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Asteroid Near-Earth

2025 DQ4

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(2025 DQ4)

Where is it now

Distance from Sun
1.158 AU
True anomaly
184.65°
Distance from Earth
2.152 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 DQ4 — 1.158 AU from the Sun 2025 DQ4
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 DQ4 is 2.152 AU from Earth today (17.9 light-minutes).

In the sky

Right ascension
13h 20m 03s
Declination
-07° 01′ 51″
Constellation
Virgo
Distance from Earth
2.15 AU
Elongation from the Sun
3.23° — 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
0.813 AU
Eccentricity
0.4284
Inclination
2.5°
Orbital period
267.6 days
Perihelion
0.465 AU
Aphelion
1.161 AU
Longitude of ascending node
122.62°
Argument of periapsis
250.9°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 8.6 LD
0.0222 AU
Tisserand (Jupiter)
7.117

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
44
Data arc
12 days
First observed
22 February 2025
Last observed
6 March 2025
Residual RMS
0.49 ″
Solution · Otto Matic
7 March 2025

Visual & observation

Absolute magnitude (H)
24.77

Discovery & classification

Aten Near-Earth Object

Close approaches 93 on record

Flyby geometry
Ecliptic flyby of 2025 DQ4 at 2028-04-24 07:44 UTC Top-down view of the ecliptic, Earth at the centre, for the 2028-04-24 07:44 UTC close approach of 2025 DQ4. Catalogue miss distance 53.2 LD · 2.04 × 10⁷ km. The curve is the geocentric path from 2028-04-21 to 2028-04-27, 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 53.2 LD · 2.04 × 10⁷ km 2028-04-24 07:44 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2028-04-24 07:44 UTC close approach of 2025 DQ4. Catalogue miss distance 53.2 LD · 2.04 × 10⁷ km. The curve is the geocentric path from 2028-04-21 to 2028-04-27, 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
2028-04-24 07:44:00 Earth 0.1366 AU 53.2 LD 8.8 km/s
2032-02-26 13:59:00 Venus 0.1032 AU 40.2 LD 10.8 km/s
2033-02-05 20:54:00 Venus 0.0566 AU 22.0 LD 13.2 km/s
2035-10-28 18:12:00 Venus 0.1074 AU 41.8 LD 20.6 km/s
2036-02-29 12:17:00 Earth 0.0907 AU 35.3 LD 9.1 km/s
2039-05-05 04:09:00 Earth 0.0973 AU 37.9 LD 9.1 km/s
2047-03-14 02:23:00 Earth 0.141 AU 54.9 LD 8.8 km/s
2047-07-15 11:17:00 Venus 0.1126 AU 43.8 LD 10.3 km/s
2048-06-24 15:54:00 Venus 0.0502 AU 19.5 LD 13.6 km/s
2050-05-11 01:58:00 Earth 0.0465 AU 18.1 LD 10.7 km/s

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

Sources