About Sedna
90377 Sedna is a distant trans-Neptunian object on one of the most extreme orbits known. Its aphelion is ~937 AU and its orbital period about 11,400 years. Its highly eccentric, distantly-bound orbit — never coming closer than 76 AU from the Sun — makes it a candidate first member of the hypothetical inner Oort Cloud. Its orbit is part of the observational evidence supporting the hypothesized “Planet Nine.”
Physical Properties
Orbit
Gallery
Hand-picked mission imagery of Sedna sourced from NASA and partner archives. Click any photo for full resolution and source attribution.
Imagery on this page is provided by the original mission teams. Full attribution terms: Image Rights & Credits.
Sources & Further Reading
- Wikipedia — extensive cross-referenced article
- Brown, Trujillo & Rabinowitz 2004 u2014 Discovery of Sedna
Numerical values (radius, mass, orbital elements, temperatures) are drawn from NASA NSSDC Planetary Fact Sheets, JPL Horizons, and the JPL Small-Body Database. Last refreshed: 2026-06-08 01:37:02.