2013 WR45 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.79 AU to 1.24 AU from the Sun; one orbit takes 374 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 1.193 AU
- True anomaly
- 149.37°
- Distance from Earth
- 1.214 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
- 19h 08m 05s
- Declination
- -18° 12′ 50″
- Constellation
- Sagittarius
- Distance from Earth
- 1.22 AU
- Elongation from the Sun
- 64.53° — well clear of the Sun
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
- 1.016 AU
- Eccentricity
- 0.2214
- Inclination
- 4.36°
- Orbital period
- 374 days
- Perihelion
- 0.791 AU
- Aphelion
- 1.241 AU
- Longitude of ascending node
- 241.94°
- Argument of periapsis
- 303.29°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 13.4 LD
- 0.0344 AU
- Tisserand (Jupiter)
- 5.981
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 22
- Data arc
- 25 days
- First observed
- 27 November 2013
- Last observed
- 22 December 2013
- Residual RMS
- 0.3 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 25.7
Discovery & classification
Close approaches 30 on record
Top-down view of the ecliptic, Earth at the centre, for the 2065-07-10 20:15 UTC close approach of 2013 WR45. Catalogue miss distance 30.9 LD · 1.19 × 10⁷ km. The curve is the geocentric path from 2065-07-07 to 2065-07-13, 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 |
|---|---|---|---|---|
| 2029-08-02 04:48:00 | Venus | 0.1084 AU | 42.2 LD | 4.5 km/s |
| 2065-07-10 20:15:00 | Earth | 0.0795 AU | 30.9 LD | 8.5 km/s |
| 2066-07-17 21:04:00 | Earth | 0.1982 AU | 77.1 LD | 12.3 km/s |
| 2067-07-24 12:03:00 | Earth | 0.3281 AU | 127.7 LD | 16.2 km/s |
| 2068-07-29 19:06:00 | Earth | 0.4586 AU | 178.5 LD | 20.2 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