Where is it now
- Distance from Sun
- 0.859 AU
- True anomaly
- 258.2°
- Distance from Earth
- 1.419 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
- 15h 44m 50s
- Declination
- -35° 05′ 23″
- Constellation
- Lupus
- Distance from Earth
- 1.41 AU
- Elongation from the Sun
- 36.62° — near the Sun — look low at dusk or dawn
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
- 0.897 AU
- Eccentricity
- 0.326
- Inclination
- 26.43°
- Orbital period
- 310.2 days
- Perihelion
- 0.604 AU
- Aphelion
- 1.189 AU
- Longitude of ascending node
- 36.89°
- Argument of periapsis
- 353.65°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 68.3 LD
- 0.1755 AU
- Tisserand (Jupiter)
- 6.506
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 55
- Data arc
- 33 days
- First observed
- 11 April 2022
- Last observed
- 14 May 2022
- Residual RMS
- 0.53 ″
- Solution · Otto Matic
- 14 May 2022
Visual & observation
- Absolute magnitude (H)
- 22.65
Discovery & classification
Close approaches 183 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-02 11:22 UTC close approach of 2022 HU1. Catalogue miss distance 132.1 LD · 5.08 × 10⁷ km. The curve is the geocentric path from 2027-03-30 to 2027-04-05, 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 |
|---|---|---|---|---|
| 2027-04-02 11:22:00 | Earth | 0.3394 AU | 132.1 LD | 15.4 km/s |
| 2027-10-19 03:59:00 | Earth | 0.3983 AU | 155.0 LD | 21.7 km/s |
| 2028-05-14 21:32:00 | Earth | 0.2833 AU | 110.2 LD | 16.6 km/s |
| 2028-08-22 22:52:00 | Venus | 0.1315 AU | 51.2 LD | 18.7 km/s |
| 2032-12-15 11:04:00 | Earth | 0.4162 AU | 162.0 LD | 18.6 km/s |
| 2033-04-20 13:11:00 | Earth | 0.2103 AU | 81.8 LD | 13.8 km/s |
| 2033-09-13 17:36:00 | Earth | 0.4531 AU | 176.4 LD | 19.2 km/s |
| 2035-06-17 11:26:00 | Venus | 0.1479 AU | 57.6 LD | 19 km/s |
| 2038-03-26 09:24:00 | Earth | 0.4703 AU | 183.0 LD | 19.3 km/s |
| 2038-11-10 14:21:00 | Earth | 0.385 AU | 149.8 LD | 21.5 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