Taygete (moon)
A small retrograde irregular moon of Jupiter.
Taygete, also called Jupiter XX and originally labeled S/2000 J 9, is a tiny, irregular moon of Jupiter that moves in a retrograde orbit. A University of Hawaiʻi team headed by Scott S. Sheppard spotted it in 2000. The moon received its permanent name in October 2002, after Taygete, a Pleiad—daughter of the Titan Atlas and mother of Lacedaemon by Zeus (Jupiter).
This satellite circles Jupiter at an average distance of 23.3 million kilometers, taking 732 days to complete one orbit. Its path is tilted 165° to the ecliptic, moves backward relative to Jupiter’s rotation, and has an eccentricity of 0.248. Taygete belongs to the Carme group, a cluster of irregular retrograde moons whose orbits cluster between 22.7 and 23.5 million kilometers from Jupiter, with inclinations around 165° and eccentricities from 0.24 to 0.28.
Estimates put Taygete’s diameter at about 5 kilometers, assuming a 4% albedo. Like most Carme group members (Kalyke is the exception), it appears light red, with color indices B−V=0.56 and V−R=0.52, similar to D-type asteroids.
Taygete likely did not form near Jupiter but was captured later. Along with other Carme group moons, which share similar orbits, it is probably a fragment of a larger, captured heliocentric asteroid that broke apart.
Quick Facts
- Pronounced
- t · eɪ · ˈ · ɪ · dʒ · ə · t · iː
- Adjective
- Taygetean ˌ · t · eɪ · ə · dʒ · ə · ˈ · t · iː · ə · n
- Named After
- Τᾱϋγέτη Tāÿgetē
- Mpc Name
- Jupiter XX
- Discoverer
- Scott S. Sheppard / David C. Jewitt / Yanga R. Fernandez / Eugene A. Magnier
- Discovery Site
- Mauna Kea Observatory
- Discovered
- 25 November 2000
- Satellite Of
- Jupiter
- Group
- Carme group
- Epoch
- 23 March 2018 (JD 2458200.5)
- Observation Arc
- 2000 · 2025 / 2025-12-21 (last obs)
- Semimajor
- 0.1507123 AU
Facts from the source article.
Lore & Background
Taygete was discovered in 2000 by a team of astronomers from the University of Hawaiʻi led by Scott S. Sheppard, and given the temporary designation S/2000 J 9. It was named in October 2002 after Taygete, one of the Pleiades, daughter of the Titan Atlas and mother of Lacedaemon by Zeus (Jupiter).
Taygete orbits Jupiter at an average distance of 23.3 million kilometers in 732 days, at an inclination of 165° to the ecliptic, in a retrograde direction and with an eccentricity of 0.248. It belongs to the Carme group, a tightly packed set of irregular retrograde moons orbiting Jupiter at a distance ranging between 22.7–23.5 million km, at an inclination of about 165°, and eccentricities between 0.24 and 0.28.
Its estimated diameter is 5 kilometers, assuming an albedo of 4%. Like most other members of the Carme group (the exception is Kalyke), it is light red in color (B−V=0.56, V−R=0.52), similar to D-type asteroids. Taygete probably did not form near Jupiter but was captured by Jupiter later, and like other Carme group members, is likely the remnant of a broken, captured heliocentric asteroid.
Reader's Guide
Taygete is significant as a member of the Carme group, a collection of irregular retrograde moons that share similar orbital parameters, suggesting a common origin. Its discovery in 2000 by the University of Hawaiʻi team led by Scott S. Sheppard added to the growing catalog of Jupiter's irregular satellites, which provide insights into the capture and fragmentation history of small bodies in the outer Solar System. The moon's light red color, similar to D-type asteroids, supports the hypothesis that it originated as a heliocentric asteroid that was later captured by Jupiter's gravity and subsequently broken apart, with Taygete being one of the surviving fragments. Its retrograde orbit and high inclination (165°) are characteristic of captured objects rather than moons that formed in situ. The naming after Taygete, a Pleiad from Greek mythology, continues the tradition of naming Jupiter's moons after mythological figures associated with the god Jupiter (Zeus). As a very small moon (only 5 km in diameter), Taygete represents the faint, distant population of Jovian satellites that are challenging to observe but crucial for understanding the dynamical evolution of the Jovian system.
Did You Know?
- Taygete orbits Jupiter in a retrograde direction at an inclination of 165° to the ecliptic.
- It belongs to the Carme group, a set of irregular retrograde moons with similar orbits.
More in Moons of Jupiter 1-24
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