An interstellar object is any astronomical body, such as an asteroid, comet, or rogue planet, located in interstellar space and not gravitationally bound to a star. These objects offer valuable insights into planetary formation and the composition of other star systems. The study of these objects helps scientists to better understand the universe beyond our solar system, including the prevalence and characteristics of planetary systems elsewhere.
In the early 1980s, C/1980 E1, initially bound to the Sun, passed near Jupiter and gained enough speed to escape the Solar System. This event in 1980 changed its orbit from elliptical to hyperbolic, making it the most eccentric object known at the time and setting it on a course for interstellar space.
In 1996 comet Hyakutake C/1996 B2 was discovered with atypical chemical makeups for comets in the Solar System and there is the possibility that it may have been captured into a heliocentric orbit while passing through the Solar System.
On July 28, 2006 a multi-centimeter intergalactic meteor hit the atmosphere above the Special Astrophysical Observatory of the Russian Academy of Sciences.
In 2007, Afanasiev et al. reported the likely detection of a multi-centimeter intergalactic meteor hitting the atmosphere above the Special Astrophysical Observatory of the Russian Academy of Sciences on 28 July 2006.
On January 8, 2014, CNEOS 2014-01-08 (IM1), a 0.46-ton meteor, burned up in Earth's atmosphere. It exploded near Papua New Guinea at an altitude of 18.7 km.
In 2014 a paper was published, claiming the anomalous properties of CNEOS 2014-01-08 meteoroid are better described as measurement error rather than genuine parameters.
On March 9, 2017, CNEOS 2017-03-09 (IM2), a meteor with a mass of roughly 6.3 tons, burned up in the Earth's atmosphere.
In October 2017, a dim object, initially named C/2017 U1, was discovered by the Pan-STARRS telescope. It was later renamed A/2017 U1 after no cometary activity was observed. After its interstellar nature was confirmed, it was renamed again to 1I/ʻOumuamua, signifying it as the first interstellar object discovered.
In 2017, astronomers Amir Siraj and Avi Loeb identified several centaur candidates, such as 2017 SV13, which are orbiting the Sun but may have been captured in the distant past as interstellar objects.
In 2017, the Initiative for Interstellar Studies (i4is) launched Project Lyra to assess the feasibility of a mission to ʻOumuamua.
In 2017, the first interstellar object, 1I/ʻOumuamua, was discovered traveling through the Solar System. These objects have a high hyperbolic excess velocity, meaning they originated outside of the Solar System, having been ejected from their host star.
In 2017, the first large interstellar object (1I/ʻOumuamua) was detected in the solar system. These objects are expected to be detected more frequently with new telescopes.
In September 2018, astronomers proposed several potential home star systems for ʻOumuamua, suggesting where it may have originated from its interstellar journey.
In November 2018, Harvard astronomers Amir Siraj and Avi Loeb predicted the existence of hundreds of ʻOumuamua-size interstellar objects in the Solar System and identified some centaur candidates.
In 2018, astronomers found that comet C/2018 V1 (Machholz–Fujikawa–Iwamoto) has a 72.6% probability of having an extrasolar provenance although an origin in the Oort cloud could not be excluded.
In August 2019, comet 2I/Borisov was discovered, and it had a high eccentricity.
On September 13, 2019, the Gran Telescopio Canarias obtained a visible spectrum of 2I/Borisov, revealing a surface composition similar to typical Oort Cloud comets. The IAU Working Group named the comet 2I/Borisov.
In 2019, a preprint suggested that the meteor CNEOS 2014-01-08 (IM1) had been of interstellar origin.
In 2019, the interstellar object 2I/Borisov was detected. The expectation is that future telescopes will detect interstellar objects more frequently.
On March 12, 2020, astronomers reported observational evidence of "ongoing nucleus fragmentation" from Borisov.
In April 2022, the U.S. Space Command declassified and confirmed the velocity of a potential interstellar meteor based on data collected from its planetary defense sensors.
In September 2022, astronomers Amir Siraj and Avi Loeb reported the discovery of a candidate interstellar meteor, CNEOS 2017-03-09, that impacted Earth in 2017 and is considered a possible interstellar object.
In November 2022, a paper was published claiming the anomalous properties of CNEOS 2014-01-08 are better described as measurement error rather than genuine parameters.
In May 2023, astronomers reported the possible capture of other interstellar objects in Near Earth Orbit (NEO) over the years.
In September 1, 2023, Further related studies were reported on CNEOS 2014-01-08.
In July 2025, 3I/ATLAS was discovered with a record eccentricity of 6.1.
On July 1, 2025, a third interstellar object, 3I/ATLAS, was discovered by ATLAS at a distance of 4.5 AU from the Sun with a record setting eccentricity.
On October 29, 2025, 3I/ATLAS will reach perihelion at a distance of 1.357 AU from the Sun.
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