Where is it now
- Distance from Sun
- 0.891 AU
- True anomaly
- 238.96°
- Distance from Earth
- 0.148 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
- 16h 24m 20s
- Declination
- -05° 20′ 07″
- Constellation
- Ophiuchus
- Distance from Earth
- 0.15 AU
- Elongation from the Sun
- 41.43° — near the Sun — look low at dusk or dawn
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
- 0.827 AU
- Eccentricity
- 0.2603
- Inclination
- 4.35°
- Orbital period
- 274.8 days
- Perihelion
- 0.612 AU
- Aphelion
- 1.042 AU
- Longitude of ascending node
- 343.46°
- Argument of periapsis
- 158.27°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.8 LD
- 0.0045 AU
- Tisserand (Jupiter)
- 7.059
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 44
- Data arc
- 3 days
- First observed
- 6 September 2023
- Last observed
- 9 September 2023
- Residual RMS
- 0.36 ″
- Solution · Otto Matic
- 19 September 2023
Visual & observation
- Absolute magnitude (H)
- 28.45
Discovery & classification
Close approaches 72 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-08-02 02:26 UTC close approach of 2023 RL. Catalogue miss distance 18.8 LD · 7.22 × 10⁶ km. The curve is the geocentric path from 2029-07-30 to 2029-08-05, 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 |
|---|---|---|---|---|
| 2026-12-16 21:42:00 | Venus | 0.0966 AU | 37.6 LD | 8 km/s |
| 2029-08-02 02:26:00 | Earth | 0.0483 AU | 18.8 LD | 5 km/s |
| 2032-07-18 12:35:00 | Earth | 0.0771 AU | 30.0 LD | 6.6 km/s |
| 2032-11-13 12:57:00 | Earth | 0.2494 AU | 97.1 LD | 4 km/s |
| 2033-10-12 10:21:00 | Venus | 0.1066 AU | 41.5 LD | 8.2 km/s |
| 2035-07-17 01:23:00 | Earth | 0.1537 AU | 59.8 LD | 9.5 km/s |
| 2035-12-07 07:15:00 | Earth | 0.2958 AU | 115.1 LD | 7.3 km/s |
| 2038-07-18 19:12:00 | Earth | 0.2473 AU | 96.2 LD | 12.6 km/s |
| 2038-12-23 23:24:00 | Earth | 0.3278 AU | 127.6 LD | 9.4 km/s |
| 2040-08-26 16:10:00 | Venus | 0.0732 AU | 28.5 LD | 7.7 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