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Asteroid Near-Earth

2025 MR89

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(2025 MR89)

Where is it now

Distance from Sun
0.713 AU
True anomaly
92.48°
Distance from Earth
1.694 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 MR89 — 0.713 AU from the Sun 2025 MR89
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 MR89 is 1.694 AU from Earth today (14.1 light-minutes).

In the sky

Right ascension
13h 48m 15s
Declination
-14° 02′ 42″
Constellation
Virgo
Distance from Earth
1.7 AU
Elongation from the Sun
6.66° — too close to the Sun to observe

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
0.807 AU
Eccentricity
0.3624
Inclination
7.74°
Orbital period
265 days
Perihelion
0.515 AU
Aphelion
1.1 AU
Longitude of ascending node
274.24°
Argument of periapsis
210.62°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 0.5 LD
0.0012 AU
Tisserand (Jupiter)
7.172

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
81
Data arc
27 days
First observed
26 June 2025
Last observed
23 July 2025
Residual RMS
0.56 ″
Solution · Otto Matic
14 August 2025

Visual & observation

Absolute magnitude (H)
26.33

Discovery & classification

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

Aten Near-Earth Object

Close approaches 34 on record

Flyby geometry
Ecliptic flyby of 2025 MR89 at 2033-07-14 11:12 UTC Top-down view of the ecliptic, Earth at the centre, for the 2033-07-14 11:12 UTC close approach of 2025 MR89. Catalogue miss distance 37.1 LD · 1.42 × 10⁷ km. The curve is the geocentric path from 2033-07-11 to 2033-07-17, 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 north of the ecliptic. The path is a geocentric ecliptic ephemeris from JPL Horizons. The inset is a heliocentric view and is approximate. Sun 37.1 LD · 1.42 × 10⁷ km 2033-07-14 11:12 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2033-07-14 11:12 UTC close approach of 2025 MR89. Catalogue miss distance 37.1 LD · 1.42 × 10⁷ km. The curve is the geocentric path from 2033-07-11 to 2033-07-17, 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 north 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
2028-01-15 20:47:00 Venus 0.1497 AU 58.2 LD 17.9 km/s
2028-12-27 15:22:00 Venus 0.1197 AU 46.6 LD 10.9 km/s
2033-07-14 11:12:00 Earth 0.0952 AU 37.1 LD 7.3 km/s
2040-05-23 07:38:00 Venus 0.1296 AU 50.4 LD 12 km/s
2041-08-12 10:31:00 Earth 0.1203 AU 46.8 LD 7.4 km/s
2046-06-25 10:22:00 Earth 0.1674 AU 65.1 LD 13.9 km/s
2048-05-07 15:19:00 Venus 0.1245 AU 48.4 LD 16 km/s
2049-04-16 11:17:00 Venus 0.1029 AU 40.0 LD 12.5 km/s
2049-08-30 05:39:00 Earth 0.1308 AU 50.9 LD 9.5 km/s
2054-06-24 06:35:00 Earth 0.0412 AU 16.1 LD 10 km/s

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

Sources