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Pandora (moon) - Wikipedia, the free encyclopedia

Pandora (moon)

From Wikipedia, the free encyclopedia

There is also an asteroid called 55 Pandora.
Pandora

Pandora, as imaged by Cassini
Discovery
Discovered by Collins, Voyager 1
Discovered in October, 1980
Orbital characteristics [1]
Epoch 31 December 2003 (JD 2453005.5)
Semimajor axis 141,720 ± 10 km
Eccentricity 0.0042
Revolution period 0.628504213 d
Inclination
to Saturn's equator
0.050 ± 0.004°
Is a satellite of Saturn
Physical characteristics
Diameter 81 km (103×80×64 km) [2]
Surface area ~21,000 km²
Volume ~270,000 km³
Mass 1.356 ± 0.022 ×1017 kg [1]
Mean density 0.49 ± 0.08 g/cm³
Surface gravity 0.0034 m/s2
Escape velocity ~0.019 km/s
Rotation period synchronous
Axial tilt zero
Albedo 0.6
Surface temp.
min mean max
~78 K
Atmospheric pressure none

Pandora (pan-dor'-a, IPA: [pænˈdɔrə], Greek Πανδώρα) is an inner satellite of Saturn. It was discovered in 1980 from photos taken by the Voyager 1 probe, and was designated 1980 S 26.[3] In 1985 it was officially named after Pandora from Greek mythology. It is also designated as Saturn XVII.[4]

Pandora is the outer shepherd satellite of the F Ring. It is more heavily cratered than nearby Prometheus, and has at least two large craters 30 km in diameter.[citation needed]

From its very low density and relatively high albedo, it seems likely that Pandora is a very porous icy body. There is a lot of uncertainty in these values, however, so this remains to be confirmed.[citation needed]

The orbit of Pandora appears to be chaotic, as a consequence of a mean motion resonance with Prometheus. 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. Pandora also has a 3:2 mean-motion resonance with Mimas [1].

[edit] References

  1. ^ a b c d J.N. Spitale et al (2006). "The orbits of Saturn's small satellites derived from combined historic and Cassini imaging observations". The Astronomical Journal 132: 692.
  2. ^ C.C. Porco et al. (2006). "Physical characteristics and possible accretionary origins for Saturn's small satellites". Bulletin of the American Astronomical Society 37: 768.
  3. ^ Smith, B. A. (October 31, 1980). IAU Circular No. 3532. Retrieved on 2006-08-07.
  4. ^ Planet and Satellite Names and Discoverers. Gazetteer of Planetary Nomenclature. USGS Astrogeology (July 21, 2006). Retrieved on 2006-08-07.

[edit] External links

Pandora as seen from the Cassini probe in 2005; the rings of Saturn are in the background.
Enlarge
Pandora as seen from the Cassini probe in 2005; the rings of Saturn are in the background.
... | S/2004 S 3 | Pandora | Epimetheus | ...


edit Saturn's natural satellites
Pan · Daphnis · Atlas · Prometheus · S/2004 S 6 · S/2004 S 4 · S/2004 S 3 · Pandora · Epimetheus and Janus
Mimas · Methone · Pallene · Enceladus · Telesto, Tethys, and Calypso · Helene, Dione, and Polydeuces · Rhea · Titan · Hyperion · Iapetus
Kiviuq · Ijiraq · Phoebe · Paaliaq · Skathi · Albiorix · S/2004 S 11 · Erriapo · S/2006 S 8 · Siarnaq · S/2004 S 13 · S/2006 S 4 · Tarvos
S/2004 S 19 · Mundilfari · S/2006 S 6 · S/2006 S 1 · S/2004 S 17 · Narvi · S/2004 S 15 · S/2004 S 10 · Suttungr · S/2004 S 12 · S/2004 S 18
S/2004 S 9 · S/2004 S 14 · S/2004 S 7 · Thrymr · S/2006 S 3 · S/2006 S 7 · S/2006 S 2 · S/2004 S 16 · S/2006 S 2 · Ymir · S/2006 S 5 · S/2004 S 8
See also: Pronunciation key | Rings of Saturn | Cassini-Huygens | Themis

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