Rhea

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Details

Rhea is Saturn's second-largest moon, a cold icy body with an old, heavily cratered surface. Cassini also detected an extremely thin oxygen and carbon dioxide exosphere around it, making this quiet-looking moon chemically more interesting than it first appears.

Rhea matters because it is large enough to be one of Saturn's major moons, yet quiet enough to preserve an ancient surface. It is cold, airless in any ordinary sense, and heavily cratered, closer in mood to an old icy archive than to an active plume world like Enceladus.

That apparent stillness is the point. NASA describes Rhea as mostly ice with rock mixed through it, farther from Saturn than Dione and Tethys and less affected by tidal heating. Without enough internal warmth to erase old craters widely, its surface keeps a memory of impacts that more active moons can blur or rewrite.

Cassini added a subtle twist: Rhea has an extremely thin exosphere containing oxygen and carbon dioxide. That does not make it Earth-like, but it does make the surface chemistry more interesting. Rhea shows that a quiet icy moon can still participate in processes driven by radiation, ice, and planetary magnetospheres.

668km
Visual creditNASA / JPL / Space Science Institute / Public domainSource: Wikimedia Commons

Key facts

Category
Moons
Object class
Large icy moon
Composition
Water ice and rock
Temperature
~99 K sunlit surface
Scale fact
1,528 kmdiameter
Estimated age
~4.5 billion years
Host
Saturn

Scale context

Where Rhea sits on the full axis

By size on the journey, Rhea sits between Oberon and Titania. The band below compares Rhea with nearby Large icy moon objects so the size jump stays easy to read.

Shared physical scale
3,938km
Rhea1,528 km
Titania1,600 km
Titan5,150 km

Together, these objects make the size change around Rhea easy to compare at a glance.

Sources

References for Rhea

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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