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Asteroid Near-Earth

2026 EE2

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(2026 EE2)

Where is it now

Distance from Sun
0.804 AU
True anomaly
343.09°
Distance from Earth
0.233 AU
As of
22 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 2026 EE2 — 0.804 AU from the Sun 2026 EE2
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2026 EE2 is 0.233 AU from Earth today (1.9 light-minutes).

In the sky

Right ascension
12h 11m 46s
Declination
-32° 47′ 20″
Constellation
Hydra
Distance from Earth
0.23 AU
Elongation from the Sun
31.1° — 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
0.941 AU
Eccentricity
0.1498
Inclination
12.23°
Orbital period
333.3 days
Perihelion
0.8 AU
Aphelion
1.082 AU
Longitude of ascending node
172.31°
Argument of periapsis
237.73°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 2.0 LD
0.0051 AU
Tisserand (Jupiter)
6.353

Orbit quality

Orbit reasonably well determined (uncertainty code 3).

Observations used
139
Data arc
12 days
First observed
10 March 2026
Last observed
22 March 2026
Residual RMS
0.38 ″
Solution · Otto Matic
30 July 2026

Visual & observation

Absolute magnitude (H)
25

Discovery & classification

Aten Near-Earth Object

Close approaches 62 on record

Flyby geometry
Ecliptic flyby of 2026 EE2 at 2037-08-02 17:44 UTC Top-down view of the ecliptic, Earth at the centre, for the 2037-08-02 17:44 UTC close approach of 2026 EE2. Catalogue miss distance 69.6 LD · 2.68 × 10⁷ km. The curve is the geocentric path from 2037-07-30 to 2037-08-05, 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 69.6 LD · 2.68 × 10⁷ km 2037-08-02 17:44 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2037-08-02 17:44 UTC close approach of 2026 EE2. Catalogue miss distance 69.6 LD · 2.68 × 10⁷ km. The curve is the geocentric path from 2037-07-30 to 2037-08-05, 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
2026-09-29 14:06:00 Earth 0.1845 AU 71.8 LD 8 km/s
2026-10-18 23:34:00 Venus 0.129 AU 50.2 LD 9.2 km/s
2037-08-02 17:44:00 Earth 0.1789 AU 69.6 LD 8.9 km/s
2047-03-22 11:44:00 Earth 0.1357 AU 52.8 LD 6.5 km/s
2047-09-03 17:17:00 Earth 0.1421 AU 55.3 LD 7.8 km/s
2051-05-23 23:58:00 Venus 0.1002 AU 39.0 LD 8 km/s
2057-03-12 10:11:00 Earth 0.0496 AU 19.3 LD 8.1 km/s
2068-08-20 17:48:00 Earth 0.1383 AU 53.8 LD 7.9 km/s
2078-03-12 11:38:00 Earth 0.0307 AU 12.0 LD 7.8 km/s
2078-10-08 10:39:00 Earth 0.1993 AU 77.6 LD 7.9 km/s

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

Sources