Cyllene (moon)

Moon of Jupiter that comes after Chaldene
Cyllene
Discovery
Discovered byScott S. Sheppard et al.
Discovery date2003
Designations
Designation
Jupiter XLVIII
Pronunciation/səˈln/[1]
Named after
Κυλλήνη Kyllēnē
S/2003 J 13
AdjectivesCyllenean /sɪləˈnən/[a]
Orbital characteristics[4]
Epoch 2026-01-01
Periapsis13.9 million km
Apoapsis33.83 million km
23.9 million km
Eccentricity0.416
−754.4 days
Inclination144.5°
Satellite ofJupiter
GroupPasiphae group
Physical characteristics
2 km[5]
Spectral type
B–V = 0.73 ± 0.07, V–R = 0.46 ± 0.07[6]
23.2

Cyllene /səˈln/, also known as Jupiter XLVIII, is an irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaiʻi led by Scott S. Sheppard in 2003, receiving the temporary designation S/2003 J 13.[7][8] It gets as far as 33.8 million km from Jupiter.[4]

Cyllene is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23.9 million km in 754 days (2.0 years), at an inclination of 145° to the ecliptic, in a retrograde direction and with an eccentricity of 0.416.[4]

It was named in March 2005 after Cyllene, a naiad (stream nymph) or oread (mountain nymph) associated with Mount Cyllene, Greece.[9] She was a daughter of Zeus (Jupiter).

It belongs to the Pasiphae group, irregular retrograde moons orbiting Jupiter at distances ranging between 22.8 and 24.1 million km, and with inclinations ranging between 144.5° and 158.3°.

Notes

  1. ^ The adjective 'Cyllenean' is also used for Mercury,[2] though rarely, as for that referent the form is normally 'Cyllenian' /səˈlniən/.[3]

References

  1. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  2. ^ Thomas Chase (1882) Six books of the Æneid of Virgil (1877), p. 252
  3. ^ "Cyllenian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  4. ^ a b c Horizons output. "Jovian Osculating Orbital Elements for Cyllene (548)". Retrieved 2025-12-19.
  5. ^ S.S. Sheppard (2019), Moons of Jupiter, Carnegie Science, on line
  6. ^ Graykowski, Ariel; Jewitt, David (2018-04-05). "Colors and Shapes of the Irregular Planetary Satellites". The Astronomical Journal. 155 (4): 184. arXiv:1803.01907. doi:10.3847/1538-3881/aab49b. ISSN 1538-3881.
  7. ^ IAUC 8116: Satellites of Jupiter and Saturn Archived 2006-05-05 at the Wayback Machine 2003 April (discovery)
  8. ^ MPEC 2003-G09: S/2003 J 13 2003 April (discovery and ephemeris)
  9. ^ IAUC 8502: Satellites of Jupiter 2005 March (naming the moon)
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