| Discovery | |||||||
|---|---|---|---|---|---|---|---|
| Discovered by | William Herschel | ||||||
| Discovered on | September 17, 1789 | ||||||
| Orbital characteristics | |||||||
| Semimajor axis | 185,404 km | ||||||
| Eccentricity | 0.0202 * | ||||||
| Orbital period | 0.9424218 d * | ||||||
| Inclination | 1.51° (to Saturn's equator) | ||||||
| Is a satellite of | Saturn | ||||||
| Physical characteristics | |||||||
| Mean diameter | 396.6 km (414.8×394.4×381.4 km)* | (0.0311 Earths)||||||
| Surface area | ~1,990,000 km2 | ||||||
| Volume | ~32,900,000 km3 | ||||||
| Mass | 3.84 kg | (6.4 Earths)||||||
| Mean density | 1.17 g/cm3 | ||||||
| Surface gravity | ~0.065 m/s2 | ||||||
| Escape velocity | ~0.16 km/s | ||||||
| Rotation period | synchronous | ||||||
| Axial tilt | zero | ||||||
| Albedo | 0.77 | ||||||
| Surface temp. | |||||||
| min | mean | max |
|---|---|---|
| ? K | ~64 K | ? K |
Mimas was one of the Titans of Greek mythology. The name "Mimas", indeed the names of all seven then-known satellites of Saturn, were suggested by Herschel's son John Herschel in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope *. He named them after Titans specifically because Saturn, known as Kronos in Greek mythology, was the leader of the Titans.
According to Liddell and Scott's Greek-English Lexicon, the adjectival form of Mimas/Mimans would be Mimantean (the genitive case is Mimantis, Greek Μῑμάντις). In practice, anglicisms such as Mimasian and Mimian are very occasionally seen, but more commonly writers simply use the phrase 'of Mimas'.
Mimas (NASA) PIA06176.jpg Mimas' most distinctive feature is a colossal impact crater 130 km across, named Herschel after the moon's discoverer. Herschel's diameter is almost a third of the moon's own diameter; 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 4,000 km in diameter, wider than Canada. The impact that made this crater must have nearly shattered Mimas: fractures can be seen on the opposite side of Mimas that may have been created by shock waves from the impact travelling through the moon's body.
The surface is saturated with 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 features on Mimas: craters and chasmata (chasms). See also: List of geological features on Mimas.
Mimas is responsible for clearing the material from the Cassini Division, the gap between Saturn's two widest rings, A Ring and B Ring.
Мимас (спътник) | Mimas (satèl·lit) | Mimas | Mimas (měsíc) | Mimas (måne) | Mimas (Mond) | Mimas (luna) | Mimas (lune) | Mimas (mjesec) | Mimas (astronomia) | Mimas (satelles) | Mimas (maan) | ミマス (衛星) | Mimas | Saturnmånen Mimas | Mimas (księżyc) | Mimas (satélite) | Мимас (спутник) | Mimas (mesiac) | Мима | Mimas | Mimas | Mimas (uydu) | 土卫一
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It uses material from the
"Mimas (moon)".
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