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Asteroid Near-Earth

2022 UL11

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(2022 UL11)

Where is it now

Distance from Sun
0.817 AU
True anomaly
219.65°
Distance from Earth
0.787 AU
As of
15 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 2022 UL11 — 0.817 AU from the Sun 2022 UL11
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2022 UL11 is 0.787 AU from Earth today (6.5 light-minutes).

In the sky

Right ascension
10h 07m 19s
Declination
+08° 56′ 20″
Constellation
Leo
Distance from Earth
0.79 AU
Elongation from the Sun
52.52° — near the Sun — look low at dusk or dawn

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
0.669 AU
Eccentricity
0.4901
Inclination
3.62°
Orbital period
200 days
Perihelion
0.341 AU
Aphelion
0.997 AU
Longitude of ascending node
212.19°
Argument of periapsis
0.76°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.8 LD
0.0021 AU
Tisserand (Jupiter)
8.398

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
46
Data arc
3 days
First observed
26 October 2022
Last observed
29 October 2022
Residual RMS
0.41 ″
Solution · Otto Matic
28 January 2024

Visual & observation

Absolute magnitude (H)
29.15

Discovery & classification

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

Aten Near-Earth Object

Close approaches 231 on record

Flyby geometry
Ecliptic flyby of 2022 UL11 at 2027-11-09 23:30 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-11-09 23:30 UTC close approach of 2022 UL11. Catalogue miss distance 115.2 LD · 4.43 × 10⁷ km. The curve is the geocentric path from 2027-11-06 to 2027-11-12, 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 115.2 LD · 4.43 × 10⁷ km 2027-11-09 23:30 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-11-09 23:30 UTC close approach of 2022 UL11. Catalogue miss distance 115.2 LD · 4.43 × 10⁷ km. The curve is the geocentric path from 2027-11-06 to 2027-11-12, 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
2026-11-28 07:50:00 Mercury 0.0528 AU 20.5 LD 25.8 km/s
2026-11-28 07:50:00 Merc 0.0528 AU 20.5 LD 25.8 km/s
2027-11-09 23:30:00 Earth 0.296 AU 115.2 LD 19.4 km/s
2028-10-11 20:39:00 Earth 0.0592 AU 23.0 LD 10.9 km/s
2031-03-16 21:48:00 Venus 0.1055 AU 41.0 LD 22.1 km/s
2031-05-07 22:14:00 Mercury 0.0882 AU 34.3 LD 30.7 km/s
2031-05-07 22:14:00 Merc 0.0882 AU 34.3 LD 30.7 km/s
2032-12-08 00:15:00 Mercury 0.0605 AU 23.5 LD 23 km/s
2032-12-08 00:15:00 Merc 0.0605 AU 23.5 LD 23 km/s
2033-11-13 00:43:00 Earth 0.1626 AU 63.3 LD 14.6 km/s

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

Sources