Where is it now
- Distance from Sun
- 0.776 AU
- True anomaly
- 9.05°
- Distance from Earth
- 1.464 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
- 15h 47m 21s
- Declination
- -16° 49′ 16″
- Constellation
- Libra
- Distance from Earth
- 1.46 AU
- Elongation from the Sun
- 29.8° — 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
- 0.914 AU
- Eccentricity
- 0.1517
- Inclination
- 5.85°
- Orbital period
- 319 days
- Perihelion
- 0.775 AU
- Aphelion
- 1.052 AU
- Longitude of ascending node
- 177.62°
- Argument of periapsis
- 90.66°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 20.7 LD
- 0.0531 AU
- Tisserand (Jupiter)
- 6.519
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 69
- Data arc
- 7.25 years
- First observed
- 6 November 2014
- Last observed
- 4 February 2022
- Residual RMS
- 0.58 ″
- Solution · Otto Matic
- 1 March 2023
Visual & observation
- Absolute magnitude (H)
- 22.39
Discovery & classification
Close approaches 137 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-09-27 20:04 UTC close approach of 2014 YF. Catalogue miss distance 50.7 LD · 1.95 × 10⁷ km. The curve is the geocentric path from 2028-09-24 to 2028-09-30, 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 |
|---|---|---|---|---|
| 2028-09-27 20:04:00 | Earth | 0.1303 AU | 50.7 LD | 3.8 km/s |
| 2028-12-10 01:26:00 | Earth | 0.1232 AU | 47.9 LD | 3.5 km/s |
| 2029-03-26 19:50:00 | Earth | 0.1526 AU | 59.4 LD | 4.1 km/s |
| 2030-04-02 13:36:00 | Venus | 0.1252 AU | 48.7 LD | 6.8 km/s |
| 2030-05-17 22:32:00 | Venus | 0.1343 AU | 52.3 LD | 2.3 km/s |
| 2035-08-28 11:53:00 | Earth | 0.1869 AU | 72.7 LD | 5 km/s |
| 2036-02-22 22:56:00 | Earth | 0.0789 AU | 30.7 LD | 4 km/s |
| 2040-09-05 17:28:00 | Venus | 0.0949 AU | 36.9 LD | 4.4 km/s |
| 2041-11-11 19:25:00 | Earth | 0.4919 AU | 191.4 LD | 19.9 km/s |
| 2042-08-08 08:35:00 | Earth | 0.2194 AU | 85.4 LD | 5.9 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