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Asteroid Near-Earth

2022 UM1

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(2022 UM1)

Where is it now

Distance from Sun
1.071 AU
True anomaly
193.07°
Distance from Earth
0.775 AU
As of
19 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 2022 UM1 — 1.071 AU from the Sun 2022 UM1
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2022 UM1 is 0.775 AU from Earth today (6.4 light-minutes).

In the sky

Right ascension
09h 12m 41s
Declination
+23° 25′ 12″
Constellation
Cancer
Distance from Earth
0.77 AU
Elongation from the Sun
73.28° — well clear of the Sun

Favours the northern hemisphere; low or below the horizon from far south.

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
0.838 AU
Eccentricity
0.2919
Inclination
6.78°
Orbital period
280.2 days
Perihelion
0.593 AU
Aphelion
1.083 AU
Longitude of ascending node
22.57°
Argument of periapsis
214.55°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 2.0 LD
0.0052 AU
Tisserand (Jupiter)
6.971

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
42
Data arc
11 days
First observed
18 October 2022
Last observed
29 October 2022
Residual RMS
0.54 ″
Solution · Otto Matic
29 October 2022

Visual & observation

Absolute magnitude (H)
27.21

Discovery & classification

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

Aten Near-Earth Object

Close approaches 118 on record

Flyby geometry
Ecliptic flyby of 2022 UM1 at 2029-06-29 02:26 UTC Top-down view of the ecliptic, Earth at the centre, for the 2029-06-29 02:26 UTC close approach of 2022 UM1. Catalogue miss distance 155.3 LD · 5.97 × 10⁷ km. The curve is the geocentric path from 2029-06-26 to 2029-07-02, 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 155.3 LD · 5.97 × 10⁷ km 2029-06-29 02:26 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2029-06-29 02:26 UTC close approach of 2022 UM1. Catalogue miss distance 155.3 LD · 5.97 × 10⁷ km. The curve is the geocentric path from 2029-06-26 to 2029-07-02, 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
2027-01-14 17:43:00 Venus 0.0209 AU 8.1 LD 9.7 km/s
2029-06-29 02:26:00 Earth 0.3991 AU 155.3 LD 12.4 km/s
2029-12-29 04:52:00 Earth 0.2129 AU 82.8 LD 13.3 km/s
2030-02-09 05:50:00 Venus 0.0178 AU 6.9 LD 10.9 km/s
2032-11-06 20:55:00 Earth 0.1055 AU 41.1 LD 6.6 km/s
2033-02-18 00:29:00 Earth 0.2672 AU 104.0 LD 5.8 km/s
2033-03-04 19:20:00 Venus 0.083 AU 32.3 LD 14.2 km/s
2035-10-15 23:48:00 Earth 0.2296 AU 89.4 LD 15.2 km/s
2036-04-18 22:20:00 Earth 0.3953 AU 153.8 LD 13.8 km/s
2039-06-03 07:44:00 Earth 0.4221 AU 164.3 LD 14.6 km/s

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

Sources