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Sedna

90377 Sedna, 2003 VB12

Potential dwarf planet of the Solar System

Proper NameSedna
Minor Planet Designation90377 Sedna
Provisional Designation2003 VB12
Orbital Period12,678.58 years
Distance from the SunSemi-Major Axis: 81,339,284,000 km (543.72 AU)
Perihelion: 11,397,060,000 km (76.18 AU)
Aphelion: 151,281,507,000 km (1,011.25 AU)
Eccentricity0.8599
Rotation Period10 hours, 16 minutes
Mean Diameter906 km
MoonsNone known
Parent starThe Sun, yellow dwarf
Other planets in this systemMercury, terrestrial planet
Venus, terrestrial planet
Earth, terrestrial planet
Mars, terrestrial planet
Jupiter, gas giant
Saturn, gas giant
Uranus, ice giant
Neptune, ice giant
Numerous dwarf planets, asteroids and other bodies

A tiny and distant planetoid that pursues an extreme orbit out into the depths of the Solar System, far from the Sun, and potentially belonging to the group of bodies known as dwarf planets. Discovered in 2003, Sedna is still something of mystery. It is currently classified as part of the group of bodies designated as the 'scattered disc', objects thrown out into elongated orbits by the planet Neptune, though in Sedna's case this classification is controversial.

Sedna in the Solar System

Sedna's orbit is exceptionally eccentric in nature: at its most distant, Sedna can reach a distance of some 936 AU from the Sun, or about 1% of a light year. At present, however, it is approaching its perihelion point, its closest approach to the heart of the Solar System. This will bring it to within some 76 AU of the Sun, a point still immensely distant (far beyond the orbit of Pluto) which it will probably reach in the year 2076. In the skies of Earth, Sedna is presently passing through Taurus, in the direction of Orion and Gemini.

The origins of Sedna's extreme orbit are still mysterious, and a range of possibilities remain open. Sedna appears to have formed on the outer fringes of the Solar System following a far less eccentric orbit, an orbit that was then perturbed by another body. The identity of that body is unclear - if indeed it existed at all. It may have been another star during the early development of the Solar System, or perhaps even a more massive planet yet to be discovered in a distant orbit of the Sun.

Physical Characteristics

Sedna is a small body by comparison with similar objects, with an estimated diameter of a little over nine hundred kilometres. By comparison, Pluto has a diameter more than twice this value, and Earth's Moon is nearly four times Sedna's diameter. Early observations of Sedna soon after its discovery hinted that it might have an even tinier body orbiting it as a moon, but further investigation suggests that this is not in fact the case.

In common with similar planetoids, Sedna's surface is covered with frozen methane, water and nitrogen, with the methane in particular creating a distinct reddish hue. These frigid conditions explain Sedna's name, which comes from an Inuit sea-goddess believed to dwell in the frozen depths of the northern oceans.

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