2014 WW202 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.81 AU to 1.26 AU from the Sun; one orbit takes 382 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.842 AU
- True anomaly
- 41°
- Distance from Earth
- 1.8 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
- 15h 21m 20s
- Declination
- -17° 17′ 20″
- Constellation
- Libra
- Distance from Earth
- 1.8 AU
- Elongation from the Sun
- 10.34° — too close to the Sun to observe
Favours the southern hemisphere; low or below the horizon from far north.
From your location
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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
- 0.2183
- Inclination
- 3.02°
- Orbital period
- 382 days
- Perihelion
- 0.805 AU
- Aphelion
- 1.255 AU
- Longitude of ascending node
- 191.6°
- Argument of periapsis
- 10.84°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 19.5 LD
- 0.0502 AU
- Tisserand (Jupiter)
- 5.918
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 12
- Data arc
- 4 days
- First observed
- 24 November 2014
- Last observed
- 28 November 2014
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 24.4
Discovery & classification
Close approaches 31 on record
Top-down view of the ecliptic, Earth at the centre, for the 2080-12-25 16:44 UTC close approach of 2014 WW202. Catalogue miss distance 160.1 LD · 6.16 × 10⁷ km. The curve is the geocentric path from 2080-12-22 to 2080-12-28, 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 |
|---|---|---|---|---|
| 2080-12-25 16:44:00 | Earth | 0.4114 AU | 160.1 LD | 19.1 km/s |
| 2082-01-08 00:58:00 | Earth | 0.1274 AU | 49.6 LD | 10.2 km/s |
| 2085-07-24 10:18:00 | Earth | 0.056 AU | 21.8 LD | 5.9 km/s |
| 2086-08-05 11:34:00 | Earth | 0.2592 AU | 100.9 LD | 14.1 km/s |
| 2149-12-23 05:48:00 | Earth | 0.493 AU | 191.9 LD | 21.7 km/s |
| 2150-02-25 01:43:00 | Venus | 0.0925 AU | 36.0 LD | 3.8 km/s |
| 2151-01-05 05:02:00 | Earth | 0.2143 AU | 83.4 LD | 13 km/s |
| 2155-08-02 17:26:00 | Earth | 0.1672 AU | 65.1 LD | 11.4 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