Where is it now
- Distance from Sun
- 1.36 AU
- True anomaly
- 194.5°
- Distance from Earth
- 0.484 AU
- As of
- 21 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
- 05h 06m 17s
- Declination
- +08° 55′ 11″
- Constellation
- Orion
- Distance from Earth
- 0.48 AU
- Elongation from the Sun
- 131.11° — well clear of the Sun
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
- 0.925 AU
- Eccentricity
- 0.5224
- Inclination
- 5.15°
- Orbital period
- 324.8 days
- Perihelion
- 0.442 AU
- Aphelion
- 1.408 AU
- Longitude of ascending node
- 153.25°
- Argument of periapsis
- 55.64°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 3.3 LD
- 0.0084 AU
- Tisserand (Jupiter)
- 6.343
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 61
- Data arc
- 8 years
- First observed
- 8 September 2016
- Last observed
- 9 September 2024
- Residual RMS
- 0.62 ″
- Solution · Otto Matic
- 13 September 2024
Visual & observation
- Absolute magnitude (H)
- 23.65
Discovery & classification
Close approaches 287 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-12-10 13:08 UTC close approach of 2016 RJ20. Catalogue miss distance 86.4 LD · 3.32 × 10⁷ km. The curve is the geocentric path from 2026-12-07 to 2026-12-13, 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 |
|---|---|---|---|---|
| 2026-12-10 13:08:00 | Earth | 0.222 AU | 86.4 LD | 11.1 km/s |
| 2027-11-27 11:32:00 | Earth | 0.4546 AU | 176.9 LD | 30.3 km/s |
| 2029-10-25 20:06:00 | Merc | 0.0332 AU | 12.9 LD | 19.2 km/s |
| 2029-10-25 20:06:00 | Mercury | 0.0332 AU | 12.9 LD | 19.2 km/s |
| 2030-02-25 02:52:00 | Mars | 0.0847 AU | 33.0 LD | 9.5 km/s |
| 2032-07-07 15:11:00 | Merc | 0.0835 AU | 32.5 LD | 20.6 km/s |
| 2032-07-07 15:11:00 | Mercury | 0.0835 AU | 32.5 LD | 20.6 km/s |
| 2032-08-31 05:02:00 | Earth | 0.0304 AU | 11.8 LD | 15.3 km/s |
| 2033-10-15 03:55:00 | Earth | 0.4149 AU | 161.5 LD | 12.5 km/s |
| 2034-12-09 22:11:00 | Earth | 0.2264 AU | 88.1 LD | 11.1 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