| Orbital diagram of 2014 SV349 | |
| Discovery [1] [2] | |
|---|---|
| Discovered by | S. S. Sheppard |
| Discovery site | Cerro Tololo Obs. |
| Discovery date | 19 September 2014 |
| Designations | |
| 2014 SV349 | |
| Orbital characteristics [3] | |
| Epoch 1 July 2021 (JD 2459396.5) | |
| Uncertainty parameter 5 [1] ·6 [3] | |
| Observation arc | 2.83 yr (1,035 d) |
| Aphelion | 88.398 AU |
| Perihelion | 35.026 AU |
| 61.712 AU | |
| Eccentricity | 0.4324 |
| 484.81 yr (177,075 d) | |
| 297.13° | |
| 0° 0m 7.2s / day | |
| Inclination | 17.785° |
| 56.651° | |
| 23.717° | |
| Physical characteristics | |
| 423 km (est.) [4] [6] | |
| 5.1 [1] [3] | |
2014 SV349 is a large trans-Neptunian object from the scattered disc located in the outermost region of the Solar System. The object is a dwarf planet candidate and measures approximately 423 kilometers (260 miles) in diameter. It was discovered on 19 September 2014, by American astronomer Scott Sheppard at the Cerro Tololo Observatory, Chile. [1]
This minor planet orbits the Sun at a distance of 35.0–88.4 AU once every 484 years and 10 months (177,075 days; semi-major axis of 61.71 AU). Its orbit has an eccentricity of 0.43 and an inclination of 18° with respect to the ecliptic. [3] 2014 SV349 is moving closer to the Sun and will come to perihelion in 2106. [3] As of 2025 [update] , it is at 59.1 AU from the Sun. [7]
It is classified as a scattered disc object, [4] or "near-scattered" object in the classification of the Deep Ecliptic Survey, [5] that still gravitationally interacts with Neptune (30.1 AU) due to its relatively low perihelion of 35.0 AU, contrary to the extended-scattered/detached objects and sednoids which never approach Neptune as close.
Based on a generic magnitude-to-diameter conversion, 2014 SV349 measures approximately 423 kilometers (260 miles) in diameter, for an assumed albedo of 0.9 and a magnitude of 5.1. [4] [6]