Skip to content
Public Universe
Asteroid Near-Earth

2023 UR3

Add to an observing list or journal →

(2023 UR3)

Where is it now

Distance from Sun
1.128 AU
True anomaly
164.52°
Distance from Earth
0.83 AU
As of
23 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 2023 UR3 — 1.128 AU from the Sun 2023 UR3
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2023 UR3 is 0.83 AU from Earth today (6.9 light-minutes).

In the sky

Right ascension
09h 30m 49s
Declination
+28° 55′ 04″
Constellation
Leo
Distance from Earth
0.83 AU
Elongation from the Sun
75.97° — 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
0.965 AU
Eccentricity
0.178
Inclination
12.67°
Orbital period
346.3 days
Perihelion
0.793 AU
Aphelion
1.137 AU
Longitude of ascending node
25.45°
Argument of periapsis
245.75°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 3.4 LD
0.0086 AU
Tisserand (Jupiter)
6.218

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
20
Data arc
2 days
First observed
19 October 2023
Last observed
21 October 2023
Residual RMS
0.39 ″
Solution · Otto Matic
22 October 2023

Visual & observation

Absolute magnitude (H)
26.27

Discovery & classification

Aten Near-Earth Object

Close approaches 71 on record

Flyby geometry
Ecliptic flyby of 2023 UR3 at 2027-02-25 17:38 UTC Top-down view of the ecliptic, Earth at the centre, for the 2027-02-25 17:38 UTC close approach of 2023 UR3. Catalogue miss distance 160.2 LD · 6.16 × 10⁷ km. The curve is the geocentric path from 2027-02-22 to 2027-02-28, 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 160.2 LD · 6.16 × 10⁷ km 2027-02-25 17:38 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2027-02-25 17:38 UTC close approach of 2023 UR3. Catalogue miss distance 160.2 LD · 6.16 × 10⁷ km. The curve is the geocentric path from 2027-02-22 to 2027-02-28, 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
2027-02-25 17:38:00 Earth 0.4116 AU 160.2 LD 18.8 km/s
2040-10-28 16:20:00 Earth 0.3851 AU 149.9 LD 18.6 km/s
2041-10-18 12:25:00 Earth 0.0679 AU 26.4 LD 10.1 km/s
2042-11-15 21:04:00 Earth 0.2232 AU 86.9 LD 6.7 km/s
2043-05-24 17:03:00 Earth 0.2488 AU 96.8 LD 8.3 km/s
2044-03-27 09:48:00 Earth 0.1033 AU 40.2 LD 8.9 km/s
2045-03-02 12:55:00 Earth 0.3249 AU 126.5 LD 16.2 km/s
2046-03-17 14:34:00 Venus 0.1401 AU 54.5 LD 6.6 km/s
2059-10-23 12:26:00 Earth 0.2188 AU 85.1 LD 13.9 km/s
2060-10-18 19:36:00 Earth 0.0951 AU 37.0 LD 7.1 km/s

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

Sources