(53319) 1999 JM8
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- The correct title of this article is (53319) 1999 JM8. It features superscript or subscript characters that are substituted or omitted because of technical limitations.
| Discovery | |
|---|---|
| Discovered by: | LINEAR |
| Discovery date: | May 13, 1999 |
| Orbital characteristics | |
| Epoch December 1, 2005 (JD 2453705.5) | |
| Aphelion | 667.93 Gm (4.46 AU) |
| Perihelion: | 142.03 Gm (0.95 AU) |
| Semi-major axis: | 404.98 Gm (2.71 AU) |
| Eccentricity: | .65 |
| Orbital period: | 1626.91 d (4.45 a) |
| Avg. orbital speed: | 16.01 km/s |
| Mean anomaly: | 151.84° |
| Inclination: | 13.83° |
| Longitude of ascending node: | 133.90° |
| Argument of perihelion: | 166.25° |
| Physical characteristics | |
| Dimensions: | 3.5 km |
| Rotation period: | 136 h |
| Temperature: | ~ K |
| Spectral type: | X |
| Absolute magnitude: | 15.1 |
(53319) 1999 JM8 (also written (53319) 1999 JM8) is a near-Earth asteroid and Mars-crosser asteroid discovered by LINEAR. Radar imaging by Goldstone and Arecibo has revealed the asteroid to be 3.5 km in diameter. Like the asteroid 4179 Toutatis, its rotation speed is unusually slow and possibly chaotic. Its shape is bizarre, and is vaguely reminiscent of a roast chicken.
It passed closer than 30 Gm to the Earth five times in the last century (5 Gm in 1990), but its closest approach in the 21st century will be at 38.3 Gm, in 2075.
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| Vulcanoids · Near-Earth asteroids · Main belt · Jupiter Trojans · Centaurs · Damocloids · Neptune Trojans · Comets · Trans-Neptunians (Kuiper belt • Scattered disc objects • Oort cloud) |
| For other objects and regions, see Asteroid groups and families, Binary asteroids, Asteroid moons, meteoroids and the Solar System. For a complete listing, see List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |