Mimas (moon)
Moon of Saturn / From Wikipedia, the free encyclopedia
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Mimas /ˈmaɪməs/, also designated Saturn I, is a moon of Saturn discovered in 1789 by William Herschel.[11] It is named after Mimas, a son of Gaia in Greek mythology.
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Discovery | |
---|---|
Discovered by | William Herschel |
Discovery date | 17 September 1789[1] |
Designations | |
Designation | Saturn I |
Pronunciation | /ˈmaɪməs/[2] or as Greco-Latin Mimas (approximated /ˈmiːməs/) |
Named after | Μίμας Mimās |
Adjectives | Mimantean,[3] Mimantian[4] (both /mɪˈmæntiən/) |
Orbital characteristics [5] | |
Periapsis | 181902 km |
Apoapsis | 189176 km |
185539 km | |
Eccentricity | 0.0196 |
0.942421959 d | |
Average orbital speed | 14.28 km/s (calculated) |
Inclination | 1.574° (to Saturn's equator) |
Satellite of | Saturn |
Physical characteristics | |
Dimensions | 415.6 × 393.4 × 381.2 km (0.0311 Earths)[6] |
Mean radius | 198.2±0.4 km [6] |
490000–500000 km2 | |
Volume | 32600000±200000 km3 |
Mass | (3.7493±0.0031)×1019 kg [7][8] (6.3×10−6 Earths) |
Mean density | 1.1479±0.007 g/cm3 [6] |
0.064 m/s2 (0.00648 g) | |
0.159 km/s | |
synchronous | |
zero | |
Albedo | 0.962±0.004 (geometric)[9] |
Temperature | ≈ 64 K |
12.9 [10] | |
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.[citation needed]