(506479) 2003 HB57, is an extreme trans-Neptunian object of the extended scattered disc in the outermost region of the Solar System, approximately 180 kilometers in diameter. It was discovered by astronomers at the Mauna Kea Observatory on 26 April 2003.[4]
| Discovery[1] | |
|---|---|
| Discovered by | Mauna Kea Obs. |
| Discovery site | Mauna Kea Obs. |
| Discovery date | 26 April 2003 |
| Designations | |
| (506479) 2003 HB57 | |
| 2003 HB57 | |
| TNO[1] · E-SDO[2][3] distant[4] · detached | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 4 | |
| Observation arc | 13.94 yr (5,090 days) |
| Aphelion | 294.21 AU |
| Perihelion | 38.109 AU |
| 166.16 AU | |
| Eccentricity | 0.7706 |
| 2141.87 yr (782,317 days) | |
| 1.4255° | |
| 0° 0m 1.8s / day | |
| Inclination | 15.473° |
| 197.82° | |
| 11.013° | |
| Physical characteristics | |
| 147 km[2] 200 km[5] | |
| 0.04[5] 0.09[2] | |
| BR[2] | |
| 7.4[1] · 7.6[5] | |
Description
edit2003 HB57 orbits the Sun at a distance of 38.1–294.2 AU once every 2141 years and 10 months (782,317 days). Its orbit has an eccentricity of 0.77 and an inclination of 15° with respect to the ecliptic.[1]
Extended scattered disc
editIt is one of a small group of extreme trans-Neptunian objects with perihelion distances of 30 AU or more, and semi-major axes of 150 AU or more.[6] Such objects can not have reached their present-day orbits without the gravitational influence of some perturbing object, which lead to the speculation of planet nine.[7][8]
Physical characterization
edit2003 HB57 has a BR-type spectrum and an estimated diameter of 147 and 200 kilometers based on an assumed albedo of 0.09 and 0.04, respectively.[2][5]
References
edit- ^ a b c d e "JPL Small-Body Database Browser: 506479 (2003 HB57)" (2017-04-02 last obs.). Jet Propulsion Laboratory. Retrieved 9 December 2017.
- ^ a b c d e Johnston, Wm. Robert (15 October 2017). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 16 November 2017.
- ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 9 December 2017.
- ^ a b "506479 (2003 HB57)". Minor Planet Center. Retrieved 9 December 2017.
- ^ a b c d Michael E. Brown. "How many dwarf planets are there in the outer solar system?". California Institute of Technology. Retrieved 30 July 2017.
- ^ minorplanetcenter.net: q>30, a>150
- ^ Sheppard, Scott S.; Trujillo, Chadwick (December 2016). "New Extreme Trans-Neptunian Objects: Toward a Super-Earth in the Outer Solar System". The Astronomical Journal. 152 (6): 18. arXiv:1608.08772. Bibcode:2016AJ....152..221S. doi:10.3847/1538-3881/152/6/221. S2CID 119187392.
- ^ de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (21 October 2016). "Finding Planet Nine: apsidal anti-alignment Monte Carlo results". Monthly Notices of the Royal Astronomical Society. 462 (2): 1972–1977. arXiv:1607.05633. Bibcode:2016MNRAS.462.1972D. doi:10.1093/mnras/stw1778. S2CID 119212828.
External links
edit- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Discovery Circumstances: Numbered Minor Planets (505001)-(510000) – Minor Planet Center
- (506479) 2003 HB57 at AstDyS-2, Asteroids—Dynamic Site
- (506479) 2003 HB57 at the JPL Small-Body Database
