Triton

Triton

Moon· orbits Neptune

Triton is Neptune's largest moon and the only large moon orbiting backwards (retrograde) — a captured Kuiper-belt world with a young nitrogen-ice surface and active nitrogen geysers, seen by Voyager 2 in 1989.

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Key facts

Mass
2.14 × 10²² kg
0.291 Moon masses
Radius
1,353 km
78% of our Moon's radius
Surface gravity
0.78 m/s²
8% of Earth's
Day length
5.9 days
Orbit around Neptune
5.88 Earth days

Science

Physical

Mass
2.14 × 10²² kg · 0.291 Moon masses
Radius
1,353 km · 78% of our Moon's radius
Density
2,064 kg/m³ · 2.1× water
Surface gravity
0.78 m/s² · 8% of Earth's
Escape velocity
1.45 km/s · 13% of Earth's

Orbit around Neptune

Distance from Neptune
2,704,826 km
Orbital period
5.9 days
Eccentricity
0
Inclination
157.30 °

Rotation

Rotation period
5.9 days
Tidal locking
Tidally locked to its parent

Atmosphere

Composition
Tenuous N₂ with traces of CH₄ and CO
Surface pressure
1.4 Pa

Temperature

Surface
38 K (-235 °C)

Composition

Bulk composition
A nitrogen-ice surface (with CO₂, CO and methane ices) over a water-ice crust and a large rocky core; one of the coldest measured surfaces in the Solar System.

Radiation & temperature

Insolation
0.00112 S⊕ · 1/893 of the sunlight Earth receives
Bond albedo
0.76 · reflects 76% of incoming sunlight
Equilibrium temperature
36 K (-238 °C)
Surface temperature
38 K (-235 °C)

Discovery & history

Discovered
October 10, 1846
By
William Lassell
Method
Visual discovery (telescopic)
Name
Triton, a sea-god son of Poseidon (Neptune) in Greek myth.

William Lassell discovered Triton just 17 days after Neptune itself was found in 1846. It orbits backwards — the only large moon to do so — marking it as a captured Kuiper Belt object. Voyager 2 found it geologically active, with nitrogen geysers erupting from one of the coldest surfaces ever measured.

Images

Images from open archives · credit shown per image