2024 GE3 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.76 AU to 1.27 AU from the Sun; one orbit takes 374 days. Orbit from the JPL solution of 14 April 2024.
Where is it now
- Distance from Sun
- 1.135 AU
- True anomaly
- 129.92°
- Distance from Earth
- 0.63 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
- 09h 09m 28s
- Declination
- +13° 27′ 07″
- Constellation
- Cancer
- Distance from Earth
- 0.63 AU
- Elongation from the Sun
- 85.95° — 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
- 1.016 AU
- Eccentricity
- 0.2514
- Inclination
- 1.78°
- Orbital period
- 374 days
- Perihelion
- 0.761 AU
- Aphelion
- 1.271 AU
- Longitude of ascending node
- 195.28°
- Argument of periapsis
- 109.71°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 1.7 LD
- 0.0043 AU
- Tisserand (Jupiter)
- 5.977
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 35
- Data arc
- 4 days
- First observed
- 10 April 2024
- Last observed
- 14 April 2024
- Residual RMS
- 0.48 ″
- Solution · Otto Matic
- 14 April 2024
Visual & observation
- Absolute magnitude (H)
- 26.08
Discovery & classification
Close approaches 56 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-02-06 23:49 UTC close approach of 2024 GE3. Catalogue miss distance 109.5 LD · 4.21 × 10⁷ km. The curve is the geocentric path from 2027-02-03 to 2027-02-09, 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 |
|---|---|---|---|---|
| 2027-02-06 23:49:00 | Earth | 0.2814 AU | 109.5 LD | 7.3 km/s |
| 2027-07-21 01:33:00 | Earth | 0.2557 AU | 99.5 LD | 8.9 km/s |
| 2028-01-20 02:49:00 | Earth | 0.2877 AU | 112.0 LD | 7.4 km/s |
| 2028-08-15 04:33:00 | Earth | 0.247 AU | 96.1 LD | 8.5 km/s |
| 2028-12-31 10:13:00 | Earth | 0.266 AU | 103.5 LD | 6.9 km/s |
| 2029-09-14 11:21:00 | Earth | 0.2044 AU | 79.6 LD | 6.7 km/s |
| 2029-12-08 07:22:00 | Earth | 0.2093 AU | 81.5 LD | 5.8 km/s |
| 2030-11-03 18:30:00 | Earth | 0.0895 AU | 34.8 LD | 5.5 km/s |
| 2031-11-08 21:16:00 | Earth | 0.06 AU | 23.3 LD | 9.8 km/s |
| 2032-11-14 11:10:00 | Earth | 0.2119 AU | 82.5 LD | 14.5 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