Where is it now
- Distance from Sun
- 0.685 AU
- True anomaly
- 113.66°
- Distance from Earth
- 0.857 AU
- As of
- 15 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
- 11h 05m 52s
- Declination
- +16° 29′ 21″
- Constellation
- Leo
- Distance from Earth
- 0.86 AU
- Elongation from the Sun
- 43.1° — near the Sun — look low at dusk or dawn
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.714 AU
- Eccentricity
- 0.4712
- Inclination
- 23.85°
- Orbital period
- 220.5 days
- Perihelion
- 0.378 AU
- Aphelion
- 1.051 AU
- Longitude of ascending node
- 290.11°
- Argument of periapsis
- 33.18°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 18.5 LD
- 0.0476 AU
- Tisserand (Jupiter)
- 7.883
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 84
- Data arc
- 15.09 years
- First observed
- 16 January 2010
- Last observed
- 16 February 2025
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 16 February 2025
Physical properties
- Mean radius
- 0.11 km
Visual & observation
- Geometric albedo
- 0.103
- Absolute magnitude (H)
- 21.4
Discovery & classification
Also known as 2010 BY20
Close approaches 171 on record
Top-down view of the ecliptic, Earth at the centre, for the 2048-01-18 03:55 UTC close approach of 2016 DL. Catalogue miss distance 53.1 LD · 2.04 × 10⁷ km. The curve is the geocentric path from 2048-01-15 to 2048-01-21, 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 |
|---|---|---|---|---|
| 2048-01-18 03:55:00 | Earth | 0.1364 AU | 53.1 LD | 13.7 km/s |
| 2051-01-15 08:26:00 | Earth | 0.0593 AU | 23.1 LD | 15 km/s |
| 2053-05-16 20:36:00 | Venus | 0.1205 AU | 46.9 LD | 23.9 km/s |
| 2053-12-26 23:45:00 | Venus | 0.1072 AU | 41.7 LD | 21.2 km/s |
| 2054-01-15 17:08:00 | Earth | 0.0778 AU | 30.3 LD | 17.1 km/s |
| 2054-08-09 08:36:00 | Venus | 0.1376 AU | 53.6 LD | 19.3 km/s |
| 2057-01-17 21:27:00 | Earth | 0.1703 AU | 66.3 LD | 19.9 km/s |
| 2058-01-19 01:43:00 | Merc | 0.0877 AU | 34.1 LD | 32.1 km/s |
| 2058-01-19 01:43:00 | Mercury | 0.0877 AU | 34.1 LD | 32.1 km/s |
| 2059-04-05 08:25:00 | Merc | 0.0678 AU | 26.4 LD | 30.6 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