Haumea

Haumea

Dwarf Planet· orbits the Sun

Haumea is a dwarf planet in the Kuiper belt spun into an egg shape by a ≈3.9-hour rotation, one of the fastest of any large body. It has two moons and a thin ring. No spacecraft has visited.

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

Key facts

Mass
4.01 × 10²¹ kg
0.0546 Moon masses
Radius
780 km
12% of Earth's radius
Surface gravity
0.439 m/s²
4% of Earth's gravity
Day length
3.92 hours
Year
283 Earth years
103,318 Earth days
Distance from Sun
43.1 AU
Moons
2
Hiʻiaka & Namaka

Science

Physical

Mass
4.01 × 10²¹ kg · 0.0546 Moon masses
Mean radius
780 km · 12% of Earth's radius
Density
2,015 kg/m³ · 2× water
Computed from mass and radius
Surface gravity
0.439 m/s² · 4% of Earth's gravity
Computed from mass and radius
Escape velocity
828 m/s · 7% of Earth's escape velocity
Computed from mass and radius

Orbital

Distance from the Sun
49.7 AU
Computed from the position at the selected time
Semi-major axis
43.1 AU
Computed from the cached state vector
Eccentricity
0.1938
Computed from the cached state vector
Inclination
24.83 °
Computed from the cached state vector
Orbital period
282.87 years
Computed from the cached state vector
Perihelion
34.7 AU
Computed from the orbital elements
Aphelion
51.4 AU
Computed from the orbital elements
Mean orbital velocity
4.54 km/s
Computed from the orbital elements

Rotation

Rotation period
3.92 hours

Composition

Bulk composition
A surface of nearly pure crystalline water ice over a predominantly rocky body, inferred from spectroscopy and its high density; the rapid spin stretches it into an ellipsoid.
Surface imagery
No real surface imagery exists — this object has never been visited; color is approximate, inferred from spectroscopy.

Radiation & temperature

Insolation
0.000539 S⊕ · 1/1,857 of the sunlight Earth receives
Computed from the distance to the Sun (inverse-square; Earth's sunlight = 1), before any atmosphere.
Geometric albedo
0.66
V-band geometric albedo; Bond albedo not directly measured.
Equilibrium temperature
32 K (-241 °C)
Computed from albedo + distance from the Sun (airless black body); uses the geometric albedo as an estimate

Discovery & history

Discovered
December 28, 2004
By
Teams led by Mike Brown (Caltech) and José Luis Ortiz (Spain), amid a priority dispute
Method
Photographic plates
Name
The Hawaiian goddess of fertility and childbirth; its moons are named for her daughters.

Haumea was first detected on 28 December 2004 by a team led by Mike Brown at Caltech — who codenamed it 'Santa' for its Christmas-time discovery — and independently reported in 2005 by José Luis Ortiz's group in Spain from 2003 images (provisional designation 2003 EL61), sparking a lasting priority dispute. It is one of the fastest-spinning large bodies known, whirling around every ~3.9 hours into an elongated, egg-like shape, and in 2017 a stellar occultation revealed a ring — the first found around a trans-Neptunian object. It was named for Haumea, the Hawaiian goddess of fertility and childbirth; its two moons, Hiʻiaka and Namaka, are named for her daughters.

Images

Images from open archives · credit shown per image