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Asteroid Near-Earth

2013 FQ10

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(2013 FQ10)

Where is it now

Distance from Sun
1.115 AU
True anomaly
180.28°
Distance from Earth
2.084 AU
As of
21 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.

Sun Earth — 0.995 AU from the Sun Earth 2013 FQ10 — 1.115 AU from the Sun 2013 FQ10
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2013 FQ10 is 2.084 AU from Earth today (17.3 light-minutes).

In the sky

Right ascension
13h 12m 28s
Declination
-07° 29′ 32″
Constellation
Virgo
Distance from Earth
2.08 AU
Elongation from the Sun
9.7° — 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.

How do I find my coordinates?

Google Maps on a computer

  1. Right-click the spot where you'll be observing.
  2. The first line of the menu is the coordinates, e.g. 51.50722, -0.12758 — click it and they're copied.
  3. Paste them above.

Google Maps on a phone

  1. Press and hold the spot to drop a pin.
  2. The coordinates appear in the search bar (or on the pin's card) — tap to copy, then paste above.

A full Google Maps link works too, but the short maps.app.goo.gl share links don't carry coordinates — copy the numbers instead. We round to about a kilometre; that's all the sky calculation needs.

Know your what3words address? Paste it, e.g. ///filled.count.soap. This is optional — the three words are sent to what3words to convert them, and we don't store the address or the result.

Your location stays in your browser and is sent only for this calculation. Using a what3words address is optional; if you do, the three words go to what3words to be converted and we don't record them. Set a location first, then you can save an email alert for this object. See our privacy policy.

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
0.935 AU
Eccentricity
0.1927
Inclination
16.86°
Orbital period
330 days
Perihelion
0.754 AU
Aphelion
1.115 AU
Longitude of ascending node
189.84°
Argument of periapsis
180.14°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 45.1 LD
0.116 AU
Tisserand (Jupiter)
6.363

Orbit quality

Orbit very well determined (uncertainty code 1).

Observations used
119
Data arc
9.04 years
First observed
20 March 2013
Last observed
3 April 2022
Residual RMS
0.48 ″
Solution · Otto Matic
1 September 2023

Visual & observation

Absolute magnitude (H)
22.52

Discovery & classification

Aten Near-Earth Object

Close approaches 145 on record

Flyby geometry
Ecliptic flyby of 2013 FQ10 at 2031-02-21 23:56 UTC Top-down view of the ecliptic, Earth at the centre, for the 2031-02-21 23:56 UTC close approach of 2013 FQ10. Catalogue miss distance 127.0 LD · 4.88 × 10⁷ km. The curve is the geocentric path from 2031-02-18 to 2031-02-24, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate. approximate Sun 127.0 LD · 4.88 × 10⁷ km 2031-02-21 23:56 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2031-02-21 23:56 UTC close approach of 2013 FQ10. Catalogue miss distance 127.0 LD · 4.88 × 10⁷ km. The curve is the geocentric path from 2031-02-18 to 2031-02-24, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate.

When (UTC) Body Distance Lunar distances Relative speed
2031-02-21 23:56:00 Earth 0.3263 AU 127.0 LD 13.1 km/s
2031-10-18 03:14:00 Earth 0.2465 AU 95.9 LD 12.3 km/s
2032-04-12 00:10:00 Earth 0.1379 AU 53.7 LD 9.5 km/s
2035-05-27 18:58:00 Venus 0.0368 AU 14.3 LD 11.8 km/s
2040-02-22 03:42:00 Earth 0.4899 AU 190.7 LD 18.7 km/s
2040-11-16 14:05:00 Earth 0.271 AU 105.5 LD 10.9 km/s
2041-03-25 01:41:00 Earth 0.1243 AU 48.4 LD 9.2 km/s
2041-08-24 04:32:00 Earth 0.2834 AU 110.3 LD 11.3 km/s
2042-05-01 18:08:00 Earth 0.3854 AU 150.0 LD 15.7 km/s
2048-12-11 14:30:00 Venus 0.0784 AU 30.5 LD 12.7 km/s

Next ten from today. 1 lunar distance = 384,400 km. Source: JPL close-approach data.

Sources