2025 VR1 is an asteroid in the Aten orbit class. Its orbit takes it from 0.73 AU to 1.25 AU from the Sun; one orbit takes 359.7 days. Orbit from the JPL solution of 13 November 2025.
Where is it now
- Distance from Sun
- 1.02 AU
- True anomaly
- 248.44°
- Distance from Earth
- 0.095 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 01m 10s
- Declination
- +20° 59′ 19″
- Constellation
- Cancer
- Distance from Earth
- 0.09 AU
- Elongation from the Sun
- 102.93° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 0.99 AU
- Eccentricity
- 0.2635
- Inclination
- 3.9°
- Orbital period
- 359.7 days
- Perihelion
- 0.729 AU
- Aphelion
- 1.251 AU
- Longitude of ascending node
- 226.77°
- Argument of periapsis
- 290.3°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 2.2 LD
- 0.0057 AU
- Tisserand (Jupiter)
- 6.096
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 23
- Data arc
- 2 days
- First observed
- 10 November 2025
- Last observed
- 12 November 2025
- Residual RMS
- 0.35 ″
- Solution · Otto Matic
- 13 November 2025
Visual & observation
- Absolute magnitude (H)
- 27.34
Discovery & classification
Close approaches 51 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-11 02:46 UTC close approach of 2025 VR1. Catalogue miss distance 39.0 LD · 1.5 × 10⁷ km. The curve is the geocentric path from 2026-11-08 to 2026-11-14, 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 |
|---|---|---|---|---|
| 2026-11-11 02:46:00 | Earth | 0.1002 AU | 39.0 LD | 10.8 km/s |
| 2027-11-07 12:12:00 | Earth | 0.1969 AU | 76.6 LD | 13.7 km/s |
| 2079-06-23 03:30:00 | Earth | 0.1254 AU | 48.8 LD | 11.2 km/s |
| 2080-06-18 13:48:00 | Earth | 0.0539 AU | 21.0 LD | 8.7 km/s |
| 2081-06-15 10:38:00 | Earth | 0.0681 AU | 26.5 LD | 6.4 km/s |
| 2083-07-21 13:59:00 | Earth | 0.1994 AU | 77.6 LD | 5.5 km/s |
| 2089-10-18 03:12:00 | Earth | 0.1786 AU | 69.5 LD | 5.6 km/s |
| 2089-12-30 02:25:00 | Earth | 0.1965 AU | 76.5 LD | 5.6 km/s |
| 2090-11-09 06:04:00 | Earth | 0.1127 AU | 43.8 LD | 5.1 km/s |
| 2091-11-15 06:55:00 | Earth | 0.0291 AU | 11.3 LD | 7.1 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