2018 AM12
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Where is it now
- Distance from Sun
- 0.968 AU
- True anomaly
- 124.12°
- Distance from Earth
- 1.209 AU
- As of
- 21 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
- 10h 39m 33s
- Declination
- +09° 54′ 00″
- Constellation
- Leo
- Distance from Earth
- 1.21 AU
- Elongation from the Sun
- 51.02° — 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
- 0.917 AU
- Eccentricity
- 0.1162
- Inclination
- 21.67°
- Orbital period
- 320.9 days
- Perihelion
- 0.811 AU
- Aphelion
- 1.024 AU
- Longitude of ascending node
- 288.83°
- Argument of periapsis
- 51.05°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.8 LD
- 0.0071 AU
- Tisserand (Jupiter)
- 6.448
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 128
- Data arc
- 14.06 years
- First observed
- 9 January 2011
- Last observed
- 31 January 2025
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 31 January 2025
Physical properties
- Rotation period
- 0.21 hours
Visual & observation
- Absolute magnitude (H)
- 21.16
Discovery & classification
Close approaches 64 on record
Top-down view of the ecliptic, Earth at the centre, for the 2040-01-08 14:10 UTC close approach of 2018 AM12. Catalogue miss distance 73.1 LD · 2.81 × 10⁷ km. The curve is the geocentric path from 2040-01-05 to 2040-01-11, 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. At closest approach the object is south of the ecliptic. 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 |
|---|---|---|---|---|
| 2040-01-08 14:10:00 | Earth | 0.1879 AU | 73.1 LD | 11.6 km/s |
| 2047-01-09 12:16:00 | Earth | 0.0325 AU | 12.6 LD | 11.4 km/s |
| 2047-06-26 13:30:00 | Earth | 0.1835 AU | 71.4 LD | 13 km/s |
| 2054-01-11 05:35:00 | Earth | 0.0729 AU | 28.4 LD | 12.3 km/s |
| 2054-07-08 00:00:00 | Earth | 0.1715 AU | 66.7 LD | 12.7 km/s |
| 2070-04-24 13:00:00 | Venus | 0.1396 AU | 54.3 LD | 14.6 km/s |
| 2076-06-19 05:28:00 | Venus | 0.1235 AU | 48.1 LD | 14.7 km/s |
| 2082-08-14 20:50:00 | Venus | 0.1172 AU | 45.6 LD | 14.9 km/s |
| 2083-01-08 16:59:00 | Earth | 0.1077 AU | 41.9 LD | 11.2 km/s |
| 2088-10-09 12:36:00 | Venus | 0.1307 AU | 50.9 LD | 15.4 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB