Where is it now
- Distance from Sun
- 0.82 AU
- True anomaly
- 128.81°
- Distance from Earth
- 1.476 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
- 11h 39m 11s
- Declination
- -05° 54′ 19″
- Constellation
- Virgo
- Distance from Earth
- 1.48 AU
- Elongation from the Sun
- 31.98° — 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
- 0.918 AU
- Eccentricity
- 0.7101
- Inclination
- 17.24°
- Orbital period
- 321.3 days
- Perihelion
- 0.266 AU
- Aphelion
- 1.57 AU
- Longitude of ascending node
- 266.98°
- Argument of periapsis
- 102.77°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 68.3 LD
- 0.1755 AU
- Tisserand (Jupiter)
- 6.232
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 95
- Data arc
- 15.11 years
- First observed
- 17 February 2010
- Last observed
- 30 March 2025
- Residual RMS
- 0.56 ″
- Solution · Otto Matic
- 1 April 2025
Visual & observation
- Absolute magnitude (H)
- 19.06
Discovery & classification
- Discovered by
- Pan-STARRS 1
- Discovery date
- 13 April 2018
- Discovery site
- Haleakala
Also known as 2018 GY4
Close approaches 126 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-05-15 21:20 UTC close approach of 678989. Catalogue miss distance 68.9 LD · 2.65 × 10⁷ km. The curve is the geocentric path from 2035-05-12 to 2035-05-18, 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 south 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 |
|---|---|---|---|---|
| 2032-11-17 02:02:00 | Merc | 0.0588 AU | 22.9 LD | 43.3 km/s |
| 2032-11-17 02:02:00 | Mercury | 0.0588 AU | 22.9 LD | 43.3 km/s |
| 2035-05-15 21:20:00 | Earth | 0.1772 AU | 68.9 LD | 23.2 km/s |
| 2035-07-09 19:11:00 | Merc | 0.0802 AU | 31.2 LD | 28.5 km/s |
| 2035-07-09 19:11:00 | Mercury | 0.0802 AU | 31.2 LD | 28.5 km/s |
| 2043-05-17 00:58:00 | Merc | 0.0653 AU | 25.4 LD | 32.1 km/s |
| 2043-05-17 00:58:00 | Mercury | 0.0653 AU | 25.4 LD | 32.1 km/s |
| 2046-11-11 07:54:00 | Venus | 0.1286 AU | 50.0 LD | 35.3 km/s |
| 2053-01-06 18:14:00 | Venus | 0.0997 AU | 38.8 LD | 33.6 km/s |
| 2053-02-09 19:41:00 | Mercury | 0.0718 AU | 27.9 LD | 45.2 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