(5407) 1992 AX
| Discovery[1] | |
|---|---|
| Discovered by | Seiji Ueda and Hiroshi Kaneda |
| Discovery site | Kushiro, Hokkaidō |
| Discovery date | 4 January 1992 |
| Designations | |
| 1987 BH2 | |
| Orbital characteristics[1][2] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 23380 days (64.01 yr) |
| Aphelion | 2.3484 AU (351.32 Gm) |
| Perihelion | 1.3279 AU (198.65 Gm) |
| 1.8382 AU (274.99 Gm) | |
| Eccentricity | 0.27758 |
| 2.49 yr (910.29 d) | |
| 149.33° | |
| 0° 23m 43.728s / day | |
| Inclination | 11.390° |
| 117.76° | |
| 108.73° | |
| Known satellites | 1 |
| Earth MOID | 0.376704 AU (56.3541 Gm) |
| Jupiter MOID | 2.70035 AU (403.967 Gm) |
| Proper orbital elements | |
Proper mean motion | 0.3955 deg / yr |
Proper orbital period |
910.2402 yr (332465.234 d) |
| Physical characteristics | |
| Dimensions | 4 km (2.5 mi)[3] |
| 2.5488 h (0.10620 d) | |
Sidereal rotation period | 2.5488 h[1] |
| 0.16[2] | |
| S[1] | |
| 13.9[1] | |
|
| |
(5407) 1992 AX is a Mars-crossing minor planet. It was discovered by Seiji Ueda and Hiroshi Kaneda in Kushiro, Hokkaidō, on January 4, 1992.
Mars-Crossing
1992 AX makes occasional close approaches to Mars. Its next close approach, on January 22, 2027, will bring it 11,260,000 km (0.0753 AU) from Mars.[1]
Moon
1992 AX has one natural satellite, S/1997 (5407) 1. However, the true presence of a moon is still considered inconclusive.[2] If it exists, the moon completes one orbit around 1992 AX every 13.5196 hours at a distance of 6.8 km. S/1997 (5407) 1 is 1.2 km wide.[2] From the surface of 1992 AX, S/1997 (5407) 1 would have an angular diameter of roughly 14.3°.[lower-alpha 1] For comparison, the Sun appears to be 0.5° from Earth.
Gallery

Orbit of 1992 AX
See also
Notes
- ↑ Calculated by solving the equation
.
References
- 1 2 3 4 5 6 "JPL Small-Body Database Browser: 5407 (1992 AX)". Jet Propulsion Laboratory. Retrieved 4 April 2016.
- 1 2 3 4 Johnston, W.M. (September 1, 2005). "(5407) 1992 AX". Johnston Archive. Retrieved 27 November 2013.
- ↑ "Two-Period Lightcurves of 1996 FG 3, 1998 PG, and (5407) 1992 AX: One Probable and Two Possible Binary Asteroids". Icarus 146 (1): 190–203. July 2000. Bibcode:2000Icar..146..190P. doi:10.1006/icar.2000.6375.
External links
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