Where is it now
- Distance from Sun
- 0.627 AU
- True anomaly
- 359.24°
- Distance from Earth
- 1.481 AU
- As of
- 24 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 04m 20s
- Declination
- +01° 09′ 42″
- Constellation
- Virgo
- Distance from Earth
- 1.48 AU
- Elongation from the Sun
- 18.65° — 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
- 0.971 AU
- Eccentricity
- 0.3541
- Inclination
- 24.7°
- Orbital period
- 349.3 days
- Perihelion
- 0.627 AU
- Aphelion
- 1.314 AU
- Longitude of ascending node
- 28.95°
- Argument of periapsis
- 133.5°
- Epoch · J2000
- 2459145.5
- Orbit class · ATE
- Aten
- Earth MOID · 37.5 LD
- 0.0963 AU
- Tisserand (Jupiter)
- 6.094
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 13
- Data arc
- 10 days
- First observed
- 17 October 2020
- Last observed
- 27 October 2020
- Residual RMS
- 0.56 ″
- Solution · Otto Matic
- 14 September 2023
Visual & observation
- Absolute magnitude (H)
- 24.18
Discovery & classification
Close approaches 32 on record
Top-down view of the ecliptic, Earth at the centre, for the 2086-10-26 23:27 UTC close approach of 2020 UK6. Catalogue miss distance 70.9 LD · 2.73 × 10⁷ km. The curve is the geocentric path from 2086-10-23 to 2086-10-29, 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 |
|---|---|---|---|---|
| 2086-10-26 23:27:00 | Earth | 0.1822 AU | 70.9 LD | 13.5 km/s |
| 2087-10-30 18:19:00 | Earth | 0.1241 AU | 48.3 LD | 16.8 km/s |
| 2088-10-24 04:06:00 | Earth | 0.3377 AU | 131.4 LD | 22.9 km/s |
| 2094-10-22 23:17:00 | Venus | 0.1456 AU | 56.7 LD | 21.2 km/s |
| 2109-10-31 10:58:00 | Earth | 0.1013 AU | 39.4 LD | 15 km/s |
| 2110-10-28 20:19:00 | Earth | 0.2402 AU | 93.5 LD | 20.2 km/s |
| 2111-10-20 21:42:00 | Earth | 0.4759 AU | 185.2 LD | 27 km/s |
| 2198-10-29 13:09:00 | Earth | 0.1578 AU | 61.4 LD | 13.8 km/s |
| 2199-10-31 15:04:00 | Earth | 0.1507 AU | 58.6 LD | 17.6 km/s |
| 2200-10-25 05:07:00 | Earth | 0.3766 AU | 146.6 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