Where is it now
- Distance from Sun
- 0.901 AU
- True anomaly
- 144.63°
- Distance from Earth
- 1.499 AU
- As of
- 15 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 35m 28s
- Declination
- +13° 58′ 10″
- Constellation
- Leo
- Distance from Earth
- 1.5 AU
- Elongation from the Sun
- 35.88° — 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
- 0.724 AU
- Eccentricity
- 0.392
- Inclination
- 45.48°
- Orbital period
- 225.2 days
- Perihelion
- 0.441 AU
- Aphelion
- 1.008 AU
- Longitude of ascending node
- 325.89°
- Argument of periapsis
- 9.72°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.5 LD
- 0.0115 AU
- Tisserand (Jupiter)
- 7.663
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 141
- Data arc
- 19.02 years
- First observed
- 22 February 2007
- Last observed
- 28 February 2026
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 28 February 2026
Visual & observation
- Absolute magnitude (H)
- 19.96
Discovery & classification
Close approaches 117 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-02-14 18:50 UTC close approach of 2020 CL1. Catalogue miss distance 39.4 LD · 1.51 × 10⁷ km. The curve is the geocentric path from 2028-02-11 to 2028-02-17, 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 south 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 |
|---|---|---|---|---|
| 2028-02-14 18:50:00 | Earth | 0.1011 AU | 39.4 LD | 21.7 km/s |
| 2035-03-21 16:55:00 | Mercury | 0.0741 AU | 28.8 LD | 37.6 km/s |
| 2035-03-21 16:55:00 | Merc | 0.0741 AU | 28.8 LD | 37.6 km/s |
| 2036-02-15 06:29:00 | Earth | 0.0237 AU | 9.2 LD | 21.7 km/s |
| 2040-10-06 01:47:00 | Merc | 0.0384 AU | 14.9 LD | 37.8 km/s |
| 2040-10-06 01:47:00 | Mercury | 0.0384 AU | 14.9 LD | 37.8 km/s |
| 2044-02-15 19:23:00 | Earth | 0.0451 AU | 17.5 LD | 22 km/s |
| 2050-08-19 07:48:00 | Mercury | 0.0863 AU | 33.6 LD | 37.8 km/s |
| 2050-08-19 07:48:00 | Merc | 0.0863 AU | 33.6 LD | 37.8 km/s |
| 2052-02-16 17:00:00 | Earth | 0.1218 AU | 47.4 LD | 22.7 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