Where is it now
- Distance from Sun
- 0.602 AU
- True anomaly
- 61.41°
- Distance from Earth
- 1.239 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
- 12h 23m 27s
- Declination
- +14° 24′ 56″
- Constellation
- Coma Berenices
- Distance from Earth
- 1.25 AU
- Elongation from the Sun
- 28.6° — 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
- 0.788 AU
- Eccentricity
- 0.3373
- Inclination
- 34.11°
- Orbital period
- 255.7 days
- Perihelion
- 0.522 AU
- Aphelion
- 1.054 AU
- Longitude of ascending node
- 22.71°
- Argument of periapsis
- 37.75°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 17.6 LD
- 0.0451 AU
- Tisserand (Jupiter)
- 7.207
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 40
- Data arc
- 11.93 years
- First observed
- 17 May 2014
- Last observed
- 23 April 2026
- Residual RMS
- 0.31 ″
- Solution · Otto Matic
- 26 April 2026
Visual & observation
- Absolute magnitude (H)
- 19.72
Discovery & classification
Close approaches 22 on record
Top-down view of the ecliptic, Earth at the centre, for the 2033-04-11 15:05 UTC close approach of 2026 HG2. Catalogue miss distance 70.1 LD · 2.7 × 10⁷ km. The curve is the geocentric path from 2033-04-08 to 2033-04-14, 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 south 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 |
|---|---|---|---|---|
| 2033-04-11 15:05:00 | Earth | 0.1802 AU | 70.1 LD | 16.7 km/s |
| 2040-04-11 09:41:00 | Earth | 0.1857 AU | 72.2 LD | 16.7 km/s |
| 2047-04-12 03:03:00 | Earth | 0.1924 AU | 74.9 LD | 16.7 km/s |
| 2126-04-21 09:30:00 | Earth | 0.1895 AU | 73.8 LD | 21.1 km/s |
| 2133-04-20 16:52:00 | Earth | 0.1756 AU | 68.3 LD | 20.8 km/s |
| 2140-04-20 03:14:00 | Earth | 0.1664 AU | 64.7 LD | 20.6 km/s |
| 2147-04-20 15:08:00 | Earth | 0.158 AU | 61.5 LD | 20.4 km/s |
| 2154-04-20 06:23:00 | Earth | 0.1538 AU | 59.8 LD | 20.3 km/s |
| 2161-04-20 01:02:00 | Earth | 0.154 AU | 59.9 LD | 20.3 km/s |
| 2168-04-19 21:35:00 | Earth | 0.1558 AU | 60.6 LD | 20.4 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