Where is it now
- Distance from Sun
- 1.118 AU
- True anomaly
- 201.46°
- Distance from Earth
- 0.56 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
- 16h 22m 12s
- Declination
- +72° 35′ 46″
- Constellation
- Ursa Minor
- Distance from Earth
- 0.56 AU
- Elongation from the Sun
- 87.13° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.874 AU
- Eccentricity
- 0.3207
- Inclination
- 30.47°
- Orbital period
- 298.5 days
- Perihelion
- 0.594 AU
- Aphelion
- 1.154 AU
- Longitude of ascending node
- 287.45°
- Argument of periapsis
- 262.07°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 65.4 LD
- 0.1682 AU
- Tisserand (Jupiter)
- 6.622
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 47
- Data arc
- 4.97 years
- First observed
- 27 August 2021
- Last observed
- 15 August 2026
- Residual RMS
- 0.51 ″
- Solution · Otto Matic
- 16 August 2026
Visual & observation
- Absolute magnitude (H)
- 20.85
Discovery & classification
Close approaches 64 on record
Top-down view of the ecliptic, Earth at the centre, for the 2030-07-21 11:45 UTC close approach of 2021 QF1. Catalogue miss distance 66.2 LD · 2.54 × 10⁷ km. The curve is the geocentric path from 2030-07-18 to 2030-07-24, 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 north 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 |
|---|---|---|---|---|
| 2027-03-29 13:46:00 | Venus | 0.0773 AU | 30.1 LD | 23.3 km/s |
| 2029-09-12 03:25:00 | Venus | 0.0704 AU | 27.4 LD | 21.9 km/s |
| 2030-07-21 11:45:00 | Earth | 0.17 AU | 66.2 LD | 19 km/s |
| 2032-02-27 00:59:00 | Venus | 0.1091 AU | 42.5 LD | 20.7 km/s |
| 2039-07-17 07:55:00 | Earth | 0.1719 AU | 66.9 LD | 18.1 km/s |
| 2041-09-17 21:36:00 | Venus | 0.1165 AU | 45.3 LD | 20.8 km/s |
| 2044-03-03 09:22:00 | Venus | 0.0593 AU | 23.1 LD | 21.9 km/s |
| 2046-08-17 16:18:00 | Venus | 0.0425 AU | 16.6 LD | 23.2 km/s |
| 2048-07-12 03:22:00 | Earth | 0.1939 AU | 75.5 LD | 17.4 km/s |
| 2049-01-30 15:24:00 | Venus | 0.0932 AU | 36.3 LD | 25 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