Where is it now
- Distance from Sun
- 1.166 AU
- True anomaly
- 138.35°
- Distance from Earth
- 1.7 AU
- As of
- 24 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 40m 45s
- Declination
- +12° 31′ 42″
- Constellation
- Leo
- Distance from Earth
- 1.7 AU
- Elongation from the Sun
- 41.87° — 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
- 0.971 AU
- Eccentricity
- 0.4201
- Inclination
- 14.11°
- Orbital period
- 349.5 days
- Perihelion
- 0.563 AU
- Aphelion
- 1.379 AU
- Longitude of ascending node
- 51.21°
- Argument of periapsis
- 305.9°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 9.0 LD
- 0.0232 AU
- Tisserand (Jupiter)
- 6.119
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 151
- Data arc
- 4.17 years
- First observed
- 8 March 2022
- Last observed
- 10 May 2026
- Residual RMS
- 0.27 ″
- Solution · Otto Matic
- 26 August 2026
Visual & observation
- Absolute magnitude (H)
- 22.8
Discovery & classification
Close approaches 50 on record
Top-down view of the ecliptic, Earth at the centre, for the 2048-05-15 11:47 UTC close approach of 2025 HF12. Catalogue miss distance 20.7 LD · 7.95 × 10⁶ km. The curve is the geocentric path from 2048-05-12 to 2048-05-18, 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 |
|---|---|---|---|---|
| 2048-05-15 11:47:00 | Earth | 0.0532 AU | 20.7 LD | 15.8 km/s |
| 2068-09-22 21:07:00 | Venus | 0.1411 AU | 54.9 LD | 20.8 km/s |
| 2069-05-14 15:50:00 | Earth | 0.1888 AU | 73.5 LD | 10.6 km/s |
| 2070-05-15 15:47:00 | Earth | 0.0676 AU | 26.3 LD | 16.2 km/s |
| 2077-05-02 13:55:00 | Venus | 0.1069 AU | 41.6 LD | 19 km/s |
| 2085-12-10 15:10:00 | Venus | 0.0844 AU | 32.8 LD | 17.7 km/s |
| 2091-05-15 07:41:00 | Earth | 0.1876 AU | 73.0 LD | 10.6 km/s |
| 2092-05-15 06:25:00 | Earth | 0.0684 AU | 26.6 LD | 16.2 km/s |
| 2094-07-21 09:05:00 | Venus | 0.0737 AU | 28.7 LD | 17 km/s |
| 2103-03-02 12:38:00 | Venus | 0.0688 AU | 26.8 LD | 16.6 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