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System of two stars orbiting each other
A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars are among
Binary_star
Potential conditions for extraterrestrial life in binary star systems
Planets in binary star systems may be candidates for supporting extraterrestrial life. Their habitability is determined by many factors from a variety
Habitability of binary star systems
Habitability_of_binary_star_systems
Collapsed core of a massive star
been detected are pulsars or a part of a binary system. Neutron stars in a binary system with a main sequence star can pull in large amounts of gas from
Neutron_star
Binary star system whose component stars are very close
In astronomy, a contact binary is a binary star system whose component stars are so close that they touch each other or have merged to share their gaseous
Contact_binary
Small number of stars that orbit each other
comets). A star system of two stars is known as a binary star, binary star system or physical double star. Systems with four or more components are rare
Star_system
Japanese manga series and its adaptations
digital outlets. An action role-playing game, titled Made in Abyss: Binary Star Falling into Darkness (メイドインアビス 闇を目指した連星, Meido in Abisu Yami o Mezashita
Made_in_Abyss
American hip hop group
Binary Star is an underground hip-hop duo from Pontiac, Michigan. The duo consists of rapper One Be Lo (also known as OneManArmy), rapper Senim Silla
Binary_Star_(hip-hop_group)
Pair of stars that appear close to each other
optical telescopes. This occurs because the pair either forms a binary star (i.e. a binary system of stars in mutual orbit, gravitationally bound to each
Double_star
Double stars that show a significant interaction between their components
An Interacting binary star is a type of binary star in which one or both of the component stars has filled or exceeded its Roche lobe, also known as a
Interacting_binary_star
American rapper (born 1976)
Pontiac, Michigan. He is well respected for being one half of the rap duo Binary Star, and has released a number of well-received solo albums. He is a member
One_Be_Lo
Two astronomical bodies which orbit each other
considered a binary because they are different kinds of objects. Astronomy portal Binary asteroid Binary star Contact binary Contact binary (small Solar
Binary_system
list (link) Gatewood, George (2005-08-01). "An Astrometric Study of the Binary Star α Ophiuchi". The Astronomical Journal. 130 (2): 809–814. Bibcode:2005AJ
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Open cluster in the constellation Taurus
eventually be reduced to a remnant containing about a dozen star systems, most of them binary or multiple, which will remain vulnerable to ongoing dissipative
Hyades_(star_cluster)
American rapper)
from Pontiac, Michigan, best known as one of the two MCs in rap duo Binary Star, along with One Be Lo. Senim Silla co-hosted the Foreally Show with lifelong
Senim_Silla
Model for the accretion of a uniform gas by a massive body
interstellar medium by neutron stars and black holes, or wind mass transfer in binary star systems. It is named after Hermann Bondi, Fred Hoyle, and Raymond Lyttleton
Bondi–Hoyle–Lyttleton accretion
Bondi–Hoyle–Lyttleton_accretion
Astronomic function
astronomy, the binary mass function or simply mass function is a function that constrains the mass of the unseen component (typically a star or exoplanet)
Binary_mass_function
2000 studio album by Binary Star
Universe is the second and final studio album from American hip hop duo Binary Star (Senim Silla & One Be Lo), released on October 31, 2000. The release
Masters of the Universe (Binary Star album)
Masters_of_the_Universe_(Binary_Star_album)
Common gas atmosphere of a binary star system
envelope (CE) is gas that contains a binary-star system. The gas does not rotate at the same rate as the embedded binary system. A system with such a configuration
Common_envelope
System. It is thought that most black holes are solitary, but black holes in binary or larger systems are much easier to detect. Solitary black holes can generally
List of nearest known black holes
List_of_nearest_known_black_holes
System consisting of two black holes in close orbit around each other
black holes themselves, binary black hole systems are classified as either stellar-mass—involving remnants of high-mass binary star systems or formed by
Binary_black_hole
Extrasolar planet of the binary Kepler-14 system
in orbit around the primary star of the binary Kepler-14 system. It is currently the only planet known to exist in this star system. Kepler-14b is 8.4 times
Kepler-14b
Coming together of two stars
of two stars caused by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation
Stellar_collision
Large self-illuminated object in space
paradox, where the most-evolved star in a system is the least massive. The evolution of binary star and higher-order star systems is intensely researched
Star
Stars that appear green
350 light years away. Another is the Sigma Cassiopeiae (σ Cas) star system, a binary star 1,500 light-years from Earth. σ Cas‑A is a greenish-hued magnitude 5
Green_star_(astronomy)
Class of binary stars
lifetime and the mass-transfer rate in an X-ray binary depends on the evolutionary status of the donor star, the mass ratio between the stellar components
X-ray_binary
Topics referred to by the same term
children Binary-coded decimal, a method for encoding for decimal digits in binary sequences Binary star, a star system with two stars in it X-ray binary, a
Binary
Type of binary star
high-mass X-ray binary (HMXB or HMXRB) is a binary star system containing a compact object (typically a black hole or neutron star) and a normal star more massive
High-mass_X-ray_binary
Astronomical category of stars
In astronomy, the term iron star has been used for two observed types of star: Binary stars with highly variable emission and stellar spectral type Fe
Iron_star
Zodiac constellation in the northern hemisphere
470 years. A wide-set red dwarf star is also a part of the system; this star is an Algol-type eclipsing binary star with a period of 19.5 hours; its
Gemini_(constellation)
Pulsar in the constellation Aquila
1913+16) is a binary star system composed of a neutron star and a pulsar which orbit around their common center of mass. It is the first binary pulsar ever
Hulse–Taylor_pulsar
Circumbinary exoplanet orbiting TOI-1338
BEBOP-1 b or EBLM J0608-59 b) is a Saturn-sized exoplanet orbiting the binary star system TOI-1338. It is a circumbinary planet, meaning it orbits both
TOI-1338_b
Type of neutron star with beams of radiation
tools for astronomers. For example, observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence of gravitational
Pulsar
Stellar core remnant
Sirius binary star. In 1910, Henry Norris Russell, Edward Charles Pickering and Williamina Fleming discovered that, despite being a dim star, 40 Eridani
White_dwarf
Astronomical objects
Bursting Pulsar Vela Junior LMC N49 Intermediate-mass X-ray binary High-mass X-ray binaries Centaurus X-3 Circinus X-1 GX 301-2 Hercules X-1 Kesteven 79
List_of_neutron_stars
Binary star system
D9 is a binary star system located in the S Cluster, a dense group of stars orbiting Sagittarius A* (Sgr A*), the supermassive black hole at the center
D9_(star)
Brightest star in Earth's night sky
twice as bright as Canopus, the next brightest star. Sirius is a binary star consisting of a main-sequence star of spectral type A0 or A1, termed Sirius A
Sirius
Triple-star system in the constellation Norma
Apep is a triple star system containing a Wolf–Rayet binary and a hot supergiant, located in the constellation of Norma. Named after the serpent deity
Apep_(star_system)
1999 studio album by Binary Star
Waterworld is the debut album from Michigan hip hop duo Binary Star. The album was self-released, with only 1,000 copies printed. A rearranged, remixed
Waterworld (Binary Star album)
Waterworld_(Binary_Star_album)
Class of astronomical objects
A symbiotic binary is a type of binary star system, often simply called a symbiotic star. They usually contain a white dwarf with a companion red giant
Symbiotic_binary
Accumulation of matter around a star
disc is one which orbits around the secondary (i.e. less massive) star of the binary star system. This type of disc will only form when a high enough level
Circumstellar_disc
Constellation in the northern celestial hemisphere
Dziban) is a binary star divisible in binoculars and small amateur telescopes, 72 light-years from Earth. The primary is a yellow-white star of magnitude
Draco_(constellation)
2015 detection made by LIGO interferometers
inferred only indirectly, via their effect on the timing of pulsars in binary star systems. The waveform, detected by both LIGO observatories, matched the
First observation of gravitational waves
First_observation_of_gravitational_waves
Type of stellar binary
A visual binary is a gravitationally bound binary star system that can be visually resolved as two separate stars, as opposed to a singular point source
Visual_binary
Exoplanet orbiting Kepler-16
exoplanet consisting of half gas and half rock and ice. It orbits a binary star, Kepler-16, with a period of 229 days. "It is the first confirmed, unambiguous
Kepler-16b
double star, though the latter can also refer to an optical double star, a type of optical illusion which is entirely distinct from true binary star systems
Glossary_of_astronomy
Binary stars in the Big Dipper asterism
Ursae Majoris (80 UMa), is a binary star, the pair together forming a sextuple system. Mizar was the first known binary star system, claimed to be discovered
Mizar_and_Alcor
American actor (born 1984)
Billions. Dillon identifies as non-binary and uses singular they pronouns. Their role on Billions is the first non-binary main character on North American
Asia_Kate_Dillon
Constellation in the northern celestial hemisphere
Another eclipsing binary in Auriga, part of the Haedi asterism with Eta Aurigae, is Zeta Aurigae (Saclateni), an eclipsing binary star at a distance of
Auriga
Topics referred to by the same term
theory Binary system (astronomy), a system of two celestial bodies on a mutual orbit Binary asteroid Binary star Contact binary Contact binary (asteroid)
Binary system (disambiguation)
Binary_system_(disambiguation)
Number expressed in the base-2 numeral system
A binary number is a number expressed in the base-2 numeral system or binary numeral system, a method for representing numbers that uses only two symbols
Binary_number
Recurrent nova in the constellation Corona Borealis
T Coronae Borealis is a binary star and a recurrent nova about 3,000 light-years (920 parsecs) away in the constellation Corona Borealis. Its apparent
T_Coronae_Borealis
Long-period exoplanet orbiting b Centauri
b (sometimes b Centauri (AB)b) is a circumbinary planet orbiting the binary star system b Centauri, located in the southern constellation Centaurus. The
B_Centauri_b
Binary star system in the constellation Taurus
designation 27 Tauri, is a binary star system in the constellation of Taurus. It is a member of the Pleiades, an open star cluster (M45). It is 444 light-years
Atlas_(star)
Constellation in the northern celestial hemisphere
the smallest constellation, Crux. Its brightest star, Alpheratz (Alpha Andromedae), is a binary star that has also been counted as a part of Pegasus,
Andromeda_(constellation)
Constellation in the southern hemisphere
Eridani is a binary star 290 light-years from Earth. The primary is a yellow-hued star of magnitude 4.8 and the secondary is a blue-green star of magnitude
Eridanus
Star in the constellation Ophiuchus
is a binary star system located 16.7 light-years away from the Earth. It is in the constellation Ophiuchus. At magnitude 4 it appears as a dim star visible
70_Ophiuchi
Star in the constellation of Draco
Draconis or α Draconis, is a binary star system in the northern constellation of Draco. A relatively inconspicuous star in the night sky of the Northern
Thuban
Constellation straddling the celestial equator
a yellow star of magnitude 3.4 and the secondary is a blue star of magnitude 6.7. However, there are several dimmer double stars and binary stars in Hydra
Hydra_(constellation)
Japanese manga artist (born 1979)
LovePlus Dewy's Adventure (水精デューイの大冒険!!) (Character design) Made in Abyss: Binary Star Falling into Darkness (Original story supervisor) ジグソーパズルのアップルワン◆「つくしあきひと」のジグソーパズル
Akihito_Tsukushi
Type of variable stellar binary
Heartbeat stars are variable binary star systems in eccentric orbits with vibrations caused by tidal forces. The name "heartbeat" comes from the similarity
Heartbeat_star
Binary star system in the constellation Cetus
Mira (pronounced /ˈmaɪrə/, MY-rə) is a binary star system in the constellation Cetus. It has the Bayer designation Omicron Ceti, which is Latinized from
Mira
Binary star system in the constellation Pictor
J0608-59) is an eclipsing binary star system located in the constellation Pictor, about 1,300 light-years (400 pc) from Earth. The binary system consists of
TOI-1338
Binary star in the constellation Cepheus
is an eclipsing binary star system located in the constellation Cepheus. It is both a B[e] star and shell star. As a 5th magnitude star, it is visible
VV_Cephei
Topics referred to by the same term
**, symbol in astronomical notation representing: Binary star Double star Multiple star Multiple star system 2018 Winter Paralympics (**), whose logo is
**
Set of isotopes in nuclear astrophysics
p-nuclei from the γ-process. A neutron star in a binary star system can also accrete matter from the companion star on its surface. Combined hydrogen and
P-nuclei
Substellar object
about 8%±6%. Brown dwarf binaries have a higher companion-to-host ratio q=MB/MA for lower mass binaries. Binaries with a M-type star as a primary have for
Brown_dwarf
Binary star system in which two massive stars emit powerful stellar winds
A colliding-wind binary is a binary star system in which the two members are massive stars that emit powerful, radiatively-driven stellar winds. The location
Colliding-wind_binary
Star system in the Centaurus constellation
that together form the binary star system α Centauri AB. To the naked eye, these two main components appear to be a single star with an apparent magnitude
Alpha_Centauri
Zodiac constellation in the northern hemisphere
its absolute magnitude is 2.1. It is a spectroscopic binary star, one in which the companion star is only known through analysis of the spectra. The spectral
Aries_(constellation)
Quantities used in astronomy
used to calculate the relative apparent position of components of a binary star system. For (amateur) astronomers who want to observe double stars, it
Thiele−Innes_elements
Five-star system in the constellation Orion
which orbits Aa with an orbital period of 152 years Delta Ori C, a binary star with an orbital period of 30 days, also known as HD 36485 Delta Ori Ca
Mintaka
Type of planet
forms in a binary star system when one of the stars becomes a red giant and mass transfers from it to an accretion disk around the other star where the
Second_generation_planet
Star whose brightness fluctuates, as seen from Earth
preserved historical document of the discovery of a variable star, the eclipsing binary Algol, but the validity of this claim has been questioned. Aboriginal
Variable_star
Small Magellanic Cloud star in the constellation Tucana
HV 2112 is a cool luminous variable star in the Small Magellanic Cloud. Until 2018, it was considered to be the most likely candidate for a Thorne–Żytkow
HV_2112
Class of star
transfer in a binary star system. The mass transfer occurred when the now-observed giant star was on the main sequence. Its companion, the donor star, was a
Barium_star
Constellation in the southern celestial hemisphere
brighter than magnitude 5 . Other notable objects in Caelum are RR Caeli, a binary star with one known planet approximately 20.13 parsecs (65.7 ly) away; X Caeli
Caelum
Constellation in the northern celestial hemisphere
There are several prominent double stars and binary stars in Cepheus. Omicron Cephei is a binary star with a period of 800 years. The system, 211 light-years
Cepheus_(constellation)
Binary star system
Kepler-14 is a binary star system targeted by the Kepler spacecraft. It is host to one known planet: the Jupiter-like Kepler-14b. The star system was identified
Kepler-14
system. Stars in binary systems (or other multiples) are listed by their total or combined brightness if they appear as a single star to the naked eye
List_of_brightest_stars
Binary star in the Pleiades star cluster
Pleione is a binary star system in the Pleiades star cluster, within the constellation of Taurus. It has the variable star designation BU Tauri (BU Tau)
Pleione_(star)
Variable star in the constellation Cassiopeia
(V523 Cas) is an eclipsing binary star system located in the constellation of Cassiopeia. It is classified as an overcontact binary of the W Ursae Majoris
V523_Cassiopeiae
Planetary nebula located in the constellation Lyra
central star is a close binary central star of PNe (CSPN) that shows evidence of passing through a common-envelope (CE) phase. The central star is a ∼140-kK
ETHOS_1
Circumbinary planetary-mass object orbiting ROXs 42B
ROXs 42Bb is a directly imaged planetary-mass companion to the binary M star ROXs 42B, a likely member of the Rho Ophiuchi cloud complex. The companion
ROXs_42Bb
Gravitationally-binding region around a star in a binary system
lobe is the region around a star in a binary system within which orbiting material is gravitationally bound to that star. It is an approximately teardrop-shaped
Roche_lobe
Binary star with at least seven exoplanets 41 light-years away
55 Cancri is a binary star system located 41 light-years away from the Sun in the zodiac constellation of Cancer. It has the Bayer designation Rho1 Cancri
55_Cancri
American actor (born 1997)
playing Adira Tal in Star Trek: Discovery. They are the franchise's first openly non-binary actor and played its first non-binary role. Del Barrio has
Blu_del_Barrio
Nuclear explosion in a white dwarf star
usually created in a close binary star system consisting of a white dwarf and either a main sequence, subgiant, or red giant star. If the orbital period of
Nova
Binary star in the constellation Lynx
XO-5, formally named Absolutno, is a likely binary star system, made up of a G-type dwarf and a red dwarf companion, located approximately 893 light-years
XO-5
Jamaican astronomer
dynamics of interacting binary stars systems. However, her pioneering research in the tomography of interacting binary star systems and cataclysmic variable
Mercedes_Richards
Binary star in the constellation Scorpius
of the Sun. Antares appears as a single star when viewed with the naked eye, but it is actually a binary star system, with its two components called α
Antares
Astronomical phenomenon due to the gravitational lens effect
detect exoplanets, study limb darkening in distant stars, constrain the binary star population, and constrain the structure of the Milky Way's disk. Microlensing
Gravitational_microlensing
Constellation in the northern celestial hemisphere
19.13 ly away. It is a binary star made up of a G-dwarf star similar to the Sun, of apparent magnitude 3.45, and a K-dwarf star of apparent magnitude 7
Cassiopeia_(constellation)
Circumbinary exoplanet orbiting TOI-1338
TOI-1338 c (also known as BEBOP-1 c) is a gas giant exoplanet orbiting the binary star system TOI-1338. The planet and its two stars are located in the constellation
TOI-1338_c
orbit binary star systems (and 39 orbit multiple star systems with three or more stars). Specifically, they orbit what are known as "wide" binary star systems
Physics_and_Star_Wars
Binary star in the constellation Capricornus
Delta Capricorni is the brightest star in the constellation of Capricornus, the Sea Goat. It is a binary star system whose components are seen to eclipse
Delta_Capricorni
Constellation in the Southern Celestial Hemisphere
magnitudes 4.22 and 4.29. S Antliae is an eclipsing binary star system, changing in brightness as one star passes in front of the other. Sharing a common envelope
Antlia
Planet that orbits two stars instead of one
binary system have stable orbits around one of the two stars, closer in than the orbital distance of the other star (see Habitability of binary star systems)
Circumbinary_planet
Star in the constellation Draco
is a binary star system containing a G-type main-sequence star similar to the Sun. The primary component is called TrES-2A or TrES-2 parent star in reference
TrES-2_(star)
Planetary nebula located in Cassiopeia
was produced by V664 Cassiopeia, a binary star system. The distinct fist-shape of this nebula comes from the star system moving rapidly across the galaxy
HFG1
Temperate gas giant in Kepler-47 system
Object of Interest designation KOI-3154.02) is an exoplanet orbiting the binary star system Kepler-47, the outermost of three such planets discovered by NASA's
Kepler-47c
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BINARY STAR
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