Where is it now
- Distance from Sun
- 0.697 AU
- True anomaly
- 339.61°
- Distance from Earth
- 1.152 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
- 16h 16m 26s
- Declination
- -14° 42′ 40″
- Constellation
- Scorpius
- Distance from Earth
- 1.15 AU
- Elongation from the Sun
- 36.99° — 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
- 0.907 AU
- Eccentricity
- 0.2405
- Inclination
- 14.07°
- Orbital period
- 315.5 days
- Perihelion
- 0.689 AU
- Aphelion
- 1.125 AU
- Longitude of ascending node
- 255.27°
- Argument of periapsis
- 70.63°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 15.6 LD
- 0.0401 AU
- Tisserand (Jupiter)
- 6.523
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 90
- Data arc
- 7.25 years
- First observed
- 23 December 2014
- Last observed
- 23 March 2022
- Residual RMS
- 0.41 ″
- Solution · Otto Matic
- 1 March 2023
Visual & observation
- Absolute magnitude (H)
- 21.58
Discovery & classification
Close approaches 160 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-01-05 18:01 UTC close approach of 2015 AH. Catalogue miss distance 96.0 LD · 3.69 × 10⁷ km. The curve is the geocentric path from 2028-01-02 to 2028-01-08, 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 |
|---|---|---|---|---|
| 2028-01-05 18:01:00 | Earth | 0.2466 AU | 96.0 LD | 7.4 km/s |
| 2028-06-10 14:34:00 | Earth | 0.2483 AU | 96.6 LD | 10.1 km/s |
| 2033-12-15 11:18:00 | Earth | 0.0569 AU | 22.2 LD | 11.2 km/s |
| 2034-07-26 15:01:00 | Earth | 0.3535 AU | 137.6 LD | 11.3 km/s |
| 2035-04-12 13:13:00 | Earth | 0.3172 AU | 123.4 LD | 16.7 km/s |
| 2039-12-29 03:48:00 | Earth | 0.3653 AU | 142.2 LD | 20 km/s |
| 2040-09-14 23:21:00 | Earth | 0.3669 AU | 142.8 LD | 9.6 km/s |
| 2041-05-09 01:33:00 | Earth | 0.1643 AU | 63.9 LD | 9.9 km/s |
| 2046-12-11 18:02:00 | Earth | 0.1533 AU | 59.7 LD | 7.8 km/s |
| 2047-06-28 10:36:00 | Earth | 0.2943 AU | 114.5 LD | 10.7 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