Mimas (moon)



         


Mimas
Discovery
Discovered by William Herschel
Discovered on September 17, 1789
Orbital characteristics
Semimajor axis 185,520 km
Eccentricity 0.0202
Orbital period 22 h 37 min 5 s
Inclination 1.53 °
Is a satellite of Saturn
Physical characteristics
Mean diameter 397.2 km
Mass 3.84×1019 kg
Mean density 1.17 g/cm3
Surface gravity 0.077 m/s2
Rotation period 22 h 37 min 5 s
(synchronous)
Axial tilt 0.005 °
Albedo 0.77
Atmosphere none

Mimas ("MY muss") is a moon of Saturn that was discovered in 1789 by William Herschel. It is named after Mimas, a son of Gaia in Greek mythology. It is also designated Saturn I.

The name "Mimas" and the names of all seven satellites of Saturn then known were suggested by Herschel's son John Herschel in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope .

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Physical characteristics

Mimas' low density (1.17) indicates that it is composed mostly of water ice with only a small amount of rock.

Mimas' most distinctive feature is a colossal impact crater 130 km across, named Herschel after the moon's discoverer. Herschel covers almost 1/3 of the diameter of the entire moon; its walls are approximately 5 km high, parts of its floor measure 10 km deep, and its central peak rises 6 km above the crater floor. If there were a crater of an equivalent scale on Earth it would be over 4000 km in diameter, wider than Canada. The impact that made this crater must have nearly disrupted Mimas entirely; fractures can be seen on the opposite side of Mimas that may be due to the shock waves from the impact travelling through the moon's body.

The surface is saturated with other smaller impact craters, but no others are anywhere near the size of Herschel. Although Mimas is heavily cratered, the cratering is not uniform. Most of the surface is covered with craters greater than 40 km in diameter but in the south polar region, craters greater than 20 km are generally lacking. This suggests that some process removed the larger craters from these areas.

Scientists officially recognise two types of geological feature on Mimas: craters and chasmata (chasms). See also: List of geological features on Mimas

The Cassini-Huygens orbiter is due to perform a flyby of Mimas on August 1, 2005.

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Mimas in Fiction and Film


... | Janus, Epimetheus | Mimas | S/2004 S 1 | ...


Saturn
Janus' group | Mimas | Enceladus | Tethys | Dione | Rhea
Titan | Hyperion | Iapetus | Siarnaq's group | Phoebe's group
(For other moons, see: Saturn's natural satellites)






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