Where is it now
- Distance from Sun
- 0.918 AU
- True anomaly
- 240.38°
- Distance from Earth
- 1.24 AU
- As of
- 19 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 51m 46s
- Declination
- -13° 11′ 14″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.24 AU
- Elongation from the Sun
- 46.79° — near the Sun — look low at dusk or dawn
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
- 0.858 AU
- Eccentricity
- 0.2717
- Inclination
- 12.58°
- Orbital period
- 290.1 days
- Perihelion
- 0.625 AU
- Aphelion
- 1.091 AU
- Longitude of ascending node
- 217.4°
- Argument of periapsis
- 208.13°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 11.7 LD
- 0.0302 AU
- Tisserand (Jupiter)
- 6.83
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 60
- Data arc
- 18 days
- First observed
- 30 April 2023
- Last observed
- 18 May 2023
- Residual RMS
- 0.53 ″
- Solution · Otto Matic
- 2 June 2023
Visual & observation
- Absolute magnitude (H)
- 24.73
Discovery & classification
Close approaches 167 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-05-19 12:52 UTC close approach of 2023 HQ7. Catalogue miss distance 53.7 LD · 2.06 × 10⁷ km. The curve is the geocentric path from 2027-05-16 to 2027-05-22, 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 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 |
|---|---|---|---|---|
| 2027-05-19 12:52:00 | Earth | 0.138 AU | 53.7 LD | 7.6 km/s |
| 2031-01-13 08:11:00 | Earth | 0.3579 AU | 139.3 LD | 10.1 km/s |
| 2031-06-21 15:52:00 | Earth | 0.211 AU | 82.1 LD | 8.8 km/s |
| 2031-09-12 17:45:00 | Venus | 0.1386 AU | 53.9 LD | 14.6 km/s |
| 2034-12-18 00:34:00 | Earth | 0.3744 AU | 145.7 LD | 13.1 km/s |
| 2035-06-27 08:45:00 | Earth | 0.3234 AU | 125.8 LD | 13.9 km/s |
| 2037-04-13 09:01:00 | Venus | 0.0871 AU | 33.9 LD | 12.6 km/s |
| 2038-04-29 15:09:00 | Earth | 0.4691 AU | 182.6 LD | 21.5 km/s |
| 2038-11-24 20:05:00 | Earth | 0.37 AU | 144.0 LD | 14.2 km/s |
| 2039-06-22 00:51:00 | Earth | 0.476 AU | 185.3 LD | 19.6 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