Moons of Saturn, Part 2 Codexery

Tethys (moon)

Tethys is Saturn's fifth-largest moon, made almost entirely of water ice.

Tethys (moon)

Tethys is the fifth-largest moon orbiting Saturn, with a diameter of about 1,060 kilometers (660 miles). Giovanni Domenico Cassini spotted it in 1684, and it takes its name from the Titaness Tethys in Greek mythology. Its density is the lowest among all the major moons in the Solar System—just 0.98 grams per cubic centimeter—which suggests it is mostly water ice, with only a tiny amount of rock mixed in.

Quick Facts

Pronounced
ˈ · t · iː · θ · ɪ · s or ˈ · t · ɛ · θ · ɪ · s
Mpc Name
Saturn III
Adjectives
Tethyan ˈ · t · iː · θ · i · ə · n · ,_ · ' · t · ɛ · -
Named After
Τηθύς Tēthys
Discoverer
G. D. Cassini
Discovered
11 March 1684
Periapsis
294 · 590 km
Apoapsis
294 · 649 km
Eccentricity
0.0001Jacobson 2010 SAT339
Avg Speed
11.35 km/s
Inclination
1.12° (to Saturn's equator)
Satellite Of
Saturn

Facts from the source article.

Lore & Background

Tethys was discovered by Giovanni Domenico Cassini in 1684 together with Dione, using a large aerial telescope at the Paris Observatory. Cassini originally named the four new moons Sidera Lodoicea to honor King Louis XIV of France. The modern name Tethys was suggested by John Herschel in 1847, following the convention of naming Saturn's moons after Titans. Tethys is also designated Saturn III.

The moon's surface is very bright, the second-brightest of Saturn's moons after Enceladus, and neutral in color. It is heavily cratered and cut by large faults and trench-like graben. The largest impact crater, Odysseus, is about 400 km in diameter, while the largest graben, Ithaca Chasma, is about 100 km wide and more than 2,000 km long. A small part of the surface is covered by smooth plains that may be cryovolcanic in origin. Tethys has two co-orbital moons, Telesto and Calypso, which orbit near its Lagrange points.

Tethys formed from the Saturnian sub-nebula—a disk of gas and dust that surrounded Saturn soon after its formation. It has been observed by several space probes, including Pioneer 11 (1979), Voyager 1 (1980), Voyager 2 (1981), and most extensively by Cassini–Huygens (2004–2017).

Reader's Guide

Tethys is notable for its extremely low density, the lowest among all major moons in the Solar System, which confirms it is composed almost entirely of water ice with only a small fraction of rock. Its surface is one of the most reflective at visual wavelengths, with a visual albedo of 1.229, largely due to sandblasting by particles from Saturn's E-ring. The moon's surface features include the massive Odysseus impact basin and the extensive Ithaca Chasma graben, which may be related. Tethys also exhibits a distinctive color pattern: its trailing hemisphere is redder and darker, while the leading hemisphere has a dark bluish equatorial band that gives it a 'Pac-Man'-like appearance in mid-infrared temperature maps. The moon's interior is likely homogeneous, and a subsurface ocean is considered unlikely. Tethys's legacy includes its role in the numbering scheme of Saturn's moons and its extensive study by the Cassini mission, which provided the most detailed observations of this icy world.

Did You Know?

More in Moons of Saturn, Part 2 1-24

Spotted an error? Know more?

Reader corrections go straight into our review queue. Suggest an edit · How this site is sourced

Comments

Loading…
Open in the interactive codex →