Where is it now
- Distance from Sun
- 1.062 AU
- True anomaly
- 197.62°
- Distance from Earth
- 1.683 AU
- As of
- 21 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
- 16h 15m 53s
- Declination
- -15° 50′ 33″
- Constellation
- Scorpius
- Distance from Earth
- 1.68 AU
- Elongation from the Sun
- 36.37° — 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
- 0.923 AU
- Eccentricity
- 0.161
- Inclination
- 15.55°
- Orbital period
- 323.7 days
- Perihelion
- 0.774 AU
- Aphelion
- 1.071 AU
- Longitude of ascending node
- 246.25°
- Argument of periapsis
- 195.47°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 19.4 LD
- 0.0498 AU
- Tisserand (Jupiter)
- 6.441
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 87
- Data arc
- 8.1 years
- First observed
- 30 May 2013
- Last observed
- 5 July 2021
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 6 July 2021
Visual & observation
- Absolute magnitude (H)
- 23.51
Discovery & classification
Close approaches 131 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-05-14 18:01 UTC close approach of 2013 KH6. Catalogue miss distance 128.4 LD · 4.93 × 10⁷ km. The curve is the geocentric path from 2028-05-11 to 2028-05-17, 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 |
|---|---|---|---|---|
| 2028-05-14 18:01:00 | Earth | 0.3299 AU | 128.4 LD | 14.2 km/s |
| 2028-12-17 05:23:00 | Earth | 0.2257 AU | 87.9 LD | 10.7 km/s |
| 2029-06-22 04:14:00 | Earth | 0.2638 AU | 102.7 LD | 10.5 km/s |
| 2034-04-05 02:34:00 | Venus | 0.0734 AU | 28.6 LD | 12.2 km/s |
| 2036-05-15 20:45:00 | Earth | 0.1851 AU | 72.0 LD | 10.5 km/s |
| 2036-11-23 07:47:00 | Earth | 0.2073 AU | 80.7 LD | 10.8 km/s |
| 2037-06-30 17:55:00 | Earth | 0.3951 AU | 153.8 LD | 13.9 km/s |
| 2044-05-22 20:12:00 | Earth | 0.0608 AU | 23.6 LD | 8.4 km/s |
| 2044-10-29 15:44:00 | Earth | 0.2236 AU | 87.0 LD | 10.3 km/s |
| 2052-01-30 05:48:00 | Earth | 0.2796 AU | 108.8 LD | 8 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