Where is it now
- Distance from Sun
- 0.439 AU
- True anomaly
- 334.3°
- Distance from Earth
- 1.117 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 56m 19s
- Declination
- -04° 01′ 59″
- Constellation
- Virgo
- Distance from Earth
- 1.13 AU
- Elongation from the Sun
- 22.67° — 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
- 0.681 AU
- Eccentricity
- 0.3723
- Inclination
- 23.33°
- Orbital period
- 205.4 days
- Perihelion
- 0.428 AU
- Aphelion
- 0.935 AU
- Longitude of ascending node
- 273.41°
- Argument of periapsis
- 230.43°
- Epoch · J2000
- 2461200.5
- Orbit class · IEO
- Atira (interior-Earth object)
- Earth MOID · 76.8 LD
- 0.1974 AU
- Tisserand (Jupiter)
- 8.254
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 291
- Data arc
- 20.75 years
- First observed
- 26 September 2005
- Last observed
- 26 June 2026
- Residual RMS
- 0.5 ″
- Solution · Otto Matic
- 26 June 2026
Physical properties
- Rotation period
- 1.39 hours
Visual & observation
- Absolute magnitude (H)
- 17.63
Discovery & classification
- Discovered by
- CSS
- Discovery date
- 5 October 2005
- Discovery site
- Catalina
Also known as 2005 TG45
Close approaches 43 on record
Top-down view of the ecliptic, Earth at the centre, for the 2090-07-14 07:46 UTC close approach of 413563. Catalogue miss distance 77.6 LD · 2.98 × 10⁷ km. The curve is the geocentric path from 2090-07-11 to 2090-07-17, 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 |
|---|---|---|---|---|
| 2030-04-20 02:00:00 | Venus | 0.1127 AU | 43.9 LD | 23.4 km/s |
| 2037-01-22 09:42:00 | Venus | 0.0251 AU | 9.8 LD | 19.3 km/s |
| 2043-10-30 12:05:00 | Venus | 0.1341 AU | 52.2 LD | 16.6 km/s |
| 2049-12-26 01:34:00 | Venus | 0.0967 AU | 37.6 LD | 22.8 km/s |
| 2056-09-29 14:05:00 | Venus | 0.0375 AU | 14.6 LD | 18.7 km/s |
| 2069-09-01 14:25:00 | Venus | 0.0612 AU | 23.8 LD | 21.4 km/s |
| 2076-06-06 19:51:00 | Venus | 0.0717 AU | 27.9 LD | 17.7 km/s |
| 2089-05-09 09:01:00 | Venus | 0.0335 AU | 13.0 LD | 20.3 km/s |
| 2090-07-14 07:46:00 | Earth | 0.1995 AU | 77.6 LD | 14.1 km/s |
| 2096-02-13 06:53:00 | Venus | 0.0918 AU | 35.7 LD | 17.3 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