Where is it now
- Distance from Sun
- 0.809 AU
- True anomaly
- 276.37°
- Distance from Earth
- 1.724 AU
- As of
- 22 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 51m 25s
- Declination
- -06° 29′ 24″
- Constellation
- Virgo
- Distance from Earth
- 1.72 AU
- Elongation from the Sun
- 15.31° — too close to the Sun to observe
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
- 0.947 AU
- Eccentricity
- 0.3376
- Inclination
- 3.77°
- Orbital period
- 336.5 days
- Perihelion
- 0.627 AU
- Aphelion
- 1.266 AU
- Longitude of ascending node
- 324.63°
- Argument of periapsis
- 294.02°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.0 LD
- 0.0026 AU
- Tisserand (Jupiter)
- 6.297
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 23
- Data arc
- 10 days
- First observed
- 31 January 2022
- Last observed
- 10 February 2022
- Residual RMS
- 0.3 ″
- Solution · Otto Matic
- 28 July 2026
Visual & observation
- Absolute magnitude (H)
- 25.95
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 54 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-10-26 02:01 UTC close approach of 2022 BU6. Catalogue miss distance 76.1 LD · 2.93 × 10⁷ km. The curve is the geocentric path from 2031-10-23 to 2031-10-29, 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 |
|---|---|---|---|---|
| 2027-12-06 17:45:00 | Venus | 0.0632 AU | 24.6 LD | 13 km/s |
| 2029-10-09 19:37:00 | Venus | 0.0525 AU | 20.4 LD | 12.4 km/s |
| 2031-08-14 15:44:00 | Venus | 0.05 AU | 19.5 LD | 12.2 km/s |
| 2031-10-26 02:01:00 | Earth | 0.1956 AU | 76.1 LD | 7.1 km/s |
| 2033-06-19 03:54:00 | Venus | 0.0541 AU | 21.1 LD | 12.5 km/s |
| 2034-02-10 16:15:00 | Earth | 0.0498 AU | 19.4 LD | 12.2 km/s |
| 2035-04-24 23:35:00 | Venus | 0.0603 AU | 23.5 LD | 12.9 km/s |
| 2037-02-27 23:55:00 | Venus | 0.0709 AU | 27.6 LD | 13.4 km/s |
| 2039-01-04 11:22:00 | Venus | 0.0899 AU | 35.0 LD | 14.4 km/s |
| 2040-11-10 04:16:00 | Venus | 0.1155 AU | 44.9 LD | 15.7 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