|Discovered by||William Herschel|
|Discovery date||17 September 1789|
|Pronunciation||//, or as Greek Μίμας|
|Orbital characteristics |
Average orbital speed
|14.28 km/s (calculated)|
|Inclination||1.574° (to Saturn's equator)|
|Dimensions||415.6 × 393.4 × 381.2 km|
|198.2±0.4 km |
|Mass||(3.7493±0.0031)×1019 kg |
|1.1479±0.007 g/cm3 |
|0.064 m/s2 (0.00648 g)|
|Temperature||≈ 64 K|
With a diameter of 396 kilometres (246 mi) it is the smallest astronomical body that is known to still be rounded in shape because of self-gravitation. However, Mimas is not actually in hydrostatic equilibrium for its current rotation.
Mimas was discovered by the astronomer William Herschel on 17 September 1789. He recorded his discovery as follows: "The great light of my forty-foot [12 m] telescope was so useful that on the 17th of September, 1789, I remarked the seventh satellite, then situated at its greatest western elongation."
Mimas is named after one of the Giants in Greek mythology, Mimas. The names of all seven then-known satellites of Saturn, including Mimas, were suggested by William Herschel's son John in his 1847 publication Results of Astronomical Observations made at the Cape of Good Hope. He named them after Titans specifically because Saturn (the Roman equivalent of Cronus in Greek mythology), was the leader of the Titans and ruler of the world for some time. Mimas was a son of the Greek goddess Gaia.
The surface area of Mimas is slightly less than the land area of Spain. The low density of Mimas, 1.15 g/cm3, indicates that it is composed mostly of water ice with only a small amount of rock. Due to the tidal forces acting on it, Mimas is noticeably prolate; its longest axis is about 10% longer than the shortest. The ellipsoidal shape of Mimas is especially noticeable in some recent images from the Cassini probe.
Mimas's most distinctive feature is a giant impact crater 130 km (81 mi) across, named Herschel after the discoverer of Mimas. Herschel's diameter is almost a third of Mimas's own diameter; its walls are approximately 5 km (3 mi) high, parts of its floor measure 10 km (6 mi) deep, and its central peak rises 6 km (4 mi) above the crater floor. If there were a crater of an equivalent scale on Earth (in relative size) it would be over 4,000 km (2,500 mi) in diameter, wider than Australia. 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 Mimas's core.
The Mimantean 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 larger than 40 km (25 mi) in diameter, but in the south polar region, there are generally no craters larger than 20 km (12 mi) in diameter.
A number of features in Saturn's rings are related to resonances with Mimas. Mimas is responsible for clearing the material from the Cassini Division, the gap between Saturn's two widest rings, the A Ring and B Ring. Particles in the Huygens Gap at the inner edge of the Cassini division are in a 2:1 orbital resonance with Mimas. They orbit twice for each orbit of Mimas. The repeated pulls by Mimas on the Cassini division particles, always in the same direction in space, force them into new orbits outside the gap. The boundary between the C and B rings is in a 3:1 resonance with Mimas. Recently, the G Ring was found to be in a 7:6 co-rotation eccentricity resonance[clarification needed] with Mimas; the ring's inner edge is about 15,000 km (9,300 mi) inside Mimas's orbit.
In 2014, researchers noted that the librational motion of Mimas has a component that cannot be explained by its orbit alone, and concluded that it was due to either an interior that is not in hydrostatic equilibrium (an elongated core) or an internal ocean. However, in 2017 it was concluded that an ocean would lead to surface tidal stresses comparable to or greater than those on tectonically active Europa. Thus, the lack of evidence for surface cracking or other tectonic activity on Mimas argues against the presence of such an ocean. Since formation of a core would likely have led to formation of an internal ocean in the past, probably leading to geologic activity, this explanation for the libration is also problematic. The presence of an asymmetric mass anomaly associated with the crater Herschel is another possible explanation for the libration.
Mimas was imaged several times by the Cassini orbiter, which entered into orbit around Saturn in 2004. A close flyby occurred on February 13, 2010, when Cassini passed by Mimas at 9,500 km (5,900 mi).
In popular cultureEdit
When seen from certain angles, Mimas resembles the Death Star, a fictional space station and superweapon known from the 1977 film Star Wars. Herschel resembles the concave disc of the Death Star's "superlaser". This is coincidental, as the film was made nearly three years before Mimas was resolved well enough to see the crater.
In 2010, NASA revealed a temperature map of Mimas, using images obtained by Cassini. The warmest regions, which are along one edge of Mimas, create a shape similar to the video game character Pac-Man, with Herschel Crater assuming the role of an "edible dot" or "power pellet" known from Pac-Man gameplay.
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- As reported by William Lassell, Monthly Notices of the Royal Astronomical Society, Vol. 8, No. 3, pp. 42–43 (January 14, 1848)
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- Young, Kelly (2005-02-11). "Saturn's moon is Death Star's twin". New Scientist. Retrieved 2008-08-21.
Saturn's diminutive moon, Mimas, poses as the Death Star – the planet-destroying space station from the movie Star Wars – in an image recently captured by NASA's Cassini spacecraft.
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|Wikimedia Commons has media related to Mimas (moon).|
- Cassini mission page – Mimas
- Mimas Profile at NASA's Solar System Exploration site
- The Planetary Society: Mimas
- Google Mimas 3D, interactive map of the moon
- Mimas page at The Nine Planets
- Views of the Solar System – Mimas
- Cassini images of Mimas
- Images of Mimas at JPL's Planetary Photojournal
- 3D shape model of Mimas (requires WebGL)
- Paul Schenk's Mimas blog entry and movie of Mimas's rotation on YouTube
- Mimas global and polar basemaps (June 2012) from Cassini images
- Mimas atlas (July 2010) from Cassini images
- Mimas nomenclature and Mimas map with feature names from the USGS planetary nomenclature page
- Figure "J" is Mimas transiting Saturn in 1979, imaged by Pioneer 11 from here