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Prometheus (moon)

Moon of Saturn


Moon of Saturn

FieldValue
namePrometheus
imagePrometheus 12-26-09b.jpg
captionPrometheus image from Cassini (December 26, 2009)
pronounced
adjectivePromethean, -ian
named_afterΠρομηθεύς Promētheys
mpc_nameSaturn XVI
discovererStewart A. Collins
D. Carlson
Voyager 1
discovered24 October 1980
orbit_ref
epoch31 December 2003 (JD )
semimajor
eccentricity
period
inclinationto Saturn's equator
satellite_ofSaturn
groupInner shepherd moon of the F Ring
dimensionskm
(± km)
mean_diameter
volume
mass
density
surface_grav
escape_velocitykm/s at longest axis
to km/s at poles
rotationsynchronous
axial_tiltzero
albedo0.6
single_temperature≈ 74 K

D. Carlson Voyager 1 (± km) to km/s at poles

Prometheus is an inner satellite of Saturn. It was discovered on 24 October 1980 from images taken by the Voyager 1 probe, and was provisionally designated S/1980 S 27.

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

Prometheus is extremely elongated, measuring approximately 137 x 81 x 56 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 is likely that Prometheus is a very porous icy body. There is much uncertainty in these values, however, and so this remains to be confirmed.

Interactions with F Ring and other moons

Prometheus is a shepherd satellite for the inner edge of Saturn's narrow F Ring. Pandora orbits just outside the F Ring, and has traditionally been viewed as an outer shepherd of the ring; however, recent studies indicate that only Prometheus contributes to the confinement of the ring.{{cite web | access-date = 2015-04-17 }}

Images from the Cassini probe show that Prometheus's gravitational influence creates kinks and knots in the F Ring as it shepherds material from it. The orbit of Prometheus appears to be chaotic, due to a series of four 121:118 mean-motion resonances with Pandora. The most appreciable changes in their orbits occur approximately every 6.2 years, when the periapsis of Pandora lines up with the apoapsis of Prometheus, as they approach to within approximately 1400 km. Prometheus is itself a significant perturber of Atlas, with which it is in a 53:54 mean-longitude resonance.

Prometheus also participates in a 17:15 mean-motion resonance with Epimetheus, but only while it is on the outer orbit relative to Janus. No such configuration with Janus exists.

References

Notes

Citations

Sources

  • {{cite journal | access-date = 2011-12-29
  • {{cite journal | access-date = 2011-12-29
  • {{cite web | access-date = 2011-12-29
  • {{cite journal
  • {{cite journal |doi-access = free

References

  1. "Prometheus". [[Oxford University Press]].
  2. "Promethean". [[Oxford University Press]].
  3. (April 2014). "Saturn's F Ring core: Calm in the midst of chaos". Icarus.
  4. Cooper, N. J.. (2014-12-24). "SATURNʼS INNER SATELLITES: ORBITS, MASSES, AND THE CHAOTIC MOTION OF ATLAS FROM NEW CASSINI IMAGING OBSERVATIONS". The Astronomical Journal.
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