Where is it now
- Distance from Sun
- 0.658 AU
- True anomaly
- 296.29°
- Distance from Earth
- 1.105 AU
- As of
- 21 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 35m 26s
- Declination
- +02° 23′ 41″
- Constellation
- Leo
- Distance from Earth
- 1.11 AU
- Elongation from the Sun
- 35.64° — 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
- 0.929 AU
- Eccentricity
- 0.4048
- Inclination
- 2.2°
- Orbital period
- 326.9 days
- Perihelion
- 0.553 AU
- Aphelion
- 1.305 AU
- Longitude of ascending node
- 280.19°
- Argument of periapsis
- 252.98°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.8 LD
- 0.0124 AU
- Tisserand (Jupiter)
- 6.375
Orbit quality
Orbit reasonably well determined (uncertainty code 4).
- Observations used
- 30
- Data arc
- 32 days
- First observed
- 11 October 2024
- Last observed
- 12 November 2024
- Residual RMS
- 0.45 ″
- Solution · Otto Matic
- 12 November 2024
Visual & observation
- Absolute magnitude (H)
- 23.99
Discovery & classification
Close approaches 126 on record
Top-down view of the ecliptic, Earth at the centre, for the 2031-07-21 17:54 UTC close approach of 2024 UK5. Catalogue miss distance 8.54 LD · 3.28 × 10⁶ km. The curve is the geocentric path from 2031-07-18 to 2031-07-24, 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 |
|---|---|---|---|---|
| 2029-08-26 23:28:00 | Venus | 0.0154 AU | 6.0 LD | 14 km/s |
| 2031-07-21 17:54:00 | Earth | 0.0219 AU | 8.5 LD | 11.3 km/s |
| 2032-04-12 17:51:00 | Earth | 0.4273 AU | 166.3 LD | 15.9 km/s |
| 2032-09-25 04:51:00 | Earth | 0.2978 AU | 115.9 LD | 9.5 km/s |
| 2033-02-01 01:06:00 | Earth | 0.3905 AU | 152.0 LD | 14 km/s |
| 2033-11-09 10:28:00 | Earth | 0.1493 AU | 58.1 LD | 16.3 km/s |
| 2039-07-01 06:46:00 | Venus | 0.0154 AU | 6.0 LD | 14.1 km/s |
| 2039-07-31 19:37:00 | Earth | 0.2851 AU | 110.9 LD | 20.5 km/s |
| 2040-05-26 06:55:00 | Earth | 0.3328 AU | 129.5 LD | 9.1 km/s |
| 2040-08-21 00:35:00 | Earth | 0.2592 AU | 100.9 LD | 8.9 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