202683
Add to an observing list or journal →202683 (2006 US216)
Where is it now
- Distance from Sun
- 0.942 AU
- True anomaly
- 197.01°
- Distance from Earth
- 1.033 AU
- As of
- 15 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
- 09h 56m 00s
- Declination
- +09° 22′ 33″
- Constellation
- Leo
- Distance from Earth
- 1.03 AU
- Elongation from the Sun
- 55.23° — 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
- 0.637 AU
- Eccentricity
- 0.5623
- Inclination
- 3.44°
- Orbital period
- 185.7 days
- Perihelion
- 0.279 AU
- Aphelion
- 0.995 AU
- Longitude of ascending node
- 193.22°
- Argument of periapsis
- 56.45°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 17.2 LD
- 0.0442 AU
- Tisserand (Jupiter)
- 8.745
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 89
- Data arc
- 11.17 years
- First observed
- 6 November 2005
- Last observed
- 7 January 2017
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 13 April 2021
Visual & observation
- Absolute magnitude (H)
- 19.78
Discovery & classification
- Discovered by
- Mt. Lemmon Survey
- Discovery date
- 30 October 2006
- Discovery site
- Mount Lemmon
Also known as 2006 US216
Close approaches 396 on record
Top-down view of the ecliptic, Earth at the centre, for the 2032-12-09 00:57 UTC close approach of 202683. Catalogue miss distance 163.2 LD · 6.28 × 10⁷ km. The curve is the geocentric path from 2032-12-06 to 2032-12-12, 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 |
|---|---|---|---|---|
| 2029-06-01 03:51:00 | Venus | 0.071 AU | 27.6 LD | 20.6 km/s |
| 2031-01-05 16:23:00 | Mercury | 0.0834 AU | 32.5 LD | 27.7 km/s |
| 2031-01-05 16:23:00 | Merc | 0.0834 AU | 32.5 LD | 27.7 km/s |
| 2032-12-09 00:57:00 | Earth | 0.4195 AU | 163.2 LD | 26.2 km/s |
| 2033-12-12 19:00:00 | Earth | 0.3304 AU | 128.6 LD | 22.8 km/s |
| 2034-03-10 16:35:00 | Venus | 0.0686 AU | 26.7 LD | 23.1 km/s |
| 2034-12-16 01:49:00 | Earth | 0.242 AU | 94.2 LD | 19.4 km/s |
| 2035-08-04 00:03:00 | Merc | 0.0822 AU | 32.0 LD | 27.8 km/s |
| 2035-08-04 00:03:00 | Mercury | 0.0822 AU | 32.0 LD | 27.8 km/s |
| 2035-12-18 04:58:00 | Earth | 0.158 AU | 61.5 LD | 16.1 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