2016 RU33 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.8 AU to 1.25 AU from the Sun; one orbit takes 378.4 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.236 AU
- True anomaly
- 197.1°
- Distance from Earth
- 1.843 AU
- As of
- 3 November 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
- 17h 17m 16s
- Declination
- -26° 02′ 20″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.85 AU
- Elongation from the Sun
- 38.59° — near the Sun — look low at dusk or dawn
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
- 1.024 AU
- Eccentricity
- 0.223
- Inclination
- 5.44°
- Orbital period
- 378.4 days
- Perihelion
- 0.795 AU
- Aphelion
- 1.252 AU
- Longitude of ascending node
- 344.66°
- Argument of periapsis
- 108.21°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 5.8 LD
- 0.0149 AU
- Tisserand (Jupiter)
- 5.943
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 28
- Data arc
- 7 days
- First observed
- 10 September 2016
- Last observed
- 17 September 2016
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 27.5
Discovery & classification
Close approaches 90 on record
Top-down view of the ecliptic, Earth at the centre, for the 2043-08-30 14:19 UTC close approach of 2016 RU33. Catalogue miss distance 156.2 LD · 6 × 10⁷ km. The curve is the geocentric path from 2043-08-27 to 2043-09-02, 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 |
|---|---|---|---|---|
| 2032-06-21 14:58:00 | Venus | 0.0991 AU | 38.6 LD | 4.8 km/s |
| 2043-08-30 14:19:00 | Earth | 0.4013 AU | 156.2 LD | 18.4 km/s |
| 2044-09-08 18:55:00 | Earth | 0.1813 AU | 70.6 LD | 11.9 km/s |
| 2045-09-16 23:03:00 | Earth | 0.0441 AU | 17.1 LD | 5.7 km/s |
| 2046-07-31 21:40:00 | Earth | 0.2144 AU | 83.5 LD | 5.4 km/s |
| 2047-06-22 05:40:00 | Earth | 0.258 AU | 100.4 LD | 5.9 km/s |
| 2048-01-27 00:25:00 | Earth | 0.1778 AU | 69.2 LD | 6.1 km/s |
| 2048-05-08 08:45:00 | Earth | 0.2104 AU | 81.9 LD | 4.8 km/s |
| 2049-03-25 23:02:00 | Earth | 0.0361 AU | 14.0 LD | 6.9 km/s |
| 2050-04-08 11:00:00 | Earth | 0.2389 AU | 93.0 LD | 13.5 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