Where is it now
- Distance from Sun
- 0.897 AU
- True anomaly
- 176.97°
- Distance from Earth
- 0.209 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 55m 47s
- Declination
- +11° 53′ 48″
- Constellation
- Leo
- Distance from Earth
- 0.21 AU
- Elongation from the Sun
- 56.08° — 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
- 0.618 AU
- Eccentricity
- 0.4544
- Inclination
- 2.95°
- Orbital period
- 177.3 days
- Perihelion
- 0.337 AU
- Aphelion
- 0.898 AU
- Longitude of ascending node
- 211.13°
- Argument of periapsis
- 5.46°
- Epoch · J2000
- 2461200.5
- Orbit class · IEO
- Atira (interior-Earth object)
- Earth MOID · 37.1 LD
- 0.0954 AU
- Tisserand (Jupiter)
- 9.039
Orbit quality
Orbit very well determined (uncertainty code 1).
- Observations used
- 72
- Data arc
- 9.76 years
- First observed
- 13 December 2004
- Last observed
- 16 September 2014
- Residual RMS
- 0.22 ″
- Solution · Otto Matic
- 13 April 2021
Visual & observation
- Absolute magnitude (H)
- 20.45
Discovery & classification
- Discovered by
- Tholen, D. J.
- Discovery date
- 13 December 2004
- Discovery site
- Mauna Kea
Also known as 2004 XZ130
Close approaches 418 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-04 00:02 UTC close approach of 164294. Catalogue miss distance 76.4 LD · 2.94 × 10⁷ km. The curve is the geocentric path from 2026-11-01 to 2026-11-07, 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 |
|---|---|---|---|---|
| 2026-11-04 00:02:00 | Earth | 0.1963 AU | 76.4 LD | 11.2 km/s |
| 2026-11-15 11:43:00 | Venus | 0.1272 AU | 49.5 LD | 11.6 km/s |
| 2027-10-31 01:31:00 | Earth | 0.3479 AU | 135.4 LD | 17 km/s |
| 2029-05-10 06:12:00 | Venus | 0.0908 AU | 35.3 LD | 19.3 km/s |
| 2031-01-23 13:23:00 | Venus | 0.0991 AU | 38.6 LD | 12 km/s |
| 2036-02-13 01:08:00 | Venus | 0.0844 AU | 32.8 LD | 12.1 km/s |
| 2037-10-28 14:17:00 | Venus | 0.1109 AU | 43.2 LD | 19.4 km/s |
| 2039-11-01 15:35:00 | Earth | 0.3801 AU | 147.9 LD | 18.7 km/s |
| 2040-01-19 01:52:00 | Earth | 0.4578 AU | 178.2 LD | 7.5 km/s |
| 2040-04-22 08:47:00 | Venus | 0.1355 AU | 52.7 LD | 11.5 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