Where is it now
- Distance from Sun
- 0.931 AU
- True anomaly
- 90.2°
- Distance from Earth
- 0.567 AU
- As of
- 22 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
- 09h 35m 57s
- Declination
- +11° 16′ 15″
- Constellation
- Leo
- Distance from Earth
- 0.57 AU
- Elongation from the Sun
- 66.83° — well clear of the Sun
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.
Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.
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
- 0.936 AU
- Eccentricity
- 0.0749
- Inclination
- 1.83°
- Orbital period
- 330.9 days
- Perihelion
- 0.866 AU
- Aphelion
- 1.006 AU
- Longitude of ascending node
- 136.36°
- Argument of periapsis
- 196.75°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.9 LD
- 0.0126 AU
- Tisserand (Jupiter)
- 6.403
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 25
- Data arc
- 3 days
- First observed
- 6 February 2026
- Last observed
- 9 February 2026
- Residual RMS
- 0.33 ″
- Solution · Otto Matic
- 9 February 2026
Visual & observation
- Absolute magnitude (H)
- 28.94
Discovery & classification
Close approaches 30 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-09-09 12:05 UTC close approach of 2026 CQ. Catalogue miss distance 54.8 LD · 2.11 × 10⁷ km. The curve is the geocentric path from 2035-09-06 to 2035-09-12, 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 |
|---|---|---|---|---|
| 2035-09-09 12:05:00 | Earth | 0.1409 AU | 54.8 LD | 3.7 km/s |
| 2036-03-28 12:37:00 | Earth | 0.1687 AU | 65.7 LD | 7.1 km/s |
| 2036-07-13 01:24:00 | Venus | 0.1458 AU | 56.7 LD | 1.7 km/s |
| 2045-01-02 22:13:00 | Earth | 0.0852 AU | 33.2 LD | 4.6 km/s |
| 2045-06-26 03:20:00 | Earth | 0.1236 AU | 48.1 LD | 3 km/s |
| 2053-10-11 14:41:00 | Venus | 0.1448 AU | 56.4 LD | 1.7 km/s |
| 2065-03-24 22:39:00 | Earth | 0.1822 AU | 70.9 LD | 7.6 km/s |
| 2073-12-29 20:06:00 | Earth | 0.0893 AU | 34.8 LD | 4.7 km/s |
| 2093-09-03 08:53:00 | Earth | 0.1402 AU | 54.5 LD | 3.6 km/s |
| 2094-03-21 17:26:00 | Earth | 0.1603 AU | 62.4 LD | 6.9 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