2017 QG33 is an asteroid in the Aten orbit class. Its orbit takes it from 0.68 AU to 1.28 AU from the Sun; one orbit takes 354.4 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.739 AU
- True anomaly
- 50.32°
- Distance from Earth
- 1.622 AU
- As of
- 2 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
- 13h 23m 03s
- Declination
- -11° 22′ 04″
- Constellation
- Virgo
- Distance from Earth
- 1.62 AU
- Elongation from the Sun
- 17.43° — too close to the Sun to observe
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
- 0.98 AU
- Eccentricity
- 0.3108
- Inclination
- 8.54°
- Orbital period
- 354.4 days
- Perihelion
- 0.675 AU
- Aphelion
- 1.285 AU
- Longitude of ascending node
- 321.18°
- Argument of periapsis
- 168.07°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 47.2 LD
- 0.1213 AU
- Tisserand (Jupiter)
- 6.125
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 38
- Data arc
- 777 days
- First observed
- 23 August 2017
- Last observed
- 9 October 2019
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 23.5
Discovery & classification
Close approaches 173 on record
Top-down view of the ecliptic, Earth at the centre, for the 2043-06-11 13:45 UTC close approach of 2017 QG33. Catalogue miss distance 173.6 LD · 6.67 × 10⁷ km. The curve is the geocentric path from 2043-06-08 to 2043-06-14, 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 |
|---|---|---|---|---|
| 2030-08-04 02:32:00 | Venus | 0.1361 AU | 53.0 LD | 13.5 km/s |
| 2037-06-03 10:20:00 | Venus | 0.042 AU | 16.3 LD | 9.4 km/s |
| 2043-06-11 13:45:00 | Earth | 0.446 AU | 173.6 LD | 21.5 km/s |
| 2044-04-06 20:26:00 | Venus | 0.102 AU | 39.7 LD | 10.9 km/s |
| 2044-06-02 18:32:00 | Earth | 0.2826 AU | 110.0 LD | 16.1 km/s |
| 2045-05-26 22:00:00 | Earth | 0.1596 AU | 62.1 LD | 10.7 km/s |
| 2046-06-05 05:41:00 | Earth | 0.1851 AU | 72.0 LD | 6.5 km/s |
| 2047-03-20 06:30:00 | Earth | 0.271 AU | 105.5 LD | 9.8 km/s |
| 2047-07-07 12:06:00 | Earth | 0.2505 AU | 97.5 LD | 7.8 km/s |
| 2048-02-20 14:04:00 | Earth | 0.302 AU | 117.5 LD | 11.9 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