Where is it now
- Distance from Sun
- 1.276 AU
- True anomaly
- 158.5°
- Distance from Earth
- 1.6 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
- 11h 45m 21s
- Declination
- +33° 04′ 49″
- Constellation
- Ursa Major
- Distance from Earth
- 1.6 AU
- Elongation from the Sun
- 53.07° — 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
- 0.931 AU
- Eccentricity
- 0.4477
- Inclination
- 40.51°
- Orbital period
- 328 days
- Perihelion
- 0.514 AU
- Aphelion
- 1.348 AU
- Longitude of ascending node
- 358.45°
- Argument of periapsis
- 313.72°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 25.3 LD
- 0.065 AU
- Tisserand (Jupiter)
- 6.165
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 102
- Data arc
- 26.06 years
- First observed
- 12 March 2000
- Last observed
- 5 April 2026
- Residual RMS
- 0.56 ″
- Solution · Otto Matic
- 5 April 2026
Visual & observation
- Absolute magnitude (H)
- 20.67
Discovery & classification
Also known as 2026 DU11
Close approaches 25 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-03-24 02:55 UTC close approach of 2000 EZ106. Catalogue miss distance 71.8 LD · 2.76 × 10⁷ km. The curve is the geocentric path from 2035-03-21 to 2035-03-27, 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 |
|---|---|---|---|---|
| 2035-03-24 02:55:00 | Earth | 0.1846 AU | 71.8 LD | 20.6 km/s |
| 2044-03-22 20:19:00 | Earth | 0.1003 AU | 39.0 LD | 21.8 km/s |
| 2053-03-21 15:30:00 | Earth | 0.0674 AU | 26.2 LD | 23.3 km/s |
| 2062-03-19 14:23:00 | Earth | 0.1335 AU | 51.9 LD | 25.3 km/s |
| 2088-03-23 10:25:00 | Earth | 0.1426 AU | 55.5 LD | 21.1 km/s |
| 2097-03-22 16:15:00 | Earth | 0.0722 AU | 28.1 LD | 22.5 km/s |
| 2106-03-22 02:51:00 | Earth | 0.0917 AU | 35.7 LD | 24.2 km/s |
| 2115-03-19 17:29:00 | Earth | 0.177 AU | 68.9 LD | 26.4 km/s |
| 2132-03-24 16:59:00 | Earth | 0.191 AU | 74.3 LD | 20.6 km/s |
| 2141-03-24 13:07:00 | Earth | 0.1054 AU | 41.0 LD | 21.7 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