2018 AU11 is an asteroid in the Aten orbit class. Its orbit takes it from 0.62 AU to 1.33 AU from the Sun; one orbit takes 352.7 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.82 AU
- True anomaly
- 275.01°
- Distance from Earth
- 1.508 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
- 12h 10m 27s
- Declination
- +01° 56′ 35″
- Constellation
- Virgo
- Distance from Earth
- 1.51 AU
- Elongation from the Sun
- 30.2° — near the Sun — look low at dusk or dawn
Visible from both hemispheres.
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
- 0.977 AU
- Eccentricity
- 0.3653
- Inclination
- 10.36°
- Orbital period
- 352.7 days
- Perihelion
- 0.62 AU
- Aphelion
- 1.334 AU
- Longitude of ascending node
- 114.01°
- Argument of periapsis
- 114.78°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.6 LD
- 0.0066 AU
- Tisserand (Jupiter)
- 6.12
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 32
- Data arc
- 6 days
- First observed
- 10 January 2018
- Last observed
- 16 January 2018
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 25.3
Discovery & classification
Close approaches 94 on record
Top-down view of the ecliptic, Earth at the centre, for the 2037-09-21 07:56 UTC close approach of 2018 AU11. Catalogue miss distance 169.6 LD · 6.52 × 10⁷ km. The curve is the geocentric path from 2037-09-18 to 2037-09-24, 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 |
|---|---|---|---|---|
| 2030-09-16 15:01:00 | Venus | 0.1442 AU | 56.1 LD | 18 km/s |
| 2032-10-24 21:23:00 | Venus | 0.1089 AU | 42.4 LD | 16.8 km/s |
| 2037-09-21 07:56:00 | Earth | 0.4357 AU | 169.6 LD | 24.5 km/s |
| 2038-09-11 17:55:00 | Earth | 0.2491 AU | 96.9 LD | 18.3 km/s |
| 2039-07-29 21:57:00 | Venus | 0.0575 AU | 22.4 LD | 14.3 km/s |
| 2039-08-31 20:10:00 | Earth | 0.1323 AU | 51.5 LD | 12.3 km/s |
| 2042-11-09 23:13:00 | Earth | 0.3931 AU | 153.0 LD | 9.7 km/s |
| 2043-12-01 15:22:00 | Earth | 0.3657 AU | 142.3 LD | 9.7 km/s |
| 2046-01-17 07:41:00 | Earth | 0.1063 AU | 41.4 LD | 9.7 km/s |
| 2046-05-04 05:46:00 | Venus | 0.0384 AU | 14.9 LD | 13.3 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