Methone (moon)
Methone as seen by Cassini taken in September, 2010
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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.
It 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.
Methone 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]
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]
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Discovery image of Methone on June 1, 2004[8]
[edit] References
Explanatory
- ^ Early press releases of the discovery mentioned the first person to see the moon in Cassini images. This bit of trivia was blown out of proportion in the following months, with this individual being credited as the "discoverer" by some sources. Because the discovery was a large team effort, involving tens of people and hundreds of hours of distributed work, a conscious decision was made by the IAU to officially and correctly assign any credit to "the Cassini Imaging team" and to avoid unfairly singling out any one individual as the discoverer.
Citations
Sources
- "Cassini Imaging Science Team". Cassini Imaging Central Laboratory for OPerationS. http://ciclops.org/team/iss_team.php. Retrieved 2012-01-01.
- Green, Daniel W. E. (August 16, 2004). "S/2004 S 1 and S/2004 S 2" (discovery). IAU Circular 8389. http://www.cbat.eps.harvard.edu/iauc/08300/08389.html. Retrieved 2012-01-01.
- Green, Daniel W. E. (January 21, 2005). "S/2004 S 1 and S/2004 S 2" (naming the moon). IAU Circular 8471. http://www.cbat.eps.harvard.edu/iauc/08400/08471.html. Retrieved 2012-01-01.
- "PIA06105: Cassini Uncovers New Moon". Photojournal. JPL/NASA. August 16, 2004. http://photojournal.jpl.nasa.gov/catalog/PIA06105. Retrieved 2012-01-01.
- Porco, C. C.; Baker, E.; Barbara, J.; Beurle, K.; Brahic, A.; Burns, J. A.; Charnoz, S.; Cooper, N. et al (February 25, 2005). "Cassini Imaging Science: Initial Results on Saturn's Rings and Small Satellites". Science 307 (5713): 1226–1236. doi:10.1126/science.1108056. PMID 15731439.
- Spitale, J. N.; Jacobson, R. A.; Porco, C. C.; Owen, W. M., Jr. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal 132 (2): 692–710. Bibcode 2006AJ....132..692S. doi:10.1086/505206.
- Thomas, P. C. (July 2010). "Sizes, shapes, and derived properties of the saturnian satellites after the Cassini nominal mission". Icarus 208 (1): 395–401. Bibcode 2010Icar..208..395T. doi:10.1016/j.icarus.2010.01.025. http://www.ciclops.org/media/sp/2011/6794_16344_0.pdf.
[edit] External links
| Wikimedia Commons has media related to: Methone |
- Methone Profile by NASA's Solar System Exploration
- IAU Working Group for Planetary System Nomenclature
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