Skip to content
Public Universe
Asteroid Near-Earth

2025 VM5

Add to an observing list or journal →

(2025 VM5)

Where is it now

Distance from Sun
0.977 AU
True anomaly
244.32°
Distance from Earth
0.593 AU
As of
21 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 2025 VM5 — 0.977 AU from the Sun 2025 VM5
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 VM5 is 0.593 AU from Earth today (4.9 light-minutes).

In the sky

Right ascension
09h 24m 37s
Declination
+15° 39′ 30″
Constellation
Leo
Distance from Earth
0.59 AU
Elongation from the Sun
70.63° — 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
0.933 AU
Eccentricity
0.1656
Inclination
1.46°
Orbital period
328.9 days
Perihelion
0.778 AU
Aphelion
1.087 AU
Longitude of ascending node
254.35°
Argument of periapsis
284.66°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 2.5 LD
0.0065 AU
Tisserand (Jupiter)
6.414

Orbit quality

Orbit reasonably well determined (uncertainty code 5).

Observations used
57
Data arc
6 days
First observed
14 November 2025
Last observed
20 November 2025
Residual RMS
0.46 ″
Solution · Otto Matic
11 March 2026

Visual & observation

Absolute magnitude (H)
26.98

Discovery & classification

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

Aten Near-Earth Object

Close approaches 29 on record

Flyby geometry
Ecliptic flyby of 2025 VM5 at 2034-11-20 23:32 UTC Top-down view of the ecliptic, Earth at the centre, for the 2034-11-20 23:32 UTC close approach of 2025 VM5. Catalogue miss distance 6.42 LD · 2.47 × 10⁶ km. The curve is the geocentric path from 2034-11-17 to 2034-11-23, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate. approximate Sun 6.42 LD · 2.47 × 10⁶ km 2034-11-20 23:32 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2034-11-20 23:32 UTC close approach of 2025 VM5. Catalogue miss distance 6.42 LD · 2.47 × 10⁶ km. The curve is the geocentric path from 2034-11-17 to 2034-11-23, 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 approximate: a two-body Kepler propagation of the catalogue orbital elements, not a numerical integration. The Moon’s position is approximate. The inset is a heliocentric view and is approximate.

When (UTC) Body Distance Lunar distances Relative speed
2027-02-24 04:19:00 Venus 0.1263 AU 49.2 LD 2.8 km/s
2034-11-20 23:32:00 Earth 0.0165 AU 6.4 LD 4 km/s
2038-09-03 23:37:00 Venus 0.1315 AU 51.2 LD 2 km/s
2040-09-10 14:38:00 Venus 0.1439 AU 56.0 LD 3.2 km/s
2043-07-31 00:06:00 Earth 0.0275 AU 10.7 LD 4 km/s
2071-07-31 13:59:00 Earth 0.0309 AU 12.0 LD 3.9 km/s
2080-07-28 23:21:00 Earth 0.1112 AU 43.3 LD 7.7 km/s
2081-11-18 10:10:00 Earth 0.1632 AU 63.5 LD 9.5 km/s
2090-11-21 15:57:00 Moon 0.0036 AU 1.4 LD 4.4 km/s

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

Sources