2015 FU284 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.44 AU to 1.61 AU from the Sun; one orbit takes 379 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.603 AU
- True anomaly
- 76.13°
- Distance from Earth
- 0.537 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 44m 27s
- Declination
- -28° 17′ 12″
- Constellation
- Scorpius
- Distance from Earth
- 0.53 AU
- Elongation from the Sun
- 31.85° — near the Sun — look low at dusk or dawn
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
- 1.025 AU
- Eccentricity
- 0.5747
- Inclination
- 14.52°
- Orbital period
- 379 days
- Perihelion
- 0.436 AU
- Aphelion
- 1.614 AU
- Longitude of ascending node
- 175.16°
- Argument of periapsis
- 123.21°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 0.9 LD
- 0.0024 AU
- Tisserand (Jupiter)
- 5.78
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 26
- First observed
- 16 March 2015
- Last observed
- 16 March 2015
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 28.3
Discovery & classification
Close approaches 38 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-28 13:39 UTC close approach of 2015 FU284. Catalogue miss distance 122.7 LD · 4.72 × 10⁷ km. The curve is the geocentric path from 2026-11-25 to 2026-12-01, 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 |
|---|---|---|---|---|
| 2026-11-28 13:39:00 | Earth | 0.3153 AU | 122.7 LD | 26.4 km/s |
| 2027-09-21 02:00:00 | Venus | 0.0723 AU | 28.1 LD | 20.2 km/s |
| 2027-12-09 12:08:00 | Earth | 0.4976 AU | 193.6 LD | 33.5 km/s |
| 2040-05-08 10:33:00 | Venus | 0.0997 AU | 38.8 LD | 25.6 km/s |
| 2041-03-03 21:16:00 | Earth | 0.3239 AU | 126.0 LD | 29.6 km/s |
| 2042-03-13 05:14:00 | Earth | 0.1003 AU | 39.0 LD | 22.7 km/s |
| 2043-03-20 02:52:00 | Earth | 0.1257 AU | 48.9 LD | 16.4 km/s |
| 2044-04-29 18:13:00 | Venus | 0.0526 AU | 20.5 LD | 21.7 km/s |
| 2106-11-15 21:19:00 | Earth | 0.2249 AU | 87.5 LD | 18 km/s |
| 2107-09-07 19:12:00 | Venus | 0.1038 AU | 40.4 LD | 26.8 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