2022 GO3 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.67 AU to 1.34 AU from the Sun; one orbit takes 369.2 days. Orbit from the JPL solution of 10 April 2022.
Where is it now
- Distance from Sun
- 1.126 AU
- True anomaly
- 232.13°
- Distance from Earth
- 1.456 AU
- As of
- 3 November 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
- 18h 07m 25s
- Declination
- -18° 23′ 35″
- Constellation
- Sagittarius
- Distance from Earth
- 1.46 AU
- Elongation from the Sun
- 50.46° — near the Sun — look low at dusk or dawn
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
- 1.007 AU
- Eccentricity
- 0.3338
- Inclination
- 7.71°
- Orbital period
- 369.2 days
- Perihelion
- 0.671 AU
- Aphelion
- 1.343 AU
- Longitude of ascending node
- 192.42°
- Argument of periapsis
- 249.91°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.7 LD
- 0.0043 AU
- Tisserand (Jupiter)
- 5.988
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 19
- Data arc
- 7 days
- First observed
- 3 April 2022
- Last observed
- 10 April 2022
- Residual RMS
- 0.5 ″
- Solution · Otto Matic
- 10 April 2022
Visual & observation
- Absolute magnitude (H)
- 26.85
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 64 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-12 21:08 UTC close approach of 2022 GO3. Catalogue miss distance 114.7 LD · 4.41 × 10⁷ km. The curve is the geocentric path from 2027-04-09 to 2027-04-15, 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 |
|---|---|---|---|---|
| 2027-04-12 21:08:00 | Earth | 0.2946 AU | 114.7 LD | 18.9 km/s |
| 2028-01-15 12:15:00 | Venus | 0.0453 AU | 17.6 LD | 12.1 km/s |
| 2028-04-15 03:31:00 | Earth | 0.3588 AU | 139.6 LD | 20.8 km/s |
| 2029-04-18 00:37:00 | Earth | 0.4167 AU | 162.2 LD | 22.6 km/s |
| 2030-04-20 23:04:00 | Earth | 0.4743 AU | 184.6 LD | 24.3 km/s |
| 2039-04-10 21:24:00 | Venus | 0.1209 AU | 47.0 LD | 8.1 km/s |
| 2042-03-05 01:04:00 | Venus | 0.139 AU | 54.1 LD | 16.2 km/s |
| 2053-04-20 21:16:00 | Venus | 0.0709 AU | 27.6 LD | 8.4 km/s |
| 2067-05-31 17:38:00 | Venus | 0.0392 AU | 15.3 LD | 11.9 km/s |
| 2100-08-08 06:10:00 | Earth | 0.4769 AU | 185.6 LD | 24 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