Where is it now
- Distance from Sun
- 1.234 AU
- True anomaly
- 199.18°
- Distance from Earth
- 0.763 AU
- As of
- 24 October 2026
Two-body Kepler propagation — accurate to ~0.1% for major planets over decades, less so for highly-perturbed bodies. Use JPL Horizons for high precision.
In the sky
- Right ascension
- 09h 03m 50s
- Declination
- +48° 02′ 23″
- Constellation
- Ursa Major
- Distance from Earth
- 0.76 AU
- Elongation from the Sun
- 88.21° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
From your location
See how high it is right now, whether it is up after civil twilight, and when it rises and sets where you are.
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Two-body approximation, good to about a degree for the planets — enough to find the constellation and know whether it is up.
Orbital elements
- Semi-major axis
- 0.973 AU
- Eccentricity
- 0.2985
- Inclination
- 24.07°
- Orbital period
- 350.3 days
- Perihelion
- 0.682 AU
- Aphelion
- 1.263 AU
- Longitude of ascending node
- 292.01°
- Argument of periapsis
- 291.85°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.0 LD
- 0.0102 AU
- Tisserand (Jupiter)
- 6.104
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 85
- Data arc
- 7 days
- First observed
- 10 January 2026
- Last observed
- 17 January 2026
- Residual RMS
- 0.57 ″
- Solution · Otto Matic
- 17 January 2026
Visual & observation
- Absolute magnitude (H)
- 25.1
Discovery & classification
Close approaches 32 on record
Top-down view of the ecliptic, Earth at the centre, for the 2049-01-14 23:18 UTC close approach of 2026 AX1. Catalogue miss distance 46.9 LD · 1.8 × 10⁷ km. The curve is the geocentric path from 2049-01-11 to 2049-01-17, with a mark at UTC midnights and an arrow for the direction of motion. The circle is the Moon’s mean orbit; the Moon is plotted at closest approach. A ray shows the Sun’s direction. The labelled distance is the full separation. The drawn radius is the part that lies in the ecliptic plane. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate.
| When (UTC) | Body | Distance | Lunar distances | Relative speed |
|---|---|---|---|---|
| 2034-01-03 17:11:00 | Venus | 0.0673 AU | 26.2 LD | 17.6 km/s |
| 2042-08-19 03:16:00 | Venus | 0.0947 AU | 36.9 LD | 20.4 km/s |
| 2049-01-14 23:18:00 | Earth | 0.1205 AU | 46.9 LD | 13.4 km/s |
| 2050-01-09 21:08:00 | Earth | 0.1286 AU | 50.0 LD | 17.9 km/s |
| 2066-08-13 04:18:00 | Venus | 0.0576 AU | 22.4 LD | 17.9 km/s |
| 2073-01-12 13:19:00 | Earth | 0.0319 AU | 12.4 LD | 15.8 km/s |
| 2075-03-28 02:18:00 | Venus | 0.0901 AU | 35.1 LD | 20.3 km/s |
| 2116-06-10 16:04:00 | Venus | 0.1291 AU | 50.3 LD | 16.7 km/s |
| 2118-01-16 05:53:00 | Earth | 0.0996 AU | 38.8 LD | 13.7 km/s |
| 2119-01-10 09:29:00 | Earth | 0.1586 AU | 61.7 LD | 18.6 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB