Cassini image from 20 May 2012
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Discovery
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| Discovered by | CICLOPS Team [1] |
| Discovery date | June 1, 2004 |
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Designations
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| Pronunciation | |
| Adjective | Methonean |
| Epoch June 20, 2004 (JD 2453177.5) | |
| Semi-major axis | 194,440 ± 20 km |
| Eccentricity | 0.0001 |
| Orbital period | 1.009573975 d [3] |
| Inclination | 0.007 ± 0.003° (to Saturn's equator) |
| Satellite of | Saturn |
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Physical characteristics
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| Mean radius | 1.6 ± 0.6 km [4] |
| Rotation period | synchronous |
| Axial tilt | zero |
Methone is a very small natural satellite of Saturn lying between the orbits of Mimas and Enceladus.
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Contents
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Methone was first seen by the Cassini Imaging Team[1][5][6] and given the temporary designation S/2004 S 1. Methone is also named Saturn XXXII (32). The Cassini–Huygens spacecraft has made two visits to Methone and its closest approach was made on May 20, 2012 with a minimum distance of 1,900 km from it.
The name Methone was approved by the IAU Working Group on Planetary System Nomenclature on January 21, 2005.[7] It was ratified at the IAU General Assembly in 2006. Methone was one of the Alkyonides, the seven beautiful daughters of the Giant Alkyoneus.[a]
In May 2012, the Cassini spacecraft obtained its first close-up photographs of Methone, revealing an egg-shaped moonlet with a remarkably smooth surface, with no visible craters.[8]
Methone's orbit is visibly affected by a perturbing mean longitude resonance with the much larger Mimas. This causes its osculating orbital elements to vary with an amplitude of about 20 km in semi-major axis, and 5° in longitude on a timescale of about 450 days. Eccentricity also varies on different timescales between 0.0011 and 0.0037, and inclination between about 0.003° and 0.020°.[2]
Discovery image of Methone on June 1, 2004[9]
Explanatory
Citations
Sources
| Wikimedia Commons has media related to: Methone |
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