Where is it now
- Distance from Sun
- 0.989 AU
- True anomaly
- 215.62°
- Distance from Earth
- 1.882 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
- 12h 37m 09s
- Declination
- -00° 31′ 41″
- Constellation
- Virgo
- Distance from Earth
- 1.88 AU
- Elongation from the Sun
- 18.5° — 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
- 0.852 AU
- Eccentricity
- 0.2225
- Inclination
- 6.4°
- Orbital period
- 287.4 days
- Perihelion
- 0.663 AU
- Aphelion
- 1.042 AU
- Longitude of ascending node
- 98.3°
- Argument of periapsis
- 215.87°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.0 LD
- 0.0027 AU
- Tisserand (Jupiter)
- 6.889
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 40
- Data arc
- 19 days
- First observed
- 3 January 2025
- Last observed
- 22 January 2025
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 27 January 2025
Visual & observation
- Absolute magnitude (H)
- 26.89
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2035-12-26 08:22 UTC close approach of 2025 AC1. Catalogue miss distance 32.5 LD · 1.25 × 10⁷ km. The curve is the geocentric path from 2035-12-23 to 2035-12-29, 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 |
|---|---|---|---|---|
| 2031-02-05 12:49:00 | Venus | 0.0633 AU | 24.6 LD | 9.1 km/s |
| 2035-12-26 08:22:00 | Earth | 0.0836 AU | 32.5 LD | 8.7 km/s |
| 2036-07-04 17:32:00 | Venus | 0.064 AU | 24.9 LD | 6 km/s |
| 2040-03-08 22:02:00 | Earth | 0.1125 AU | 43.8 LD | 6.7 km/s |
| 2041-12-13 06:48:00 | Venus | 0.0605 AU | 23.5 LD | 9.4 km/s |
| 2050-10-12 14:03:00 | Venus | 0.0524 AU | 20.4 LD | 8.3 km/s |
| 2051-02-05 10:35:00 | Earth | 0.0935 AU | 36.4 LD | 5.3 km/s |
| 2056-03-10 10:35:00 | Venus | 0.0637 AU | 24.8 LD | 6 km/s |
| 2061-08-19 09:34:00 | Venus | 0.0756 AU | 29.4 LD | 10.2 km/s |
| 2061-12-28 07:27:00 | Earth | 0.0059 AU | 2.3 LD | 6.5 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