Where is it now
- Distance from Sun
- 0.94 AU
- True anomaly
- 133.02°
- Distance from Earth
- 1.936 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
- 13h 35m 08s
- Declination
- -09° 15′ 26″
- Constellation
- Virgo
- Distance from Earth
- 1.94 AU
- Elongation from the Sun
- 1.43° — 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
- 0.815 AU
- Eccentricity
- 0.4304
- Inclination
- 2.67°
- Orbital period
- 268.8 days
- Perihelion
- 0.464 AU
- Aphelion
- 1.166 AU
- Longitude of ascending node
- 55.04°
- Argument of periapsis
- 18.02°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 6.1 LD
- 0.0158 AU
- Tisserand (Jupiter)
- 7.097
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 113
- Data arc
- 17.15 years
- First observed
- 28 April 2000
- Last observed
- 22 June 2017
- Residual RMS
- 0.54 ″
- Solution · Otto Matic
- 14 April 2021
Physical properties
- Rotation period
- 0.22 hours
Visual & observation
- Absolute magnitude (H)
- 23.7
Discovery & classification
Close approaches 208 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-05-08 20:47 UTC close approach of 2000 HB24. Catalogue miss distance 43.1 LD · 1.66 × 10⁷ km. The curve is the geocentric path from 2028-05-05 to 2028-05-11, 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 |
|---|---|---|---|---|
| 2028-05-08 20:47:00 | Earth | 0.1108 AU | 43.1 LD | 8.5 km/s |
| 2028-09-28 01:33:00 | Earth | 0.4256 AU | 165.6 LD | 12.5 km/s |
| 2031-02-03 08:08:00 | Earth | 0.4328 AU | 168.4 LD | 13.7 km/s |
| 2031-07-01 22:45:00 | Earth | 0.1024 AU | 39.8 LD | 8.6 km/s |
| 2032-08-06 19:12:00 | Venus | 0.0768 AU | 29.9 LD | 19.1 km/s |
| 2034-07-09 06:25:00 | Earth | 0.1953 AU | 76.0 LD | 16.7 km/s |
| 2035-05-03 11:11:00 | Venus | 0.1093 AU | 42.5 LD | 10.2 km/s |
| 2036-04-13 09:17:00 | Venus | 0.0155 AU | 6.0 LD | 15.8 km/s |
| 2036-05-07 05:19:00 | Earth | 0.4222 AU | 164.3 LD | 24.2 km/s |
| 2037-06-27 06:26:00 | Earth | 0.4913 AU | 191.2 LD | 26.4 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB