2017 QW17
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Where is it now
- Distance from Sun
- 1.051 AU
- True anomaly
- 141.74°
- Distance from Earth
- 1.019 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
- 18h 03m 25s
- Declination
- -25° 27′ 45″
- Constellation
- Sagittarius
- Distance from Earth
- 1.02 AU
- Elongation from the Sun
- 62.99° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
From your location
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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
- 0.888 AU
- Eccentricity
- 0.6452
- Inclination
- 12.34°
- Orbital period
- 305.6 days
- Perihelion
- 0.315 AU
- Aphelion
- 1.461 AU
- Longitude of ascending node
- 337.05°
- Argument of periapsis
- 208.73°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 17.2 LD
- 0.0442 AU
- Tisserand (Jupiter)
- 6.477
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 196
- Data arc
- 6.14 years
- First observed
- 20 August 2017
- Last observed
- 10 October 2023
- Residual RMS
- 0.48 ″
- Solution · Otto Matic
- 2 May 2026
Visual & observation
- Absolute magnitude (H)
- 21.63
Discovery & classification
Close approaches 180 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-08-19 04:37 UTC close approach of 2017 QW17. Catalogue miss distance 17.8 LD · 6.83 × 10⁶ km. The curve is the geocentric path from 2027-08-16 to 2027-08-22, 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 |
|---|---|---|---|---|
| 2027-08-19 04:37:00 | Earth | 0.0457 AU | 17.8 LD | 19.9 km/s |
| 2032-07-14 13:22:00 | Merc | 0.0693 AU | 27.0 LD | 33.8 km/s |
| 2032-07-14 13:22:00 | Mercury | 0.0693 AU | 27.0 LD | 33.8 km/s |
| 2032-08-21 10:30:00 | Earth | 0.1096 AU | 42.7 LD | 23.1 km/s |
| 2033-06-04 13:15:00 | Venus | 0.0914 AU | 35.6 LD | 22 km/s |
| 2034-03-16 08:11:00 | Merc | 0.0873 AU | 34.0 LD | 23.5 km/s |
| 2034-03-16 08:11:00 | Mercury | 0.0873 AU | 34.0 LD | 23.5 km/s |
| 2037-07-02 13:29:00 | Mercury | 0.0867 AU | 33.7 LD | 22.7 km/s |
| 2037-07-02 13:29:00 | Merc | 0.0867 AU | 33.7 LD | 22.7 km/s |
| 2039-03-03 11:12:00 | Merc | 0.0598 AU | 23.3 LD | 37.7 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