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Asteroid Near-Earth

2011 GE3

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(2011 GE3)

Where is it now

Distance from Sun
1.043 AU
True anomaly
191.93°
Distance from Earth
1.999 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 2011 GE3 — 1.043 AU from the Sun 2011 GE3
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2011 GE3 is 1.999 AU from Earth today (16.6 light-minutes).

In the sky

Right ascension
14h 11m 17s
Declination
-15° 08′ 40″
Constellation
Virgo
Distance from Earth
2 AU
Elongation from the Sun
11.73° — too close to the Sun to observe

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.

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
0.815 AU
Eccentricity
0.2925
Inclination
6.24°
Orbital period
268.5 days
Perihelion
0.576 AU
Aphelion
1.053 AU
Longitude of ascending node
13.19°
Argument of periapsis
21.26°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 5.6 LD
0.0143 AU
Tisserand (Jupiter)
7.141

Orbit quality

Orbit very well determined (uncertainty code 1).

Observations used
54
Data arc
11.02 years
First observed
2 April 2011
Last observed
8 April 2022
Residual RMS
0.46 ″
Solution · Otto Matic
9 April 2022

Visual & observation

Absolute magnitude (H)
25.88

Discovery & classification

Aten Near-Earth Object

Close approaches 244 on record

Flyby geometry
Ecliptic flyby of 2011 GE3 at 2027-11-15 19:25 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-11-15 19:25 UTC close approach of 2011 GE3. Catalogue miss distance 159.4 LD · 6.13 × 10⁷ km. The curve is the geocentric path from 2027-11-12 to 2027-11-18, 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. Sun 159.4 LD · 6.13 × 10⁷ km 2027-11-15 19:25 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-11-15 19:25 UTC close approach of 2011 GE3. Catalogue miss distance 159.4 LD · 6.13 × 10⁷ km. The curve is the geocentric path from 2027-11-12 to 2027-11-18, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2027-11-15 19:25:00 Earth 0.4095 AU 159.4 LD 14.4 km/s
2028-05-14 01:47:00 Earth 0.4562 AU 177.5 LD 20.6 km/s
2029-06-05 18:45:00 Venus 0.0525 AU 20.4 LD 11.6 km/s
2030-10-06 14:58:00 Earth 0.4135 AU 160.9 LD 14.7 km/s
2033-02-07 17:29:00 Venus 0.0947 AU 36.8 LD 6.6 km/s
2033-03-23 03:46:00 Earth 0.1803 AU 70.2 LD 12.1 km/s
2033-08-23 13:37:00 Earth 0.3553 AU 138.3 LD 10.1 km/s
2036-05-01 06:52:00 Earth 0.0685 AU 26.7 LD 6 km/s
2036-09-13 22:28:00 Venus 0.1495 AU 58.2 LD 9 km/s
2038-12-06 22:30:00 Earth 0.3839 AU 149.4 LD 12.3 km/s

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

Sources