Tarqeq (Saturn LII): a small prograde irregular moon of Saturn
Tarqeq (Saturn LII, S/2007 S 1) is a small, non-spherical prograde irregular satellite of Saturn discovered in 2007. It belongs to the Inuit group and orbits at about 17.9 million km with a ~895-day period.
Tarqeq, designated Saturn LII and provisionally S/2007 S 1, is one of Saturn's numerous small irregular moons. Announced in April 2007, it was identified from a set of ground-based observations spanning early 2006 to 2007. Tarqeq is diminutive (roughly 7 km across), follows a distant, inclined orbit and is classified with the prograde Inuit group of Saturnian satellites. Its name derives from an Inuit lunar deity.
Image gallery
1 ImageDiscovery and designation
The discovery of Tarqeq was reported on April 13, 2007 by a team led by Scott S. Sheppard and David C. Jewitt, with contributions from Jan Kleyna and Brian G. Marsden. The observations used to confirm its motion and orbit were collected between January 5, 2006 and March 22, 2007. After initial detection as a moving point of light, follow-up imaging established its orbital parameters and secured its provisional label S/2007 S 1 before the International Astronomical Union assigned the permanent satellite number Saturn LII and the name Tarqeq.
Orbit and classification
Tarqeq is an irregular satellite, meaning it orbits far from Saturn with a significant inclination and non-zero eccentricity compared with the regular, close-in moons. Key orbital characteristics are:
- Semi-major axis: approximately 17,910,000 km from Saturn
- Orbital period: about 894.86 days
- Inclination: roughly 49.90° to the ecliptic (about 49.77° to Saturn's equator)
- Eccentricity: about 0.1081 (eccentricity measures orbital elongation)
These properties place Tarqeq among the prograde irregular satellites; it travels in the same general direction as Saturn’s rotation but on a distant, tilted path. It is grouped with other similarly inclined, prograde moons known as the Inuit group.
Physical characteristics
Tarqeq is very small, with an estimated diameter near 7 km, and is not spherical. Like many small irregular satellites it is likely a fragmentary body rather than a world that has reached hydrostatic equilibrium. Observational data are limited: optical measurements indicate a faint object, and basic properties such as surface composition, albedo, and detailed shape remain poorly constrained. Given its membership in the Inuit group, Tarqeq may share compositional traits with those relatives, which are often assumed to be mixtures of rock and ice formed or modified by collisions.
Name and cultural origin
The name Tarqeq comes from Inuit mythology, where Tarqeq is associated with the moon. The choice follows the convention of naming Saturnian Inuit-group satellites after figures from Inuit culture and legend. The formal adoption of mythological names helps avoid confusion with provisional designations and emphasizes the international tradition of drawing on diverse cultures for astronomical names. For background on the cultural reference see Inuit traditions.
Context and scientific importance
Although Tarqeq is too small to host geological activity, such irregular satellites are scientifically valuable. They provide clues to the collisional and capture history of the Saturnian system and to the population of small bodies in the outer Solar System. Studies of orbital clustering, color and reflectivity, and dynamics can indicate whether groups like the Inuit formed by the breakup of a larger progenitor or were captured and later perturbed. Tarqeq and its peers therefore help astronomers reconstruct Saturn's past environment and the processes that populate giant-planet satellite systems.
Observation and challenges
Detecting and tracking tiny moons like Tarqeq requires large telescopes and repeated, carefully timed imaging to distinguish orbital motion from background stars. Their faintness and slow motion against the sky make follow-up essential to secure orbits. Published discovery notices and orbital updates are typically circulated through professional channels; the initial reports associated with Tarqeq credited the discoverers and their observing campaign. Additional observational work is needed to refine Tarqeq's physical measurements and to determine how closely it matches other members of the Inuit group in color and composition.
For original discovery information and subsequent orbit refinements consult announcements and databases maintained by professional groups and observatories; the primary discovery team included Scott S. Sheppard and David C. Jewitt, with context on the orbital plane provided by references to the ecliptic and discussions of orbital eccentricity. Further cultural naming context can be explored via sources on the Inuit moon lore.
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AlegsaOnline.com Tarqeq (Saturn LII): a small prograde irregular moon of Saturn Leandro Alegsa
URL: https://en.alegsaonline.com/art/96422