Dione

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Dione
Discovery
Discovered byGiovanni Domenico Cassini
Orbital characteristics
377,400 km
Eccentricity0.0022
2.736915 days
10.03 km/s
Known satellitesHelene, Polydeuces
Physical characteristics
Dimensions1122.8 × 1122.8 × 1122.8 km
561.4 km
3,959,000 km²
Volume741,000,000 km³
Mass1.09552 × 10^21 kg
Mean density
1.478 g/cm³
0.232 m/s²
0.515 km/s
synchronous
zero
Albedo0.998
Temperature87 K

Dione is a natural satellite of Saturn. It was discovered by the Italian astronomer Giovanni Domenico Cassini in 1684. Dione is the fifteenth-largest moon in the Solar System and the fourth-largest moon of Saturn.

Physical characteristics[edit | edit source]

Dione has a mean radius of 561.4 km and a mass of 1.09552 × 10^21 kg. Its density is 1.478 g/cm³, which suggests that it is composed of a mixture of water ice and silicate rock. The surface of Dione is heavily cratered, with a number of bright ice cliffs and fractures.

Orbit and rotation[edit | edit source]

Dione orbits Saturn at a distance of approximately 377,400 km. It has a very low orbital eccentricity of 0.0022 and completes one orbit around Saturn in about 2.736915 days. Dione is in synchronous rotation with Saturn, meaning that it always shows the same face to the planet.

Surface features[edit | edit source]

The surface of Dione is marked by a variety of geological features, including craters, chasms, and ice cliffs. The most prominent feature is the Janiculum Dorsa, a large ridge that stretches across the moon's surface. Other notable features include the Carrel Crater and the Padua Chasmata.

Subsatellites[edit | edit source]

Dione has two known trojan moons, Helene and Polydeuces, which share its orbit around Saturn.

Exploration[edit | edit source]

Dione has been studied by several spacecraft, including the Voyager missions and the Cassini spacecraft. These missions have provided detailed images and data about Dione's surface and composition.

See also[edit | edit source]

Related pages[edit | edit source]

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Contributors: Prab R. Tumpati, MD