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EntityQ17420· pop 53· linked from 104 articles

Also known as Jupiter XLVIII, S/2003 J 13

moon of Jupiter

AI overview

Cyllene is one of Jupiter's many moons that orbits far from the planet in a distant and irregular path. It is of scientific interest because studying its orbit and characteristics helps astronomers understand Jupiter's system of moons and how celestial bodies form and move in space.

AI-generated from the Wikipedia summary — may contain errors.

Key facts

Discovered by
Scott S. Sheppard et al.
Designation
Jupiter XLVIII
Pronunciation
/ s ə ˈ l iː n iː /
Named after
Κυλλήνη Kyllēnē
Alternative names
S/2003 J 13
Adjectives
Cyllenean / s ɪ l ə ˈ n iː ə n /
Observation arc
16 years, 2018-04-18 (last obs)
Periapsis
13.9 million km
Apoapsis
33.83 million km
Semi major axis
23.9 million km
Orbital period sidereal
−754.4 days
Inclination
144.5°
Satellite of
Jupiter
Group
Pasiphae group
Mean diameter
2 km
Spectral type
B–V = 0.73 ± 0.07, V–R = 0.46 ± 0.07
Absolute magnitude h
16.34 (28 obs)

via Wikipedia infobox

Wikidata facts

Diameter
2
Mass
15
Orbital period
7751.94
Show 9 more facts
time of discovery or invention
2003-02-09
provisional designation
S/2003 J 13
albedo
0.04
orbital eccentricity
0.4116
semi-major axis of an orbit
23396289
apparent magnitude
23.2
surface gravity
0.00081
name
Júpiter XLVIII
orbital inclination
140
Sources (4)

via Wikidata · CC0

~1 min read

Article

Cyllene /səˈliːniː/, 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. It gets as far as 33.8 million kilometres (21,000,000 mi) from Jupiter.

Cyllene is about 2 kilometres (1.2 mi) in diameter, and orbits Jupiter at an average distance of 23.9 million kilometres (14,900,000 mi) in 754 days (2.06 yr), at an inclination of 145° to the ecliptic, in a retrograde direction and with an eccentricity of 0.416. The orbital elements are continuously changing due to solar and planetary perturbations. In October 2014, the moon reached 0.253 AU (37.8 million km; 23.5 million mi) from Jupiter, and in October 2015 approached within 0.0616 AU (9.22 million km; 5.73 million mi) of Jupiter.

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