Where is it now
- Distance from Sun
- 1.225 AU
- True anomaly
- 179.39°
- Distance from Earth
- 2.115 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
- 15h 03m 54s
- Declination
- -16° 23′ 09″
- Constellation
- Libra
- Distance from Earth
- 2.12 AU
- Elongation from the Sun
- 19.6° — too close to the Sun to observe
Favours the southern hemisphere; low or below the horizon from far north.
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
- 0.91 AU
- Eccentricity
- 0.3458
- Inclination
- 1.83°
- Orbital period
- 317 days
- Perihelion
- 0.595 AU
- Aphelion
- 1.225 AU
- Longitude of ascending node
- 186.6°
- Argument of periapsis
- 237.87°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.6 LD
- 0.0015 AU
- Tisserand (Jupiter)
- 6.503
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 13
- Data arc
- 24 hours
- First observed
- 2 April 2022
- Last observed
- 3 April 2022
- Residual RMS
- 0.19 ″
- Solution · Otto Matic
- 28 July 2026
Visual & observation
- Absolute magnitude (H)
- 29.34
Discovery & classification
Close approaches 38 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-04-02 00:15 UTC close approach of 2022 GX2. Catalogue miss distance 44.7 LD · 1.72 × 10⁷ km. The curve is the geocentric path from 2035-03-30 to 2035-04-05, 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 |
|---|---|---|---|---|
| 2028-02-17 06:14:00 | Venus | 0.1214 AU | 47.3 LD | 9.8 km/s |
| 2032-07-15 09:28:00 | Venus | 0.0912 AU | 35.5 LD | 14.6 km/s |
| 2035-04-02 00:15:00 | Earth | 0.115 AU | 44.7 LD | 13 km/s |
| 2036-07-11 07:29:00 | Earth | 0.118 AU | 45.9 LD | 6.9 km/s |
| 2038-06-08 21:59:00 | Venus | 0.0487 AU | 18.9 LD | 11.4 km/s |
| 2042-04-22 17:29:00 | Earth | 0.1658 AU | 64.5 LD | 7.1 km/s |
| 2042-11-15 17:17:00 | Venus | 0.1259 AU | 49.0 LD | 10.1 km/s |
| 2043-07-15 05:51:00 | Earth | 0.1925 AU | 74.9 LD | 15.2 km/s |
| 2047-04-19 12:12:00 | Venus | 0.0702 AU | 27.3 LD | 13.1 km/s |
| 2049-06-13 22:46:00 | Earth | 0.1966 AU | 76.5 LD | 7.3 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