Where is it now
- Distance from Sun
- 0.844 AU
- True anomaly
- 238.57°
- Distance from Earth
- 1.182 AU
- As of
- 16 October 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 43m 39s
- Declination
- +08° 15′ 25″
- Constellation
- Leo
- Distance from Earth
- 1.18 AU
- Elongation from the Sun
- 44.48° — near the Sun — look low at dusk or dawn
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
- 0.782 AU
- Eccentricity
- 0.2841
- Inclination
- 0.54°
- Orbital period
- 252.5 days
- Perihelion
- 0.56 AU
- Aphelion
- 1.004 AU
- Longitude of ascending node
- 310.35°
- Argument of periapsis
- 273.87°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 3.4 LD
- 0.0087 AU
- Tisserand (Jupiter)
- 7.398
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 32
- Data arc
- 7 days
- First observed
- 5 November 2023
- Last observed
- 12 November 2023
- Residual RMS
- 0.59 ″
- Solution · Otto Matic
- 9 December 2023
Visual & observation
- Absolute magnitude (H)
- 26.97
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 88 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-05-07 21:44 UTC close approach of 2023 VC2. Catalogue miss distance 174.8 LD · 6.72 × 10⁷ km. The curve is the geocentric path from 2028-05-04 to 2028-05-10, 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 |
|---|---|---|---|---|
| 2028-05-07 21:44:00 | Earth | 0.4492 AU | 174.8 LD | 15.6 km/s |
| 2029-02-24 10:09:00 | Venus | 0.0687 AU | 26.7 LD | 12.8 km/s |
| 2030-06-28 05:15:00 | Earth | 0.4035 AU | 157.0 LD | 11.9 km/s |
| 2030-11-26 04:41:00 | Earth | 0.4079 AU | 158.7 LD | 19.1 km/s |
| 2034-09-08 06:08:00 | Venus | 0.0703 AU | 27.4 LD | 12.9 km/s |
| 2034-10-19 02:14:00 | Earth | 0.3519 AU | 137.0 LD | 17.3 km/s |
| 2035-03-16 01:12:00 | Earth | 0.3877 AU | 150.9 LD | 11.6 km/s |
| 2037-05-08 15:21:00 | Earth | 0.448 AU | 174.3 LD | 15.5 km/s |
| 2039-05-21 03:54:00 | Venus | 0.146 AU | 56.8 LD | 8.6 km/s |
| 2039-07-02 15:20:00 | Earth | 0.3933 AU | 153.1 LD | 11.3 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