Where is it now
- Distance from Sun
- 0.79 AU
- True anomaly
- 52.64°
- Distance from Earth
- 0.908 AU
- As of
- 20 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 36m 28s
- Declination
- +03° 07′ 39″
- Constellation
- Sextans
- Distance from Earth
- 0.91 AU
- Elongation from the Sun
- 48.82° — 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
- 0.899 AU
- Eccentricity
- 0.1707
- Inclination
- 6.14°
- Orbital period
- 311.1 days
- Perihelion
- 0.745 AU
- Aphelion
- 1.052 AU
- Longitude of ascending node
- 187.69°
- Argument of periapsis
- 206.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 9.4 LD
- 0.0241 AU
- Tisserand (Jupiter)
- 6.605
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 30
- Data arc
- 12 days
- First observed
- 2 April 2020
- Last observed
- 14 April 2020
- Residual RMS
- 0.46 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.4
Discovery & classification
Close approaches 54 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-03-19 07:47 UTC close approach of 2020 GQ. Catalogue miss distance 147.1 LD · 5.66 × 10⁷ km. The curve is the geocentric path from 2031-03-16 to 2031-03-22, 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 |
|---|---|---|---|---|
| 2029-03-31 09:19:00 | Venus | 0.1082 AU | 42.1 LD | 8 km/s |
| 2031-03-19 07:47:00 | Earth | 0.3781 AU | 147.1 LD | 15.7 km/s |
| 2032-05-25 18:00:00 | Earth | 0.3494 AU | 136.0 LD | 14.2 km/s |
| 2037-03-11 14:03:00 | Earth | 0.1237 AU | 48.1 LD | 7.9 km/s |
| 2048-11-18 10:39:00 | Earth | 0.246 AU | 95.7 LD | 7.3 km/s |
| 2049-05-30 07:49:00 | Earth | 0.2077 AU | 80.8 LD | 9.5 km/s |
| 2054-03-15 01:06:00 | Earth | 0.2706 AU | 105.3 LD | 12.5 km/s |
| 2054-10-04 04:38:00 | Earth | 0.2464 AU | 95.9 LD | 7.9 km/s |
| 2055-05-22 18:25:00 | Earth | 0.4513 AU | 175.6 LD | 17.5 km/s |
| 2058-03-17 21:59:00 | Venus | 0.0832 AU | 32.4 LD | 7 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