Where is it now
- Distance from Sun
- 1.382 AU
- True anomaly
- 193.08°
- Distance from Earth
- 1.586 AU
- As of
- 20 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
- 10h 08m 39s
- Declination
- +16° 07′ 49″
- Constellation
- Leo
- Distance from Earth
- 1.58 AU
- Elongation from the Sun
- 59.93° — 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
- 0.905 AU
- Eccentricity
- 0.5835
- Inclination
- 9.09°
- Orbital period
- 314.2 days
- Perihelion
- 0.377 AU
- Aphelion
- 1.432 AU
- Longitude of ascending node
- 322.88°
- Argument of periapsis
- 312.99°
- Epoch · J2000
- 2461082.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.3 LD
- 0.0008 AU
- Tisserand (Jupiter)
- 6.421
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 20
- Data arc
- 2 days
- First observed
- 10 February 2026
- Last observed
- 12 February 2026
- Residual RMS
- 0.47 ″
- Solution · Otto Matic
- 12 February 2026
Visual & observation
- Absolute magnitude (H)
- 27.04
Discovery & classification
Close approaches 39 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-11-13 21:41 UTC close approach of 2026 CW1. Catalogue miss distance 77.6 LD · 2.98 × 10⁷ km. The curve is the geocentric path from 2029-11-10 to 2029-11-16, 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 |
|---|---|---|---|---|
| 2027-01-16 22:10:00 | Venus | 0.0916 AU | 35.6 LD | 22.1 km/s |
| 2029-11-13 21:41:00 | Earth | 0.1993 AU | 77.6 LD | 22.3 km/s |
| 2030-07-23 06:46:00 | Mercury | 0.0774 AU | 30.1 LD | 28.6 km/s |
| 2030-07-23 06:46:00 | Merc | 0.0774 AU | 30.1 LD | 28.6 km/s |
| 2031-05-09 21:27:00 | Venus | 0.0991 AU | 38.6 LD | 20.5 km/s |
| 2035-08-30 22:38:00 | Venus | 0.1187 AU | 46.2 LD | 18.7 km/s |
| 2070-02-10 17:18:00 | Earth | 0.0653 AU | 25.4 LD | 20.6 km/s |
| 2072-12-08 23:08:00 | Venus | 0.1361 AU | 53.0 LD | 23.6 km/s |
| 2073-11-11 17:50:00 | Earth | 0.1658 AU | 64.5 LD | 20.1 km/s |
| 2076-02-13 17:43:00 | Earth | 0.1505 AU | 58.6 LD | 14.7 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