellite of Saturn, approximately 500 km in diameter and located at a mean distance of 237,900 km from the center of Saturn. It was discovered in 1789 by W. Herschel.