Where is it now
- Distance from Sun
- 0.979 AU
- True anomaly
- 210.99°
- Distance from Earth
- 1.838 AU
- As of
- 21 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 27m 22s
- Declination
- -02° 58′ 04″
- Constellation
- Virgo
- Distance from Earth
- 1.84 AU
- Elongation from the Sun
- 21.22° — 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
- 0.913 AU
- Eccentricity
- 0.0873
- Inclination
- 0.1°
- Orbital period
- 318.6 days
- Perihelion
- 0.833 AU
- Aphelion
- 0.993 AU
- Longitude of ascending node
- 333.95°
- Argument of periapsis
- 340.6°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 0.0 LD
- 0.0001 AU
- Tisserand (Jupiter)
- 6.534
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 55
- Data arc
- 16 days
- First observed
- 14 January 2024
- Last observed
- 30 January 2024
- Residual RMS
- 0.47 ″
- Solution · Otto Matic
- 30 January 2024
Visual & observation
- Absolute magnitude (H)
- 28.71
Discovery & classification
Listed by JPL impact monitoring; see the Sentry table for current probabilities.
Close approaches 31 on record
Top-down view of the ecliptic, Earth at the centre, for the 2030-10-18 02:36 UTC close approach of 2024 AM4. Catalogue miss distance 49.4 LD · 1.9 × 10⁷ km. The curve is the geocentric path from 2030-10-15 to 2030-10-21, 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 |
|---|---|---|---|---|
| 2029-09-17 07:34:00 | Venus | 0.1169 AU | 45.5 LD | 2.1 km/s |
| 2030-10-18 02:36:00 | Earth | 0.1268 AU | 49.4 LD | 2.5 km/s |
| 2031-03-07 04:08:00 | Earth | 0.0799 AU | 31.1 LD | 4.5 km/s |
| 2037-01-06 19:33:00 | Earth | 0.4464 AU | 173.7 LD | 16 km/s |
| 2037-08-18 18:32:00 | Earth | 0.18 AU | 70.1 LD | 4.6 km/s |
| 2038-03-02 09:10:00 | Earth | 0.2959 AU | 115.2 LD | 11.3 km/s |
| 2040-03-14 08:41:00 | Venus | 0.1092 AU | 42.5 LD | 1.6 km/s |
| 2043-12-30 04:11:00 | Earth | 0.2221 AU | 86.5 LD | 9 km/s |
| 2044-06-25 17:32:00 | Earth | 0.1702 AU | 66.2 LD | 4.1 km/s |
| 2050-09-13 04:43:00 | Venus | 0.1169 AU | 45.5 LD | 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