Where is it now
- Distance from Sun
- 1.107 AU
- True anomaly
- 225.35°
- Distance from Earth
- 0.593 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
- 19h 36m 57s
- Declination
- -13° 08′ 43″
- Constellation
- Sagittarius
- Distance from Earth
- 0.59 AU
- Elongation from the Sun
- 84.01° — well clear of the Sun
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
- 0.954 AU
- Eccentricity
- 0.3325
- Inclination
- 4.58°
- Orbital period
- 340.1 days
- Perihelion
- 0.636 AU
- Aphelion
- 1.271 AU
- Longitude of ascending node
- 254.51°
- Argument of periapsis
- 237.5°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 1.6 LD
- 0.0042 AU
- Tisserand (Jupiter)
- 6.262
Orbit quality
Orbit poorly determined (uncertainty code 6).
- Observations used
- 48
- Data arc
- 17 days
- First observed
- 14 June 2025
- Last observed
- 1 July 2025
- Residual RMS
- 0.43 ″
- Solution · Otto Matic
- 6 July 2025
Visual & observation
- Absolute magnitude (H)
- 24.93
Discovery & classification
Close approaches 28 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-09-28 03:49 UTC close approach of 2025 LW. Catalogue miss distance 66.9 LD · 2.57 × 10⁷ km. The curve is the geocentric path from 2027-09-25 to 2027-10-01, 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 |
|---|---|---|---|---|
| 2027-09-28 03:49:00 | Earth | 0.1718 AU | 66.9 LD | 6.2 km/s |
| 2039-06-16 19:07:00 | Earth | 0.1616 AU | 62.9 LD | 6.6 km/s |
| 2041-10-09 11:20:00 | Earth | 0.0743 AU | 28.9 LD | 10.4 km/s |
| 2048-05-27 04:17:00 | Venus | 0.0839 AU | 32.6 LD | 14.4 km/s |
| 2050-04-09 04:38:00 | Venus | 0.0197 AU | 7.7 LD | 9.9 km/s |
| 2052-03-11 20:38:00 | Venus | 0.1104 AU | 43.0 LD | 8.5 km/s |
| 2052-06-02 01:13:00 | Earth | 0.0108 AU | 4.2 LD | 10 km/s |
| 2052-06-02 01:13:00 | Moon | 0.0086 AU | 3.3 LD | 9 km/s |
| 2054-03-02 12:33:00 | Venus | 0.0968 AU | 37.7 LD | 11.6 km/s |
| 2055-10-06 05:39:00 | Earth | 0.1672 AU | 65.1 LD | 14.2 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