[go: up one dir, main page]
Jump to content

Prometheus (moon)

Listen to this article
From Wikipedia, the free encyclopedia
(Redirected from Prometheus (satellite))
For the asteroid, see 1809 Prometheus.
Prometheus
Prometheus image from Cassini (December 26, 2009)
Discovery
Discovered byStewart A. Collins
D. Carlson
Voyager 1
Discovery dateOctober, 1980
Designations
Designation
Saturn XVI
Pronunciation/prəˈmiːθiːəs/[1]
Named after
Προμηθεύς Promētheys
AdjectivesPromethean, -ian /prəˈmiːθiːən/[2]
Orbital characteristics [3]
Epoch 31 December 2003 (JD 2453005.5)
139380±10 km
Eccentricity0.0022
0.612990038 d
Inclination0.008°±0.004° to Saturn's equator
Satellite ofSaturn
GroupInner shepherd moon of the F Ring
Physical characteristics
Dimensions137.0 × 81.0 × 56.2 km
(± 1.0 × 2.8 × 0.8 km)[4]: 2 
85.6±1.4 km[4]: 2 
Volume327740±1710 km3[5]: 4 
Mass(1.59720±0.00072)×1017 kg[a]
Mean density
0.4873±0.0026 g/cm3[5]: 4 
0.0007–0.0056 m/s2[4]: 3 
0.018 km/s at longest axis
to 0.028 km/s at poles
synchronous
zero
Albedo0.6
Temperature≈ 74 K

Prometheus /prəˈmiːθiːəs/ 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.[6]

In late 1985 it was officially named after Prometheus, a Titan in Greek mythology.[7] It is also designated Saturn XVI.[8]

Prometheus is extremely elongated, measuring approximately 137 km × 81 km × 56 km (85 mi × 50 mi × 35 mi). It has several ridges and valleys and a number of impact craters of about 20 km (12 mi) 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

[edit]

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.[9][10]

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.[11] The most appreciable changes in their orbits occur approximately every 6.2 years,[3] 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.[3]

Selected images

[edit]
  • Prometheus pulling material from the F Ring
    Prometheus pulling material from the F Ring
  • Prometheus tugging kinks into the F Ring
    Prometheus tugging kinks into the F Ring
  • Voyager 2 (August 25, 1981) image
    Voyager 2 (August 25, 1981) image
  • Cassini image (with moon's Saturn-facing end at lower right) reveals a surface covered with a blanket of fine material.
    Cassini image (with moon's Saturn-facing end at lower right) reveals a surface covered with a blanket of fine material.
  • Image from Jan. 27, 2010. Saturnshine illuminates the moon's night side.
    Image from Jan. 27, 2010. Saturnshine illuminates the moon's night side.
  • Brightened version of same image
    Brightened version of same image
  • Prometheus flyby (December 6, 2015)
    Prometheus flyby
    (December 6, 2015)

Animations

[edit]
  • Prometheus collides with the F ring, pulls a streamer, and leaves behind a dark channel. 12 seconds 107 kbit/s
  • Movie of Prometheus and the F Ring looped once. 5 seconds 48 kbit/s

Notes

[edit]
  1. ^ Calculated from the standard gravitational parameter GM = (1.06602±0.00048)×10−2 km3·s–2 given by Lainey et al. (2023), divided by the gravitational constant G = 6.6743×10−2 km3·kg–1·s–2.[5]

References

[edit]

Citations

[edit]
  1. ^ "Prometheus". Lexico UK English Dictionary. Oxford University Press. Archived from the original on March 20, 2020.
  2. ^ "Promethean". Lexico UK English Dictionary UK English Dictionary. Oxford University Press. Archived from the original on March 20, 2020.
  3. ^ a b c Spitale Jacobson et al. 2006.
  4. ^ a b c Thomas & Helfenstein 2020.
  5. ^ a b c Lainey et al. 2023.
  6. ^ IAUC 3532.
  7. ^ IAUC 4157.
  8. ^ USGS: Planet and Satellite Names and Discoverers.
  9. ^ Lakdawalla, E. (2014-07-05). "On the masses and motions of mini-moons: Pandora's not a "shepherd," but Prometheus still is". Planetary Society. Retrieved 2015-04-17.
  10. ^ Cuzzi, J. N.; Whizin, A. D.; Hogan, R. C.; Dobrovolskis, A. R.; Dones, L.; Showalter, M. R.; Colwell, J. E.; Scargle, J. D. (April 2014). "Saturn's F Ring core: Calm in the midst of chaos". Icarus. 232: 157–175. Bibcode:2014Icar..232..157C. doi:10.1016/j.icarus.2013.12.027. ISSN 0019-1035.
  11. ^ Renner et al. 2005.

Sources

[edit]
[edit]
Listen to this article (2 minutes)
Spoken Wikipedia icon
This audio file was created from a revision of this article dated 10 January 2010 (2010-01-10), and does not reflect subsequent edits.
(Audio help · More spoken articles)

Media related to Prometheus (moon) at Wikimedia Commons

Retrieved from "https://en.wikipedia.org/w/index.php?title=Prometheus_(moon)&oldid=1241191829"