Mimas

396 kmdiameter

Updated

396km
Visual creditCassini 2010 / NASA / JPL-Caltech / Space Science Institute / Public domainSource: Wikimedia Commons

Details

Mimas is a small, heavily cratered moon of Saturn whose icy shell is dominated by the 130-kilometer Herschel crater. A 2024 analysis of its orbital motion found evidence for a young global ocean 20–30 kilometers beneath that old-looking surface.

Herschel crater spans about one third of Mimas’s diameter. The impact may have approached the energy needed to disrupt the moon, but the cratered exterior otherwise shows little of the fractures or resurfacing associated with better-known ocean moons.

A 2024 study used Cassini measurements of Mimas’s orbital precession to infer a global ocean beneath an ice shell 20–30 kilometers thick. The authors’ thermal and orbital models indicate that the ocean formed recently on geological timescales. It is an inference from the moon’s motion rather than a direct detection of liquid water.

Key facts

Category
Moons
Object class
Icy moon
Mass
~38 quadrillion metric tons
Host
Saturn
Scale fact
396 kmdiameter
Estimated age
~4.5 billion years
Composition
Mostly water ice
Temperature
~75 K surface
Embed

Size neighbors

Objects near Mimas on the scale

On the logarithmic size axis, Mimas falls between Hyperion and 10 Hygiea. The band uses nearby Icy moon records.

Shared physical scale
895km
Mimas396 km
Miranda472 km
Tethys1,066 km
Dione1,124 km
Ariel1,160 km
Umbriel1,170 km

Sources

References for Mimas

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.

Continue with nearby objects or open the full scale.

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