(434326) 2004 JG6
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(Redirected from 2004 JG6)
| Discovery | |
|---|---|
| Discovered by | Brian A. Skiff / LONEOS |
| Discovery date | May 11, 2004 |
| Designations | |
| none | |
| Aten, Apohele Mercury-crosser Venus-crosser |
|
| Orbital characteristics | |
| Epoch October 22, 2004 (JD 2453300.5) | |
| Aphelion | 145.491 Gm (0.973 AU) |
| Perihelion | 44.480 Gm (0.297 AU) |
| 94.985 Gm (0.635 AU) | |
| Eccentricity | 0.532 |
| 184.798 d (0.51 a) | |
|
Average orbital speed
|
34.58 km/s |
| 164.532° | |
| Inclination | 18.962° |
| 37.076° | |
| 352.935° | |
| Physical characteristics | |
| Dimensions | 0.5–1.1 km[1] |
| Mass | 1.3–18.0×1011 kg |
|
Mean density
|
2.0? g/cm³ |
| 0.0001–0.0003 m/s² | |
| 0.0003–0.0006 km/s | |
| ? d | |
| Albedo | 0.10? |
| Temperature | ~349 K |
|
Spectral type
|
? |
| 18.9 | |
(434326) 2004 JG6 (also written 2004 JG6) is one of the closest orbiting objects to the Sun.
It is the second known Apohele asteroid (the first being 163693 Atira), which means its entire orbit lies within that of the Earth.[2] Its orbital period is less than that of Venus, making it one of the closest known objects to the Sun, after Mercury.2004 JG6 has an eccentric orbit that crosses the orbits of both Mercury and Venus.[2]
It was discovered by Brian A. Skiff of the LONEOS project.
See also
References
External links
- Orbital simulation from JPL (Java)
- Lua error in package.lua at line 80: module 'strict' not found.
