Rhea

Rhea

Moon· orbits Saturn

Rhea is Saturn's second-largest moon — a heavily cratered ball of water ice and rock with a tenuous oxygen–carbon-dioxide exosphere.

Open in 3D viewSee Rhea in the live, interactive 3D map

Key facts

Mass
2.31 × 10²¹ kg
0.0314 Moon masses
Radius
764 km
44% of our Moon's radius
Surface gravity
0.264 m/s²
3% of Earth's
Day length
4.5 days
Orbit around Saturn
4.52 Earth days

Science

Physical

Mass
2.31 × 10²¹ kg · 0.0314 Moon masses
Radius
764 km · 44% of our Moon's radius
Density
1,237 kg/m³ · 1.2× water
Surface gravity
0.264 m/s² · 3% of Earth's
Escape velocity
635 m/s · 6% of Earth's

Orbit around Saturn

Distance from Saturn
4,669,124 km
Orbital period
4.5 days
Eccentricity
0.001
Inclination
0.30 °

Rotation

Rotation period
4.5 days
Tidal locking
Tidally locked to its parent

Temperature

Mean
76 K (-197 °C)

Composition

Bulk composition
Mostly water ice with about a quarter rock, probably only weakly differentiated.

Radiation & temperature

Insolation
0.0112 S⊕ · 1% of the sunlight Earth receives
Bond albedo
0.50 · reflects 50% of incoming sunlight
Equilibrium temperature
76 K (-197 °C)
Measured mean temperature
76 K (-197 °C)

Discovery & history

Discovered
December 23, 1672
By
Giovanni Domenico Cassini
Method
Visual discovery (telescopic)
Name
Rhea, the Titaness mother of the gods in Greek myth.

Cassini discovered Rhea, Saturn's second-largest moon, in 1672. A heavily cratered ball of ice and rock, it briefly seemed to possess a faint ring of its own — which would have been the only ring known around a moon, though later observations cast doubt on it.

Images

Images from open archives · credit shown per image