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Asteroid Near-Earth

2024 UX10

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(2024 UX10)

Where is it now

Distance from Sun
0.774 AU
True anomaly
108.9°
Distance from Earth
0.58 AU
As of
16 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 2024 UX10 — 0.774 AU from the Sun 2024 UX10
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2024 UX10 is 0.58 AU from Earth today (4.8 light-minutes).

In the sky

Right ascension
16h 03m 37s
Declination
-48° 35′ 34″
Constellation
Norma
Distance from Earth
0.58 AU
Elongation from the Sun
51.06° — 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
0.786 AU
Eccentricity
0.3611
Inclination
27.87°
Orbital period
254.4 days
Perihelion
0.502 AU
Aphelion
1.069 AU
Longitude of ascending node
37.22°
Argument of periapsis
203.81°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 9.3 LD
0.0239 AU
Tisserand (Jupiter)
7.263

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
46
Data arc
24 hours
First observed
30 October 2024
Last observed
31 October 2024
Residual RMS
0.42 ″
Solution · Otto Matic
2 November 2024

Visual & observation

Absolute magnitude (H)
26.51

Discovery & classification

Aten Near-Earth Object

Close approaches 130 on record

Flyby geometry
Ecliptic flyby of 2024 UX10 at 2026-11-07 15:47 UTC Top-down view of the ecliptic, Earth at the centre, for the 2026-11-07 15:47 UTC close approach of 2024 UX10. Catalogue miss distance 184.5 LD · 7.09 × 10⁷ km. The curve is the geocentric path from 2026-11-04 to 2026-11-10, 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 south of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 184.5 LD · 7.09 × 10⁷ km 2026-11-07 15:47 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2026-11-07 15:47 UTC close approach of 2024 UX10. Catalogue miss distance 184.5 LD · 7.09 × 10⁷ km. The curve is the geocentric path from 2026-11-04 to 2026-11-10, 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 south 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
2026-11-07 15:47:00 Earth 0.474 AU 184.5 LD 27.2 km/s
2027-05-03 10:13:00 Earth 0.499 AU 194.2 LD 26 km/s
2031-07-10 13:23:00 Mercury 0.0722 AU 28.1 LD 21.2 km/s
2031-07-10 13:23:00 Merc 0.0722 AU 28.1 LD 21.2 km/s
2031-11-05 08:07:00 Earth 0.1817 AU 70.7 LD 14.4 km/s
2032-02-15 13:36:00 Earth 0.4731 AU 184.1 LD 14.7 km/s
2033-11-01 10:38:00 Earth 0.2799 AU 108.9 LD 21.5 km/s
2034-04-14 08:07:00 Earth 0.4779 AU 186.0 LD 24.8 km/s
2037-10-15 10:29:00 Merc 0.074 AU 28.8 LD 18.9 km/s
2037-10-15 10:29:00 Mercury 0.074 AU 28.8 LD 18.9 km/s

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

Sources