Prometheus (moon)

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Prometheus
Image:Prometheus moon.jpg
Prometheus, as imaged by Voyager 2 on August 25, 1981
Discovery
Discovered by Collins, Voyager 1
Discovery date October, 1980
Epoch 31 December 2003 (JD 2453005.5
Semi-major axis 139,380 ± 10 km
Eccentricity 0.0022
Orbital period 0.612990038 d
Inclination 0.008 ± 0.004° to Saturn's equator
Satellite of Saturn
Physical characteristics
Dimensions 119×87×61 km [2]
Mean radius 43 ± 2 km [2]
Surface area ~23,000 km2
Volume ~340,000 km3
Mass 1.566 ± 0.019 ×1017 kg [1]
Mean density 0.47 ± 0.07 g/cm3
Equatorial surface gravity ~0.003 m/s2
Escape velocity ~0.019 km/s
Rotation period synchronous
Axial tilt zero
Albedo 0.6
Temperature ~74 K

Prometheus (pronounced /proʊˈmiːθiəs/ proe-MEE-thee-əs, also /-θiuːs/ -thee-oos, or as Greek Προμηθέας) is an inner satellite of Saturn. It was discovered in 1980 (some time before October 25) from photos taken by the Voyager 1 probe, and was provisionally designated S/1980 S 27.[3]

In late 1985 it was officially named after Prometheus, a Titan in Greek mythology.[4] It is also designated Saturn XVI.[5]

This small moon is extremely elongated, measuring about 119 by 87 by 61 km. It has several ridges and valleys and a number of impact craters of about 20 km diameter are visible, but it is less cratered than nearby Pandora, Epimetheus and Janus. From its very low density and relatively high albedo, it seems likely that Prometheus is a very porous icy body. There is a lot of uncertainty in these values, however, and so this remains to be confirmed.[citation needed]

Prometheus acts as a shepherd satellite for the inner edge of Saturn's F Ring. Recent images from the Cassini probe show that the Promethean gravitational field creates kinks and knots in the F Ring as the moon 'steals' material from it. The orbit of Prometheus appears to be chaotic, as a consequence of a mean motion resonance with Pandora. The most appreciable changes in their orbits occur approximately every 6.2 years [1], when the periapsis of Pandora lines up with the apoapsis of Prometheus and the moons approach to within about 1400 km. Prometheus is itsef a significant perturber of Atlas.

Closeup of Prometheus's gravitational effect on the F Ring.
Closeup of Prometheus's gravitational effect on the F Ring.

There is also an asteroid called 1809 Prometheus.

[edit] References

  1. ^ a b c Spitale, J. N.; et al. (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal 132: 692. doi:10.1086/505206. 
  2. ^ a b Porco, C. C.; et al. (2006). "Physical Characteristics and Possible Accretionary Origins for Saturn's Small Satellites". Bulletin of the American Astronomical Society 37: 768. 
  3. ^ IAUC 3532: Satellites of Saturn 1980 October 31 (discovery)
  4. ^ IAUC 4157: Satellites of Saturn and Pluto 1986 January 3 (naming the moon)
  5. ^ Planet and Satellite Names and Discoverers. Gazetteer of Planetary Nomenclature. USGS Astrogeology (July 21, 2006). Retrieved on 2006-08-07.

[edit] External links