Where is it now
- Distance from Sun
- 0.91 AU
- True anomaly
- 261.15°
- Distance from Earth
- 1.717 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
- 15h 21m 33s
- Declination
- -18° 38′ 36″
- Constellation
- Libra
- Distance from Earth
- 1.72 AU
- Elongation from the Sun
- 24.45° — 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
- 0.909 AU
- Eccentricity
- 0.1514
- Inclination
- 0.49°
- Orbital period
- 316.7 days
- Perihelion
- 0.772 AU
- Aphelion
- 1.047 AU
- Longitude of ascending node
- 39.77°
- Argument of periapsis
- 318.79°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.1 LD
- 0.0002 AU
- Tisserand (Jupiter)
- 6.549
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 90
- Data arc
- 32 days
- First observed
- 3 February 2022
- Last observed
- 7 March 2022
- Residual RMS
- 0.42 ″
- Solution · Otto Matic
- 22 March 2022
Visual & observation
- Absolute magnitude (H)
- 27.31
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 41 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-02-07 07:17 UTC close approach of 2022 CA1. Catalogue miss distance 162.4 LD · 6.24 × 10⁷ km. The curve is the geocentric path from 2028-02-04 to 2028-02-10, 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 |
|---|---|---|---|---|
| 2028-02-07 07:17:00 | Earth | 0.4173 AU | 162.4 LD | 16.9 km/s |
| 2028-10-04 00:38:00 | Earth | 0.227 AU | 88.3 LD | 6.5 km/s |
| 2029-04-29 00:37:00 | Earth | 0.1922 AU | 74.8 LD | 9.8 km/s |
| 2030-05-05 05:23:00 | Venus | 0.1381 AU | 53.7 LD | 2.2 km/s |
| 2035-01-26 21:07:00 | Earth | 0.0265 AU | 10.3 LD | 4.7 km/s |
| 2035-07-21 23:32:00 | Earth | 0.1911 AU | 74.4 LD | 4.7 km/s |
| 2040-12-04 07:56:00 | Venus | 0.0744 AU | 28.9 LD | 1.5 km/s |
| 2048-02-09 01:49:00 | Earth | 0.4816 AU | 187.4 LD | 18.9 km/s |
| 2048-10-21 15:05:00 | Earth | 0.2076 AU | 80.8 LD | 5.8 km/s |
| 2049-05-02 14:15:00 | Earth | 0.0914 AU | 35.6 LD | 6.7 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