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AsteriaStar
Interstellar object

3I/ATLAS

The third confirmed interstellar object, discovered on 1 July 2025 by the ATLAS survey in Chile. Its orbit is the most strongly hyperbolic of the three found so far, with an eccentricity of roughly 6, and it showed cometary activity as it passed through the inner Solar System in late 2025. Some physical parameters remain preliminary, but its interstellar origin is established by the trajectory.

Confirmed interstellarHyperbolic (e ≈ 6.1) — the most strongly hyperbolic yet found

Note

Discovered in mid-2025; some physical parameters remain preliminary. The interstellar origin rests on the strongly hyperbolic orbit, not on any claim of artificial origin.

Physical & orbital character

Origin:Unbound; the most strongly hyperbolic interstellar object found to date
Activity:An active comet — a coma was detected soon after discovery
Size:Nucleus uncertain — early estimates span a few hundred metres to a few kilometres
Composition:Cometary; detailed composition still being studied

Knowledge connections

Sources

The primary and reference sources this topic draws on.

  • Minor Planet CenterIAU Minor Planet Center

    Designations and orbits of asteroids, comets, and minor bodies.

  • NASA JPLJet Propulsion Laboratory / Solar System Dynamics

    Orbital data, ephemerides, and small-body parameters for planets, asteroids, and comets.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.