Where is it now
- Distance from Sun
- 1.068 AU
- True anomaly
- 174.2°
- Distance from Earth
- 2.037 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
- 13h 01m 53s
- Declination
- -08° 46′ 10″
- Constellation
- Virgo
- Distance from Earth
- 2.04 AU
- Elongation from the Sun
- 9.65° — too close to the Sun to observe
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
- 0.856 AU
- Eccentricity
- 0.2492
- Inclination
- 5.64°
- Orbital period
- 289.4 days
- Perihelion
- 0.643 AU
- Aphelion
- 1.069 AU
- Longitude of ascending node
- 231.47°
- Argument of periapsis
- 142.44°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.6 LD
- 0.0042 AU
- Tisserand (Jupiter)
- 6.859
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 16
- Data arc
- 2 days
- First observed
- 5 May 2025
- Last observed
- 7 May 2025
- Residual RMS
- 0.64 ″
- Solution · Otto Matic
- 6 May 2025
Visual & observation
- Absolute magnitude (H)
- 25.13
Discovery & classification
Close approaches 46 on record
Top-down view of the ecliptic, Earth at the centre, for the 2040-02-22 13:53 UTC close approach of 2025 JX1. Catalogue miss distance 37.4 LD · 1.44 × 10⁷ km. The curve is the geocentric path from 2040-02-19 to 2040-02-25, 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 |
|---|---|---|---|---|
| 2027-11-11 09:04:00 | Venus | 0.148 AU | 57.6 LD | 6.1 km/s |
| 2027-12-28 23:16:00 | Venus | 0.1225 AU | 47.7 LD | 7.5 km/s |
| 2033-07-28 04:43:00 | Venus | 0.1057 AU | 41.1 LD | 7.9 km/s |
| 2039-02-22 20:19:00 | Venus | 0.0756 AU | 29.4 LD | 7.9 km/s |
| 2040-02-22 13:53:00 | Earth | 0.096 AU | 37.4 LD | 6.3 km/s |
| 2044-05-02 15:42:00 | Earth | 0.0459 AU | 17.9 LD | 5.6 km/s |
| 2044-09-16 22:32:00 | Venus | 0.0325 AU | 12.6 LD | 8.6 km/s |
| 2048-05-09 19:51:00 | Earth | 0.1694 AU | 65.9 LD | 11.6 km/s |
| 2050-04-07 19:52:00 | Venus | 0.044 AU | 17.1 LD | 10.8 km/s |
| 2055-10-26 23:59:00 | Venus | 0.1317 AU | 51.3 LD | 14.8 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