2020 VN1 is an asteroid in the Aten orbit class. Its orbit takes it from 0.92 AU to 1.04 AU from the Sun; one orbit takes 354.4 days. Orbit from the JPL solution of 13 April 2022.
Where is it now
- Distance from Sun
- 1.038 AU
- True anomaly
- 160.38°
- Distance from Earth
- 1.001 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
- 10h 42m 57s
- Declination
- +11° 23′ 20″
- Constellation
- Leo
- Distance from Earth
- 1 AU
- Elongation from the Sun
- 62.81° — 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
- 0.98 AU
- Eccentricity
- 0.0633
- Inclination
- 3.51°
- Orbital period
- 354.4 days
- Perihelion
- 0.918 AU
- Aphelion
- 1.042 AU
- Longitude of ascending node
- 43.92°
- Argument of periapsis
- 255.06°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.1 LD
- 0.0004 AU
- Tisserand (Jupiter)
- 6.173
Orbit quality
Orbit very well determined (uncertainty code 2).
- Observations used
- 146
- Data arc
- 500 days
- First observed
- 8 November 2020
- Last observed
- 23 March 2022
- Residual RMS
- 0.35 ″
- Solution · Otto Matic
- 13 April 2022
Visual & observation
- Absolute magnitude (H)
- 27.93
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 63 on record
Top-down view of the ecliptic, Earth at the centre, for the 2051-11-16 23:06 UTC close approach of 2020 VN1. Catalogue miss distance 144.5 LD · 5.56 × 10⁷ km. The curve is the geocentric path from 2051-11-13 to 2051-11-19, 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 |
|---|---|---|---|---|
| 2051-11-16 23:06:00 | Earth | 0.3714 AU | 144.5 LD | 13.7 km/s |
| 2052-11-09 12:44:00 | Earth | 0.1888 AU | 73.5 LD | 8.2 km/s |
| 2053-11-05 07:40:00 | Earth | 0.0083 AU | 3.2 LD | 3.2 km/s |
| 2054-11-05 18:18:00 | Earth | 0.031 AU | 12.1 LD | 2.3 km/s |
| 2055-09-09 01:19:00 | Earth | 0.0898 AU | 34.9 LD | 2.1 km/s |
| 2055-12-22 03:36:00 | Earth | 0.0825 AU | 32.1 LD | 2.2 km/s |
| 2056-07-23 14:31:00 | Earth | 0.1028 AU | 40.0 LD | 2.5 km/s |
| 2057-02-08 21:46:00 | Earth | 0.0916 AU | 35.6 LD | 2.1 km/s |
| 2057-06-11 23:48:00 | Earth | 0.0859 AU | 33.4 LD | 2.4 km/s |
| 2058-04-28 17:46:00 | Earth | 0.0407 AU | 15.8 LD | 2.3 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