Iapetus

Iapetus

Moon· orbits Saturn

Iapetus is Saturn's two-faced moon: one hemisphere is as dark as coal, the other as bright as snow, and a strange ridge of equatorial mountains circles much of the body.

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

Key facts

Mass
1.81 × 10²¹ kg
0.0246 Moon masses
Radius
734 km
42% of our Moon's radius
Surface gravity
0.224 m/s²
2% of Earth's
Day length
79.3 days
Orbit around Saturn
79.33 Earth days

Science

Physical

Mass
1.81 × 10²¹ kg · 0.0246 Moon masses
Radius
734 km · 42% of our Moon's radius
Density
1,089 kg/m³ · 1.1× water
Surface gravity
0.224 m/s² · 2% of Earth's
Escape velocity
573 m/s · 5% of Earth's

Orbit around Saturn

Distance from Saturn
3,076,018 km
Orbital period
79.3 days
Eccentricity
0.028
Inclination
7.60 °

Rotation

Rotation period
79.3 days
Tidal locking
Tidally locked to its parent

Temperature

Mean
115 K (-158 °C)

Composition

Bulk composition
Mostly water ice with rock; one hemisphere is coated in a thin, very dark, organic-rich dust.

Radiation & temperature

Insolation
0.0112 S⊕ · 1% of the sunlight Earth receives
Bond albedo
0.20 · reflects 20% of incoming sunlight
Equilibrium temperature
86 K (-188 °C)
Measured mean temperature
115 K (-158 °C)
Greenhouse warming
+29 K

Discovery & history

Discovered
October 25, 1671
By
Giovanni Domenico Cassini
Method
Visual discovery (telescopic)
Name
Iapetus, a Titan of Greek myth, father of Prometheus and Atlas.

Iapetus, found by Cassini in 1671, is the Solar System's great two-faced world: one hemisphere is as dark as coal, the other as bright as snow. Cassini correctly reasoned it must keep one face toward Saturn, and a strange equatorial ridge gives it the outline of a walnut.

Images

Images from open archives · credit shown per image