2026 JV1 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.72 AU to 1.33 AU from the Sun; one orbit takes 379.6 days. Orbit from the JPL solution of 26 May 2026.
Where is it now
- Distance from Sun
- 1.128 AU
- True anomaly
- 125.14°
- Distance from Earth
- 1.077 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
- 10h 36m 22s
- Declination
- +12° 55′ 02″
- Constellation
- Leo
- Distance from Earth
- 1.08 AU
- Elongation from the Sun
- 66.19° — 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
- 1.026 AU
- Eccentricity
- 0.2962
- Inclination
- 5.55°
- Orbital period
- 379.6 days
- Perihelion
- 0.722 AU
- Aphelion
- 1.33 AU
- Longitude of ascending node
- 61.54°
- Argument of periapsis
- 275.37°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 5.7 LD
- 0.0146 AU
- Tisserand (Jupiter)
- 5.916
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 45
- Data arc
- 4 days
- First observed
- 10 May 2026
- Last observed
- 14 May 2026
- Residual RMS
- 0.37 ″
- Solution · Otto Matic
- 26 May 2026
Visual & observation
- Absolute magnitude (H)
- 25.77
Discovery & classification
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2030-11-30 05:06 UTC close approach of 2026 JV1. Catalogue miss distance 57.4 LD · 2.21 × 10⁷ km. The curve is the geocentric path from 2030-11-27 to 2030-12-03, 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 |
|---|---|---|---|---|
| 2030-11-30 05:06:00 | Earth | 0.1476 AU | 57.4 LD | 5.7 km/s |
| 2031-12-12 05:53:00 | Earth | 0.104 AU | 40.5 LD | 12.7 km/s |
| 2035-11-12 14:08:00 | Venus | 0.143 AU | 55.7 LD | 12.6 km/s |
| 2039-02-03 19:05:00 | Venus | 0.0774 AU | 30.1 LD | 9.5 km/s |
| 2052-05-12 06:15:00 | Earth | 0.0476 AU | 18.5 LD | 11 km/s |
| 2052-07-28 23:45:00 | Venus | 0.0256 AU | 10.0 LD | 5.3 km/s |
| 2053-05-06 23:19:00 | Earth | 0.1898 AU | 73.9 LD | 5.5 km/s |
| 2053-06-10 04:27:00 | Earth | 0.1907 AU | 74.2 LD | 5.6 km/s |
| 2057-12-08 09:42:00 | Earth | 0.0307 AU | 11.9 LD | 10.2 km/s |
| 2066-01-05 23:14:00 | Venus | 0.1139 AU | 44.3 LD | 11.1 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