673713
Add to an observing list or journal →673713 (2015 FQ117)
Where is it now
- Distance from Sun
- 0.328 AU
- True anomaly
- 9.79°
- Distance from Earth
- 0.697 AU
- As of
- 19 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
- 14h 11m 35s
- Declination
- -10° 57′ 52″
- Constellation
- Virgo
- Distance from Earth
- 0.68 AU
- Elongation from the Sun
- 7.59° — 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
- 0.861 AU
- Eccentricity
- 0.6205
- Inclination
- 4.55°
- Orbital period
- 291.6 days
- Perihelion
- 0.327 AU
- Aphelion
- 1.395 AU
- Longitude of ascending node
- 293.85°
- Argument of periapsis
- 63.12°
- Epoch · J2000
- 2461200.5
- Orbit class · ATE
- Aten
- Earth MOID · 11.0 LD
- 0.0283 AU
- Tisserand (Jupiter)
- 6.682
Orbit quality
Orbit very well determined (uncertainty code 0).
- Observations used
- 84
- Data arc
- 7.99 years
- First observed
- 22 March 2015
- Last observed
- 19 March 2023
- Residual RMS
- 0.55 ″
- Solution · Otto Matic
- 16 April 2024
Visual & observation
- Absolute magnitude (H)
- 20.87
Discovery & classification
- Discovered by
- Pan-STARRS 1
- Discovery date
- 22 March 2015
- Discovery site
- Haleakala
Also known as 2015 FQ117
Close approaches 355 on record
Top-down view of the ecliptic, Earth at the centre, for the 2027-03-25 01:11 UTC close approach of 673713. Catalogue miss distance 156.4 LD · 6.01 × 10⁷ km. The curve is the geocentric path from 2027-03-22 to 2027-03-28, 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 south 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 |
|---|---|---|---|---|
| 2026-10-01 17:01:00 | Mercury | 0.0682 AU | 26.6 LD | 29.3 km/s |
| 2026-10-01 17:01:00 | Merc | 0.0682 AU | 26.6 LD | 29.3 km/s |
| 2027-03-25 01:11:00 | Earth | 0.4018 AU | 156.4 LD | 14.3 km/s |
| 2030-02-12 16:26:00 | Earth | 0.2596 AU | 101.0 LD | 27 km/s |
| 2031-03-28 10:15:00 | Earth | 0.3942 AU | 153.4 LD | 14.3 km/s |
| 2031-06-28 23:00:00 | Venus | 0.1333 AU | 51.9 LD | 18.3 km/s |
| 2032-06-23 02:52:00 | Venus | 0.1183 AU | 46.0 LD | 18.6 km/s |
| 2034-02-10 19:49:00 | Earth | 0.213 AU | 82.9 LD | 25.4 km/s |
| 2034-10-15 22:33:00 | Mercury | 0.0829 AU | 32.3 LD | 32.5 km/s |
| 2034-10-15 22:33:00 | Merc | 0.0829 AU | 32.3 LD | 32.5 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