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Asteroid Near-Earth

2010 FS

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(2010 FS)

Where is it now

Distance from Sun
1.025 AU
True anomaly
174.17°
Distance from Earth
2.007 AU
As of
16 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 — 0.997 AU from the Sun Earth 2010 FS — 1.025 AU from the Sun 2010 FS
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2010 FS is 2.007 AU from Earth today (16.7 light-minutes).

In the sky

Right ascension
13h 05m 02s
Declination
-05° 08′ 18″
Constellation
Virgo
Distance from Earth
2.01 AU
Elongation from the Sun
7.03° — 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
0.78 AU
Eccentricity
0.3175
Inclination
9.12°
Orbital period
251.6 days
Perihelion
0.532 AU
Aphelion
1.028 AU
Longitude of ascending node
169.74°
Argument of periapsis
206.3°
Epoch · J2000
2455276.5
Orbit class · ATE
Aten
Earth MOID · 3.4 LD
0.0087 AU
Tisserand (Jupiter)
7.396

Orbit quality

Orbit very uncertain — the object may be effectively lost (uncertainty code 8).

Observations used
42
Data arc
13 days
First observed
18 March 2010
Last observed
31 March 2010
Residual RMS
0.53 ″
Solution · Otto Matic
15 April 2021

Physical properties

Mean radius
0.01 km

Visual & observation

Geometric albedo
0.548
Absolute magnitude (H)
24.2

Discovery & classification

Aten Near-Earth Object

Close approaches 44 on record

Flyby geometry
Ecliptic flyby of 2010 FS at 2028-04-24 12:58 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-04-24 12:58 UTC close approach of 2010 FS. Catalogue miss distance 124.7 LD · 4.79 × 10⁷ km. The curve is the geocentric path from 2028-04-21 to 2028-04-27, 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. Sun 124.7 LD · 4.79 × 10⁷ km 2028-04-24 12:58 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-04-24 12:58 UTC close approach of 2010 FS. Catalogue miss distance 124.7 LD · 4.79 × 10⁷ km. The curve is the geocentric path from 2028-04-21 to 2028-04-27, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2028-04-24 12:58:00 Earth 0.3204 AU 124.7 LD 15.9 km/s
2032-03-12 11:53:00 Earth 0.2927 AU 113.9 LD 16.4 km/s
2039-04-27 00:55:00 Earth 0.209 AU 81.3 LD 11.7 km/s
2043-03-18 13:12:00 Earth 0.4305 AU 167.5 LD 20.9 km/s
2045-10-06 03:22:00 Earth 0.4686 AU 182.4 LD 17.8 km/s
2047-04-04 19:05:00 Venus 0.1374 AU 53.5 LD 14.5 km/s
2047-11-19 22:09:00 Earth 0.4351 AU 169.3 LD 14.2 km/s
2048-04-22 09:04:00 Earth 0.398 AU 154.9 LD 18.7 km/s
2052-03-10 15:37:00 Earth 0.2309 AU 89.9 LD 14.5 km/s
2068-04-24 00:04:00 Earth 0.3577 AU 139.2 LD 17.2 km/s

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

Sources