(307463) 2002 VU130
| Discovery[1][2] | |
|---|---|
| Discovered by | M. W. Buie |
| Discovery site | Kitt Peak Obs. |
| Discovery date | 7 November 2002 |
| Designations | |
| (307463) 2002 VU130 | |
| 2002 VU130 | |
| TNO[3] · plutino[4][5] | |
| Orbital characteristics[3] | |
| Epoch 1 July 2021 (JD 2459396.5) | |
| Uncertainty parameter 2[3] · 1[1] | |
| Observation arc | 13.99 yr (5,110 d) |
| Aphelion | 47.106 AU |
| Perihelion | 30.929 AU |
| 39.018 AU | |
| Eccentricity | 0.2073 |
| 243.73 yr (89,021 d) | |
| 278.86° | |
| 0° 0m 14.4s / day | |
| Inclination | 1.3761° |
| 267.86° | |
| 281.56° | |
| Physical characteristics | |
| 253 km[5][6] | |
| 0.179[5][6] | |
| 5.47[6] 5.9[3] | |
(307463) 2002 VU130 (provisional designation 2002 VU130) is a trans-Neptunian object, located in the circumstellar disc of the Kuiper belt in the outermost region of the Solar System. The resonant trans-Neptunian object belongs to the population of plutinos and measures approximately 253 kilometers (160 miles) in diameter. It was discovered on 7 November 2002, by American astronomer Marc Buie at the Kitt Peak Observatory near Tucson, Arizona. The object has not been named yet.[1]
Orbit and classification
[edit]2002 VU130 is a plutino, a population of objects in the Kuiper belt that stay in a 2:3 resonance with Neptune.[4][5] A large part of the inner Kuiper belt is formed by objects belonging to this population which is named after its largest member, Pluto. 2002 VU130 orbits the Sun at a distance of 30.9–47.1 AU once every 243 years and 9 months (89,021 days; semi-major axis of 39.02 AU). Its orbit has an eccentricity of 0.21 and an inclination of 1° with respect to the ecliptic.[3] The body's observation arc begins with its official discovery observation on 7 November 2002.[1] It is currently approaching the Sun at 39.428 AU,[7] with its perihelion-passage projected to occur in June 2076.[3]
Numbering and naming
[edit]This minor planet was numbered by the Minor Planet Center on 10 December 2011 (M.P.C. 77418).[8] As of 2021[update], it has not been named.[1] If named, it will follow the already established scheme of naming these objects after mythological entities associated with the underworld.
Physical characteristics
[edit]Diameter and albedo
[edit]Observations with Herschel's PACS instrument were published in 2011. For 2002 VU130, the measurements gave a mean-diameter of 252.9+33.6
−31.3 km with an unusually high albedo of 0.179+0.202
−0.103 and an absolute magnitude of 5.47±0.83.[6] This result has been adopted in Johnston's Archive, giving a rounded diameter of 253 kilometers (160 miles),[5] while Mike Brown estimates as similar one of 260 km with an albedo of 0.18 and an absolute magnitude of 5.5.[9]
References
[edit]- ^ a b c d e "307463 (2002 VU130)". Minor Planet Center. Retrieved 24 July 2021.
- ^ "M.P.E.C. 2002-X10 (containing 2002 VU130)". Minor Planet Electronic Circular. 3 December 2002. Retrieved 24 July 2021.
- ^ a b c d e f "JPL Small-Body Database Browser: 307463 (2002 VU130)" (2016-11-03 last obs.). Jet Propulsion Laboratory. Retrieved 24 July 2021.
- ^ a b "Orbit Fit and Astrometric record for 307463". Southwest Research Institute. Retrieved 24 July 2021.The Deep Ecliptic Survey Object Classifications
- ^ a b c d e Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 24 July 2021.
- ^ a b c d Mommert, M.; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; et al. (May 2012). "TNOs are cool: A survey of the trans-Neptunian region. V. Physical characterization of 18 Plutinos using Herschel-PACS observations". Astronomy & Astrophysics. 541: A93. arXiv:1202.3657. Bibcode:2012A&A...541A..93M. doi:10.1051/0004-6361/201118562. ISSN 0004-6361.
- ^ "Asteroid (307463) 2002 VU130 – Ephemerides". AstDyS-2, Asteroids – Dynamic Site. Retrieved 24 July 2021.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 July 2021.
- ^ Brown, Michael E. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 24 July 2021.
External links
[edit]- Orbit simulation from NASA JPL site
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- (307463) 2002 VU130, Small Bodies Data Ferret
- (307463) 2002 VU130 at the JPL Small-Body Database
