Where is it now
- Distance from Sun
- 1.048 AU
- True anomaly
- 199.93°
- Distance from Earth
- 1.848 AU
- As of
- 19 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 11m 37s
- Declination
- -24° 20′ 23″
- Constellation
- Libra
- Distance from Earth
- 1.85 AU
- Elongation from the Sun
- 25.91° — 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
- 0.849 AU
- Eccentricity
- 0.2612
- Inclination
- 16.43°
- Orbital period
- 285.6 days
- Perihelion
- 0.627 AU
- Aphelion
- 1.07 AU
- Longitude of ascending node
- 34.67°
- Argument of periapsis
- 22.6°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 12.9 LD
- 0.0331 AU
- Tisserand (Jupiter)
- 6.879
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 37
- Data arc
- 7 days
- First observed
- 26 April 2006
- Last observed
- 3 May 2006
- Residual RMS
- 0.39 ″
- Solution · Otto Matic
- 14 April 2021
Visual & observation
- Absolute magnitude (H)
- 23.6
Discovery & classification
Close approaches 57 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-11-28 22:03 UTC close approach of 2006 HV50. Catalogue miss distance 146.7 LD · 5.64 × 10⁷ km. The curve is the geocentric path from 2027-11-25 to 2027-12-01, 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 |
|---|---|---|---|---|
| 2027-11-28 22:03:00 | Earth | 0.3769 AU | 146.7 LD | 15 km/s |
| 2028-06-04 15:37:00 | Earth | 0.4514 AU | 175.7 LD | 17.6 km/s |
| 2028-08-14 20:03:00 | Venus | 0.0729 AU | 28.4 LD | 12.2 km/s |
| 2031-04-18 12:03:00 | Earth | 0.1237 AU | 48.2 LD | 11.5 km/s |
| 2035-06-01 02:05:00 | Earth | 0.286 AU | 111.3 LD | 11.7 km/s |
| 2037-03-17 22:50:00 | Venus | 0.1195 AU | 46.5 LD | 14.4 km/s |
| 2038-04-21 05:07:00 | Earth | 0.3332 AU | 129.7 LD | 17.2 km/s |
| 2049-04-20 21:04:00 | Earth | 0.0396 AU | 15.4 LD | 9.7 km/s |
| 2053-06-04 21:02:00 | Earth | 0.3592 AU | 139.8 LD | 14.2 km/s |
| 2056-04-18 14:09:00 | Earth | 0.2441 AU | 95.0 LD | 14.7 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