2025 GL is an asteroid in the Apollo orbit class. Its orbit takes it from 0.82 AU to 1.19 AU from the Sun; one orbit takes 368.2 days. Orbit from the JPL solution of 20 April 2025.
Where is it now
- Distance from Sun
- 0.986 AU
- True anomaly
- 265.56°
- Distance from Earth
- 0.721 AU
- As of
- 3 November 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 25m 47s
- Declination
- -23° 52′ 50″
- Constellation
- Sagittarius
- Distance from Earth
- 0.72 AU
- Elongation from the Sun
- 68.15° — well clear of the Sun
Favours the southern hemisphere; low or below the horizon from far north.
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
- 1.005 AU
- Eccentricity
- 0.1833
- Inclination
- 5.3°
- Orbital period
- 368.2 days
- Perihelion
- 0.821 AU
- Aphelion
- 1.19 AU
- Longitude of ascending node
- 13.7°
- Argument of periapsis
- 79.27°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.2 LD
- 0.003 AU
- Tisserand (Jupiter)
- 6.036
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 62
- Data arc
- 24 hours
- First observed
- 3 April 2025
- Last observed
- 4 April 2025
- Residual RMS
- 0.54 ″
- Solution · Otto Matic
- 20 April 2025
Visual & observation
- Absolute magnitude (H)
- 29.46
Discovery & classification
Close approaches 90 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-04-05 05:05 UTC close approach of 2025 GL. Catalogue miss distance 29.8 LD · 1.15 × 10⁷ km. The curve is the geocentric path from 2027-04-02 to 2027-04-08, 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. 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 |
|---|---|---|---|---|
| 2027-04-05 05:05:00 | Earth | 0.0766 AU | 29.8 LD | 7.8 km/s |
| 2028-04-06 23:30:00 | Earth | 0.1354 AU | 52.7 LD | 9.4 km/s |
| 2029-04-09 21:34:00 | Earth | 0.1973 AU | 76.8 LD | 11.2 km/s |
| 2036-03-05 11:08:00 | Venus | 0.1217 AU | 47.4 LD | 2.3 km/s |
| 2050-04-27 07:11:00 | Venus | 0.1185 AU | 46.1 LD | 2.2 km/s |
| 2064-06-25 20:07:00 | Venus | 0.127 AU | 49.4 LD | 2.4 km/s |
| 2109-09-12 00:02:00 | Earth | 0.1854 AU | 72.1 LD | 10.8 km/s |
| 2110-09-15 09:25:00 | Earth | 0.1269 AU | 49.4 LD | 9.1 km/s |
| 2111-09-18 15:58:00 | Earth | 0.0735 AU | 28.6 LD | 7.5 km/s |
| 2112-09-20 22:07:00 | Earth | 0.0339 AU | 13.2 LD | 6.2 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