Where is it now
- Distance from Sun
- 1.067 AU
- True anomaly
- 189.73°
- Distance from Earth
- 0.189 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
- 02h 55m 12s
- Declination
- -60° 52′ 33″
- Constellation
- Horologium
- Distance from Earth
- 0.19 AU
- Elongation from the Sun
- 107.04° — well clear of the Sun
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
- 0.883 AU
- Eccentricity
- 0.2136
- Inclination
- 14.78°
- Orbital period
- 302.9 days
- Perihelion
- 0.694 AU
- Aphelion
- 1.071 AU
- Longitude of ascending node
- 165.87°
- Argument of periapsis
- 30.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 8.0 LD
- 0.0205 AU
- Tisserand (Jupiter)
- 6.674
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 193
- Data arc
- 4 days
- First observed
- 6 September 2021
- Last observed
- 10 September 2021
- Residual RMS
- 0.44 ″
- Solution · Otto Matic
- 10 August 2022
Visual & observation
- Absolute magnitude (H)
- 25.38
Discovery & classification
Close approaches 164 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-01-21 17:45 UTC close approach of 2021 RG2. Catalogue miss distance 95.1 LD · 3.66 × 10⁷ km. The curve is the geocentric path from 2027-01-18 to 2027-01-24, 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 |
|---|---|---|---|---|
| 2027-01-21 17:45:00 | Earth | 0.2444 AU | 95.1 LD | 9.7 km/s |
| 2031-06-03 07:27:00 | Earth | 0.347 AU | 135.0 LD | 7.5 km/s |
| 2031-10-20 06:53:00 | Earth | 0.2383 AU | 92.7 LD | 8.4 km/s |
| 2036-04-04 01:34:00 | Venus | 0.1279 AU | 49.8 LD | 13.7 km/s |
| 2036-05-02 11:19:00 | Earth | 0.3523 AU | 137.1 LD | 11 km/s |
| 2036-11-21 11:45:00 | Earth | 0.3273 AU | 127.4 LD | 12 km/s |
| 2038-10-06 04:02:00 | Venus | 0.0478 AU | 18.6 LD | 10.5 km/s |
| 2040-09-09 03:32:00 | Earth | 0.3602 AU | 140.2 LD | 17.8 km/s |
| 2041-04-07 23:56:00 | Earth | 0.3299 AU | 128.4 LD | 12.4 km/s |
| 2041-11-15 21:40:00 | Earth | 0.4535 AU | 176.5 LD | 17.3 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