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Calypso (moon)

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Trojan moon of Saturn
Not to be confused with53 Kalypso, an asteroid in theasteroid belt, orCallisto (moon), a moon ofJupiter.
Calypso
Calypso image fromCassini
(February 13, 2010)
Discovery
Discovered by
  • Dan Pascu
  • P. Kenneth Seidelmann
  • William A. Baum
  • Douglas G. Currie
Discovery dateMarch 13, 1980
Designations
Designation
Saturn XIV
Pronunciation/kəˈlɪps/[1]
Named after
ΚαλυψώKalypsō
Tethys C
S/1980 S 25
AdjectivesCalypsoan/kælɪpˈs.ən/,[2] Calypsonian/kælɪpˈsniən/[3]
Orbital characteristics
295000 km[4]
Eccentricity0.001[4]
1.887803 d[4]
Inclination1.56° (to Saturn's equator)
Satellite ofSaturn
GroupL5 Tethys trojan
Physical characteristics
Dimensions29.4 × 18.6 × 12.8 km
(± 0.6 × 1.8 × 0.6 km)[5]: 2 
19.0±0.8 km[5]: 2 
Volume3591 km3[a]
Mass≈2×1015 kg (assumed; unmeasured)[b]
≈0.5 g/cm3 (assumed; unmeasured)[5]: 3 
0.0009–0.0013 m/s2[5]: 3 
≈ 0.004 km/s at longest axis
to ≈ 0.006 km/s at poles
synchronous
zero
Albedo1.34±0.10 (geometric) [6]

Calypso is amoon ofSaturn. It was discovered in 1980, from ground-based observations, by Dan Pascu, P. Kenneth Seidelmann,William A. Baum, and Douglas G. Currie, and wasprovisionally designatedS/1980 S 25 (the 25th satellite of Saturn discovered in 1980).[7] Several other apparitions of it were recorded in the following months:S/1980 S 29,S/1980 S 30,[8]S/1980 S 32,[9] andS/1981 S 2.[10] In 1983 it was officially named afterCalypso ofGreek mythology.[c] It is also designatedSaturn XIV orTethys C.

Calypso is co-orbital with the moonTethys, and resides in Tethys's trailingLagrangian point (L5), 60 degrees behind Tethys. This relationship was first identified bySeidelmannet al. in 1981.[11] The moonTelesto resides in the other (leading) Lagrangian point of Tethys, 60 degrees in the other direction from Tethys. Calypso and Telesto have been termed "Tethys trojans", by analogy to thetrojan asteroids, and are half of the four presently knowntrojan moons.

Like many other small Saturnian moons and smallasteroids, Calypso is irregularly shaped, has overlapping large craters, and appears to also have loose surface material capable of smoothing the craters' appearance. Its surface is one of the most reflective (at visual wavelengths) in the Solar System, with a visualgeometric albedo of 1.34.[6] This very high albedo is the result of the sandblasting of particles fromSaturn's E-ring, a faint ring composed of small, water-ice particles generated byEnceladus's south polar geysers.[12]

Gallery

[edit]
  • Another February 13, 2010 image showing flow-like albedo features
    Another February 13, 2010 image showing flow-likealbedo features
  • Cassini image from September 23, 2005
    Cassini image from September 23, 2005
  • Calypso as seen by Voyager 2 (August 1981)
    Calypso as seen byVoyager 2 (August 1981)

See also

[edit]

Notes

[edit]
  1. ^Calculated from Calypso's volume-equivalent sphere radius of9.5±0.4 km given by Thomas et al. (2020)[5]: 2 
  2. ^Calculated by multiplying Calypso's volume with its assumed density of500 kg/m3.
  3. ^ Transactions of the International Astronomical Union, Vol. XVIIIA, 1982 (confirms Janus, names Epimetheus, Telesto, Calypso) (mentioned inIAUC 3872:Satellites of Jupiter and Saturn, September 30, 1983)

References

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Citations

[edit]
  1. ^"Calypso".Lexico UK English Dictionary.Oxford University Press. Archived fromthe original on March 22, 2020.
  2. ^The Emerson Society Quarterly, vol. 50, p. 56, 1968
  3. ^"Calypsonian".Lexico UK English Dictionary UK English Dictionary.Oxford University Press. Archived fromthe original on March 22, 2020.
  4. ^abc"Planetary Satellite Mean Orbital Parameters".Jet Propulsion Laboratory. Retrieved5 June 2023.
  5. ^abcdeThomas & Helfenstein 2020.
  6. ^abVerbiscer French et al. 2007.
  7. ^IAUC 3496.
  8. ^IAUC 3549.
  9. ^IAUC 3605.
  10. ^IAUC 3593.
  11. ^Seidelmann Harrington et al. 1981.
  12. ^Mason 2010.

Sources

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External links

[edit]
Wikimedia Commons has media related toCalypso.
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