Epimetheus

130 kmmaximum extent

Explore Epimetheus to scale

Updated

130km
Visual creditCassini 2007 / NASA / JPL / Space Science Institute / Public domainSource: Wikimedia Commons

Details

Epimetheus is a porous, cratered inner moon of Saturn that shares two neighboring orbits with Janus. About every four years, the pair exchange momentum and swap which moon follows the inner path.

Epimetheus and Janus follow orbits separated by only about 50 kilometers. Roughly every four years the inner, faster moon catches the outer one; their gravitational interaction transfers momentum, and each moves onto the other path while they remain about 15,000 kilometers apart at closest approach. Voyager 1 confirmed in 1980 that the conflicting earlier observations belonged to two moons, not one.

Cassini images show Epimetheus as an irregular, cratered body with a flattened south-polar region. Its low density supports a porous, ice-rich structure, while dust knocked from Epimetheus and Janus may supply the faint ring along their shared orbit.

Key facts

Category
Moons
Object class
Co-orbital inner moon
Composition
Water ice (porous rubble pile)
Temperature
78 K surface
Scale fact
130 kmmaximum extent
Mass
~526 trillion metric tons
Host
Saturn

Size neighbors

Objects near Epimetheus on the scale

On the logarithmic size axis, Epimetheus falls between 21 Lutetia and Prometheus. The band uses nearby Co-orbital inner moon records.

Shared physical scale
155km
Epimetheus130 km
Janus203 km

Sources

References for Epimetheus

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

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