Where is it now
- Distance from Sun
- 0.837 AU
- True anomaly
- 60.18°
- Distance from Earth
- 0.564 AU
- As of
- 22 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
- 17h 45m 12s
- Declination
- -29° 09′ 27″
- Constellation
- Sagittarius
- Distance from Earth
- 0.56 AU
- Elongation from the Sun
- 57.35° — 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
- 0.943 AU
- Eccentricity
- 0.1795
- Inclination
- 7.09°
- Orbital period
- 334.3 days
- Perihelion
- 0.773 AU
- Aphelion
- 1.112 AU
- Longitude of ascending node
- 142.48°
- Argument of periapsis
- 152.57°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 24.0 LD
- 0.0615 AU
- Tisserand (Jupiter)
- 6.351
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 36
- Data arc
- 11.07 years
- First observed
- 10 February 2007
- Last observed
- 7 March 2018
- Residual RMS
- 0.6 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 25.1
Discovery & classification
Also known as 2018 EY2
Close approaches 137 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-27 04:36 UTC close approach of 2007 CM26. Catalogue miss distance 178.9 LD · 6.88 × 10⁷ km. The curve is the geocentric path from 2026-11-24 to 2026-11-30, 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 |
|---|---|---|---|---|
| 2026-11-27 04:36:00 | Earth | 0.4596 AU | 178.9 LD | 19.4 km/s |
| 2027-10-20 05:36:00 | Earth | 0.1454 AU | 56.6 LD | 4.4 km/s |
| 2027-12-06 03:39:00 | Earth | 0.1404 AU | 54.6 LD | 4.6 km/s |
| 2028-06-30 08:43:00 | Earth | 0.2502 AU | 97.4 LD | 7.9 km/s |
| 2029-03-11 19:00:00 | Earth | 0.1336 AU | 52.0 LD | 9.5 km/s |
| 2032-03-24 03:25:00 | Venus | 0.0772 AU | 30.0 LD | 5.2 km/s |
| 2034-02-01 21:36:00 | Venus | 0.0998 AU | 38.8 LD | 3.9 km/s |
| 2037-11-23 07:11:00 | Earth | 0.37 AU | 144.0 LD | 16.4 km/s |
| 2038-09-18 17:48:00 | Earth | 0.1845 AU | 71.8 LD | 6.2 km/s |
| 2039-01-05 16:42:00 | Earth | 0.1474 AU | 57.4 LD | 5.5 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