2014 GA is an asteroid in the Apollo orbit class. Its orbit takes it from 0.97 AU to 1.09 AU from the Sun; one orbit takes 381.6 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.002 AU
- True anomaly
- 294.62°
- Distance from Earth
- 1.981 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
- 14h 11m 45s
- Declination
- -15° 00′ 10″
- Constellation
- Virgo
- Distance from Earth
- 1.98 AU
- Elongation from the Sun
- 6.52° — too close to the Sun to observe
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
- 1.03 AU
- Eccentricity
- 0.0589
- Inclination
- 9.65°
- Orbital period
- 381.6 days
- Perihelion
- 0.969 AU
- Aphelion
- 1.09 AU
- Longitude of ascending node
- 10.08°
- Argument of periapsis
- 264.31°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 7.6 LD
- 0.0197 AU
- Tisserand (Jupiter)
- 5.929
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 41
- Data arc
- 5 days
- First observed
- 1 April 2014
- Last observed
- 6 April 2014
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.4
Discovery & classification
Close approaches 27 on record
Top-down view of the ecliptic, Earth at the centre, for the 2036-03-26 21:20 UTC close approach of 2014 GA. Catalogue miss distance 131.3 LD · 5.05 × 10⁷ km. The curve is the geocentric path from 2036-03-23 to 2036-03-29, 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 |
|---|---|---|---|---|
| 2036-03-26 21:20:00 | Earth | 0.3375 AU | 131.3 LD | 13.1 km/s |
| 2037-04-02 10:20:00 | Earth | 0.0621 AU | 24.2 LD | 6.4 km/s |
| 2038-09-29 02:43:00 | Earth | 0.0386 AU | 15.0 LD | 5.8 km/s |
| 2039-10-02 17:50:00 | Earth | 0.3082 AU | 119.9 LD | 12.2 km/s |
| 2059-03-28 07:32:00 | Earth | 0.3498 AU | 136.1 LD | 13.4 km/s |
| 2060-04-02 16:57:00 | Earth | 0.0711 AU | 27.7 LD | 6.5 km/s |
| 2061-09-29 01:31:00 | Earth | 0.038 AU | 14.8 LD | 5.8 km/s |
| 2062-10-03 02:48:00 | Earth | 0.315 AU | 122.6 LD | 12.4 km/s |
| 2082-04-01 12:10:00 | Earth | 0.233 AU | 90.7 LD | 10.3 km/s |
| 2084-09-28 20:58:00 | Earth | 0.1787 AU | 69.5 LD | 8.9 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