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Asteroid Near-Earth

2025 XP2

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(2025 XP2)

Where is it now

Distance from Sun
1 AU
True anomaly
191.07°
Distance from Earth
1.012 AU
As of
20 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 — 0.996 AU from the Sun Earth 2025 XP2 — 1 AU from the Sun 2025 XP2
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 XP2 is 1.012 AU from Earth today (8.4 light-minutes).

In the sky

Right ascension
09h 58m 12s
Declination
+10° 46′ 50″
Constellation
Leo
Distance from Earth
1.01 AU
Elongation from the Sun
59.79° — 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
0.882 AU
Eccentricity
0.1374
Inclination
7.51°
Orbital period
302.7 days
Perihelion
0.761 AU
Aphelion
1.003 AU
Longitude of ascending node
256.88°
Argument of periapsis
0.41°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 7.0 LD
0.0181 AU
Tisserand (Jupiter)
6.707

Orbit quality

Orbit poorly determined (uncertainty code 6).

Observations used
43
Data arc
10 days
First observed
11 December 2025
Last observed
21 December 2025
Residual RMS
0.67 ″
Solution · Otto Matic
1 September 2026

Visual & observation

Absolute magnitude (H)
27.76

Discovery & classification

Aten Near-Earth Object

Close approaches 39 on record

Flyby geometry
Ecliptic flyby of 2025 XP2 at 2031-01-05 15:30 UTC Top-down view of the ecliptic, Earth at the centre, for the 2031-01-05 15:30 UTC close approach of 2025 XP2. Catalogue miss distance 56.5 LD · 2.17 × 10⁷ km. The curve is the geocentric path from 2031-01-02 to 2031-01-08, 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 56.5 LD · 2.17 × 10⁷ km 2031-01-05 15:30 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2031-01-05 15:30 UTC close approach of 2025 XP2. Catalogue miss distance 56.5 LD · 2.17 × 10⁷ km. The curve is the geocentric path from 2031-01-02 to 2031-01-08, 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
2027-03-11 06:27:00 Venus 0.1227 AU 47.8 LD 8.8 km/s
2029-08-30 03:52:00 Venus 0.073 AU 28.4 LD 7.4 km/s
2031-01-05 15:30:00 Earth 0.1452 AU 56.5 LD 7.4 km/s
2048-09-22 10:19:00 Venus 0.0507 AU 19.7 LD 7.2 km/s
2049-11-16 23:33:00 Earth 0.1283 AU 49.9 LD 7.1 km/s
2051-03-14 04:57:00 Venus 0.1403 AU 54.6 LD 9.1 km/s
2054-12-13 11:36:00 Earth 0.0245 AU 9.5 LD 4.6 km/s
2072-09-18 07:15:00 Venus 0.0806 AU 31.4 LD 7.8 km/s
2073-11-25 06:57:00 Earth 0.0531 AU 20.7 LD 5.2 km/s
2075-03-09 22:01:00 Venus 0.0787 AU 30.6 LD 7.6 km/s

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

Sources