2016 CG18 is an asteroid in the Aten orbit class. Its orbit takes it from 0.89 AU to 1.07 AU from the Sun; one orbit takes 355.9 days. Orbit from the JPL solution of 28 July 2026.
Where is it now
- Distance from Sun
- 0.974 AU
- True anomaly
- 270.29°
- Distance from Earth
- 1.546 AU
- As of
- 2 November 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
- 12h 10m 47s
- Declination
- -01° 41′ 41″
- Constellation
- Virgo
- Distance from Earth
- 1.55 AU
- Elongation from the Sun
- 37.72° — 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
- 0.983 AU
- Eccentricity
- 0.0922
- Inclination
- 5.7°
- Orbital period
- 355.9 days
- Perihelion
- 0.892 AU
- Aphelion
- 1.073 AU
- Longitude of ascending node
- 316.84°
- Argument of periapsis
- 276.91°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.2 LD
- 0.0005 AU
- Tisserand (Jupiter)
- 6.156
Orbit quality
Orbit reasonably well determined (uncertainty code 4).
- Observations used
- 106
- Data arc
- 3 days
- First observed
- 3 February 2016
- Last observed
- 6 February 2016
- Residual RMS
- 0.41 ″
- Solution · Otto Matic
- 28 July 2026
Visual & observation
- Absolute magnitude (H)
- 28.5
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 16 on record
Top-down view of the ecliptic, Earth at the centre, for the 2050-09-06 02:50 UTC close approach of 2016 CG18. Catalogue miss distance 56.2 LD · 2.16 × 10⁷ km. The curve is the geocentric path from 2050-09-03 to 2050-09-09, 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 |
|---|---|---|---|---|
| 2050-09-06 02:50:00 | Earth | 0.1445 AU | 56.2 LD | 7.7 km/s |
| 2051-08-23 17:01:00 | Earth | 0.0365 AU | 14.2 LD | 4 km/s |
| 2052-06-26 17:24:00 | Earth | 0.1305 AU | 50.8 LD | 3.7 km/s |
| 2054-02-05 07:39:00 | Earth | 0.0097 AU | 3.8 LD | 4.1 km/s |
| 2055-02-03 03:18:00 | Earth | 0.0758 AU | 29.5 LD | 6.1 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