Discovery[1] | |
---|---|
Discovered by | Michael Brown Chad Trujillo David Rabinowitz |
Discovery date | 14 November 2003 |
Designations | |
(90377) Sedna | |
Pronunciation | /ˈsɛdnə/ |
Named after | Sedna (Inuit goddess of sea and marine animals) |
2003 VB12 | |
TNO[2] · detached sednoid[3] dwarf planet | |
Adjectives | Sednian[4] |
Symbol | (mostly astrological) |
Orbital characteristics[2] | |
Epoch 31 May 2020 (JD 2458900.5) | |
Uncertainty parameter 2 | |
Observation arc | 30 years |
Earliest precovery date | 25 September 1990 |
Aphelion | 937 AU (140 billion km)[5][a] |
Perihelion | 76.19 AU (11.4 billion km)[6][5][7] |
506 AU (76 billion km)[5] or 0.007 ly | |
Eccentricity | 0.8496[5] |
11390 yr (barycentric)[a] | |
11,408 Gregorian years | |
Average orbital speed | 1.04 km/s |
358.117° | |
0° 0m 0.289s / day | |
Inclination | 11.9307° |
144.248° | |
≈ 18 July 2076[6][7] | |
311.352° | |
Physical characteristics | |
Dimensions | 906+314 −258 km[8] > 1025±135 km (occultation chord)[9] |
10.273±0.002 h (~18 h less likely)[10] | |
0.410+0.393 −0.186[8] | |
Temperature | ≈ 12 K (see note) |
(red) B−V=1.24; V−R=0.78[11] | |
20.8 (opposition)[12] 20.5 (perihelic)[13] | |
1.83±0.05[14] 1.3[2] | |
Sedna (minor-planet designation: 90377 Sedna) is a dwarf planet in the outermost reaches of the Solar System, orbiting the Sun beyond the orbit of Neptune. Discovered in 2003, the planetoid's surface is one of the reddest known among Solar System bodies. Spectroscopy has revealed Sedna's surface to be mostly a mixture of the solid ices of water, methane, and nitrogen, along with widespread deposits of reddish-colored tholins, a chemical makeup similar to those of some other trans-Neptunian objects. Within the range of uncertainties, it is tied with the dwarf planet Ceres in the asteroid belt as the largest dwarf planet not known to have a moon. Its diameter is roughly 1,000 km (most likely in between those of Ceres and Saturn's moon Tethys). Owing to its lack of known moons, the Keplerian laws of planetary motion cannot be employed for determining its mass, and the precise figure remains as yet unknown.
Sedna's orbit is one of the widest known in the Solar System. Its aphelion, the farthest point from the Sun in its elliptical orbit, is located 937 astronomical units (AU) away.[5] This is some 31 times the distance of Neptune's aphelion, and 19 times that of Pluto, spending most of its highly elongated orbit well beyond the heliopause, the boundary beyond which the influence of particles from interstellar space dominates over that of the Sun. Sedna's orbit is also one of the most narrow and elliptical discovered, with an eccentricity of 0.8496. This means that its perihelion, or point of closest approach to the Sun, at 76 AU is around 12.3 times closer than its aphelion. At perihelion, Sedna is only 55% further than Pluto's aphelion. As of January 2024[update], Sedna is near perihelion, 83.55 AU (12.50 billion km) from the Sun,[15] and 2.8 times farther away than Neptune. The dwarf planets Eris and Gonggong are presently farther away from the Sun than Sedna. It is suggested that an exploratory fly-by mission to Sedna near its perihelion through a Jupiter gravity assist could be completed in 24.5 years.[16]
Due to its exceptionally elongated orbit, the dwarf planet takes approximately 11,400 years, over 11 millennia, to return to the same point in its orbit around the Sun. The International Astronomical Union (IAU) initially considered Sedna to be a member of the scattered disc, a group of objects sent into high-eccentricity orbits by the gravitational influence of Neptune. However, several astronomers who worked in the associated field contested this classification as even its perihelion is far too distant for it to have been scattered by any of the currently known planets. This has led some astronomers to informally refer to it as the first known member of the inner Oort cloud. The dwarf planet is also the prototype of a new orbit class of objects named after itself, the sednoids, which include 2012 VP113 and Leleākūhonua, all celestial bodies with large perihelion distances and extremely elongated orbits.
The astronomer Michael E. Brown, co-discoverer of Sedna, believes that studying Sedna's unusual orbit could yield valuable information on the origin and early evolution of the Solar System.[17][18] It might have been perturbed into its orbit by a star within the Sun's birth cluster, or captured from a nearby wandering star, or to have been sent into its present orbit through a close gravitational encounter with the hypothetical 9th planet, sometime during the solar system's formation. The statistically unusual clustering to one side of the solar system of the aphelions of Sedna and other similar objects is speculated to be the evidence for the existence of a planet beyond the orbit of Neptune, which would by itself orbit on the opposing side of the Sun.[19][20][21]
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