Where is it now
- Distance from Sun
- 0.378 AU
- True anomaly
- 27.3°
- Distance from Earth
- 0.665 AU
- As of
- 15 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
- 12h 30m 19s
- Declination
- -13° 44′ 16″
- Constellation
- Corvus
- Distance from Earth
- 0.67 AU
- Elongation from the Sun
- 14.41° — too close to the Sun to observe
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
- 0.708 AU
- Eccentricity
- 0.4857
- Inclination
- 23.35°
- Orbital period
- 217.4 days
- Perihelion
- 0.364 AU
- Aphelion
- 1.051 AU
- Longitude of ascending node
- 177.59°
- Argument of periapsis
- 196.51°
- Epoch · J2000
- 2452725.5
- Orbit class · ATE
- Aten
- Earth MOID · 5.4 LD
- 0.0139 AU
- Tisserand (Jupiter)
- 7.946
Orbit quality
Orbit very uncertain — the object may be effectively lost (uncertainty code 8).
- Observations used
- 27
- Data arc
- 7 days
- First observed
- 24 March 2003
- Last observed
- 31 March 2003
- Residual RMS
- 0.71 ″
- Solution · Otto Matic
- 14 April 2021
Visual & observation
- Absolute magnitude (H)
- 23
Discovery & classification
Close approaches 55 on record
Top-down view of the ecliptic, Earth at the centre, for the 2062-04-11 01:38 UTC close approach of 2003 FK1. Catalogue miss distance 110.4 LD · 4.24 × 10⁷ km. The curve is the geocentric path from 2062-04-08 to 2062-04-14, 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 |
|---|---|---|---|---|
| 2062-04-11 01:38:00 | Earth | 0.2836 AU | 110.4 LD | 16.7 km/s |
| 2064-11-16 08:59:00 | Mercury | 0.034 AU | 13.2 LD | 28.6 km/s |
| 2064-11-16 08:59:00 | Merc | 0.034 AU | 13.2 LD | 28.6 km/s |
| 2065-04-11 22:12:00 | Earth | 0.3734 AU | 145.3 LD | 20.2 km/s |
| 2066-03-24 21:56:00 | Earth | 0.4541 AU | 176.7 LD | 27.2 km/s |
| 2068-04-09 15:59:00 | Earth | 0.4741 AU | 184.5 LD | 24.2 km/s |
| 2069-03-20 03:43:00 | Earth | 0.3305 AU | 128.6 LD | 23.2 km/s |
| 2122-03-17 04:25:00 | Earth | 0.14 AU | 54.5 LD | 17.4 km/s |
| 2125-03-17 23:07:00 | Earth | 0.0208 AU | 8.1 LD | 14.6 km/s |
| 2125-07-31 04:41:00 | Merc | 0.0798 AU | 31.1 LD | 33.3 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