Where is it now
- Distance from Sun
- 1.273 AU
- True anomaly
- 175.46°
- Distance from Earth
- 2.267 AU
- As of
- 22 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
- 13h 46m 13s
- Declination
- -12° 46′ 13″
- Constellation
- Virgo
- Distance from Earth
- 2.27 AU
- Elongation from the Sun
- 1.74° — too close to the Sun to observe
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
- 0.946 AU
- Eccentricity
- 0.3486
- Inclination
- 4.04°
- Orbital period
- 335.9 days
- Perihelion
- 0.616 AU
- Aphelion
- 1.275 AU
- Longitude of ascending node
- 256.66°
- Argument of periapsis
- 136.49°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 7.0 LD
- 0.0181 AU
- Tisserand (Jupiter)
- 6.299
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 19
- Data arc
- 24 hours
- First observed
- 23 June 2022
- Last observed
- 24 June 2022
- Residual RMS
- 0.29 ″
- Solution · Otto Matic
- 24 June 2022
Visual & observation
- Absolute magnitude (H)
- 25.32
Discovery & classification
Close approaches 71 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-02-24 17:06 UTC close approach of 2022 MO1. Catalogue miss distance 74.0 LD · 2.85 × 10⁷ km. The curve is the geocentric path from 2031-02-21 to 2031-02-27, 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 |
|---|---|---|---|---|
| 2031-02-24 17:06:00 | Earth | 0.1902 AU | 74.0 LD | 15.7 km/s |
| 2031-12-22 16:49:00 | Earth | 0.2927 AU | 113.9 LD | 9.4 km/s |
| 2032-03-27 09:41:00 | Earth | 0.2462 AU | 95.8 LD | 7.9 km/s |
| 2032-10-17 08:54:00 | Earth | 0.3808 AU | 148.2 LD | 14.2 km/s |
| 2033-05-31 11:15:00 | Earth | 0.1996 AU | 77.7 LD | 7.4 km/s |
| 2034-06-14 22:26:00 | Earth | 0.2482 AU | 96.6 LD | 17.7 km/s |
| 2042-03-06 08:08:00 | Earth | 0.4116 AU | 160.2 LD | 22.8 km/s |
| 2043-02-18 22:35:00 | Earth | 0.1074 AU | 41.8 LD | 7.8 km/s |
| 2045-06-22 05:01:00 | Earth | 0.0306 AU | 11.9 LD | 11 km/s |
| 2054-02-20 19:42:00 | Earth | 0.0976 AU | 38.0 LD | 12.4 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