2023 VR1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.71 AU to 1.36 AU from the Sun; one orbit takes 385.7 days. Orbit from the JPL solution of 18 November 2023.
Where is it now
- Distance from Sun
- 0.749 AU
- True anomaly
- 36.56°
- Distance from Earth
- 1.087 AU
- As of
- 4 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
- 17h 35m 57s
- Declination
- -21° 33′ 41″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.09 AU
- Elongation from the Sun
- 41.99° — 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
- 1.037 AU
- Eccentricity
- 0.3113
- Inclination
- 2.71°
- Orbital period
- 385.7 days
- Perihelion
- 0.714 AU
- Aphelion
- 1.36 AU
- Longitude of ascending node
- 216.88°
- Argument of periapsis
- 73.02°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.9 LD
- 0.005 AU
- Tisserand (Jupiter)
- 5.865
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 33
- Data arc
- 9 days
- First observed
- 4 November 2023
- Last observed
- 13 November 2023
- Residual RMS
- 0.38 ″
- Solution · Otto Matic
- 18 November 2023
Visual & observation
- Absolute magnitude (H)
- 25.83
Discovery & classification
Close approaches 22 on record
Top-down view of the ecliptic, Earth at the centre, for the 2038-03-20 08:45 UTC close approach of 2023 VR1. Catalogue miss distance 89.4 LD · 3.44 × 10⁷ km. The curve is the geocentric path from 2038-03-17 to 2038-03-23, 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 |
|---|---|---|---|---|
| 2027-10-13 13:40:00 | Venus | 0.1416 AU | 55.1 LD | 13.9 km/s |
| 2035-03-04 15:18:00 | Venus | 0.0964 AU | 37.5 LD | 11.7 km/s |
| 2038-03-20 08:45:00 | Earth | 0.2297 AU | 89.4 LD | 16.9 km/s |
| 2039-04-03 19:08:00 | Earth | 0.1152 AU | 44.8 LD | 6.7 km/s |
| 2042-10-23 07:23:00 | Earth | 0.0427 AU | 16.6 LD | 8.8 km/s |
| 2043-11-05 19:52:00 | Earth | 0.2882 AU | 112.2 LD | 18.7 km/s |
| 2049-12-05 10:48:00 | Venus | 0.1433 AU | 55.8 LD | 14 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