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Asteroid Near-Earth

2025 MX1

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(2025 MX1)

Where is it now

Distance from Sun
1.04 AU
True anomaly
176.18°
Distance from Earth
1.87 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 2025 MX1 — 1.04 AU from the Sun 2025 MX1
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 MX1 is 1.87 AU from Earth today (15.5 light-minutes).

In the sky

Right ascension
14h 59m 27s
Declination
-17° 58′ 09″
Constellation
Libra
Distance from Earth
1.87 AU
Elongation from the Sun
23.82° — 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
0.785 AU
Eccentricity
0.3264
Inclination
5.21°
Orbital period
253.9 days
Perihelion
0.529 AU
Aphelion
1.041 AU
Longitude of ascending node
268.96°
Argument of periapsis
164.83°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 1.5 LD
0.0039 AU
Tisserand (Jupiter)
7.363

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
16
Data arc
2 days
First observed
20 June 2025
Last observed
22 June 2025
Residual RMS
0.79 ″
Solution · Otto Matic
22 June 2025

Visual & observation

Absolute magnitude (H)
28.89

Discovery & classification

Aten Near-Earth Object

Close approaches 17 on record

Flyby geometry
Ecliptic flyby of 2025 MX1 at 2034-05-11 08:46 UTC Top-down view of the ecliptic, Earth at the centre, for the 2034-05-11 08:46 UTC close approach of 2025 MX1. Catalogue miss distance 30.3 LD · 1.17 × 10⁷ km. The curve is the geocentric path from 2034-05-08 to 2034-05-14, 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 30.3 LD · 1.17 × 10⁷ km 2034-05-11 08:46 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2034-05-11 08:46 UTC close approach of 2025 MX1. Catalogue miss distance 30.3 LD · 1.17 × 10⁷ km. The curve is the geocentric path from 2034-05-08 to 2034-05-14, 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
2030-09-24 03:29:00 Venus 0.1057 AU 41.2 LD 11.5 km/s
2034-05-11 08:46:00 Earth 0.0779 AU 30.3 LD 7.7 km/s
2040-03-31 06:42:00 Venus 0.1162 AU 45.2 LD 14 km/s
2041-06-28 03:44:00 Earth 0.0387 AU 15.1 LD 7.6 km/s
2046-09-15 21:07:00 Venus 0.1199 AU 46.7 LD 9.2 km/s
2050-05-27 01:09:00 Earth 0.0435 AU 16.9 LD 6 km/s
2052-04-10 16:22:00 Venus 0.1372 AU 53.4 LD 15.7 km/s
2057-06-30 01:12:00 Earth 0.1632 AU 63.5 LD 11.6 km/s
2059-05-09 14:18:00 Earth 0.1512 AU 58.8 LD 10.5 km/s
2061-10-13 00:21:00 Venus 0.106 AU 41.2 LD 12.4 km/s

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

Sources