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Longer titles found: Habitability of binary star systems (view)

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Made in Abyss (3,891 words) [view diff] case mismatch in snippet view article find links to article

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, Made in Abyss: Yami o Mezashita

WZ Andromedae (520 words) [view diff] exact match in snippet view article find links to article

WZ Andromedae (abbreviated to WZ And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 11.6, but drops

KPD 1930+2752 (531 words) [view diff] exact match in snippet view article find links to article

KPD 1930+2752 is a binary star system including a subdwarf B star and a probable white dwarf with relatively high mass. Due to the nature of this astronomical

Psi6 Aurigae (427 words) [view diff] exact match in snippet view article find links to article

Psi6 Aurigae, Latinized from ψ6 Aurigae, is a spectroscopic binary star in the northern constellation of Auriga. It is a dim, naked eye star with an apparent

Position angle (377 words) [view diff] exact match in snippet view article find links to article

pole. As the example illustrates, if one were observing a hypothetical binary star with a PA of 30°, that means an imaginary line in the eyepiece drawn

One Be Lo (1,697 words) [view diff] case mismatch in snippet view article find links to article

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

QR Andromedae (721 words) [view diff] exact match in snippet view article find links to article

QR Andromedae (often abbreviated to QR And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 12.16

DS Andromedae (744 words) [view diff] exact match in snippet view article find links to article

DS Andromedae (often abbreviated to DS And) is an eclipsing binary star in the constellation Andromeda and a member of the open cluster NGC 752. Its maximum

Kepler-453b (169 words) [view diff] no match in snippet view article find links to article

Kepler-453b is a transiting circumbinary exoplanet in the binary-star system Kepler-453. It orbits the binary system in the habitable zone every 240.5

One Be Lo (1,697 words) [view diff] case mismatch in snippet view article find links to article

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

R Canis Majoris (712 words) [view diff] exact match in snippet view article find links to article

R Canis Majoris is an eclipsing interacting binary star system in the constellation Canis Major. It varies from magnitude 5.7 to 6.34. The system is unusual

HD 59686 Ab (226 words) [view diff] exact match in snippet view article find links to article

Ab is an exoplanet that orbits the giant star HD 59686 A in a close binary star system. It has a nearly circular orbit with a period of 300 days and

KOI-74 (369 words) [view diff] exact match in snippet view article find links to article

KOI-74 (KIC 6889235) is an eclipsing binary star in the constellation of Cygnus. The primary star is an A-type main-sequence star with a temperature of

NGC 2899 (565 words) [view diff] exact match in snippet view article find links to article

significant equatorial structure. This shape is believed to result from a binary star system. The mean expansion rate is 43 to 56 km/s, with high velocity

KX Andromedae (589 words) [view diff] exact match in snippet view article find links to article

KX Andromedae (often abbreviated to KX And) is a spectroscopic binary star in the constellation Andromeda. Its apparent visual magnitude varies between

CN Andromedae (607 words) [view diff] exact match in snippet view article find links to article

CN Andromedae (CN And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 9.62 and drops down to a minimum

List of nearest known black holes (1,311 words) [view diff] exact match in snippet view article find links to article

solution has a mass of 5.6 MSol. 4,700±800 1.44±0.25 A0620-00 (V616 Mon) Binary star system with orbit t=7.75 h 06h 22m 44.503s −00° 20′ 44.72″ 1986 A BH

AC Herculis (722 words) [view diff] exact match in snippet view article find links to article

AC Herculis, is an RV Tauri variable and spectroscopic binary star in the constellation of Hercules. It varies in brightness between apparent magnitudes

Kepler-451 (547 words) [view diff] exact match in snippet view article find links to article

and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf B star and a small

F Centauri (419 words) [view diff] exact match in snippet view article find links to article

F Centauri is a suspected astrometric binary star system in the southern constellation of Centaurus. It has a reddish hue and is visible to the naked

BX Andromedae (715 words) [view diff] exact match in snippet view article find links to article

BX Andromedae (BX And) is an eclipsing binary star in the constellation Andromeda. Its maximum apparent visual magnitude is 8.87. Within a cycle of approximately

Kepler-451 (547 words) [view diff] exact match in snippet view article find links to article

and abbreviated to 2M1938+4603) is an eclipsing post-common envelope binary star system that comprises two stars, a pulsating subdwarf B star and a small

KIC 9832227 (752 words) [view diff] exact match in snippet view article find links to article

KIC 9832227 is a contact binary star system in the constellation Cygnus, located about 2,060 light-years away. It is also identified as an eclipsing binary

35 Cygni (647 words) [view diff] exact match in snippet view article find links to article

35 Cygni is a spectroscopic binary star in the constellation Cygnus. Its apparent magnitude is 5.18. Located around 1,000 parsecs (3,300 ly) distant,

4 Sagittarii (454 words) [view diff] exact match in snippet view article find links to article

4 Sagittarii is a suspected astrometric binary star system in the zodiac constellation of Sagittarius, located approximately 390 light years away based

4U 0614+091 (121 words) [view diff] exact match in snippet view article find links to article

4U 0614+091 is a low-mass X-ray binary star system which features a neutron star and a low-mass companion star. The binary system lies 10,000 light-years

BB Doradus (318 words) [view diff] exact match in snippet view article find links to article

BB Dor is a cataclysmic variable, a pre-nova star, thus a close pair binary star system. It is composed of a red dwarf and a white dwarf. Observations

AB Doradus (1,013 words) [view diff] exact match in snippet view article find links to article

four components consisting of a pair of binary star systems separated by an angle of about 9″. The binary star AB Doradus Ba/Bb orbits the primary AB Doradus

Gliese 15 Ac (415 words) [view diff] exact match in snippet view article find links to article

star Gliese 15 A (Groombridge 34 A, GX Andromedae), which is part of a binary star system located about 11.6 light-years from the Sun. The planet was first

HD 10307 (831 words) [view diff] exact match in snippet view article find links to article

HD 10307 (HR 483) is a spectroscopic binary star in the constellation Andromeda. The primary is similar to the Sun in mass, temperature and metal content

AB Doradus (1,013 words) [view diff] exact match in snippet view article find links to article

four components consisting of a pair of binary star systems separated by an angle of about 9″. The binary star AB Doradus Ba/Bb orbits the primary AB Doradus

6 Andromedae (720 words) [view diff] exact match in snippet view article find links to article

6 Andromedae is an astrometric binary star system in the northern constellation of Andromeda. The designation comes from the star catalogue of John Flamsteed

NGC 6881 (135 words) [view diff] exact match in snippet view article find links to article

light-year from one tip to the other. The symmetry could be due to a binary star at the nebula's centre. "NGC 6881". SIMBAD. Centre de données astronomiques

C3 Centauri (523 words) [view diff] exact match in snippet view article find links to article

C3 Centauri is a suspected astrometric binary star system in the southern constellation of Centaurus. It has an orange hue and is dimly visible to the

J Centauri (467 words) [view diff] exact match in snippet view article find links to article

velocity at the equator is at least 223 km/s. It is believed to be a binary star system. This star may be a member of the Scorpio-Centaurus OB association

17 Aquarii (348 words) [view diff] exact match in snippet view article find links to article

17 Aquarii, abbreviated 17 Aqr, is a spectroscopic binary star system in the constellation of Aquarius. 17 Aquarii is the Flamsteed designation. It appears

Kepler-89 (486 words) [view diff] exact match in snippet view article find links to article

is a star with four confirmed planets. Kepler-89 is a possible wide binary star. The discovery of four planets orbiting the star was announced October

10 Andromedae (426 words) [view diff] exact match in snippet view article find links to article

10 Andromedae, abbreviated 10 And, is an astrometric binary star system in the northern constellation of Andromeda. 10 Andromedae is the Flamsteed designation

IC 348 (416 words) [view diff] exact match in snippet view article find links to article

angular diameter of 20″. The most massive stars in the cluster are the binary star system BD+31°643, which has a combined spectral class of B5. Based upon

HD 76728 (475 words) [view diff] exact match in snippet view article find links to article

HD 76728 is a suspected astrometric binary star system in the constellation Carina. It has the Bayer designation c Carinae; HD 76728 is the identifier

Xi Cancri (768 words) [view diff] exact match in snippet view article find links to article

Xi Cancri (ξ Cancri, abbreviated Xi Cnc, ξ Cnc) is a spectroscopic binary star system in the zodiac constellation of Cancer. It is visible to the naked

V3903 Sagittarii (726 words) [view diff] exact match in snippet view article find links to article

known as 11 Sagittarii, or its abbreviation 11 Sgr) is an eclipsing binary star system in the constellation Sagittiarus. It creates an H II region LBN

Kepler-411 (909 words) [view diff] exact match in snippet view article find links to article

Kepler-411 is a binary star system. Its primary star Kepler-411A is a K-type main-sequence star, orbited by the red dwarf star Kepler-411B on a wide orbit

J Centauri (467 words) [view diff] exact match in snippet view article find links to article

velocity at the equator is at least 223 km/s. It is believed to be a binary star system. This star may be a member of the Scorpio-Centaurus OB association

Kepler-560b (237 words) [view diff] exact match in snippet view article find links to article

Kepler-560 Bb, is a confirmed exoplanet orbiting the secondary star of the binary star system Kepler-560. It is only 287 light-years away. Though not listed

Winnecke 4 (774 words) [view diff] exact match in snippet view article find links to article

parsecs (470 ± 1 light-year) respectively. HD 238108 is itself a genuine binary star, with an 18th magnitude white dwarf companion 5 arcseconds away and a

Messier 73 (823 words) [view diff] exact match in snippet view article find links to article

2170±22, and 2290±24 light-years from the Sun, with the second being a binary star. M73 was discovered by Charles Messier in 1780 who originally described

HD 106760 (479 words) [view diff] exact match in snippet view article find links to article

HD 106760 is a single-lined spectroscopic binary star system in the northern constellation of Coma Berenices. It is faintly visible to the naked eye,

HD 102776 (786 words) [view diff] exact match in snippet view article find links to article

known by its Bayer designation j Centauri, is a suspected astrometric binary star system in the southern constellation of Centaurus. It has a blue-white

V4641 Sagittarii (733 words) [view diff] exact match in snippet view article find links to article

V4641 Sagittarii is a variable X-ray binary star system in the constellation Sagittarius. It is the source of one of the fastest superluminal jets in

HD 106760 (479 words) [view diff] exact match in snippet view article find links to article

HD 106760 is a single-lined spectroscopic binary star system in the northern constellation of Coma Berenices. It is faintly visible to the naked eye,

HD 34790 (448 words) [view diff] exact match in snippet view article find links to article

HD 34790 is a double-lined spectroscopic binary star system in the northern constellation of Auriga. It has a combined apparent magnitude of 5.66, which

Messier 73 (823 words) [view diff] exact match in snippet view article find links to article

2170±22, and 2290±24 light-years from the Sun, with the second being a binary star. M73 was discovered by Charles Messier in 1780 who originally described

12 Persei (482 words) [view diff] exact match in snippet view article find links to article

12 Persei (12 Per) is a double-lined spectroscopic binary star system in the northern constellation Perseus. Its combined apparent magnitude is 4.94,

HD 112028 (426 words) [view diff] exact match in snippet view article find links to article

main sequence stars. HD 112028 and HD 112014 together are known as the binary star Struve 1694. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia

36 G. Doradus (637 words) [view diff] exact match in snippet view article find links to article

36 G. Doradus (HD 40409) is a suspected astrometric binary star system in the southern constellation of Dorado. It is a faint system but visible to the

59 Persei (448 words) [view diff] exact match in snippet view article find links to article

59 Persei is a suspected astrometric binary star system in the northern constellation of Perseus. It is visible to the naked eye as a dim, white-hued

HD 102776 (786 words) [view diff] exact match in snippet view article find links to article

known by its Bayer designation j Centauri, is a suspected astrometric binary star system in the southern constellation of Centaurus. It has a blue-white

Eridanus (constellation) (1,498 words) [view diff] exact match in snippet view article

name, which means "the footstool". Theta Eridani, called Acamar, is a binary star with blue-white components, distinguishable in small amateur telescopes

HD 34790 (448 words) [view diff] exact match in snippet view article find links to article

HD 34790 is a double-lined spectroscopic binary star system in the northern constellation of Auriga. It has a combined apparent magnitude of 5.66, which

HD 38282 (701 words) [view diff] exact match in snippet view article find links to article

HD 38282 (R144, BAT99-118, Brey 89) is a massive spectroscopic binary star in the Tarantula Nebula (Large Magellanic Cloud), consisting of two hydrogen-rich

HD 22663 (367 words) [view diff] exact match in snippet view article find links to article

HD 22663 (y Eridani) is a candidate astrometric binary star system in the equatorial constellation of Eridanus. It is visible to the naked eye with an

Xi Cygni (549 words) [view diff] exact match in snippet view article find links to article

ξ Cygni (Latinised as Xi Cygni) is a spectroscopic binary star in the constellation Cygnus, made up of a K-type supergiant star (primary) and an A-type

AG Virginis (1,035 words) [view diff] exact match in snippet view article find links to article

AG Virginis is an eclipsing binary star system in the equatorial constellation of Virgo. With a maximum apparent visual magnitude of 8.51 it is too faint

HD 91190 (369 words) [view diff] exact match in snippet view article find links to article

HD 91190 is a suspected astrometric binary star system in the northern circumpolar constellation of Draco. It is faintly visible to the naked eye, having

GCIRS 16SW (696 words) [view diff] exact match in snippet view article find links to article

GCIRS 16SW, also known as S97, is a contact binary star located in the Galactic Center. It is composed of two hot massive stars of equal size that orbit

10 Boötis (482 words) [view diff] exact match in snippet view article find links to article

10 Boötis is a suspected astrometric binary star system in the northern constellation of Boötes, located around 528 light years away from the Sun. It

Tau2 Hydrae (469 words) [view diff] exact match in snippet view article find links to article

Tau2 Hydrae is a probable astrometric binary star system in the equatorial constellation of Hydra. Based upon an annual parallax shift of 6.30 mas as

LS Canis Majoris (358 words) [view diff] exact match in snippet view article find links to article

LS Canis Majoris is an eclipsing binary star located around 1,510 light years from Earth in the constellation Canis Major. Its apparent magnitude ranges

Tau2 Hydrae (469 words) [view diff] exact match in snippet view article find links to article

Tau2 Hydrae is a probable astrometric binary star system in the equatorial constellation of Hydra. Based upon an annual parallax shift of 6.30 mas as

LS Canis Majoris (358 words) [view diff] exact match in snippet view article find links to article

LS Canis Majoris is an eclipsing binary star located around 1,510 light years from Earth in the constellation Canis Major. Its apparent magnitude ranges

HD 110073 (516 words) [view diff] exact match in snippet view article find links to article

a radial velocity of +15 km/s. This is a single-lined spectroscopic binary star system that belongs to the Pleiades stream. As of 2011, the pair had

12 Aquarii (339 words) [view diff] exact match in snippet view article find links to article

velocity of +1.1 km/s. The magnitude 5.88 primary, component A, is itself a binary star with a separation of 0.05″–0.07″ and an orbital period of around 18.5 yr

WZ Cephei (322 words) [view diff] exact match in snippet view article find links to article

WZ Cephei is an eclipsing binary star of W Ursae Majoris-type in the constellation of Cepheus, located 880 light years away from the Sun. The stars orbit

WR 22 (1,401 words) [view diff] exact match in snippet view article find links to article

WR 22, also known as V429 Carinae or HR 4188, is an eclipsing binary star system in the constellation Carina. The system contains a Wolf-Rayet (WR) star

LH 54-425 (863 words) [view diff] exact match in snippet view article find links to article

LH 54-425 is a spectroscopic binary star system in the LH 54 OB association within the Large Magellanic Cloud in the constellation Dorado. The OB association

Lambda Hydrae (667 words) [view diff] exact match in snippet view article find links to article

λ Hydrae, Latinised as Lambda Hydrae, is a spectroscopic binary star in the constellation Hydra. Its apparent magnitude is 3.61 Located around 33.3 parsecs

20 Cancri (381 words) [view diff] exact match in snippet view article find links to article

20 Cancri is an astrometric binary star system in the constellation Cancer, located about 372 light-years away from the Sun. This system has the Bayer

FL Lyrae (623 words) [view diff] exact match in snippet view article find links to article

FL Lyrae is the variable star designation for an eclipsing binary star system in the northern constellation of Lyra. The combined apparent magnitude of

NGC 6025 (669 words) [view diff] exact match in snippet view article find links to article

compared to the Sun; more so than the Hyades cluster. Seven spectroscopic binary star systems have been identified. Only one blue straggler has been found

HD 126053 (842 words) [view diff] exact match in snippet view article find links to article

It shares a common proper motion through space with the spectroscopic binary star system HD 122742, and in the past the three may have formed a triple

GRS 1915+105 (804 words) [view diff] exact match in snippet view article find links to article

GRS 1915+105 or V1487 Aquilae is an X-ray binary star system containing a main sequence star and a black hole. Transfer of material from the star to the

6 Draconis (580 words) [view diff] exact match in snippet view article find links to article

6 Draconis is a single-lined spectroscopic binary star system in the northern constellation of Draco, located about 430 light years away from the Sun

U Coronae Borealis (198 words) [view diff] exact match in snippet view article find links to article

U Coronae Borealis (U CrB) is an Algol-type eclipsing binary star system in the constellation Corona Borealis. Its apparent magnitude varies between 7

14 Aquilae (524 words) [view diff] exact match in snippet view article find links to article

14 Aquilae is a probable spectroscopic binary star system in the equatorial constellation of Aquila. 14 Aquilae is the Flamsteed designation though it

14 Aquilae (524 words) [view diff] exact match in snippet view article find links to article

14 Aquilae is a probable spectroscopic binary star system in the equatorial constellation of Aquila. 14 Aquilae is the Flamsteed designation though it

51 Andromedae (747 words) [view diff] exact match in snippet view article find links to article

of the mythological, chained-to-the-rocks princess, the other being binary star system Gamma Andromedae. At an estimated age of 1.7 billion years, this

Chi Cancri (541 words) [view diff] exact match in snippet view article find links to article

Chi Cancri, Latinized from χ Cancri, is a candidate astrometric binary star system in the northern zodiac constellation of Cancer. It has a yellow-white

WASP-11b/HAT-P-10b (686 words) [view diff] exact match in snippet view article find links to article

dividing line between the class I and class II planets. The planet is in a binary star system, the second star is WASP-11 B, with a mass 0.34 ± 0.05 of the

Eta Andromedae (787 words) [view diff] exact match in snippet view article find links to article

Eta Andromedae, also named Kui, is a spectroscopic binary star system in the northern constellation of Andromeda. It consists of two G-type evolved stars

HD 42818 (688 words) [view diff] exact match in snippet view article find links to article

HD 42818 is a suspected astrometric binary star system in the northern circumpolar constellation of Camelopardalis. It is visible to the naked eye with

7 Tauri (546 words) [view diff] exact match in snippet view article find links to article

equivalent to a distance of around 593 light years from the Sun. 7 Tauri is a binary star with two nearly equal components about 0.7″ apart, designated as A and

UW Coronae Borealis (355 words) [view diff] exact match in snippet view article find links to article

Coronae Borealis, also known as MS 1603.6+2600, is a low-mass X-ray binary star system in the constellation Corona Borealis. Astronomer Simon Morris

Omicron Aurigae (589 words) [view diff] exact match in snippet view article find links to article

Omicron Aurigae, Latinized from ο Aurigae, is an astrometric binary star system in the northern constellation of Auriga. With an apparent visual magnitude

LTT 3780 (585 words) [view diff] exact match in snippet view article find links to article

as TOI-732 or LP 729-54, is the brighter component of a wide visual binary star system in the constellation Hydra. This star is host to a pair of orbiting

NGC 2360 (531 words) [view diff] exact match in snippet view article find links to article

Gamma Canis Majoris and less than one degree northwest of the eclipsing binary star R Canis Majoris; it has a combined apparent magnitude of 7.2. It is 13

LTT 3780 (585 words) [view diff] exact match in snippet view article find links to article

as TOI-732 or LP 729-54, is the brighter component of a wide visual binary star system in the constellation Hydra. This star is host to a pair of orbiting

Chi Cancri (541 words) [view diff] exact match in snippet view article find links to article

Chi Cancri, Latinized from χ Cancri, is a candidate astrometric binary star system in the northern zodiac constellation of Cancer. It has a yellow-white

GG Lupi (514 words) [view diff] exact match in snippet view article find links to article

GG Lupi is an eclipsing binary star in the southern constellation of Lupus. Most of the time it is a magnitude 5.6 object, making it faintly visible to

15 Orionis (600 words) [view diff] exact match in snippet view article find links to article

15 Orionis is a suspected astrometric binary star system in the equatorial constellation of Orion, near the border with Taurus. It is visible to the naked

HD 176051 (681 words) [view diff] exact match in snippet view article find links to article

HD 176051 is a spectroscopic binary star system approximately 49 light years away from Earth in the constellation Lyra. The pair orbit with a period of

Senim Silla (174 words) [view diff] case mismatch in snippet view article find links to article

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

111 Herculis (605 words) [view diff] exact match in snippet view article find links to article

111 Herculis is a suspected astrometric binary star system located 92 light years from the Sun in the northern constellation Hercules. It is visible to

Delta Trianguli (840 words) [view diff] exact match in snippet view article find links to article

Delta Trianguli, Latinized from Delta Tri, is a spectroscopic binary star system approximately 35 light-years (11 pc) away in the constellation of Triangulum

2 Camelopardalis (451 words) [view diff] exact match in snippet view article find links to article

be relatively massive for its luminosity, it was suspected of being a binary star itself, but the current estimate of component C's magnitude as a single

Theta Carinae (898 words) [view diff] exact match in snippet view article find links to article

θ Carinae, Latinized as Theta Carinae, is a spectroscopic binary star in the southern constellation of Carina. With an apparent visual magnitude of 2