2013 QV1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.75 AU to 1.32 AU from the Sun; one orbit takes 384.8 days. Orbit from the JPL solution of 15 April 2021.
Where is it now
- Distance from Sun
- 0.875 AU
- True anomaly
- 290.14°
- Distance from Earth
- 1.107 AU
- As of
- 4 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
- 11h 48m 58s
- Declination
- +09° 00′ 18″
- Constellation
- Virgo
- Distance from Earth
- 1.11 AU
- Elongation from the Sun
- 48.89° — 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
- 1.035 AU
- Eccentricity
- 0.2739
- Inclination
- 17.61°
- Orbital period
- 384.8 days
- Perihelion
- 0.752 AU
- Aphelion
- 1.319 AU
- Longitude of ascending node
- 324.85°
- Argument of periapsis
- 218.37°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 58.7 LD
- 0.1508 AU
- Tisserand (Jupiter)
- 5.843
Orbit quality
Orbit reasonably well determined (uncertainty code 3).
- Observations used
- 75
- Data arc
- 352 days
- First observed
- 15 August 2013
- Last observed
- 2 August 2014
- Residual RMS
- 0.47 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 22
Discovery & classification
Close approaches 139 on record
Top-down view of the ecliptic, Earth at the centre, for the 2029-12-28 09:12 UTC close approach of 2013 QV1. Catalogue miss distance 111.4 LD · 4.28 × 10⁷ km. The curve is the geocentric path from 2029-12-25 to 2029-12-31, 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 |
|---|---|---|---|---|
| 2029-12-28 09:12:00 | Earth | 0.2864 AU | 111.4 LD | 16.4 km/s |
| 2031-02-02 22:55:00 | Earth | 0.1808 AU | 70.4 LD | 12.5 km/s |
| 2031-10-01 18:08:00 | Earth | 0.4065 AU | 158.2 LD | 9.6 km/s |
| 2032-03-21 08:10:00 | Earth | 0.2972 AU | 115.7 LD | 12.5 km/s |
| 2032-08-29 20:17:00 | Earth | 0.3187 AU | 124.0 LD | 10.3 km/s |
| 2033-08-03 08:24:00 | Earth | 0.1743 AU | 67.8 LD | 10.4 km/s |
| 2034-07-27 16:39:00 | Earth | 0.2472 AU | 96.2 LD | 15.5 km/s |
| 2050-01-03 07:43:00 | Earth | 0.2421 AU | 94.2 LD | 15.1 km/s |
| 2051-02-11 19:50:00 | Earth | 0.1979 AU | 77.0 LD | 12.5 km/s |
| 2051-09-24 17:10:00 | Earth | 0.396 AU | 154.1 LD | 9.9 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