Skip to content
Public Universe
Asteroid Near-Earth

2025 QV4

Add to an observing list or journal →

(2025 QV4)

Where is it now

Distance from Sun
0.502 AU
True anomaly
278.4°
Distance from Earth
1.026 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 QV4 — 0.502 AU from the Sun 2025 QV4
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 QV4 is 1.026 AU from Earth today (8.5 light-minutes).

In the sky

Right ascension
11h 57m 14s
Declination
+07° 37′ 51″
Constellation
Virgo
Distance from Earth
1.03 AU
Elongation from the Sun
28.26° — near the Sun — look low at dusk or dawn

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
0.782 AU
Eccentricity
0.5535
Inclination
19.12°
Orbital period
252.7 days
Perihelion
0.349 AU
Aphelion
1.215 AU
Longitude of ascending node
329.62°
Argument of periapsis
212.28°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 1.6 LD
0.004 AU
Tisserand (Jupiter)
7.262

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
98
Data arc
3 days
First observed
23 August 2025
Last observed
26 August 2025
Residual RMS
0.26 ″
Solution · Otto Matic
27 August 2025

Visual & observation

Absolute magnitude (H)
25.21

Discovery & classification

Aten Near-Earth Object

Close approaches 94 on record

Flyby geometry
Ecliptic flyby of 2025 QV4 at 2034-08-22 14:13 UTC Top-down view of the ecliptic, Earth at the centre, for the 2034-08-22 14:13 UTC close approach of 2025 QV4. Catalogue miss distance 15.8 LD · 6.07 × 10⁶ km. The curve is the geocentric path from 2034-08-19 to 2034-08-25, 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 20 Aug 25 Aug 15.8 LD · 6.07 × 10⁶ km 2034-08-22 14:13 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2034-08-22 14:13 UTC close approach of 2025 QV4. Catalogue miss distance 15.8 LD · 6.07 × 10⁶ km. The curve is the geocentric path from 2034-08-19 to 2034-08-25, 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
2034-08-22 14:13:00 Earth 0.0406 AU 15.8 LD 16 km/s
2041-05-06 21:19:00 Mercury 0.071 AU 27.6 LD 24 km/s
2041-05-06 21:19:00 Merc 0.071 AU 27.6 LD 24 km/s
2043-08-23 23:55:00 Earth 0.0923 AU 35.9 LD 14.9 km/s
2046-11-17 20:47:00 Mercury 0.0603 AU 23.5 LD 33.3 km/s
2046-11-17 20:47:00 Merc 0.0603 AU 23.5 LD 33.3 km/s
2052-08-26 06:16:00 Earth 0.1477 AU 57.5 LD 14 km/s
2061-08-31 10:25:00 Earth 0.1981 AU 77.1 LD 13.6 km/s
2062-10-12 03:09:00 Mercury 0.0501 AU 19.5 LD 27.2 km/s
2062-10-12 03:09:00 Merc 0.0501 AU 19.5 LD 27.2 km/s

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

Sources