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Star in the constellation Scorpius
G Scorpii (abbreviated G Sco), also named Fuyue, is a giant star in the constellation of Scorpius. It has an apparent magnitude of +3.19. It is approximately
G_Scorpii
Star in the constellation Scorpius
18 Scorpii is a solitary star located at a distance of some 46.1 light-years (14.13 parsecs) from the Sun at the northern edge of the Scorpius constellation
18_Scorpii
Triple star system in the constellation Scorpius
consisting of λ Scorpii, ε Scorpii, ζ1 Scorpii, ζ2 Scorpii, η Scorpii, θ Scorpii, ι1 Scorpii, ι2 Scorpii, κ Scorpii, μ1 Scorpii, and υ Scorpii. Consequently
Lambda_Scorpii
Star in the constellation Scorpius
Scorpii, Epsilon Scorpii, Zeta1 Scorpii and Zeta2 Scorpii, Eta Scorpii, Iota1 Scorpii and Iota2 Scorpii, Kappa Scorpii, Lambda Scorpii, Mu1 Scorpii and
Theta_Scorpii
Multi-star system in the constellation of Scorpius
both of β1 Scorpii and β2 Scorpii, π Scorpii, ρ Scorpii and δ Scorpii, . Consequently, the Chinese name for both of β1 Scorpii and β2 Scorpii is 房宿四 (Fáng
Beta_Scorpii
Triple-star system in the constellation Scorpius
Gliese 667 (142 G. Scorpii) is a triple-star system in the constellation Scorpius lying at a distance of about 7.2 parsecs (23 light-years) from Earth
Gliese_667
Goldilocks super-Earth orbiting Gliese 667 C
habitable exoplanets Sloane, Stephen A.; Guinan, Edward F.; Engle, Scott G. (June 2023). "Super-Earth GJ 667Cc: Age and XUV Irradiances of the Temperate-zone
Gliese_667_Cc
Binary star system in the constellation Scorpius
Delta Scorpii (Latinised from δ Scorpii, abbreviated Delta Sco, δ Sco) is a binary star (the presence of a third star in the system is being debated)
Delta_Scorpii
Binary star in the constellation Scorpius
designation α Scorpii, which is Latinised to Alpha Scorpii. Often referred to as "the heart of the scorpion", Antares is flanked by σ Scorpii and τ Scorpii near
Antares
Star naming system
constellations have uppercase letter designations, like B Centauri and G Scorpii. These letters were assigned by later astronomers, notably Lacaille in
Bayer_designation
Multiple star system in the constellation of Scorpius
Sigma Scorpii (or σ Scorpii, abbreviated Sigma Sco or σ Sco), is a multiple star system in the constellation of Scorpius, located near the red supergiant
Sigma_Scorpii
Star in the constellation Scorpius
HD 147513 (62 G. Scorpii) is a star in the southern constellation of Scorpius. It was first catalogued by Italian astronomer Giuseppe Piazzi in his star
HD_147513
Variable star
ω2 Scorpii, Latinised as Omega2 Scorpii, is a suspected variable star in the zodiac constellation of Scorpius. A component of the visual double star ω
Omega2_Scorpii
Multiple star system in the constellation Scorpius
Nu Scorpii (ν Scorpii, abbreviated Nu Sco, ν Sco) is a multiple star system in the constellation of Scorpius. It is most likely a septuple star system
Nu_Scorpii
Star in the constellation Scorpius
V1309 Scorpii (also known as V1309 Sco) is a contact binary that merged into a single star in 2008 in a process known as a luminous red nova. It was the
V1309_Scorpii
Binary star system in the constellation Scorpius
AR Scorpii (AR Sco) is a binary star system that consists of a pulsar-like white dwarf and a red dwarf star. It is located close to the ecliptic plane
AR_Scorpii
Star in the constellation of Scorpius
Tau Scorpii, Latinized from τ Scorpii, formally named Paikauhale /ˌpaɪkaʊˈhɑːleɪ/, is a star in the southern zodiac constellation of Scorpius. The apparent
Tau_Scorpii
Binary star in the constellation Scorpius
of Epsilon Scorpii, Mu1 Scorpii, Zeta Scorpii, Eta Scorpii, Theta Scorpii, Iota Scorpii, Kappa Scorpii, Lambda Scorpii and Upsilon Scorpii. Consequently
Epsilon_Scorpii
Guinan, Edward F.; Eaton, J. A.; Wasatonic, R.; Stewart, H.; Engle, S. G.; McCook, G. P. (November 2010). "Times-Series Photometry & Spectroscopy of the
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Star in the constellation Scorpius
consisting κ Scorpii, μ1 Scorpii, ε Scorpii, ζ1 Scorpii and ζ2 Scorpii, η Scorpii, θ Scorpii, ι1 Scorpii and ι2 Scorpii, λ Scorpii and υ Scorpii. Consequently
Kappa_Scorpii
Multiple stellar system in the constellation Scorpius
Rho Scorpii (ρ Scorpii, abbreviated Rho Sco, ρ Sco) is a double star in the constellation of Scorpius. It has an apparent visual magnitude of +3.87, which
Rho_Scorpii
Recurrent nova system first seen in 1863
U Scorpii (U Sco) is a recurrent nova system, one of 10 known recurring novae in the Milky Way galaxy. Located near the northern edge of the constellation
U_Scorpii
Star in the constellation Scorpius
Zeta1 Scorpii (Zeta1 Sco, ζ1 Scorpii, ζ1 Sco) is a binary star in the constellation of Scorpius, composed by an B-type hypergiant star as the primary,
Zeta1_Scorpii
Binary star system in the constellation Scorpius
Scorpii, Epsilon Scorpii, Zeta1 Scorpii and Zeta2 Scorpii, Eta Scorpii, Theta Scorpii, Iota1 Scorpii and Iota2 Scorpii, Kappa Scorpii, Lambda Scorpii
Mu1_Scorpii
Star system
Xi Scorpii (ξ Sco) is part of a quintuple star system in the constellation Scorpius. It was assigned this designation by Bayer, although Ptolemy had catalogued
Xi_Scorpii
number of traditional star names, there were some coined in modern times, e.g. "Avior" for Epsilon Carinae (1930), and a number of stars named after people
List_of_proper_names_of_stars
Binary star in the constellation Scorpius
AK Scorpii is a Herbig Ae/Be star and spectroscopic binary star about 459 light-years distant in the constellation Scorpius. The star belongs to the nearby
AK_Scorpii
Red supergiant star in the constellation Scorpius
AH Scorpii (abbreviated to AH Sco) is a red supergiant or hypergiant variable star located in the constellation Scorpius. It is one of the largest stars
AH_Scorpii
and Bayer letters Now known as Eta Sagittarii (η Sgr) Now known as G Scorpii (G Sco) Now known as d Ophiuchi (d Oph) Moved into Corona Australis, but
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
Globular cluster in Scorpius
diameter". The cluster is located 5 arc minutes east-northeast of the star G Scorpii, and is some 43,000 light-years from the Sun. This is one of the most
NGC_6441
Star in the constellation of Scorpius
N Scorpii, also known as HD 148703, is a solitary, bluish-white hued star located in the southern constellation Scorpius. It has an apparent magnitude
N_Scorpii
within 25–30 light-years Lists of stars List of nearest bright stars Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary
List of star systems within 20–25 light-years
List_of_star_systems_within_20–25_light-years
High proper motion binary star system in the constellation of Scorpius
Q Scorpii, also designated as HD 159433, is an astrometric binary (100% chance) located in the southern zodiac constellation Scorpius. It has an apparent
Q_Scorpii
twenty-eight mansions of the zodiac, which forms a part of Sagittarius. The star G Scorpii (Fuyue) is named after him. The Shangshu chapter "Yue ming" 說命 represents
Fu_Yue
"HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26. Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 2006-12-26
List_of_stars_in_Scorpius
Charles I of England by Sir Charles Scarborough, his physician. Fuyue for G Scorpii, a traditional Chinese name honoring Fu Yue. Sualocin and Rotanev for
Stars_named_after_people
Systematic designations to unambiguously identify astronomical objects
letters are used, such as for A Centauri (A Cen), D Centauri (D Cen), G Scorpii (G Sco), P Cygni (P Cyg), b Sagittarii (b Sgr), d Centauri (d Cen) and s Carinae
Astronomical naming conventions
Astronomical_naming_conventions
Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D. Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Constellation in the southern celestial hemisphere
Lacaille placed it in Telescopium, Gamma was placed in Scorpius and renamed G Scorpii by Gould, Theta Telescopii reverted to its old appellation of d Ophiuchi
Telescopium
arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701. de Mello, G. F. Porto; del Peloso, E. F. & Ghezzi, L. (April 2006). "Astrobiologically
List_of_nearest_bright_stars
Star in the constellation Scorpius
Iota1 Scorpii, Latinized from ι1 Scorpii, is a star in the southern constellation of Scorpius. With an apparent visual magnitude of 3.03, this star can
Iota1_Scorpii
B-type star in the constellation of Scorpius
Mu2 Scorpii, also named Pipirima /pɪˈpɪrɪmə/, is a star in the zodiac constellation of Scorpius. It has an apparent visual magnitude of +3.56, which is
Mu2_Scorpii
Variable star in the constellation Scorpius
BM Scorpii (BM Sco) is a red supergiant and a semiregular variable star located in the constellation Scorpius. It lies approximately 490 parsecs (1,600 ly)
BM_Scorpii
Star in the constellation Scorpius
Zeta2 Scorpii (Zeta2 Sco, ζ2 Scorpii, ζ2 Sco) is a star in the constellation of Scorpius. With an apparent visual magnitude variying s between 3.59 and
Zeta2_Scorpii
Variable star in the constellation Scorpius
V915 Scorpii (HR 6392, HD 155603) is a hypergiant and semiregular variable star, located 1,718 parsecs (5,600 ly) away in the constellation Scorpius.
V915_Scorpii
Variable star
V1094 Scorpii is a young stellar object in the constellation of Scorpius, located in the young Lupus Star Forming Region. It is being orbited by a protoplanetary
V1094_Scorpii
Star in the constellation Scorpius
2 Scorpii (A Scorpii) is a double star in the southern zodiac constellation of Scorpius. The brighter component has an apparent visual magnitude of 4.69
2_Scorpii
Binary star in the constellation Scorpius
Eta Scorpii, Latinized from η Scorpii, is a binary star in the southern zodiac constellation of Scorpius. With an apparent visual magnitude of 3.33, this
Eta_Scorpii
Binary star
Paradijs, J. (January 1998). "The quiescence optical light curve of Nova Scorpii 1994 (=GRO J1655–40)". Astronomy and Astrophysics. 329: 538–550. arXiv:astro-ph/9709151
GRO_J1655−40
Star in the constellation of Scorpius
ω1 Scorpii, Latinised as Omega1 Scorpii, is a star in the zodiac constellation of Scorpius. With an apparent visual magnitude of 3.95 it can be seen with
Omega1_Scorpii
Star in the constellation Scorpius
22 Scorpii (i Scorpii) is a single star in the southern zodiac constellation of Scorpius, about one degree from Antares. It is faintly visible to the naked
22_Scorpii
the Tail mansion 魚 Yú Fish Messier 7 Ptolemy Cluster 傅說 Fù Yuè Fuyue G Scorpii Fuyue A single-star asterism in the Tail mansion. Fù Yuè became the official
List_of_Chinese_star_names
Librae (φ Lib/φ Librae) by Bode in his Uranographia Labelled as Phi Scorpii (φ Sco/φ Scorpii) in Bode’s Uranographia Labelled Psi Librae (ψ Lib/ψ Librae) by
List_of_stars_in_Libra
Flag of the Brazilian state of Maranhão
(Indigenous, black, and white Brazilians), while the star represents Beta Scorpii, which in turn represents the state of Maranhão on the Flag of Brazil.
Flag_of_Maranhão
Open cluster in the constellation of Scorpius
open cluster in the southern sky located half a degrees north of Zeta Scorpii. NGC 6231 is part of a swath of young, bluish stars in the constellation
NGC_6231
Star in the constellation Libra
as Sigma Lib or σ Lib. The star originally bore the designation Gamma Scorpii and did not receive its current designation until the new designation was
Sigma_Librae
Star that has a supergiant luminosity class, with a spectral type of F or G
Iota¹ Scorpii. Many of them are variable stars, mostly pulsating Cepheids such as δ Cephei itself. Hertzsprung–Russell diagram Spectral type O B A F G K M
Yellow_supergiant
Reflection Nebula
interstellar dust. The nebula is illuminated by two bright stars V856 Scorpii (A9V) and V1027 Scorpii (A0/3III). Notable object within the region is Herbig-Haro
Bernes_149
Variable Star in the constellation Scorpius
V861 Scorpii (also known as HD 152667, or V861 Sco) is a blue supergiant star and eclipsing binary system located in the constellation of Scorpius, within
V861_Scorpii
Index of articles associated with the same name
There are two stars with the Bayer designation ω Scorpii (omega Scorpii): ω1 Scorpii ω2 Scorpii They are separated by 0.24° on the sky, which is far enough
Omega_Scorpii
Type of neutron star with beams of radiation
also as an X-ray pulsar. In 2016, a white dwarf in the binary system AR Scorpii was identified as a pulsar (it is often mistakenly called the first discovered
Pulsar
Rotational center of the Milky Way galaxy
brightest, visually close to the Butterfly Cluster (M6) or the star Lambda Scorpii, south to the Pipe Nebula. There are around 10 million stars within one
Galactic_Center
Star in the constellation of Scorpius
151932 is a variable star. It was given its variable star designation, V919 Scorpii, in 1981. Like most extremely massive stars, HD 151932 is losing mass via
HD_151932
Nuclear explosion in a white dwarf star
magnitude 2.0 (nearly as bright as Deneb). The most recent were V1280 Scorpii, which reached magnitude 3.7 on 17 February 2007, and Nova Delphini 2013
Nova
Supermassive black hole at the center of the Milky Way
the ecliptic, visually close to the Butterfly Cluster (M6) and Lambda Scorpii. Sagittarius A* is a bright and very compact astronomical radio source
Sagittarius_A*
Triple star system in the constellation Ophiuchus
Flamsteed designation. Component C (HD 156026) was also historically called 30 Scorpii. In the culture of the Kamilaroi and Euahlayi Aboriginal peoples in New
36_Ophiuchi
Star in the constellation Scorpius
HD 142990, also known as HR 5942 and V913 Scorpii, is a star about 470 light years from the Earth, in the constellation Scorpius. It is a 5th magnitude
HD_142990
Interstellar cloud
large blue area (IC 4604), Antares in the large yellow area and Sigma Scorpii in the redish Sh2-9 area, with Messier 4 inbetween the latter two stars
Rho_Ophiuchi_cloud_complex
Star in the constellation Scutum
of three red supergiants near the Galactic Center region: UY Scuti, AH Scorpii, and KW Sagittarii. They determined that all three stars are over 1,000
UY_Scuti
Designated m Lupi by Johann Bode Designated g2 Scorpii by Johann Bode, now no longer in use Designated g1 Scorpii by Johann Bode, now no longer in use
List_of_stars_in_Lupus
Luminous blue variable star in the constellation Scorpius
HD 160529 (V905 Scorpii) is a luminous blue variable (LBV) star located in the constellation of Scorpius. With an apparent magnitude of around +6.8 it
HD_160529
entirely (e.g. Centaurus). The constellations shown are sometimes heavily affected by the selection of single stars (e.g. Hydra), distorted (e.g. Scorpius)
Flag_of_Brazil
Stellar classification distinguished by bright blue luminosity
(1973) listed "dagger standards" of Tau Scorpii (B0 V), Omega Scorpii (B1 V), 42 Orionis (B1 V), 22 Scorpii (B3 V), Rho Aurigae (B5 V), and 18 Tauri
B-type_main-sequence_star
Spectroscopic binary star system in the constellation Scorpius
V636 Scorpii is a multiple star system in the constellation Scorpius, 3,000 light years away. The primary is a Classical Cepheid (δ Cephei) variable and
V636_Scorpii
Binary star system in the constellation of Scorpius
HD 326823, also known as V1104 Scorpii, is a binary star containing a unique emission-line star, which is in the midst of transitioning to a nitrogen-rich
HD_326823
Star in the constellation Scorpius
Omicron Scorpii (ο Sco, ο Scorpii) is a star in the zodiac constellation of Scorpius. With an apparent visual magnitude of +4.57, it is visible to the
Omicron_Scorpii
Star in the constellation Scorpius
is located in the constellation of Scorpius, near the bright star Theta Scorpii. The star is in a crowded region of sky near the Galactic Center, and so
Gliese_682
Star in the constellation Libra
The Bayer designation Phi Scorpii has been associated with this star. No star is found at the position marked φ Scorpii in Johann Bayer's Uranometria
49_Librae
Type of star larger than main-sequence but smaller than a giant
B0: γ Cassiopeiae, δ Scorpii, B0.5: β Scorpii, ε Persei B1: ο Persei, β Cephei B2: γ Orionis, π Scorpii, θ Ophiuchi, λ Scorpii, ω Canis Majoris B2.5:
Subgiant
Star in the constellation Scorpius
ι2 Scorpii, Latinised as Iota2 Scorpii, is a single star in tail of the zodiac constellation of Scorpius. It has an apparent visual magnitude of +4.82
Iota2_Scorpii
Stellar explosion with a distinct red colour
Szymański, M. K.; Kubiak, M.; Pietrzyński, G.; Poleski, R.; Wyrzykowski, Ł.; Ulaczyk, K. (2011). "V1309 Scorpii: Merger of a contact binary". Astronomy &
Luminous_red_nova
Binary star in the constellation Sagittarius
state in Brazil called this star and λ Scorpii, through ι Scorpii, θ Scorpii, ν Scorpii, υ Scorpii and ρ Scorpii Taugi kusugu, "Taugi's fishing basket"
Epsilon_Sagittarii
High-mass X-ray binary
Astrophysics Supplement Series. 55: 7–14. Bibcode:1984A&AS...55....7V. Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary
4U_1700−37
A-type main sequence star in the constellation Scorpius
4 Scorpii is a single star in the southern zodiac constellation of Scorpius. With an apparent visual magnitude of +5.6, it is dimly visible to the naked
4_Scorpii
Orange-hued giant star in the constellation Scorpius
Chi Scorpii, Latinized from χ Scorpii, is a single star in the zodiac constellation of Scorpius. It has an orange hue and can be faintly seen with the
Chi_Scorpii
White-hued star in the constellation Scorpius
Psi Scorpii, which is Latinized from ψ Scorpii, is a binary star in the zodiac constellation of Scorpius. It is white in hue and has an apparent visual
Psi_Scorpii
form of constellation name] [year of discovery]" format, e.g. "Nova Cygni 1974" and "Nova Scorpii 2010". An official permanent name is usually soon assigned
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
Visual binary star system
star, in April 1986. It was given its variable star designation, V1035 Scorpii, in 1997. The blue giant varies slightly in brightness every 3.5 hours
WR_86
Nova seen in 1860
T Scorpii, or Nova Scorpii 1860, was a nova in the globular cluster Messier 80 (M80). It was discovered on 21 May 1860 by Arthur von Auwers at Koenigsberg
T_Scorpii
Coming together of two stars
2008 scientists first observed a stellar merger in Scorpius (named V1309 Scorpii), though it was not known to be the result of a stellar merger at the time
Stellar_collision
Nova seen in 1862
V728 Scorpii, also known as Nova Scorpii 1862, was a nova that occurred in the constellation of Scorpius. It was discovered on 4 October 1862 by John
V728_Scorpii
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
are still sometimes called S Doradus variables. V4029 Sagittarii V905 Scorpii Usually B-class, occasionally late O or early A: 2dFS 3235 6 Cassiopeiae
Hypergiant
Star in the constellation Scorpius
V957 Scorpii is a variable star in the constellation of Scorpius. It is a blue straggler in the open cluster Messier 7, a star that is unexpectedly hot
V957_Scorpii
Milky Way superbubble
Loop I Bubble contains the star Antares (also known as α Sco, or Alpha Scorpii), as shown on the diagram above right. Several tunnels connect the cavities
Local_Bubble
Pattern of stars recognized on Earth's night sky
from Antares (α Sco) to Beta Scorpii (β Sco) and Pi Scorpii (π Sco) are replaced with a line from Beta through Delta Scorpii (δ Sco) to Pi forming a large
Asterism_(astronomy)
Star in the constellation Scorpius
H Scorpii (H Sco) is a single star in the southern constellation Scorpius. It is faintly visible to the naked eye with an apparent visual magnitude of
H_Scorpii
years of Earth. List of star systems within 400–450 light-years Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
Star system in the constellation Cassiopeia
only two known star systems with a multiplicity of 7, the other being Nu Scorpii. The multiple star system as a whole has the designations ADS 16795, CCDM J23300+5833
AR_Cassiopeiae
atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii". Astronomy and Astrophysics. 554: A76. arXiv:1305
List_of_largest_stars
Red supergiant star in the constellation Orion
"Spatial heterodyne tnterferometry of VY Canis Majoris, Alpha Orionis, Alpha Scorpii, and R Leonis at 11 microns". Astrophysical Journal Letters. 217: L97–L100
Betelgeuse
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