Where is it now
- Distance from Sun
- 1.165 AU
- True anomaly
- 208.12°
- Distance from Earth
- 1.366 AU
- As of
- 20 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
- 17h 35m 19s
- Declination
- -12° 19′ 41″
- Constellation
- Serpens
- Distance from Earth
- 1.37 AU
- Elongation from the Sun
- 56.27° — 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
- 0.907 AU
- Eccentricity
- 0.3762
- Inclination
- 13.32°
- Orbital period
- 315.4 days
- Perihelion
- 0.566 AU
- Aphelion
- 1.248 AU
- Longitude of ascending node
- 233.86°
- Argument of periapsis
- 228.08°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 6.0 LD
- 0.0155 AU
- Tisserand (Jupiter)
- 6.49
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 21
- Data arc
- 39 days
- First observed
- 25 May 2014
- Last observed
- 3 July 2014
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.4
Discovery & classification
Close approaches 149 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-06-01 15:48 UTC close approach of 2014 KM39. Catalogue miss distance 88.8 LD · 3.41 × 10⁷ km. The curve is the geocentric path from 2027-05-29 to 2027-06-04, 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 |
|---|---|---|---|---|
| 2027-06-01 15:48:00 | Earth | 0.2281 AU | 88.8 LD | 9.2 km/s |
| 2027-12-04 16:54:00 | Earth | 0.4011 AU | 156.1 LD | 16.4 km/s |
| 2028-08-25 20:24:00 | Earth | 0.3099 AU | 120.6 LD | 17.4 km/s |
| 2033-05-11 13:17:00 | Earth | 0.0161 AU | 6.3 LD | 11.9 km/s |
| 2034-01-03 07:56:00 | Earth | 0.4375 AU | 170.3 LD | 17.2 km/s |
| 2034-09-14 01:57:00 | Earth | 0.2259 AU | 87.9 LD | 10.4 km/s |
| 2039-02-09 22:15:00 | Venus | 0.1375 AU | 53.5 LD | 19.3 km/s |
| 2039-05-18 13:21:00 | Earth | 0.2393 AU | 93.1 LD | 18.6 km/s |
| 2040-02-02 02:12:00 | Earth | 0.4327 AU | 168.4 LD | 14.8 km/s |
| 2040-07-15 03:00:00 | Earth | 0.3112 AU | 121.1 LD | 8.8 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