Polydeuces (moon)
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Discovery | |||||||
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Discovered by | Cassini Imaging Science Team | ||||||
Discovered on | 24 October 2004 | ||||||
Orbital characteristics | |||||||
mean Semimajor axis | 377,396 km[1] | ||||||
Eccentricity | 0.0192[2] | ||||||
Orbital period | 2.736915 d[1] | ||||||
Inclination | 0.1774 ± 0.0015°[2] | ||||||
Is a satellite of | Saturn | ||||||
Physical characteristics | |||||||
Mean diameter | 3.5 km[3] | ||||||
Mass | 1 − 5 ×1013 kg [4] | ||||||
Mean density | unknown | ||||||
Surface gravity | unknown | ||||||
Rotation period | assumed synchronous | ||||||
Axial tilt | unknown | ||||||
Albedo | unknown | ||||||
Surface temperature |
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Atmosphere | none |
Polydeuces (pronounced /ˌpɒlɨˈdjuːsiːz/ POL-i-DEW-seez, or as Greek Πολυδεύκης) is a very small natural satellite of Saturn that is co-orbital with Dione and librates around the trailing Lagrangian point (L5). Its diameter is estimated to be about 3.5 km.[3]
Polydeuces was discovered by the Cassini Imaging Team on October 24, 2004[5] in images taken on October 21, 2004,[6],[3] and given the temporary designation S/2004 S 5. Subsequent searches of earlier Cassini imaging showed it in images as far back as April 9, 2004[5]. Polydeuces is also designated as Saturn XXXIV.
Of the known Lagrangian co-orbitals in the Saturn system, Polydeuces wanders the furtherest from its Lagrangian point. The libration takes it away from the L5 by up to 31.4° in the direction away from Dione, and 26.1° towards it with a period of 790.931 days (for comparison L5 trails Dione by 60°).[2] Polydeuces' libration is large enough that it takes on some qualities of a tadpole orbit, as evidenced by the clear asymmetry between excursions towards and away from Dione. In the course of one such cycle, Polydeuces' orbital radius also varies by about ± 7660 km with respect to Dione's.[5]
The name Polydeuces was approved by the IAU Working Group on Planetary System Nomenclature on January 21, 2005.[7] In Greek mythology, Polydeuces is another name for Pollux, twin brother of Castor, son of Zeus and Leda.
[edit] References
- ^ a b The mean semi-major axis and period must be identical to Dione's.
- ^ a b c Spitale, J. N.; Jacobson, R. A.; Porco, C. C.; and Owen, W. M., Jr. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations" ([dead link]). The Astronomical Journal 132: 692. doi: .
- ^ a b c Porco, C. C.; et al.; Cassini Imaging Science: Initial Results on Saturn's Rings and Small Satellites, Science, Vol. 307, No. 5713 (February 25, 2005), pp. 1226-1236
- ^ based on density 0.5 − 2 g/cm³
- ^ a b c Murray, C. D.; et al. (2005). "S/2004 S 5: A new co-orbital companion for Dione". Icarus 179: 222. doi: .
- ^ C.C. Porco, et al., IAUC 8432: Satellites and Rings of Saturn 2004 November 8 (discovery)
- ^ IAUC 8471: Satellites of Saturn 2005 January 21 (naming the moon)
[edit] External links
- Polydeuces Profile by NASA's Solar System Exploration
- IAU Working Group on Planetary System Nomenclature
- Cassini news release on ring and moon discoveries, via Spaceflight Now (February 24, 2005)
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