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See searches and references containing 4 SCORPII!4 SCORPII
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
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
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
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
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
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
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
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
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
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
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
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
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
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 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
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 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
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
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
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
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
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 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
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
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
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
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
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
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
Star in the constellation Scorpius
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
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
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
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
positions was made to match the astronomical coordinates correctly. Decree No. 4, issued on 19 November 1889, legally replaced the flag used under the constitutional
Flag_of_Brazil
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
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
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*
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
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
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
Open cluster in Scorpius
is a K-type orange giant star, BM Scorpii, which contrasts sharply with its blue neighbours in photographs. BM Scorpii, is classed as a semiregular variable
Butterfly_Cluster
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
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
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
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
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
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
Candidate brown dwarf orbiting variable star
V921 Scorpii b is a candidate 60-Jupiter-mass brown dwarf orbiting V921 Scorpii, a 20-solar-mass 30,000 K Herbig Haro B0IV-class subgiant. The object is
V921_Scorpii_b
Open cluster in the constellation of Scorpius
the neighboring Sagittarius Arm of the Milky Way. Zeta1 Scorpii (spectral type O8 and magnitude 4.71.) is the brightest star in the association, and one
NGC_6231
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
Interstellar cloud
4604), Antares in the large yellow area and Sigma Scorpii in the redish Sh2-9 area, with Messier 4 inbetween the latter two stars. North is up. July 2
Rho_Ophiuchi_cloud_complex
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
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
Astronomical X-ray source
system is classified as a low-mass X-ray binary; the neutron star is roughly 1.4 solar masses, while the donor star is only 0.42 solar masses. The origin of
Scorpius_X-1
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 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
log 10 ( 10 − 0.4 ⋅ 1.81 + 10 − 0.4 ⋅ 4.173 ) {\displaystyle 1.69\approx -2.5\log _{10}\left(10^{-0.4\cdot 1.81}+10^{-0.4\cdot 4.173}\right)} Combined
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
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
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
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
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
High-mass X-ray binary
accreting neutron star. The X-ray source is eclipsed by the star every 3.4 days, but no pulsations have yet been observed. The source is one of the ten
4U_1700−37
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
Molecular cloud
Sharpless Catalog assembled by Stewart Sharpless. It is located nearby to 16 Scorpii, and may be a faint reflection nebula. It is similar to the nearby Sh 2-24
Sh_2-23
Goldilocks super-Earth orbiting Gliese 667 C
masses. The equilibrium temperature of Gliese 667 Cc is estimated to be 277.4 K (4.3 °C; 39.6 °F). It is expected to have a radius of around 1.5 R🜨, dependent
Gliese_667_Cc
HII Region
constellation, surrounding the multiple star system Sigma Scorpii. Sigma Scorpii is 1° to the northwest of Messier 4, and the nebula can be easily seen with small
Sh_2-9
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
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
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
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
Norwegian black metal band
the former Windir and Ulcus guitarist. Bakketeig plays guitar in Cor Scorpii and Mistur as well. Much like I Krig, Milorg contains songs about the Norwegian
Vreid
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
Long period pulsar in the constellation Vela
star pulsar (some objects believed to be white dwarf pulsars, such as AR Scorpii, have longer periods). Its period is more than three times longer than
PSR_J0901−4046
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
Star in the constellation of Scorpius
constellation Scorpius. It has an apparent magnitude of 4.23, making it readily visible to the naked eye. N Scorpii was initially given the Bayer designation Alpha
N_Scorpii
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
Circles of latitude
winter solstice. This is the northern limit of the visibility of the star θ Scorpii and thus of the 'tail' of the constellation Scorpius. Starting at the Prime
Circles of latitude between the 45th parallel north and the 50th parallel north
Circles_of_latitude_between_the_45th_parallel_north_and_the_50th_parallel_north
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
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
Type of variable star
0.88 111 HD 28843 5.81 B9III 1.37 146 3 Scorpii 5.87 B8III/IV 1.46 158 V957 Scorpii 5.90 B6V 258 V929 Scorpii 5.92 B8V 1.49 161 HR 7355 6.02 B2Vn 0.52
SX_Arietis_variable
Binary star system whose component stars are very close
a previous candidate for stellar merger. Luminous red nova, e.g. V1309 Scorpii (2008), may result from the merger of a contact binary. MY Camelopardalis
Contact_binary
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 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 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
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
Variable star in the constellation Scorpius
HD 159176, also known as Boss 4444 and V1036 Scorpii, is a variable star about 2,800 light years from the Earth, in the constellation Scorpius. It is
HD_159176
2013 television film
confronted by Unicron and are forced to escape. Meanwhile, in the Theta Scorpii asteroid belt, Optimus and Wheeljack find the AllSpark's container, which
Transformers Prime Beast Hunters: Predacons Rising
Transformers_Prime_Beast_Hunters:_Predacons_Rising
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
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
Star in the constellation Scorpius
25 Scorpii (abbreviated to 25 Sco) is a star in the zodiac constellation of Scorpius, located about 920 light years away from the Sun. Its apparent magnitude
25_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
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
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
Spectroscopic binary star system in the constellation Scorpius
Cepheid (δ Cephei) variable and its visual magnitude varies from 6.4 to 6.9. V636 Scorpii is a spectroscopic binary, and the fainter companion is thought
V636_Scorpii
High proper motion binary star system in the constellation of Scorpius
4.27, making it readily visible to the naked eye under ideal conditions. It lies in the tail of Scorpius, between the stars κ Scorpii and υ Scorpii and
Q_Scorpii
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
planet) approved on 1 March 2020. An additional two star names were approved on 4 April 2022. In June 2023, an additional 20 names were approved in the NameExoWorlds
List_of_proper_names_of_stars
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
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
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