Where is it now
- Distance from Sun
- 0.765 AU
- True anomaly
- 91.8°
- Distance from Earth
- 1.706 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
- 14h 30m 35s
- Declination
- -14° 02′ 22″
- Constellation
- Libra
- Distance from Earth
- 1.71 AU
- Elongation from the Sun
- 12.48° — 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.
Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.
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
- 0.87 AU
- Eccentricity
- 0.3623
- Inclination
- 2.08°
- Orbital period
- 296.5 days
- Perihelion
- 0.555 AU
- Aphelion
- 1.185 AU
- Longitude of ascending node
- 182.42°
- Argument of periapsis
- 321.92°
- Epoch · J2000
- 2459107.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.3 LD
- 0.006 AU
- Tisserand (Jupiter)
- 6.742
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 16
- Data arc
- 9 days
- First observed
- 11 September 2020
- Last observed
- 20 September 2020
- Residual RMS
- 0.63 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.8
Discovery & classification
Close approaches 33 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-07-05 06:45 UTC close approach of 2020 RV6. Catalogue miss distance 80.9 LD · 3.11 × 10⁷ km. The curve is the geocentric path from 2028-07-02 to 2028-07-08, 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 |
|---|---|---|---|---|
| 2028-07-05 06:45:00 | Earth | 0.2078 AU | 80.9 LD | 15.8 km/s |
| 2029-09-29 00:27:00 | Earth | 0.2563 AU | 99.8 LD | 17.5 km/s |
| 2030-11-05 01:25:00 | Venus | 0.0524 AU | 20.4 LD | 14.9 km/s |
| 2037-12-30 21:20:00 | Earth | 0.3809 AU | 148.3 LD | 12.7 km/s |
| 2040-05-24 02:05:00 | Venus | 0.0355 AU | 13.8 LD | 14 km/s |
| 2041-07-04 16:41:00 | Earth | 0.1828 AU | 71.2 LD | 15 km/s |
| 2042-02-11 05:29:00 | Earth | 0.432 AU | 168.1 LD | 16.5 km/s |
| 2042-09-28 05:29:00 | Earth | 0.2833 AU | 110.3 LD | 18.3 km/s |
| 2046-03-22 08:39:00 | Earth | 0.408 AU | 158.8 LD | 14.3 km/s |
| 2046-10-02 17:22:00 | Earth | 0.0574 AU | 22.4 LD | 8 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