Polydeuces

This magnified view shows tiny Polydeuces, a moon that was discovered by the Cassini spacecraft and is a mere 3 kilometers (2 miles) across.
NASA/JPL/Space Science Institute

Discovery

Polydeuces was discovered by the Cassini mission team on Oct. 21, 2004, and upon further review of Cassini images, scientists found it in images from April 9 of the same year.

Overview

Polydeuces is a small moon with a mean radius of just 0.8 miles (1.3 kilometers) orbiting Saturn at a distance of about 234,000 miles (377,000 kilometers), taking 2.7 Earth days to go around the planet.

Polydeuces is an example of a so-called "Trojan" moon it follows a larger moon in orbit around the planet (in the case of Polydeuces, the larger moon is Dione). Polydeuces is a trailing co-orbital of Dione, while the moon Helene is the leading co-orbital.

Trojan moons are found near stable "Lagrangian points" places where the gravitational pull of the planet and the larger moon become balanced. The Trojans are situated 60 degrees ahead or behind the larger moon in its orbit.

It is believed that Polydeuces can get as close as 39 degrees to Dione and then drift as far as 92 degrees from it, taking over two years to complete its journey around the Lagrange point. If verified, the extent of this wandering is the largest detected so far for any Trojan moon.

How Polydeuces Got Its Name

Originally designated S/2004 S5, Polydeuces (another name for Pollux) is named for the son of Leda and Zeus.

John Herschel suggested that the moons of Saturn be associated with mythical brothers and sisters of Kronus. (Kronus is the equivalent of the Roman god Saturn in Greek mythology.) The International Astronomical Union now controls the official naming of astronomical bodies

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