Where is it now
- Distance from Sun
- 1.338 AU
- True anomaly
- 197.06°
- Distance from Earth
- 1.64 AU
- As of
- 22 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
- 10h 19m 28s
- Declination
- +04° 33′ 38″
- Constellation
- Sextans
- Distance from Earth
- 1.64 AU
- Elongation from the Sun
- 54.69° — 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
- 0.943 AU
- Eccentricity
- 0.4767
- Inclination
- 13.13°
- Orbital period
- 334.3 days
- Perihelion
- 0.493 AU
- Aphelion
- 1.392 AU
- Longitude of ascending node
- 147.76°
- Argument of periapsis
- 131.88°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 11.7 LD
- 0.03 AU
- Tisserand (Jupiter)
- 6.249
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 21
- Data arc
- 2 days
- First observed
- 20 February 2025
- Last observed
- 22 February 2025
- Residual RMS
- 0.28 ″
- Solution · Otto Matic
- 22 February 2025
Visual & observation
- Absolute magnitude (H)
- 25.75
Discovery & classification
Close approaches 13 on record
Top-down view of the ecliptic, Earth at the centre, for the 2036-02-21 06:38 UTC close approach of 2025 DX2. Catalogue miss distance 44.5 LD · 1.71 × 10⁷ km. The curve is the geocentric path from 2036-02-18 to 2036-02-24, 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 north 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 |
|---|---|---|---|---|
| 2027-01-24 05:02:00 | Venus | 0.1434 AU | 55.8 LD | 24 km/s |
| 2036-02-21 06:38:00 | Earth | 0.1142 AU | 44.5 LD | 19.3 km/s |
| 2090-02-19 17:05:00 | Earth | 0.154 AU | 59.9 LD | 20.5 km/s |
| 2096-08-08 15:45:00 | Venus | 0.1374 AU | 53.5 LD | 13 km/s |
| 2098-06-10 02:56:00 | Venus | 0.0703 AU | 27.4 LD | 17.9 km/s |
| 2100-04-11 05:20:00 | Venus | 0.1276 AU | 49.7 LD | 23.1 km/s |
| 2111-02-25 14:53:00 | Earth | 0.1297 AU | 50.5 LD | 13 km/s |
| 2119-09-05 04:00:00 | Venus | 0.1112 AU | 43.3 LD | 22.3 km/s |
| 2122-02-25 15:34:00 | Earth | 0.043 AU | 16.7 LD | 15.3 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