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An intergalactic star, also known as an intracluster star or a rogue star, is a star not gravitationally bound to any galaxy. Although a source of much discussion in the scientific community during the late 1990s, intergalactic stars are now generally thought to have originated in galaxies, like other stars, but later expelled as the result of either colliding galaxies or of a multiple star system travelling too close to a supermassive black hole, which are found at the center of many galaxies.

Collectively, intergalactic stars are referred to as the intracluster stellar population, or IC population for short, in the scientific literature.[1]


The hypothesis that stars exist only in galaxies was disproven in 1997 with the discovery of intergalactic stars.[2] The first to be discovered were in the Virgo cluster of galaxies, where some one trillion are now surmised to exist.[3]
Collisions between galaxies are commonly thought to be a source of intergalactic stars.
Proposed mechanisms for the ejection of intergalactic stars by supermassive black holes.

The way these stars arise is still a mystery, but several scientifically credible hypotheses have been suggested and published by astrophysicists.

The most common hypothesis is that the collision of two or more galaxies can toss some stars out into the vast empty regions of intergalactic space. Although stars normally reside within galaxies, they can be expelled by gravitational forces when galaxies collide. It is commonly believed that intergalactic stars may primarily have originated from extremely small galaxies, since it is easier for stars to escape a smaller galaxy's gravitational pull, than that of a large galaxy.[4] However, when large galaxies collide, some of the gravitational disturbances might also expel stars. In 2015, a study of supernovae in intergalactic space suggested that the progenitor stars had been expelled from their host galaxies during a galactic collision between two giant ellipticals, as their supermassive black hole centres merged.[5]

Another hypothesis, that is not mutually exclusive to the galactic collisions hypothesis, is that intergalactic stars were ejected from their galaxy of origin by a close encounter with the supermassive black hole in the galaxy center, should there be one. In such a scenario, it is likely that the intergalactic star(s) was originally part of a multiple star system where the other stars were pulled into the supermassive black hole and the soon-to-be intergalactic star was accelerated and ejected away at very high speeds. Such an event could theoretically accelerate a star to such high speeds that it becomes a hypervelocity star, thereby escaping the gravitational well of the entire galaxy.[6] In this respect, model calculations (from 1988) predicts the supermassive black hole in the center of our Milky Way galaxy to expel one star every 100,000 years on average.[7]
Observation history

In 1997, the Hubble telescope discovered a large number of intergalactic stars in the Virgo cluster of galaxies. Later in the 1990s, scientists discovered another group of intergalactic stars in the Fornax cluster of galaxies.

In 2005, at the Smithsonian Center for Astrophysics, Warren Brown and his team attempted to measure the speeds of hypervelocity stars by using the Doppler Technique, by which light is observed for the similar changes that occur in sound when an object is moving away or toward something. But the speeds found are only estimated minimums, as in reality their speeds may be larger than the speeds found by the researchers. "One of the newfound exiles is moving in the direction of the constellation Ursa Major at about 1.25 million mph with respect to the galaxy. It is 240,000 light-years away. The other is headed toward the constellation Cancer, outbound at 1.43 million miles per hour and 180,000 light-years away."[8]

In the late 2000s, a diffuse glow from the intergalactic medium, but of unknown origin, was discovered. In 2012, it was suggested and shown that it might originate from intergalactic stars. Subsequent observations and studies have elaborated on the issue and described the diffuse extragalactic background radiation in more detail.[9][10]

Some Vanderbilt astronomers report that they have identified more than 675 stars at the edge of the Milky Way, between the Andromeda Galaxy and the Milky Way. They argue that these stars are hypervelocity (intergalactic) stars that were ejected from the Milky Way's galactic center. These stars are red giants with a high metallicity (a measure of the proportion of chemical elements other than hydrogen and helium within a star) indicating an inner galactic origin, since stars outside the disks of galaxies tend to have low metallicity and are older.[11]

Some recently discovered supernovae have been confirmed to have exploded hundreds of thousands of light-years from the nearest star or galaxy.[12][5] Most intergalactic star candidates found in the neighborhood of the Milky Way seem not to have an origin in the Galactic Center but in the Milky Way disk or elsewhere.[13][14]

In 2005, the Spitzer Space Telescope revealed a hitherto unknown infrared component in the background from the cosmos. Since then, several other anisotropies at other wavelengths - including blue and x-ray - have been detected with other space telescopes and they are now collectively described as the diffuse extragalactic background radiation. Several explanations have been discussed by scientists, but in 2012, it was suggested and shown how for the first time this diffuse radiation might originate from intergalactic stars. If that is the case, they might collectively comprise as much mass as that found in the galaxies. A population of such magnitude was at one point thought to explain the photon underproduction crisis, and may explain a significant part of the dark matter problem.[9][10][15][16]
Known locations

This section needs to be updated. Please update this article to reflect recent events or newly available information. (September 2019)

The first intergalactic stars were discovered in the Virgo cluster of galaxies. These are largely approximately 300,000 light years away from the nearest galaxy. Although the precise mass of the intergalactic star population cannot be known exactly, it is estimated that locally they make up 10 percent of the mass of the Virgo cluster of galaxies (and most likely, this total outweighs any of its 2500 galaxies).[17]

As of 2015, approximately 675 rogue stars have been discovered at the edge of the Milky Way, towards the Andromeda Galaxy.[11]
See also

Blue straggler – A main sequence star that is more luminous and bluer than expected
HE 0437-5439
Intergalactic dust
Intracluster medium – Superheated plasma that permeates a galaxy cluster
Rogue planet – A planetary-mass object that orbits the galaxy directly, or interstellar planet
Stellar kinematics


See "Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging" for example
"NewsCenter – Hubble Finds Intergalactic Stars (01/14/1997) – Introduction". HubbleSite. 1997-01-14. Retrieved 2010-12-09.
"NewsCenter – Hubble Finds Intergalactic Stars (01/14/1997) – Release Text". HubbleSite. 1997-01-14. Retrieved 2010-12-09.
Witze, Alexandra (2014). "Half of Stars Lurk Outside Galaxies". Nature. Nature Publishing Group. doi:10.1038/nature.2014.16288. S2CID 124585348. Retrieved 3 January 2015. [ Lonely Supernova Likely Exiled by Merging Black Holes] (27 August 2015)
Britt, Robert Roy. "Exiled stars: Milky Way Boots Members". USATODAY. Retrieved 4 January 2015.
NASA: Hyperfast Star Was Booted From Milky Way (22 July 2010)
Britt, Robert Roy. "Exiled Stars: Milky Way Boots Members". USATODAY. Retrieved 4 January 2015.
Cooray; et al. (22 October 2012). "A measurement of the intrahalo light fraction with near-infrared background anisotropies". Nature.arXiv:1210.6031v1.
Zemcov; et al. (5 November 2014). "On the Origin of Near-Infrared Extragalactic Background Light Anisotropy". Nature.arXiv:1411.1411.
Salisbury, David. "Rogue Stars Ejected From the Galaxy Found in Intergalactic Space". Vanderbilt University. Vanderbilt University. Retrieved 3 January 2015.
Stallard, Brian (7 June 2015). "Between Galaxies: Lonely Supernovae Identified". Nature World News.
Bromley, Benjamin C.; Kenyon, Scott J.; Brown, Warren R.; Geller, Margaret J. (1 November 2018). "Nearby High-speed Stars in Gaia DR2". The Astrophysical Journal. 868 (1): 25 (15 pp.).arXiv:1808.02620. Bibcode:2018ApJ...868...25B. doi:10.3847/1538-4357/aae83e. S2CID 119241516.
de la Fuente Marcos, R.; de la Fuente Marcos, C. (8 July 2019). "Flying far and fast: the distribution of distant hypervelocity star candidates from Gaia DR2 data". Astronomy and Astrophysics. 627: A104 (17 pp.).arXiv:1906.05227. Bibcode:2019A&A...627A.104D. doi:10.1051/0004-6361/201935008. S2CID 186207054.
"Colossal Gas Cloud Discovered Around Milky Way". Space. Retrieved 3 January 2015.
Choi, Charles Q. "Lost in Space: Half of All Stars Drifting Free of Galaxies". Space. Purch. Retrieved 3 January 2015.

Henry C. Ferguson; et al. (1998), "Detection of intergalactic red-giant-branch stars in the Virgo cluster", Nature, 391 (6666): 461–463,arXiv:astro-ph/9801228, Bibcode:1998Natur.391..461F, doi:10.1038/35087, S2CID 4390832


Astrophysical Journal: Confirmation of Hostless Type Ia Supernovae Using Hubble Space Telescope Imaging (2 July 2015)
Astrophysical Journal: Intracluster Supernovae in the Multi-epoch Nearby Cluster Survey (22 February 2011)



Accretion Molecular cloud Bok globule Young stellar object
Protostar Pre-main-sequence Herbig Ae/Be T Tauri FU Orionis Herbig–Haro object Hayashi track Henyey track


Main sequence Red-giant branch Horizontal branch
Red clump Asymptotic giant branch
super-AGB Blue loop Protoplanetary nebula Planetary nebula PG1159 Dredge-up OH/IR Instability strip Luminous blue variable Blue straggler Stellar population Supernova Superluminous supernova / Hypernova

Spectral classification

Early Late Main sequence
O B A F G K M Brown dwarf WR OB Subdwarf
O B Subgiant Giant
Blue Red Yellow Bright giant Supergiant
Blue Red Yellow Hypergiant
Yellow Carbon
S CN CH White dwarf Chemically peculiar
Am Ap/Bp HgMn Helium-weak Barium Extreme helium Lambda Boötis Lead Technetium Be
Shell B[e]


White dwarf
Helium planet Black dwarf Neutron
Radio-quiet Pulsar
Binary X-ray Magnetar Stellar black hole X-ray binary


Blue dwarf Green Black dwarf Exotic
Boson Electroweak Strange Preon Planck Dark Dark-energy Quark Q Black Gravastar Frozen Quasi-star Thorne–Żytkow object Iron Blitzar

Stellar nucleosynthesis

Deuterium burning Lithium burning Proton–proton chain CNO cycle Helium flash Triple-alpha process Alpha process Carbon burning Neon burning Oxygen burning Silicon burning S-process R-process Fusor Nova
Symbiotic Remnant Luminous red nova


Core Convection zone
Microturbulence Oscillations Radiation zone Atmosphere
Photosphere Starspot Chromosphere Stellar corona Stellar wind
Bubble Bipolar outflow Accretion disk Asteroseismology
Helioseismology Eddington luminosity Kelvin–Helmholtz mechanism


Designation Dynamics Effective temperature Luminosity Kinematics Magnetic field Absolute magnitude Mass Metallicity Rotation Starlight Variable Photometric system Color index Hertzsprung–Russell diagram Color–color diagram

Star systems

Contact Common envelope Eclipsing Symbiotic Multiple Cluster
Open Globular Super Planetary system


Solar System Sunlight Pole star Circumpolar Constellation Asterism Magnitude
Apparent Extinction Photographic Radial velocity Proper motion Parallax Photometric-standard


Proper names
Arabic Chinese Extremes Most massive Highest temperature Lowest temperature Largest volume Smallest volume Brightest
Historical Most luminous Nearest
Nearest bright With exoplanets Brown dwarfs White dwarfs Milky Way novae Supernovae
Candidates Remnants Planetary nebulae Timeline of stellar astronomy

Related articles

Substellar object
Brown dwarf Sub-brown dwarf Planet Galactic year Galaxy Guest Gravity Intergalactic Planet-hosting stars Tidal disruption event

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