Where is it now
- Distance from Sun
- 0.727 AU
- True anomaly
- 47.22°
- Distance from Earth
- 1.702 AU
- As of
- 19 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 54m 25s
- Declination
- -17° 31′ 45″
- Constellation
- Virgo
- Distance from Earth
- 1.7 AU
- Elongation from the Sun
- 7.75° — 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
- 0.864 AU
- Eccentricity
- 0.2048
- Inclination
- 14.24°
- Orbital period
- 293.3 days
- Perihelion
- 0.687 AU
- Aphelion
- 1.041 AU
- Longitude of ascending node
- 337.06°
- Argument of periapsis
- 195.46°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 7.8 LD
- 0.0201 AU
- Tisserand (Jupiter)
- 6.795
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 28
- Data arc
- 24 hours
- First observed
- 5 September 2020
- Last observed
- 6 September 2020
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 25.1
Discovery & classification
Close approaches 147 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-08-23 12:06 UTC close approach of 2020 RL. Catalogue miss distance 43.1 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2028-08-20 to 2028-08-26, 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. At closest approach the object is south of the ecliptic. 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 |
|---|---|---|---|---|
| 2028-08-23 12:06:00 | Earth | 0.1107 AU | 43.1 LD | 9.7 km/s |
| 2029-01-20 06:14:00 | Earth | 0.2779 AU | 108.1 LD | 10.5 km/s |
| 2030-09-15 10:50:00 | Venus | 0.0459 AU | 17.8 LD | 10.4 km/s |
| 2032-08-22 19:33:00 | Earth | 0.2194 AU | 85.4 LD | 12.4 km/s |
| 2033-02-06 20:49:00 | Earth | 0.2852 AU | 111.0 LD | 11.7 km/s |
| 2036-08-24 19:34:00 | Earth | 0.3416 AU | 132.9 LD | 15.9 km/s |
| 2037-02-24 06:45:00 | Earth | 0.297 AU | 115.6 LD | 12.4 km/s |
| 2040-08-28 06:45:00 | Earth | 0.4666 AU | 181.6 LD | 19.6 km/s |
| 2041-02-27 20:46:00 | Venus | 0.033 AU | 12.8 LD | 10.5 km/s |
| 2041-03-13 17:45:00 | Earth | 0.3119 AU | 121.4 LD | 12.6 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