Where is it now
- Distance from Sun
- 0.854 AU
- True anomaly
- 348.14°
- Distance from Earth
- 1.018 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
- 17h 15m 20s
- Declination
- -23° 02′ 46″
- Constellation
- Ophiuchus
- Distance from Earth
- 1.02 AU
- Elongation from the Sun
- 50.23° — near the Sun — look low at dusk or dawn
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
- 0.942 AU
- Eccentricity
- 0.0947
- Inclination
- 1.16°
- Orbital period
- 333.9 days
- Perihelion
- 0.853 AU
- Aphelion
- 1.031 AU
- Longitude of ascending node
- 143.06°
- Argument of periapsis
- 191.87°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 5.4 LD
- 0.014 AU
- Tisserand (Jupiter)
- 6.372
Orbit quality
Orbit reasonably well determined (uncertainty code 5).
- Observations used
- 18
- Data arc
- 37 days
- First observed
- 12 February 2018
- Last observed
- 21 March 2018
- Residual RMS
- 0.69 ″
- Solution · Otto Matic
- 15 April 2021
Visual & observation
- Absolute magnitude (H)
- 26.6
Discovery & classification
Close approaches 50 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-12-31 10:31 UTC close approach of 2018 FM2. Catalogue miss distance 93.0 LD · 3.57 × 10⁷ km. The curve is the geocentric path from 2027-12-28 to 2028-01-03, 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 |
|---|---|---|---|---|
| 2027-12-31 10:31:00 | Earth | 0.2388 AU | 93.0 LD | 10.1 km/s |
| 2028-09-02 03:14:00 | Earth | 0.1561 AU | 60.7 LD | 4.3 km/s |
| 2029-04-11 08:09:00 | Earth | 0.1313 AU | 51.1 LD | 6.7 km/s |
| 2037-10-06 08:23:00 | Venus | 0.1344 AU | 52.3 LD | 1.2 km/s |
| 2038-12-27 15:20:00 | Earth | 0.0295 AU | 11.5 LD | 3.6 km/s |
| 2039-07-12 06:05:00 | Earth | 0.1385 AU | 53.9 LD | 3.6 km/s |
| 2039-08-28 07:47:00 | Venus | 0.1368 AU | 53.2 LD | 1.4 km/s |
| 2040-04-08 20:57:00 | Earth | 0.3017 AU | 117.4 LD | 11.9 km/s |
| 2041-07-11 04:25:00 | Venus | 0.143 AU | 55.7 LD | 1.9 km/s |
| 2049-12-29 23:26:00 | Earth | 0.1911 AU | 74.4 LD | 8.6 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