Where is it now
- Distance from Sun
- 0.627 AU
- True anomaly
- 337.31°
- Distance from Earth
- 0.716 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
- 11h 14m 47s
- Declination
- -06° 56′ 10″
- Constellation
- Crater
- Distance from Earth
- 0.72 AU
- Elongation from the Sun
- 38.83° — 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
- 0.952 AU
- Eccentricity
- 0.3545
- Inclination
- 19.89°
- Orbital period
- 339.3 days
- Perihelion
- 0.615 AU
- Aphelion
- 1.29 AU
- Longitude of ascending node
- 216.95°
- Argument of periapsis
- 241.25°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.7 LD
- 0.0019 AU
- Tisserand (Jupiter)
- 6.218
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 56
- Data arc
- 10 days
- First observed
- 28 April 2023
- Last observed
- 8 May 2023
- Residual RMS
- 0.46 ″
- Solution · Otto Matic
- 5 March 2024
Visual & observation
- Absolute magnitude (H)
- 26.02
Discovery & classification
Close approaches 31 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-05-14 20:42 UTC close approach of 2023 HX6. Catalogue miss distance 170.8 LD · 6.57 × 10⁷ km. The curve is the geocentric path from 2035-05-11 to 2035-05-17, 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 |
|---|---|---|---|---|
| 2035-05-14 20:42:00 | Earth | 0.439 AU | 170.8 LD | 25.5 km/s |
| 2036-01-17 12:50:00 | Venus | 0.0732 AU | 28.5 LD | 19.7 km/s |
| 2036-04-27 19:31:00 | Earth | 0.0159 AU | 6.2 LD | 14.3 km/s |
| 2037-02-16 22:55:00 | Earth | 0.4171 AU | 162.3 LD | 10.1 km/s |
| 2037-05-20 19:21:00 | Earth | 0.3585 AU | 139.5 LD | 10.6 km/s |
| 2037-11-27 21:41:00 | Venus | 0.0432 AU | 16.8 LD | 16.8 km/s |
| 2037-12-13 14:44:00 | Earth | 0.4106 AU | 159.8 LD | 16 km/s |
| 2038-10-21 05:12:00 | Earth | 0.2545 AU | 99.0 LD | 14.4 km/s |
| 2039-09-09 23:13:00 | Earth | 0.325 AU | 126.5 LD | 19.3 km/s |
| 2039-10-12 00:28:00 | Venus | 0.1486 AU | 57.8 LD | 15.3 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