2025 VN is an asteroid in the Aten orbit class. Its orbit takes it from 0.7 AU to 1.29 AU from the Sun; one orbit takes 361.8 days. Orbit from the JPL solution of 11 November 2025.
Where is it now
- Distance from Sun
- 1.005 AU
- True anomaly
- 250.47°
- Distance from Earth
- 0.048 AU
- As of
- 2 November 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
- 08h 05m 16s
- Declination
- +11° 15′ 12″
- Constellation
- Cancer
- Distance from Earth
- 0.04 AU
- Elongation from the Sun
- 100.05° — well clear of the Sun
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
- 0.994 AU
- Eccentricity
- 0.2991
- Inclination
- 12.92°
- Orbital period
- 361.8 days
- Perihelion
- 0.697 AU
- Aphelion
- 1.291 AU
- Longitude of ascending node
- 45.47°
- Argument of periapsis
- 106.9°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.1 LD
- 0.0002 AU
- Tisserand (Jupiter)
- 6.049
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 46
- First observed
- 7 November 2025
- Last observed
- 7 November 2025
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 11 November 2025
Visual & observation
- Absolute magnitude (H)
- 27.94
Discovery & classification
Close approaches 38 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-06 09:40 UTC close approach of 2025 VN. Catalogue miss distance 22.9 LD · 8.8 × 10⁶ km. The curve is the geocentric path from 2026-11-03 to 2026-11-09, 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 |
|---|---|---|---|---|
| 2026-11-06 09:40:00 | Earth | 0.0588 AU | 22.9 LD | 12.4 km/s |
| 2027-02-11 15:18:00 | Venus | 0.114 AU | 44.4 LD | 13.6 km/s |
| 2027-11-04 11:16:00 | Earth | 0.1203 AU | 46.8 LD | 14 km/s |
| 2028-11-01 05:34:00 | Earth | 0.1833 AU | 71.4 LD | 15.7 km/s |
| 2049-11-14 01:07:00 | Venus | 0.0663 AU | 25.8 LD | 11.3 km/s |
| 2067-09-04 18:45:00 | Venus | 0.1021 AU | 39.8 LD | 6.9 km/s |
| 2072-08-21 20:12:00 | Venus | 0.1202 AU | 46.8 LD | 13.9 km/s |
| 2090-06-12 11:05:00 | Venus | 0.0911 AU | 35.4 LD | 7.1 km/s |
| 2095-05-27 00:41:00 | Venus | 0.1035 AU | 40.3 LD | 13.2 km/s |
| 2101-06-13 12:35:00 | Earth | 0.1886 AU | 73.4 LD | 14.4 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