482796
Add to an observing list or journal →482796 (2013 QJ10)
Where is it now
- Distance from Sun
- 1.073 AU
- True anomaly
- 128.97°
- Distance from Earth
- 0.873 AU
- As of
- 22 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
- 18h 41m 25s
- Declination
- -18° 00′ 08″
- Constellation
- Sagittarius
- Distance from Earth
- 0.88 AU
- Elongation from the Sun
- 69.88° — well clear of the Sun
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
- 0.959 AU
- Eccentricity
- 0.425
- Inclination
- 18.15°
- Orbital period
- 343.2 days
- Perihelion
- 0.552 AU
- Aphelion
- 1.367 AU
- Longitude of ascending node
- 327.42°
- Argument of periapsis
- 243.88°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 9.8 LD
- 0.0251 AU
- Tisserand (Jupiter)
- 6.163
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 553
- Data arc
- 15.12 years
- First observed
- 7 November 2002
- Last observed
- 20 December 2017
- Residual RMS
- 0.4 ″
- Solution · Otto Matic
- 14 April 2021
Physical properties
- Rotation period
- 14.5 hours
Visual & observation
- Absolute magnitude (H)
- 19.6
Discovery & classification
- Discovered by
- OAM
- Discovery date
- 24 August 2013
- Discovery site
- La Sagra
Also known as 2013 QJ10
Close approaches 199 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-10 02:39 UTC close approach of 482796. Catalogue miss distance 158.3 LD · 6.08 × 10⁷ km. The curve is the geocentric path from 2027-09-07 to 2027-09-13, 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. 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 |
|---|---|---|---|---|
| 2027-09-10 02:39:00 | Earth | 0.4067 AU | 158.3 LD | 27.2 km/s |
| 2028-08-25 19:30:00 | Earth | 0.057 AU | 22.2 LD | 17.1 km/s |
| 2029-08-29 20:34:00 | Earth | 0.2973 AU | 115.7 LD | 10.8 km/s |
| 2030-10-11 11:50:00 | Earth | 0.484 AU | 188.4 LD | 11.4 km/s |
| 2031-04-09 14:57:00 | Earth | 0.4833 AU | 188.1 LD | 19.1 km/s |
| 2031-11-30 00:15:00 | Earth | 0.4726 AU | 183.9 LD | 9.3 km/s |
| 2032-02-26 16:50:00 | Earth | 0.3655 AU | 142.3 LD | 16 km/s |
| 2033-01-12 08:56:00 | Earth | 0.2154 AU | 83.8 LD | 15.7 km/s |
| 2033-12-19 18:52:00 | Earth | 0.4021 AU | 156.5 LD | 25.1 km/s |
| 2036-11-03 22:34:00 | Venus | 0.0554 AU | 21.6 LD | 16.7 km/s |
Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.
Sources
- visual properties: JPL SBDB (lookup)
- physical properties: JPL SBDB (lookup)
- orbital elements: JPL SBDB