Where is it now
- Distance from Sun
- 0.828 AU
- True anomaly
- 239.12°
- Distance from Earth
- 1.212 AU
- As of
- 16 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 01m 07s
- Declination
- +12° 35′ 40″
- Constellation
- Leo
- Distance from Earth
- 1.21 AU
- Elongation from the Sun
- 42.53° — 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
- 0.785 AU
- Eccentricity
- 0.4052
- Inclination
- 8.62°
- Orbital period
- 254.1 days
- Perihelion
- 0.467 AU
- Aphelion
- 1.103 AU
- Longitude of ascending node
- 9.89°
- Argument of periapsis
- 216.9°
- Epoch · J2000
- 2460973.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.5 LD
- 0.0116 AU
- Tisserand (Jupiter)
- 7.33
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 16
- Data arc
- 9 days
- First observed
- 19 October 2025
- Last observed
- 28 October 2025
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 28 October 2025
Visual & observation
- Absolute magnitude (H)
- 26.16
Discovery & classification
Close approaches 39 on record
Top-down view of the ecliptic, Earth at the centre, for the 2039-12-14 10:57 UTC close approach of 2025 UN7. Catalogue miss distance 60.7 LD · 2.33 × 10⁷ km. The curve is the geocentric path from 2039-12-11 to 2039-12-17, 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 |
|---|---|---|---|---|
| 2028-03-27 05:47:00 | Venus | 0.1341 AU | 52.2 LD | 10.4 km/s |
| 2032-07-12 01:36:00 | Mercury | 0.0557 AU | 21.7 LD | 16.6 km/s |
| 2032-07-12 01:36:00 | Merc | 0.0557 AU | 21.7 LD | 16.6 km/s |
| 2034-09-14 23:10:00 | Venus | 0.0787 AU | 30.6 LD | 12 km/s |
| 2038-08-29 22:49:00 | Venus | 0.0793 AU | 30.9 LD | 17.4 km/s |
| 2039-12-14 10:57:00 | Earth | 0.1559 AU | 60.7 LD | 12.2 km/s |
| 2040-04-04 11:18:00 | Venus | 0.1307 AU | 50.8 LD | 21.3 km/s |
| 2041-10-08 01:27:00 | Earth | 0.0223 AU | 8.7 LD | 10.5 km/s |
| 2048-11-22 04:04:00 | Earth | 0.1527 AU | 59.4 LD | 8.7 km/s |
| 2050-09-13 07:42:00 | Venus | 0.1278 AU | 49.8 LD | 10 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