2016 GG216 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.49 AU to 1.53 AU from the Sun; one orbit takes 369.9 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.133 AU
- True anomaly
- 132.22°
- Distance from Earth
- 1.094 AU
- As of
- 3 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
- 10h 12m 25s
- Declination
- -04° 18′ 09″
- Constellation
- Sextans
- Distance from Earth
- 1.09 AU
- Elongation from the Sun
- 65.69° — 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
- 1.008 AU
- Eccentricity
- 0.5154
- Inclination
- 14.71°
- Orbital period
- 369.9 days
- Perihelion
- 0.489 AU
- Aphelion
- 1.528 AU
- Longitude of ascending node
- 171.93°
- Argument of periapsis
- 157.17°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 57.3 LD
- 0.1471 AU
- Tisserand (Jupiter)
- 5.889
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 58
- Data arc
- 4.97 years
- First observed
- 25 March 2014
- Last observed
- 14 March 2019
- Residual RMS
- 0.75 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 23.15
Discovery & classification
Close approaches 158 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-09-21 02:37 UTC close approach of 2016 GG216. Catalogue miss distance 191.6 LD · 7.37 × 10⁷ km. The curve is the geocentric path from 2031-09-18 to 2031-09-24, 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 |
|---|---|---|---|---|
| 2031-09-21 02:37:00 | Earth | 0.4924 AU | 191.6 LD | 22.8 km/s |
| 2031-10-07 20:21:00 | Venus | 0.1441 AU | 56.1 LD | 21.5 km/s |
| 2032-09-27 23:10:00 | Earth | 0.4781 AU | 186.1 LD | 21.7 km/s |
| 2033-10-06 05:15:00 | Earth | 0.4608 AU | 179.3 LD | 20.3 km/s |
| 2034-01-21 09:22:00 | Earth | 0.4895 AU | 190.5 LD | 13 km/s |
| 2034-10-14 23:31:00 | Earth | 0.4403 AU | 171.4 LD | 18.6 km/s |
| 2035-01-15 22:24:00 | Earth | 0.4631 AU | 180.2 LD | 12.5 km/s |
| 2035-10-24 12:14:00 | Earth | 0.4158 AU | 161.8 LD | 16.7 km/s |
| 2036-01-09 15:57:00 | Earth | 0.4314 AU | 167.9 LD | 11.9 km/s |
| 2036-11-03 15:40:00 | Earth | 0.386 AU | 150.2 LD | 14.4 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