2014 GC35 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.71 AU to 1.33 AU from the Sun; one orbit takes 375.5 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.884 AU
- True anomaly
- 278.13°
- Distance from Earth
- 1.674 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
- 16h 11m 01s
- Declination
- -04° 45′ 53″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.67 AU
- Elongation from the Sun
- 25.3° — 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
- 1.019 AU
- Eccentricity
- 0.3066
- Inclination
- 33.11°
- Orbital period
- 375.5 days
- Perihelion
- 0.706 AU
- Aphelion
- 1.331 AU
- Longitude of ascending node
- 198.05°
- Argument of periapsis
- 154.49°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 97.1 LD
- 0.2494 AU
- Tisserand (Jupiter)
- 5.814
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 33
- Data arc
- 374 days
- First observed
- 5 April 2014
- Last observed
- 14 April 2015
- Residual RMS
- 0.35 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 22.4
Discovery & classification
Close approaches 148 on record
Top-down view of the ecliptic, Earth at the centre, for the 2047-04-21 01:54 UTC close approach of 2014 GC35. Catalogue miss distance 187.6 LD · 7.21 × 10⁷ km. The curve is the geocentric path from 2047-04-18 to 2047-04-24, 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. At closest approach the object is north 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 |
|---|---|---|---|---|
| 2047-04-21 01:54:00 | Earth | 0.482 AU | 187.6 LD | 24.2 km/s |
| 2048-04-21 18:19:00 | Earth | 0.3681 AU | 143.3 LD | 20.9 km/s |
| 2049-04-21 04:39:00 | Earth | 0.2843 AU | 110.6 LD | 18.6 km/s |
| 2050-04-18 10:34:00 | Earth | 0.2503 AU | 97.4 LD | 17.3 km/s |
| 2051-04-14 00:34:00 | Earth | 0.2709 AU | 105.4 LD | 16.7 km/s |
| 2051-08-26 04:44:00 | Earth | 0.4761 AU | 185.3 LD | 21.2 km/s |
| 2052-04-07 13:11:00 | Earth | 0.3247 AU | 126.4 LD | 16.5 km/s |
| 2052-09-13 02:47:00 | Earth | 0.3887 AU | 151.3 LD | 21.9 km/s |
| 2053-04-01 06:09:00 | Earth | 0.3901 AU | 151.8 LD | 16.5 km/s |
| 2053-09-30 00:02:00 | Earth | 0.3113 AU | 121.1 LD | 21.9 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