(721708) 2004 BX159
Asteroid
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(721708) 2004 BX159 is an asteroid from the central region of the asteroid belt, approximately 1.2 kilometers in diameter. It was first observed at Paranal Observatory in the Atacama desert of Chile on 20 January 2004.[2] 2004 BX159 missed the virtual impactor date of 29 August 2009.[5] The asteroid was removed from the Sentry Risk Table in April 2014[6] as a result of precovery images establishing it is a harmless main belt asteroid.
(discovery: first observation only)
| Discovery[1][2] | |
|---|---|
| Discovered by | Paranal Obs. |
| Discovery site | Paranal Obs. |
| Discovery date | 20 January 2004 (discovery: first observation only) |
| Designations | |
| 2004 BX159 | |
| main-belt[1][2] · (middle) | |
| Orbital characteristics[1] | |
| Epoch 4 September 2017 (JD 2458000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 19.97 yr (7,293 days) |
| Earliest precovery date | 14 July 1997 |
| Aphelion | 2.8997 AU |
| Perihelion | 2.1632 AU |
| 2.5315 AU | |
| Eccentricity | 0.1455 |
| 4.03 yr (1,471 days) | |
| 355.95° | |
| 0° 14m 40.92s / day | |
| Inclination | 4.0931° |
| 159.75° | |
| 153.29° | |
| Physical characteristics | |
| Dimensions | 1.2 km (estimate)[3] 1.8 km (est. at 0.10)[4] |
| 16.9[1] | |
Description
2004 BX159 orbits the Sun in the central main-belt at a distance of 2.2–2.9 AU once every 4.03 years (1,471 days). Its orbit has an eccentricity of 0.15 and an inclination of 4° with respect to the ecliptic.[1]
After discovery, it was thought to be a Mars-crossing asteroid because of its poorly known orbit, and was listed on the Sentry Risk Table as a possible impactor.[5] With an observation arc of 3 days and only 8 observations, perihelion was determined to be 1.5±3 astronomical units (AU).[7]
Precovery observations in archival data of the Canada-France-Hawaii Telescope on Mauna Kea were identified in early 2014, resulting in a dramatic improvement of the orbital accuracy, sufficient to recognize the object as a regular main belt asteroid, not posing any danger to Earth.[1]
The body was subsequently linked by the Minor Planet Center with additional observations reported since 1997. It has now a well-established orbit, observed over decades, with the lowest possible uncertainty of 0.[1]
It is even known that 2004 BX159 passed 0.0036 AU (540,000 km; 330,000 mi) from asteroid 3 Juno on 18 September 1961.[1]