Where is it now
- Distance from Sun
- 0.787 AU
- True anomaly
- 281.4°
- Distance from Earth
- 1.167 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
- 16h 21m 01s
- Declination
- -32° 05′ 53″
- Constellation
- Scorpius
- Distance from Earth
- 1.16 AU
- Elongation from the Sun
- 41.74° — 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
- 0.901 AU
- Eccentricity
- 0.2801
- Inclination
- 18.14°
- Orbital period
- 312.6 days
- Perihelion
- 0.649 AU
- Aphelion
- 1.154 AU
- Longitude of ascending node
- 69.76°
- Argument of periapsis
- 317.03°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 9.4 LD
- 0.024 AU
- Tisserand (Jupiter)
- 6.531
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 97
- Data arc
- 12.17 years
- First observed
- 17 March 2010
- Last observed
- 18 May 2022
- Residual RMS
- 0.35 ″
- Solution · Otto Matic
- 1 September 2023
Physical properties
- Mean radius
- 0.16 km
Visual & observation
- Geometric albedo
- 0.034
- Absolute magnitude (H)
- 21.09
Discovery & classification
Also known as 2010 FA36 · 2010 FQ32
Close approaches 170 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-01-22 05:20 UTC close approach of 2016 KL1. Catalogue miss distance 104.8 LD · 4.03 × 10⁷ km. The curve is the geocentric path from 2027-01-19 to 2027-01-25, 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 |
|---|---|---|---|---|
| 2027-01-22 05:20:00 | Earth | 0.2692 AU | 104.8 LD | 13.1 km/s |
| 2027-10-02 04:05:00 | Earth | 0.412 AU | 160.4 LD | 13.4 km/s |
| 2028-05-28 12:13:00 | Earth | 0.2789 AU | 108.6 LD | 18.2 km/s |
| 2033-01-14 15:52:00 | Earth | 0.2584 AU | 100.6 LD | 12.9 km/s |
| 2033-09-23 14:44:00 | Earth | 0.416 AU | 161.9 LD | 12.6 km/s |
| 2034-05-27 03:49:00 | Earth | 0.3328 AU | 129.5 LD | 19.7 km/s |
| 2039-01-07 12:25:00 | Earth | 0.2537 AU | 98.7 LD | 12.9 km/s |
| 2039-04-08 12:54:00 | Earth | 0.3255 AU | 126.7 LD | 8.8 km/s |
| 2039-09-15 01:15:00 | Earth | 0.416 AU | 161.9 LD | 11.4 km/s |
| 2039-10-28 16:07:00 | Venus | 0.0946 AU | 36.8 LD | 15.2 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)
- visual properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB