An interstellar object is an astronomical object in interstellar space that is not gravitationally bound to a star. Applicable objects include asteroids, comets, and rogue planets, but not a star or stellar remnant.
This term can also be applied to an object that is on an interstellar trajectory but is temporarily passing close to a star, such as certain asteroids and comets (that is, exoasteroids and exocomets[1][2]). In the latter case, the object may be called an interstellar interloper.[3]
The first interstellar objects discovered were rogue planets, planets ejected from their original stellar system (e.g., OTS 44 or Cha 110913−773444), though they are difficult to distinguish from sub-brown dwarfs, planet-mass objects that formed in interstellar space as stars do.
The first interstellar object which was discovered traveling through the Solar System was 1I/ʻOumuamua in 2017. The second was 2I/Borisov in 2019. They both possess significant hyperbolic excess velocity, indicating they did not originate in the Solar System. The discovery of ʻOumuamua inspired the tentative identification of CNEOS 2014-01-08, also known as the Manus Island fireball, as an interstellar object that impacted the Earth by astronomers Amir Siraj and Avi Loeb in 2019.[4] This was supported by the U.S. Space Command in 2022 based on the object's velocity relative to the Sun,[5][6][7][8][9][10] In May 2023, astronomers reported the possible capture of other interstellar objects in Near Earth Orbit (NEO) over the years.[11][12] however, NASA and Other astronomers doubt this,[13][14][15][16][17][18] and still other experts found Earth-related explanations for the purported meteorite impact instead.[19]
The interstellar objects were once bound to a host star and have become unbound since. Different processes can cause planets and smaller objects (planetesimals) to become unbound from their host star.[20]
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