Where is it now
- Distance from Sun
- 0.685 AU
- True anomaly
- 62.67°
- Distance from Earth
- 1.097 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 28m 22s
- Declination
- +04° 17′ 56″
- Constellation
- Leo
- Distance from Earth
- 1.1 AU
- Elongation from the Sun
- 37.85° — 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
- 0.921 AU
- Eccentricity
- 0.3634
- Inclination
- 1.55°
- Orbital period
- 322.8 days
- Perihelion
- 0.586 AU
- Aphelion
- 1.256 AU
- Longitude of ascending node
- 345.94°
- Argument of periapsis
- 58.9°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.2 LD
- 0.0006 AU
- Tisserand (Jupiter)
- 6.434
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 69
- Data arc
- 25 days
- First observed
- 12 March 2002
- Last observed
- 6 April 2002
- Residual RMS
- 0.44 ″
- Solution · Otto Matic
- 28 July 2026
Visual & observation
- Absolute magnitude (H)
- 24.4
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 52 on record
Top-down view of the ecliptic, Earth at the centre, for the 2034-06-27 07:00 UTC close approach of 2002 EM7. Catalogue miss distance 57.3 LD · 2.2 × 10⁷ km. The curve is the geocentric path from 2034-06-24 to 2034-06-30, 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. 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 |
|---|---|---|---|---|
| 2031-03-02 14:09:00 | Venus | 0.1354 AU | 52.7 LD | 10.3 km/s |
| 2034-06-27 07:00:00 | Earth | 0.1471 AU | 57.3 LD | 14.7 km/s |
| 2037-06-04 23:37:00 | Venus | 0.0613 AU | 23.9 LD | 14.8 km/s |
| 2039-01-04 16:51:00 | Venus | 0.0362 AU | 14.1 LD | 12 km/s |
| 2040-03-08 12:42:00 | Earth | 0.0476 AU | 18.5 LD | 11.7 km/s |
| 2045-04-25 18:43:00 | Venus | 0.1348 AU | 52.5 LD | 10.2 km/s |
| 2048-03-21 01:19:00 | Earth | 0.1537 AU | 59.8 LD | 7.3 km/s |
| 2049-06-30 01:22:00 | Earth | 0.0777 AU | 30.2 LD | 8.3 km/s |
| 2051-08-01 15:09:00 | Venus | 0.1136 AU | 44.2 LD | 17.3 km/s |
| 2053-03-06 05:24:00 | Venus | 0.0702 AU | 27.3 LD | 9 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