Where is it now
- Distance from Sun
- 0.569 AU
- True anomaly
- 301.51°
- Distance from Earth
- 0.841 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 02m 32s
- Declination
- -23° 40′ 38″
- Constellation
- Scorpius
- Distance from Earth
- 0.83 AU
- Elongation from the Sun
- 34.63° — 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
- 0.917 AU
- Eccentricity
- 0.4746
- Inclination
- 19.8°
- Orbital period
- 320.6 days
- Perihelion
- 0.482 AU
- Aphelion
- 1.352 AU
- Longitude of ascending node
- 344°
- Argument of periapsis
- 44.6°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 17.2 LD
- 0.0441 AU
- Tisserand (Jupiter)
- 6.371
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 171
- Data arc
- 7.07 years
- First observed
- 1 March 2019
- Last observed
- 25 March 2026
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 5 May 2026
Visual & observation
- Absolute magnitude (H)
- 22.79
Discovery & classification
Close approaches 51 on record
Top-down view of the ecliptic, Earth at the centre, for the 2033-03-02 15:24 UTC close approach of 2026 EC. Catalogue miss distance 64.2 LD · 2.47 × 10⁷ km. The curve is the geocentric path from 2033-02-27 to 2033-03-05, 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 |
|---|---|---|---|---|
| 2028-07-17 18:42:00 | Venus | 0.1463 AU | 56.9 LD | 19 km/s |
| 2033-03-02 15:24:00 | Earth | 0.1649 AU | 64.2 LD | 20.8 km/s |
| 2034-09-07 06:07:00 | Venus | 0.1295 AU | 50.4 LD | 19.8 km/s |
| 2040-10-28 12:26:00 | Venus | 0.1256 AU | 48.9 LD | 21 km/s |
| 2046-12-20 01:10:00 | Venus | 0.1371 AU | 53.3 LD | 22.6 km/s |
| 2055-02-28 23:18:00 | Earth | 0.1586 AU | 61.7 LD | 13.6 km/s |
| 2062-02-26 20:49:00 | Earth | 0.0589 AU | 22.9 LD | 15.6 km/s |
| 2069-02-28 06:05:00 | Earth | 0.0805 AU | 31.3 LD | 18.3 km/s |
| 2074-05-10 12:29:00 | Venus | 0.135 AU | 52.5 LD | 22.1 km/s |
| 2076-03-03 16:32:00 | Earth | 0.1966 AU | 76.5 LD | 21.8 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