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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
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
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
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
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
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
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 naming system
Norma's Alpha and Beta were reassigned to Scorpius and re-designated N and H Scorpii respectively, leaving Norma with no Alpha. Francis Baily died before designating
Bayer_designation
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
Zodiac constellation in the southern celestial hemisphere
second brightest star in Scorpius. U Scorpii is the fastest known nova, with a period of about 10 years. AH Scorpii is a red supergiant star and one of
Scorpius
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 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 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
Star in the constellation Scorpius
Upsilon Scorpii (υ Scorpii, abbreviated Upsilon Sco, υ Sco), formally named Lesath /ˈliːsæθ/, is a star located in the "stinger" of the southern zodiac
Upsilon_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
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
McDonald & Woodward, ISBN 0939923785 Now known as N Scorpii (N Sco) Now known as H Scorpii (H Sco) Lacaille's Theta Telescopii (θ Tel, θ Telescopii)
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
Triple star system in the constellation of Scorpius
consisting of Pi Scorpii, Rho Scorpii, Delta Scorpii, Beta¹ Scorpii and Beta² Scorpii. Consequently, the Chinese name for Pi Scorpii itself is 房宿一 (Fáng
Pi_Scorpii
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
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
Constellation in the southern celestial hemisphere
1763 catalogue, was likewise transferred to Scorpius by Baily and named H Scorpii by Gould. Norma's brightest star, Gamma2 Normae, is only of magnitude
Norma_(constellation)
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
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
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
148478 80763 16h 29m 24.47s −26° 25′ 55.0″ 0.91 −5.24 553 M1.5Iab-b Cor Scorpii, Qalb al-Aqrab, Vespertilo; 16th brightest star; binary; semiregular variable
List_of_stars_in_Scorpius
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
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 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
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
Index of articles associated with the same name
individual stars in Scorpius by different sources: θ Scorpii (Sargas) ι1 Scorpii κ Scorpii Girtablilu Allen, R. H. (1899). Star Names: Their Lore and Meaning.
Girtab
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
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
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
Red supergiant star in the constellation Orion
Betz, A.L.; Townes, C.H.; Spears, D.L. (1977). "Spatial heterodyne tnterferometry of VY Canis Majoris, Alpha Orionis, Alpha Scorpii, and R Leonis at 11 microns"
Betelgeuse
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
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
Binary star
Hooft, F.; Heemskerk, M. H. M.; Alberts, F.; van Paradijs, J. (January 1998). "The quiescence optical light curve of Nova Scorpii 1994 (=GRO J1655–40)".
GRO_J1655−40
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 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
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
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
Goldilocks super-Earth orbiting Gliese 667 C
2019-09-15 at the Wayback Machine h h ⊙ = ( T ⊙ e f f T e f f ) 2 ∗ L a {\displaystyle {\begin{smallmatrix}{\frac {h}{{h}_{\odot }}}={\left({\frac {{{T}_{\odot
Gliese_667_Cc
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
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
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
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*
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
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
Norwegian black metal band
Cor Scorpii ("Scorpion's Heart" in Latin) is a black metal band from Sogndal Municipality, Norway, founded in 2004 by Gaute Refsnes, the former keyboardist
Cor_Scorpii
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 Scutum
Marcaide, J. M.; Hauschildt, P. H. (2013). "The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii"
UY_Scuti
Alpha Scorpii (Antares) Scorpius, the Scorpion 1 1889 1889 Maranhão Beta Scorpii (Graffias) Scorpius, the Scorpion 3 1889 1889 Ceará Epsilon Scorpii (Larawag)
Flag_of_Brazil
Norwegian black metal band
members went on to form several new bands, including Vreid, Mistur, and Cor Scorpii.[citation needed] The band formed in 1994 and released four albums over
Windir
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
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
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
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
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
Globular cluster in the constellation Scorpius
as the Galactic Center, and lies midway between the stars α Scorpii (Antares) and β Scorpii in a region rich with nebulæ. With an apparent angular diameter
Messier_80
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
Astronomical X-ray source
00967. doi:10.1093/mnras/stab2515. ISSN 0035-8711. Giacconi, R.; Gursky, H.; Paolini, F.R.; Rossi, B.B. (1962). "Evidence for X-rays from sources outside
Scorpius_X-1
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
sai.msu.su. Retrieved 2023-12-08. Wielen, R.; Schwan, H.; Dettbarn, C.; Lenhardt, H.; Jahreiß, H.; Jährling, R. (1999-01-01). "Sixth Catalogue of Fundamental
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
High-mass X-ray binary
Retrieved 4 September 2017. Jones, C.; Forman, W.; Tananbaum, H.; Schreier, E.; Gursky, H.; Kellogg, E.; Giacconi, R. (1973). "Evidence for the Binary
4U_1700−37
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
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
Binary star in the constellation Libra
Scorpii, but it was reassigned to Libra as Upsilon Librae. The star now known as Omicron Scorpii was a reinterpretation of o (Latin letter o) Scorpii
Upsilon_Librae
Stellar explosion with a distinct red colour
announced luminous red novae as a new class of stellar explosion. V1309 Scorpii is a luminous red nova that followed the merger of a contact binary in
Luminous_red_nova
China. R. Carter & brothers. p. 93. Mackworth, P. H.; Commander van Balkom; Everitt, P. F.; Sadler, D. H.; Squadron-Leader May; Bennett, D. C. T.; Hinks
List_of_proper_names_of_stars
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
Emission nebula in the constellation Scorpius
Nebula, and can be found 3° to the west-northwest of the bright star Lambda Scorpii. NGC 6334 was discovered by English astronomer John Herschel on June 7
NGC_6334
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
Aboriginal nation in eastern Australia
with the body of the Emu, reaching the maximum thickness with ε Scorpii and λ Scorpii, and tapering towards 36-Ophiuchi and 3-Sagittarii, eventually ending
Gamilaraay
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
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
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
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
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
Musical artist
style as "Sognametal". Other bands that have a Sognametal sound are Cor Scorpii, Vreid, Feigd, Mistur, and Sigtyr. He studied Sogndal history extensively
Terje_Bakken
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
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
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
constellation name] [year of discovery]" format, e.g. "Nova Cygni 1974" and "Nova Scorpii 2010". An official permanent name is usually soon assigned by the General
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
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)
original on 21 December 2009. Retrieved 25 August 2009. Born, R. "Cor Scorpii". MusicMight. Archived from the original on 14 July 2011. Retrieved 25
List of black metal bands, 0–K
List_of_black_metal_bands,_0–K
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
Nova
V1280 Scorpii (or Nova Scorpii 2007 Number 1) is the first of two novae that occurred in the constellation Scorpius during February 2007 (the second nova
V1280_Scorpii
Star in the constellation Scorpius
13 Scorpii, also known by its Bayer designation c2 Scorpii, is a binary star in the constellation Scorpius. Its apparent magnitude is 4.57, meaning it
13_Scorpii
Nearest OB association to Earth
advanced evolutionary phase, among which the red supergiant Antares (α Scorpii) stands out. Despite the young age of the group, no star formation is currently
Scorpius–Centaurus association
Scorpius–Centaurus_association
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
Star in the southern zodiac constellation of Scorpius
HD 146624 (d Scorpii) is a single, white-hued star in the southern zodiac constellation of Scorpius. It is faintly visible to the naked eye, having an
HD_146624
Star in the constellation Canis Minor
39m 18.11950s, declination −05° 13′ 29.9552″. It would be as bright as β Scorpii is in our sky. Procyon's closest neighboring star is Luyten's Star, about
Procyon
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
Star in the constellation Scorpius
1 Scorpii, or b Scorpii, is a single star in the southern zodiac constellation of Scorpius. It has an apparent magnitude of 4.63, which is bright enough
1_Scorpii
Star in the constellation Scorpius
HD 151804, also known as HR 6245 and V973 Scorpii, is a blue supergiant star about 7000 light years from the Earth, in the constellation Scorpius. It
HD_151804
J. M.; Hauschildt, P. H. (June 2013). "The atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii"
List_of_largest_stars
(1991). "The Bright star catalogue". New Haven. Bibcode:1991bsc..book.....H. Bessell, Michael S. (2005). "Standard Photometric Systems". Annual Review
List_of_brightest_stars
Small number of stars that orbit each other
Exploration: Planets Beyond our Solar System. Retrieved 29 June 2022. Nu Scorpii Archived 10 April 2020 at the Wayback Machine, entry in the Multiple Star
Star_system
HII Region
Scorpius constellation, surrounding the multiple star system Sigma Scorpii. Sigma Scorpii is 1° to the northwest of Messier 4, and the nebula can be easily
Sh_2-9
H SCORPII
H SCORPII
H SCORPII
H SCORPII
H SCORPII
H SCORPII
H SCORPII
H SCORPII
H SCORPII