2023 VR5 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.91 AU to 1.11 AU from the Sun; one orbit takes 371 days. Orbit from the JPL solution of 1 December 2023.
Where is it now
- Distance from Sun
- 1.058 AU
- True anomaly
- 237.48°
- Distance from Earth
- 0.39 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
- 20h 51m 49s
- Declination
- -18° 30′ 57″
- Constellation
- Capricornus
- Distance from Earth
- 0.39 AU
- Elongation from the Sun
- 88.73° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
From your location
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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
- 1.01 AU
- Eccentricity
- 0.1022
- Inclination
- 1.23°
- Orbital period
- 371 days
- Perihelion
- 0.907 AU
- Aphelion
- 1.114 AU
- Longitude of ascending node
- 35.14°
- Argument of periapsis
- 107.09°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 3.3 LD
- 0.0084 AU
- Tisserand (Jupiter)
- 6.026
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 23
- Data arc
- 14 days
- First observed
- 9 November 2023
- Last observed
- 23 November 2023
- Residual RMS
- 0.49 ″
- Solution · Otto Matic
- 1 December 2023
Visual & observation
- Absolute magnitude (H)
- 27.69
Discovery & classification
Close approaches 24 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-05-24 02:12 UTC close approach of 2023 VR5. Catalogue miss distance 32.1 LD · 1.23 × 10⁷ km. The curve is the geocentric path from 2027-05-21 to 2027-05-27, 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 |
|---|---|---|---|---|
| 2027-05-24 02:12:00 | Earth | 0.0824 AU | 32.1 LD | 5.1 km/s |
| 2028-05-28 20:21:00 | Earth | 0.193 AU | 75.1 LD | 8.4 km/s |
| 2029-06-03 15:31:00 | Earth | 0.3062 AU | 119.2 LD | 11.7 km/s |
| 2030-06-09 09:23:00 | Earth | 0.42 AU | 163.5 LD | 15 km/s |
| 2073-10-31 12:27:00 | Earth | 0.4684 AU | 182.3 LD | 16.8 km/s |
| 2074-11-06 04:16:00 | Earth | 0.3523 AU | 137.1 LD | 13.3 km/s |
| 2075-11-12 04:07:00 | Earth | 0.2357 AU | 91.7 LD | 9.8 km/s |
| 2076-11-16 14:59:00 | Earth | 0.1209 AU | 47.0 LD | 6.3 km/s |
| 2077-11-21 12:03:00 | Earth | 0.0152 AU | 5.9 LD | 3.1 km/s |
| 2078-11-21 13:13:00 | Earth | 0.0211 AU | 8.2 LD | 2.2 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