Where is it now
- Distance from Sun
- 0.852 AU
- True anomaly
- 103.31°
- Distance from Earth
- 0.981 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
- 10h 44m 06s
- Declination
- +15° 16′ 07″
- Constellation
- Leo
- Distance from Earth
- 0.98 AU
- Elongation from the Sun
- 51.08° — near the Sun — look low at dusk or dawn
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.875 AU
- Eccentricity
- 0.3096
- Inclination
- 9.66°
- Orbital period
- 299 days
- Perihelion
- 0.604 AU
- Aphelion
- 1.146 AU
- Longitude of ascending node
- 37.91°
- Argument of periapsis
- 309.89°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 3.6 LD
- 0.0093 AU
- Tisserand (Jupiter)
- 6.715
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 46
- Data arc
- 17 days
- First observed
- 12 April 2022
- Last observed
- 29 April 2022
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 29 April 2022
Visual & observation
- Absolute magnitude (H)
- 24.7
Discovery & classification
Close approaches 170 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-10 20:14 UTC close approach of 2022 HA1. Catalogue miss distance 186.4 LD · 7.17 × 10⁷ km. The curve is the geocentric path from 2027-04-07 to 2027-04-13, 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 |
|---|---|---|---|---|
| 2027-04-10 20:14:00 | Earth | 0.479 AU | 186.4 LD | 24.3 km/s |
| 2030-10-16 02:14:00 | Earth | 0.3692 AU | 143.7 LD | 13.4 km/s |
| 2031-04-24 00:52:00 | Earth | 0.0652 AU | 25.4 LD | 8.3 km/s |
| 2035-01-12 03:35:00 | Earth | 0.1685 AU | 65.6 LD | 10.9 km/s |
| 2035-08-14 17:01:00 | Earth | 0.4132 AU | 160.8 LD | 13.5 km/s |
| 2036-04-11 17:57:00 | Earth | 0.4395 AU | 171.1 LD | 23 km/s |
| 2039-10-23 15:04:00 | Earth | 0.3538 AU | 137.7 LD | 12.7 km/s |
| 2040-04-17 07:28:00 | Earth | 0.1155 AU | 45.0 LD | 7.5 km/s |
| 2044-01-15 09:50:00 | Earth | 0.2027 AU | 78.9 LD | 13 km/s |
| 2044-08-22 12:13:00 | Earth | 0.4174 AU | 162.4 LD | 14.1 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