2022 VN1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.69 AU to 1.38 AU from the Sun; one orbit takes 384 days. Orbit from the JPL solution of 12 January 2023.
Where is it now
- Distance from Sun
- 0.709 AU
- True anomaly
- 331.62°
- Distance from Earth
- 1.514 AU
- As of
- 3 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
- 16h 14m 23s
- Declination
- -17° 39′ 07″
- Constellation
- Scorpius
- Distance from Earth
- 1.51 AU
- Elongation from the Sun
- 22.89° — near the Sun — look low at dusk or dawn
Favours the southern hemisphere; low or below the horizon from far north.
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
- 1.034 AU
- Eccentricity
- 0.3346
- Inclination
- 10.07°
- Orbital period
- 384 days
- Perihelion
- 0.688 AU
- Aphelion
- 1.38 AU
- Longitude of ascending node
- 230.03°
- Argument of periapsis
- 74.94°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 2.6 LD
- 0.0066 AU
- Tisserand (Jupiter)
- 5.86
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 239
- Data arc
- 11 days
- First observed
- 12 November 2022
- Last observed
- 23 November 2022
- Residual RMS
- 0.28 ″
- Solution · Otto Matic
- 12 January 2023
Visual & observation
- Absolute magnitude (H)
- 25.06
Discovery & classification
Close approaches 110 on record
Top-down view of the ecliptic, Earth at the centre, for the 2037-03-25 00:12 UTC close approach of 2022 VN1. Catalogue miss distance 175.8 LD · 6.76 × 10⁷ km. The curve is the geocentric path from 2037-03-22 to 2037-03-28, 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 |
|---|---|---|---|---|
| 2035-05-20 12:54:00 | Venus | 0.1493 AU | 58.1 LD | 10.2 km/s |
| 2037-03-25 00:12:00 | Earth | 0.4519 AU | 175.8 LD | 24.7 km/s |
| 2038-04-09 06:02:00 | Earth | 0.1537 AU | 59.8 LD | 15.4 km/s |
| 2039-05-08 20:57:00 | Earth | 0.1946 AU | 75.7 LD | 8.3 km/s |
| 2040-02-21 21:09:00 | Earth | 0.4086 AU | 159.0 LD | 8.8 km/s |
| 2040-07-06 01:21:00 | Earth | 0.3403 AU | 132.4 LD | 11.9 km/s |
| 2041-01-20 10:31:00 | Earth | 0.4405 AU | 171.4 LD | 9.7 km/s |
| 2041-08-22 12:14:00 | Earth | 0.3422 AU | 133.2 LD | 11.2 km/s |
| 2041-12-20 05:33:00 | Earth | 0.3661 AU | 142.5 LD | 9 km/s |
| 2042-07-28 13:57:00 | Venus | 0.0745 AU | 29.0 LD | 10.5 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