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Asteroid Near-Earth

2011 EK

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(2011 EK)

Where is it now

Distance from Sun
0.762 AU
True anomaly
332.52°
Distance from Earth
1.153 AU
As of
20 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 — 0.996 AU from the Sun Earth 2011 EK — 0.762 AU from the Sun 2011 EK
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2011 EK is 1.153 AU from Earth today (9.6 light-minutes).

In the sky

Right ascension
16h 30m 15s
Declination
-19° 06′ 57″
Constellation
Ophiuchus
Distance from Earth
1.15 AU
Elongation from the Sun
40.81° — 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.

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
0.898 AU
Eccentricity
0.1649
Inclination
8.72°
Orbital period
310.7 days
Perihelion
0.75 AU
Aphelion
1.046 AU
Longitude of ascending node
155.28°
Argument of periapsis
178.45°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 21.6 LD
0.0555 AU
Tisserand (Jupiter)
6.606

Orbit quality

Orbit very well determined (uncertainty code 0).

Observations used
74
Data arc
11.01 years
First observed
1 March 2011
Last observed
4 March 2022
Residual RMS
0.4 ″
Solution · Otto Matic
7 August 2022

Visual & observation

Absolute magnitude (H)
22.47

Discovery & classification

Aten Near-Earth Object

Close approaches 153 on record

Flyby geometry
Ecliptic flyby of 2011 EK at 2027-10-12 21:07 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-10-12 21:07 UTC close approach of 2011 EK. Catalogue miss distance 91.8 LD · 3.53 × 10⁷ km. The curve is the geocentric path from 2027-10-09 to 2027-10-15, 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. Sun 91.8 LD · 3.53 × 10⁷ km 2027-10-12 21:07 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-10-12 21:07 UTC close approach of 2011 EK. Catalogue miss distance 91.8 LD · 3.53 × 10⁷ km. The curve is the geocentric path from 2027-10-09 to 2027-10-15, 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.

JPL Horizons

When (UTC) Body Distance Lunar distances Relative speed
2027-10-12 21:07:00 Earth 0.2359 AU 91.8 LD 7.3 km/s
2028-03-20 15:30:00 Earth 0.0921 AU 35.8 LD 6.6 km/s
2028-07-28 07:42:00 Venus 0.0989 AU 38.5 LD 6.5 km/s
2033-01-16 17:40:00 Earth 0.3539 AU 137.7 LD 14.9 km/s
2033-08-19 03:24:00 Earth 0.2629 AU 102.3 LD 9.1 km/s
2034-03-25 05:18:00 Earth 0.3739 AU 145.5 LD 15.7 km/s
2035-05-18 05:22:00 Venus 0.122 AU 47.5 LD 9.6 km/s
2039-01-27 06:24:00 Earth 0.0968 AU 37.7 LD 6.1 km/s
2039-06-24 12:56:00 Earth 0.2425 AU 94.4 LD 6.2 km/s
2044-10-08 22:47:00 Earth 0.2387 AU 92.9 LD 7.5 km/s

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

Sources