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Asteroid Near-Earth

2025 OT2

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(2025 OT2)

Where is it now

Distance from Sun
0.544 AU
True anomaly
53.71°
Distance from Earth
1.537 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 OT2 — 0.544 AU from the Sun 2025 OT2
Seen from above the ecliptic, north up, to scale. Grid: Earth's orbit in blue. 2025 OT2 is 1.537 AU from Earth today (12.8 light-minutes).

In the sky

Right ascension
13h 32m 21s
Declination
-06° 21′ 26″
Constellation
Virgo
Distance from Earth
1.54 AU
Elongation from the Sun
3.07° — 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
0.801 AU
Eccentricity
0.3998
Inclination
8.87°
Orbital period
261.9 days
Perihelion
0.481 AU
Aphelion
1.121 AU
Longitude of ascending node
126.5°
Argument of periapsis
21.63°
Epoch · J2000
2461200.5
Orbit class · ATE
Aten
Earth MOID · 10.2 LD
0.0263 AU
Tisserand (Jupiter)
7.206

Orbit quality

Orbit poorly determined (uncertainty code 7).

Observations used
33
Data arc
24 hours
First observed
25 July 2025
Last observed
26 July 2025
Residual RMS
0.63 ″
Solution · Otto Matic
27 July 2025

Visual & observation

Absolute magnitude (H)
25.85

Discovery & classification

Aten Near-Earth Object

Close approaches 32 on record

Flyby geometry
Ecliptic flyby of 2025 OT2 at 2030-07-19 05:58 UTC Top-down view of the ecliptic, Earth at the centre, for the 2030-07-19 05:58 UTC close approach of 2025 OT2. Catalogue miss distance 29.1 LD · 1.12 × 10⁷ km. The curve is the geocentric path from 2030-07-16 to 2030-07-22, 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 29.1 LD · 1.12 × 10⁷ km 2030-07-19 05:58 UTC Earth Moon Heliocentric, approximate

Top-down view of the ecliptic, Earth at the centre, for the 2030-07-19 05:58 UTC close approach of 2025 OT2. Catalogue miss distance 29.1 LD · 1.12 × 10⁷ km. The curve is the geocentric path from 2030-07-16 to 2030-07-22, 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
2028-01-27 06:12:00 Venus 0.0897 AU 34.9 LD 14.7 km/s
2030-07-19 05:58:00 Earth 0.0747 AU 29.1 LD 12.1 km/s
2032-05-16 19:48:00 Venus 0.0997 AU 38.8 LD 16.3 km/s
2035-07-21 00:52:00 Earth 0.1781 AU 69.3 LD 15.4 km/s
2036-09-04 11:03:00 Venus 0.1176 AU 45.8 LD 17.9 km/s
2038-09-24 12:14:00 Earth 0.1907 AU 74.2 LD 13.7 km/s
2040-12-23 21:51:00 Venus 0.1442 AU 56.1 LD 19.6 km/s
2043-09-24 03:39:00 Earth 0.1355 AU 52.8 LD 10.7 km/s
2068-07-22 18:57:00 Earth 0.0377 AU 14.7 LD 9.5 km/s
2072-09-17 08:40:00 Venus 0.1037 AU 40.4 LD 16.7 km/s

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

Sources