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Asteroid Near-Earth

2026 LX

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(2026 LX)

Where is it now

Distance from Sun
1.058 AU
True anomaly
223.84°
Distance from Earth
0.622 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 2026 LX — 1.058 AU from the Sun 2026 LX
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2026 LX is 0.622 AU from Earth today (5.2 light-minutes).

In the sky

Right ascension
19h 12m 04s
Declination
-22° 46′ 27″
Constellation
Sagittarius
Distance from Earth
0.62 AU
Elongation from the Sun
77.81° — well clear of the Sun

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
0.916 AU
Eccentricity
0.2824
Inclination
0.22°
Orbital period
320.1 days
Perihelion
0.657 AU
Aphelion
1.174 AU
Longitude of ascending node
70.45°
Argument of periapsis
58.94°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.2 LD
0.0005 AU
Tisserand (Jupiter)
6.487

Orbit quality

Orbit reasonably well determined (uncertainty code 4).

Observations used
44
Data arc
6 days
First observed
8 June 2026
Last observed
14 June 2026
Residual RMS
0.38 ″
Solution · Otto Matic
14 June 2026

Visual & observation

Absolute magnitude (H)
28.85

Discovery & classification

Listed by JPL impact monitoring; see the Sentry table for current probabilities.

Aten Near-Earth Object

Close approaches 69 on record

Flyby geometry
Ecliptic flyby of 2026 LX at 2027-09-26 04:41 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-09-26 04:41 UTC close approach of 2026 LX. Catalogue miss distance 56.8 LD · 2.19 × 10⁷ km. The curve is the geocentric path from 2027-09-23 to 2027-09-29, 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 56.8 LD · 2.19 × 10⁷ km 2027-09-26 04:41 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-09-26 04:41 UTC close approach of 2026 LX. Catalogue miss distance 56.8 LD · 2.19 × 10⁷ km. The curve is the geocentric path from 2027-09-23 to 2027-09-29, 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
2027-09-26 04:41:00 Earth 0.1461 AU 56.8 LD 11.9 km/s
2028-10-25 12:46:00 Venus 0.0657 AU 25.6 LD 6.4 km/s
2033-06-08 03:33:00 Earth 0.0905 AU 35.2 LD 10.2 km/s
2034-09-28 15:42:00 Earth 0.0506 AU 19.7 LD 9 km/s
2034-11-23 02:29:00 Venus 0.0116 AU 4.5 LD 7.3 km/s
2041-01-31 04:25:00 Venus 0.0523 AU 20.3 LD 6.2 km/s
2041-08-26 14:36:00 Earth 0.1427 AU 55.5 LD 5.8 km/s
2047-04-25 01:23:00 Venus 0.0636 AU 24.8 LD 6.2 km/s
2048-06-30 11:45:00 Earth 0.1277 AU 49.7 LD 5.6 km/s
2053-07-08 19:49:00 Venus 0.039 AU 15.2 LD 7.3 km/s

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

Sources