(184212) 2004 PB112
| Discovery[1] | |
|---|---|
| Discovered by | M. W. Buie |
| Discovery site | Cerro Tololo Obs. |
| Discovery date | 13 August 2004 |
| Designations | |
| (184212) 2004 PB112 | |
| 2004 PB112 | |
| TNO[2] · SDO[3][4] res 4:27[5] | |
| Orbital characteristics[2] | |
| Epoch 1 July 2021 (JD 2459396.5) | |
| Uncertainty parameter 3[2] · 0[1] | |
| Observation arc | 17.07 yr (6,236 d) |
| Aphelion | 184.60 AU |
| Perihelion | 35.333 AU |
| 109.97 AU | |
| Eccentricity | 0.6787 |
| 1153.20 yrs | |
| 3.0647° | |
| 0° 0m 3.24s / day | |
| Inclination | 15.403° |
| 356.73° | |
| 3.6578° | |
| Physical characteristics | |
Mean diameter | 154 km (est. at 0.09)[3][6] |
| 7.3[1][2] | |
(184212) 2004 PB112 (provisional designation 2004 PB112) is a trans-Neptunian object from the scattered disc, approximately 154 kilometers (96 miles) in diameter, and in a rare high-order orbital resonance ratio (4:27) with Neptune. It was discovered on 13 August 2004, by American astronomer Marc Buie at the Cerro Tololo Inter-American Observatory in Chile.[1]
Orbit and classification[edit]
2004 PB112 orbits the Sun at a distance of 35.3–184.6 AU once every 1153 years and 2 months (421,205 days; semi-major axis of 109.97 AU). Its orbit has a high eccentricity of 0.68 and an inclination of 15° with respect to the ecliptic.[2] A first precovery was taken at Cerro Tololo in 2000, extending the body's observation arc by 4 years prior to its official discovery observation.[1]
2004 PB112 reached perihelion on 5 October 2011 (JD 2455839.806).[2] It has been classified as a highly unusual 4:27 resonant trans-Neptunian object,[5]: 49 but also simply as a scattered disc object,[3] or SCATNEAR, respectively, by the Deep Ecliptic Survey.[4]
Numbering and naming[edit]
This minor planet was numbered (184212) by the Minor Planet Center on 20 April 2008 (M.P.C. 62608).[7] As of 2021[update], it has not been named.[1]
Physical characteristics[edit]
Based on a generic conversion from an absolute magnitude of 7.2, 2004 PB112 measures between 100 and 220 kilometer in diameter.[6] Johnston's Archive estimates a mean-diameter of 154 kilometers (96 miles) assuming a typical albedo of 0.09.[3]
References[edit]
- ^ a b c d e f "184212 (2004 PB112)". Minor Planet Center. Retrieved 24 April 2017.
- ^ a b c d e f "JPL Small-Body Database Browser: 184212 (2004 PB112)" (2008-10-30 last obs.). Jet Propulsion Laboratory. Retrieved 1 June 2017.
- ^ a b c d Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 24 July 2021.
- ^ a b "Orbit Fit and Astrometric record for 184212". Southwest Research Institute. Retrieved 5 January 2019.The Deep Ecliptic Survey Object Classifications
- ^ a b Brett Gladman; Brian G. Marsden; Christa VanLaerhoven. "Nomenclature in the Outer Solar System" (PDF) (PDF). Retrieved 24 April 2017.
- ^ a b "Asteroid Size Estimator". CNEOS NASA/JPL. Retrieved 24 July 2021.
- ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 July 2021.
External links[edit]
- List Of Centaurs and Scattered-Disk Objects, Minor Planet Center
- Lightcurve Database Query (LCDB), at www.minorplanet.info
- Discovery Circumstances: Numbered Minor Planets (180001)-(185000) – Minor Planet Center
- (184212) 2004 PB112 at the JPL Small-Body Database
