2022 VR1 is an asteroid in the Aten orbit class. Its orbit takes it from 0.83 AU to 1.16 AU from the Sun; one orbit takes 361.8 days. Orbit from the JPL solution of 12 November 2023.
Where is it now
- Distance from Sun
- 1.005 AU
- True anomaly
- 256.46°
- Distance from Earth
- 0.165 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
- 09h 07m 41s
- Declination
- +24° 17′ 19″
- Constellation
- Cancer
- Distance from Earth
- 0.16 AU
- Elongation from the Sun
- 89.07° — 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
- 0.994 AU
- Eccentricity
- 0.1677
- Inclination
- 5.83°
- Orbital period
- 361.8 days
- Perihelion
- 0.827 AU
- Aphelion
- 1.16 AU
- Longitude of ascending node
- 242.55°
- Argument of periapsis
- 270.61°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 4.3 LD
- 0.011 AU
- Tisserand (Jupiter)
- 6.093
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 98
- Data arc
- 377 days
- First observed
- 31 October 2022
- Last observed
- 12 November 2023
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 12 November 2023
Visual & observation
- Absolute magnitude (H)
- 24.79
Discovery & classification
Close approaches 141 on record
Top-down view of the ecliptic, Earth at the centre, for the 2026-11-12 06:10 UTC close approach of 2022 VR1. Catalogue miss distance 68.7 LD · 2.64 × 10⁷ km. The curve is the geocentric path from 2026-11-09 to 2026-11-15, 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 |
|---|---|---|---|---|
| 2026-11-12 06:10:00 | Earth | 0.1766 AU | 68.7 LD | 10.5 km/s |
| 2027-11-09 16:37:00 | Earth | 0.237 AU | 92.2 LD | 12.2 km/s |
| 2028-11-06 01:57:00 | Earth | 0.2988 AU | 116.3 LD | 14.1 km/s |
| 2029-11-03 11:59:00 | Earth | 0.3614 AU | 140.6 LD | 16 km/s |
| 2030-10-31 18:20:00 | Earth | 0.4246 AU | 165.2 LD | 17.8 km/s |
| 2031-10-28 23:04:00 | Earth | 0.4878 AU | 189.8 LD | 19.7 km/s |
| 2104-07-01 01:16:00 | Earth | 0.4571 AU | 177.9 LD | 18.5 km/s |
| 2105-06-28 08:45:00 | Earth | 0.3948 AU | 153.7 LD | 16.6 km/s |
| 2106-06-25 13:55:00 | Earth | 0.3329 AU | 129.5 LD | 14.8 km/s |
| 2107-06-22 20:08:00 | Earth | 0.2714 AU | 105.6 LD | 13 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