417217
Add to an observing list or journal →417217 (2005 YS)
Where is it now
- Distance from Sun
- 0.884 AU
- True anomaly
- 142.97°
- Distance from Earth
- 0.431 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
- 11h 25m 24s
- Declination
- +48° 27′ 01″
- Constellation
- Ursa Major
- Distance from Earth
- 0.43 AU
- Elongation from the Sun
- 63.28° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.711 AU
- Eccentricity
- 0.5503
- Inclination
- 19.6°
- Orbital period
- 219 days
- Perihelion
- 0.32 AU
- Aphelion
- 1.102 AU
- Longitude of ascending node
- 288.58°
- Argument of periapsis
- 327.93°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 11.7 LD
- 0.0301 AU
- Tisserand (Jupiter)
- 7.899
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 357
- Data arc
- 18.06 years
- First observed
- 21 December 2005
- Last observed
- 14 January 2024
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 30 January 2024
Visual & observation
- Absolute magnitude (H)
- 19.52
Discovery & classification
- Discovered by
- LINEAR
- Discovery date
- 21 December 2005
- Discovery site
- Socorro
Also known as 2005 YS
Close approaches 154 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-12-20 14:04 UTC close approach of 417217. Catalogue miss distance 79.7 LD · 3.06 × 10⁷ km. The curve is the geocentric path from 2026-12-17 to 2026-12-23, 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 |
|---|---|---|---|---|
| 2026-12-20 14:04:00 | Earth | 0.2049 AU | 79.7 LD | 13.4 km/s |
| 2029-12-21 13:22:00 | Earth | 0.1992 AU | 77.5 LD | 13.4 km/s |
| 2032-12-22 06:46:00 | Earth | 0.1944 AU | 75.7 LD | 13.4 km/s |
| 2033-02-14 19:59:00 | Venus | 0.1202 AU | 46.8 LD | 22.7 km/s |
| 2035-12-23 18:58:00 | Earth | 0.1903 AU | 74.0 LD | 13.5 km/s |
| 2038-12-24 03:35:00 | Earth | 0.1869 AU | 72.7 LD | 13.5 km/s |
| 2041-12-24 07:18:00 | Earth | 0.1846 AU | 71.8 LD | 13.5 km/s |
| 2044-12-24 11:47:00 | Earth | 0.182 AU | 70.8 LD | 13.5 km/s |
| 2047-12-25 17:11:00 | Earth | 0.1792 AU | 69.8 LD | 13.5 km/s |
| 2050-12-25 22:51:00 | Earth | 0.1762 AU | 68.6 LD | 13.5 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