Where is it now
- Distance from Sun
- 1.14 AU
- True anomaly
- 185.75°
- Distance from Earth
- 1.04 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
- 09h 32m 22s
- Declination
- +14° 40′ 10″
- Constellation
- Leo
- Distance from Earth
- 1.04 AU
- Elongation from the Sun
- 68.17° — well clear of the Sun
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
- 0.92 AU
- Eccentricity
- 0.2408
- Inclination
- 0.12°
- Orbital period
- 322.4 days
- Perihelion
- 0.699 AU
- Aphelion
- 1.142 AU
- Longitude of ascending node
- 300.89°
- Argument of periapsis
- 319.52°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.3 LD
- 0.0007 AU
- Tisserand (Jupiter)
- 6.472
Orbit quality
Orbit reasonably well determined (uncertainty code 4).
- Observations used
- 21
- First observed
- 8 February 2026
- Last observed
- 8 February 2026
- Residual RMS
- 0.45 ″
- Solution · Otto Matic
- 14 February 2026
Visual & observation
- Absolute magnitude (H)
- 30.06
Discovery & classification
Close approaches 81 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-11-21 14:20 UTC close approach of 2026 CH2. Catalogue miss distance 55.3 LD · 2.13 × 10⁷ km. The curve is the geocentric path from 2032-11-18 to 2032-11-24, 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 |
|---|---|---|---|---|
| 2027-04-17 02:55:00 | Venus | 0.0817 AU | 31.8 LD | 9.5 km/s |
| 2032-11-21 14:20:00 | Earth | 0.1422 AU | 55.3 LD | 5.7 km/s |
| 2039-10-21 06:57:00 | Earth | 0.1918 AU | 74.7 LD | 13.2 km/s |
| 2041-02-03 21:42:00 | Earth | 0.0664 AU | 25.9 LD | 5.5 km/s |
| 2041-05-05 16:19:00 | Venus | 0.0266 AU | 10.3 LD | 5.3 km/s |
| 2047-10-25 22:03:00 | Earth | 0.0845 AU | 32.9 LD | 5.3 km/s |
| 2055-06-07 03:06:00 | Venus | 0.0419 AU | 16.3 LD | 7.5 km/s |
| 2056-01-04 07:40:00 | Earth | 0.1407 AU | 54.8 LD | 5.7 km/s |
| 2061-09-19 05:14:00 | Venus | 0.0303 AU | 11.8 LD | 6.4 km/s |
| 2062-10-17 20:04:00 | Earth | 0.0365 AU | 14.2 LD | 6.2 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