2014 SV349
Trans-Neptunian object
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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]
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] | |
Orbit and classification
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.