Where is it now
- Distance from Sun
- 1.055 AU
- True anomaly
- 177.6°
- Distance from Earth
- 1.083 AU
- As of
- 16 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
- 17h 37m 04s
- Declination
- -24° 32′ 50″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.09 AU
- Elongation from the Sun
- 60.71° — well clear of the Sun
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
- 0.811 AU
- Eccentricity
- 0.3012
- Inclination
- 6.66°
- Orbital period
- 266.8 days
- Perihelion
- 0.567 AU
- Aphelion
- 1.055 AU
- Longitude of ascending node
- 330.99°
- Argument of periapsis
- 171.04°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 11.7 LD
- 0.0301 AU
- Tisserand (Jupiter)
- 7.163
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 115
- Data arc
- 24 days
- First observed
- 14 August 2024
- Last observed
- 7 September 2024
- Residual RMS
- 0.34 ″
- Solution · Otto Matic
- 11 September 2024
Visual & observation
- Absolute magnitude (H)
- 24.87
Discovery & classification
Close approaches 176 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-03-16 21:14 UTC close approach of 2024 QU. Catalogue miss distance 157.8 LD · 6.07 × 10⁷ km. The curve is the geocentric path from 2027-03-13 to 2027-03-19, 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 |
|---|---|---|---|---|
| 2027-03-16 21:14:00 | Earth | 0.4054 AU | 157.8 LD | 14 km/s |
| 2027-09-06 21:51:00 | Earth | 0.4201 AU | 163.5 LD | 19.6 km/s |
| 2029-07-28 04:40:00 | Earth | 0.4797 AU | 186.7 LD | 21.3 km/s |
| 2030-01-23 15:57:00 | Earth | 0.4121 AU | 160.4 LD | 14.8 km/s |
| 2032-07-21 20:33:00 | Earth | 0.0767 AU | 29.8 LD | 7.5 km/s |
| 2032-11-16 16:54:00 | Earth | 0.2963 AU | 115.3 LD | 5.1 km/s |
| 2033-09-01 11:34:00 | Venus | 0.1087 AU | 42.3 LD | 9.2 km/s |
| 2035-04-15 22:04:00 | Earth | 0.3607 AU | 140.4 LD | 10.2 km/s |
| 2035-09-14 12:18:00 | Earth | 0.1962 AU | 76.4 LD | 12.3 km/s |
| 2038-02-19 11:45:00 | Earth | 0.4197 AU | 163.3 LD | 15.5 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