Where is it now
- Distance from Sun
- 0.669 AU
- True anomaly
- 21.68°
- Distance from Earth
- 1.424 AU
- As of
- 19 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
- 14h 55m 46s
- Declination
- -28° 53′ 14″
- Constellation
- Hydra
- Distance from Earth
- 1.42 AU
- Elongation from the Sun
- 25.34° — 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
- 0.865 AU
- Eccentricity
- 0.2377
- Inclination
- 30.88°
- Orbital period
- 294 days
- Perihelion
- 0.66 AU
- Aphelion
- 1.071 AU
- Longitude of ascending node
- 37.21°
- Argument of periapsis
- 212.63°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 10.0 LD
- 0.0258 AU
- Tisserand (Jupiter)
- 6.693
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 54
- Data arc
- 18 days
- First observed
- 4 November 2023
- Last observed
- 22 November 2023
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 22 November 2023
Visual & observation
- Absolute magnitude (H)
- 23.22
Discovery & classification
Close approaches 97 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-11-01 16:46 UTC close approach of 2023 VH1. Catalogue miss distance 73.1 LD · 2.81 × 10⁷ km. The curve is the geocentric path from 2027-10-29 to 2027-11-04, 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. At closest approach the object is south of the ecliptic. 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 |
|---|---|---|---|---|
| 2027-11-01 16:46:00 | Earth | 0.1878 AU | 73.1 LD | 18.9 km/s |
| 2028-05-01 04:36:00 | Earth | 0.3338 AU | 129.9 LD | 20.8 km/s |
| 2031-11-04 23:07:00 | Earth | 0.3268 AU | 127.2 LD | 21.9 km/s |
| 2032-05-15 10:41:00 | Earth | 0.3754 AU | 146.1 LD | 20.8 km/s |
| 2035-11-09 01:28:00 | Earth | 0.4663 AU | 181.5 LD | 25.5 km/s |
| 2038-10-16 00:00:00 | Venus | 0.1345 AU | 52.4 LD | 21.8 km/s |
| 2040-11-08 20:05:00 | Earth | 0.4556 AU | 177.3 LD | 17.8 km/s |
| 2044-11-03 12:35:00 | Earth | 0.335 AU | 130.4 LD | 16.3 km/s |
| 2048-10-31 03:02:00 | Earth | 0.2087 AU | 81.2 LD | 15.5 km/s |
| 2052-10-29 16:41:00 | Earth | 0.0847 AU | 33.0 LD | 15.6 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