2025 FF18 is an asteroid in the Apollo orbit class. Its orbit takes it from 0.77 AU to 1.28 AU from the Sun; one orbit takes 379.4 days. Orbit from the JPL solution of 7 April 2025.
Where is it now
- Distance from Sun
- 1.175 AU
- True anomaly
- 136.55°
- Distance from Earth
- 0.626 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
- 08h 58m 48s
- Declination
- +20° 19′ 44″
- Constellation
- Cancer
- Distance from Earth
- 0.62 AU
- Elongation from the Sun
- 90.69° — well clear of the Sun
Favours the northern hemisphere; low or below the horizon from far south.
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
- 1.026 AU
- Eccentricity
- 0.2514
- Inclination
- 1.68°
- Orbital period
- 379.4 days
- Perihelion
- 0.768 AU
- Aphelion
- 1.284 AU
- Longitude of ascending node
- 358.04°
- Argument of periapsis
- 298.87°
- Epoch · J2000
- 2461200.5
- Orbit class · APO
- Apollo
- Earth MOID · 3.8 LD
- 0.0099 AU
- Tisserand (Jupiter)
- 5.932
Orbit quality
Orbit poorly determined (uncertainty code 7).
- Observations used
- 34
- Data arc
- 8 days
- First observed
- 30 March 2025
- Last observed
- 7 April 2025
- Residual RMS
- 0.44 ″
- Solution · Otto Matic
- 7 April 2025
Visual & observation
- Absolute magnitude (H)
- 25.84
Discovery & classification
Close approaches 19 on record
Top-down view of the ecliptic, Earth at the centre, for the 2028-09-05 08:17 UTC close approach of 2025 FF18. Catalogue miss distance 77.7 LD · 2.99 × 10⁷ km. The curve is the geocentric path from 2028-09-02 to 2028-09-08, 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 |
|---|---|---|---|---|
| 2028-09-05 08:17:00 | Earth | 0.1997 AU | 77.7 LD | 6.7 km/s |
| 2029-10-27 21:34:00 | Earth | 0.0193 AU | 7.5 LD | 8.4 km/s |
| 2035-11-09 19:24:00 | Venus | 0.0675 AU | 26.3 LD | 5.4 km/s |
| 2051-04-07 16:34:00 | Earth | 0.0231 AU | 9.0 LD | 8.7 km/s |
| 2052-07-09 10:36:00 | Venus | 0.1099 AU | 42.8 LD | 7.2 km/s |
| 2055-10-26 00:19:00 | Earth | 0.0777 AU | 30.2 LD | 5.8 km/s |
| 2056-11-03 15:39:00 | Earth | 0.1555 AU | 60.5 LD | 12.7 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