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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
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
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
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
List of stars with high proper motion
Omicron Columbae 0.353 +20.43 PM; RM Proxima Centauri 3.859 −21.94 PM; RM Q Scorpii 0.219 −48.14 PM; RM Ross 451 3.171 −154.3 PM; RM Ross 619 Gliese 299 5
List of stars with large proper motion
List_of_stars_with_large_proper_motion
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
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
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 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
and the designation was dropped Catalogued by Bayer as Gamma Scorpii (γ Sco, γ Scorpii), reassigned by Gould to Libra - Burnham, Robert (1978), Burnham's
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
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
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
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
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
Aldebaran α Tauri 0065 K5 III Northern 15 0.96 (0.6–1.6var) Antares α Scorpii 0550 M1.5 Iab-Ib, B2.5 V Southern 16 0.97 (0.97–1.04var) Spica α Virginis
List_of_brightest_stars
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
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
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
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*
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
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
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
Astronomical X-ray source
1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR. Liu, Q. Z.; Paradijs, J. van; Heuvel, E. P. J. van den (2007-07-01). "A catalogue
Scorpius_X-1
Apparent magnitude (V) Parallax (mas) Notes and additional references Beta² Scorpii (HR 5984) 400 Scorpius B2V 4.92 RX J1856.5−3754 400 Neutron Star 25.6 The
List of star systems within 400–450 light-years
List_of_star_systems_within_400–450_light-years
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
not known prior to that. /ˈeɪtʃərd/ Acrab β1 Scorpii Aa Scorpius Arabic The traditional name of the β Scorpii system has been rendered Akrab and Elakrab
List_of_proper_names_of_stars
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
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
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
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
Center star of NGC 4361 Nebula. WR 142 4,000 WO2 12.94 HD 326823 (V1104 Scorpii) 4,142 WNpec 9.03 HD 151932 (WR 78) 4,200 WN7h 6.45 - 6.61 EZ Canis Majoris
List_of_Wolf–Rayet_stars
atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii". Astronomy & Astrophysics. 554: A76. arXiv:1305
List_of_stars_in_Sagittarius
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
Astrophysical limit on radiation from stars
atmospheric structure and fundamental parameters of the red supergiants AH Scorpii, UY Scuti, and KW Sagittarii". Astronomy & Astrophysics. 554: A76. arXiv:1305
Eddington_luminosity
Oort cloud comet
coronograph. On 27 November ISON brightened to magnitude −2 and passed Delta Scorpii. Around the time it reached perihelion on 28 November 2013, it might have
Comet_ISON
Star that is particularly similar to the Sun
of a New Data Set,” Astronomy & Astrophysics 363, November 2000, 947 18 Scorpii at SIMBAD - Ids - Bibliography - Image. Meléndez, Jorge; Ramírez, Iván
Solar_analog
Known extent to which a planet is suitable for life
solar analogs, one that closely resembles the Sun is considered to be 18 Scorpii; unfortunately for the prospects of life existing in its proximity, the
Planetary_habitability
Star that has a supergiant luminosity class, with a spectral type of F or G
include Polaris, Alpha Leporis, Alpha Persei, Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars, mostly pulsating Cepheids such as δ Cephei
Yellow_supergiant
23m 07.0s −17° 36′ 26″ M4.5Ve 13.30 138.2280±0.0482 Gliese 667 (142 G. Scorpii) A$ 23.6232±0.0048 Scorpius 17h 18m 57.2s −34° 59′ 23″ K3V 7.07 138.0663±0
List of star systems within 20–25 light-years
List_of_star_systems_within_20–25_light-years
TOI-4559 90.704 ±0.0978 M Has one confirmed exoplanet (TOI-4559b) Xi Scorpii (Graffias) A 90.88 ± 0.05 Scorpius 16h 04m 22.191s -11° 22′ 22.60″ F4(V)
List of star systems within 90–95 light-years
List_of_star_systems_within_90–95_light-years
Type of star, larger and brighter than the Sun
Gem), an A-type subgiant; Eta Bootis (η Boo), a G-type subgiant. Delta Scorpii (δ Sco), a B-type subgiant. Bright giants are stars of luminosity class
Giant_star
Astrophysical phenomenon
such systems that conveniently advertise themselves. One example is U Scorpii. Collapsar – Star that has undergone gravitational collapse Kilonova –
Supernova
System of two stars orbiting each other
its temperature relative to the primary star. Examples: Antares (Alpha Scorpii) is a red supergiant star in a binary system with a hotter blue main-sequence
Binary_star
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
Process by which stars are named
particular name corresponded to (e.g., Alniyat could refer to Sigma Scorpii or Tau Scorpii - now Paikauhale). Some stars in entirely different constellations
Stellar designations and names
Stellar_designations_and_names
Star in the constellation Sagittarius
properties, which are only consistent with those of red supergiants. AH Scorpii BC Cygni HV 11423 IRC −10414 MY Cephei NML Cygni S Persei Stephenson 2
VX_Sagittarii
Stellar core remnant
be difficult. The highly magnetized white dwarf in the binary system AR Scorpii was identified in 2016 as the first pulsar in which the compact object
White_dwarf
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
Yadav, K. K. (2021). "Properties of white dwarf in the binary system AR Scorpii and its observed features". Modern Physics Letters A. 36 (13). arXiv:2103
List_of_smallest_known_stars
List of largest planets by size
1088/2041-8205/811/2/L30. ISSN 2041-8213. Todorov, K. O.; Luhman, K. L.; Konopacky, Q. M.; McLeod, K. K.; Apai, D.; Ghez, A. M.; Pascucci, I.; Robberto, M. (2014)
List_of_largest_exoplanets
Type of star
W43A HV 2112 S Persei VX Sagittarii V1804 Sagittarii VY Canis Majoris AH Scorpii MY Cephei PZ Cassiopeiae IRC −30308 NML Cygni IRC +10420 WOH G64 A IRAS
OH/IR_star
Eridani Achernar Alpha Eridani Acrab ʽAqrab the Scorpion عقرب عَقْرَب Beta Scorpii Acubens ʼaz-Zubānā the Claw / Dart / Sting الزبانى الْزُّبَانَى Alpha Cancri
List_of_Arabic_star_names
15: 459, Bibcode:1968ApJS...15..459G, doi:10.1086/190168 Pasquini, L.; Liu, Q.; Pallavicini, R. (July 1994), "Lithium abundances of nearby solar-like stars"
List of star systems within 65–70 light-years
List_of_star_systems_within_65–70_light-years
Type of star that is luminous, blue, and variable in brightness
η Carinae P Cygni Zeta1 Scorpii AG Carinae HR Carinae V432 Carinae (Wray 15-751) V4029 Sagittarii (HD 168607) V905 Scorpii (HD 160529) V1672 Aquilae
Luminous_blue_variable
Common gas atmosphere of a binary star system
] include: M85 OT2006-1, possible ejection of the whole envelope V1309 Scorpii, a possible star merger M31 RV V838 Monocerotis Ou 5, a planetary nebula
Common_envelope
Štefl, S.; et al. (2013). "The 2011 periastron passage of the Be binary δ Scorpii". The Astrophysical Journal. 766 (2): 119. arXiv:1302.4021. Bibcode:2013ApJ
List_of_most_massive_stars
by two red dwarfs orbiting each other Nearest septenary star system Nu Scorpii 150 parsecs (490 ly) A B3V star orbited by an unknown-type star, both orbited
List_of_star_extremes
Majoris A F8V 4.82 4.28 10h 30m 37.66s +55° 58′ 49.9″ 41.9 HD 147513 (62 G. Scorpii) G3V 5.37 4.82 16h 24m 01.19s −39° 11′ 34.7″ 42.0 Gliese 428 (it) A K7V
List_of_nearest_bright_stars
28m 13s +00° 07′ 19″ 13.3 2220 G0V b 21.66 1.01 4.2568 0.057 0 2008 V921 Scorpii Scorpius 16h 59m 07.0s −42° 42′ 09.0″ 11.0 4833 B0IVe b 60 835 2019 15
List_of_brown_dwarfs
disintegrating planetesimal, most likely an asteroid. First white dwarf that is a pulsar AR Scorpii A 2016 The star is in a binary system with a red dwarf
List_of_white_dwarfs
Stars sorted by absolute magnitude
S2CID 118510909. Mauerhan, J. C.; Cotera, A.; Dong, H.; Morris, M. R.; Wang, Q. D.; Stolovy, S. R.; Lang, C. (2010). "Isolated Wolf-Rayet Stars and O Supergiants
List_of_most_luminous_stars
Star whose brightness fluctuates, as seen from Earth
variation by modulating the mass transfer rate. An example of a DPV is V393 Scorpii. Beta Lyrae (β Lyr) variables are close eclipsing binaries, named after
Variable_star
is not documented in Yixiang Kaocheng. Sun & Kistemaker (p. 186) identify q Velorum as the principal star, citing the star catalogue of Zhou Cong of the
List_of_Chinese_star_names
Manara, C. F.; Miotello, A.; Maud, L. T.; Harsono, D. (2018-08-01). "V1094 Scorpii: A rare giant multi-ringed disk around a T Tauri star". Astronomy and Astrophysics
List of resolved circumstellar disks
List_of_resolved_circumstellar_disks
Brightness of a celestial object observed from the Earth
AU away −40.17 star η Carinae A seen from 1 AU away −40.07 star Zeta1 Scorpii seen from 1 AU away −39.66 star R136a1 seen from 1 AU away −39.47 star
Apparent_magnitude
Exoplanets confirmed or discovered from direct imaging
overridden setting (link) Macintosh B, Graham JR, Barman T, De Rosa RJ, Konopacky Q, Marley MS, et al. (2 October 2015). "Discovery and spectroscopy of the young
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
(10&15 Dec), a phase 1-trialed HIV vaccine (2 Dec), mice-tested Pillar[6]MaxQ against meth and fentanyl drug overdoses (15 Dec), first approval of a trialed
2022_in_science
Accumulation of matter around a star
evolution depend on the binary's parameters, such as the mass ratio q b {\displaystyle q_{b}} and eccentricity e b {\displaystyle e_{b}} , as well as the
Circumstellar_disc
Overview of the events of 2022 in science
mechanism of anti-aging senolytics, in particular of Dasatinib plus Quercetin (D+Q) – an increase of α-Klotho as shown in mice, human cells and in a human trial
January–March_2022_in_science
S2CID 220250511 Zang, Weicheng; et al. (2022), "OGLE-2018-BLG-0799Lb: A q ~ 2.7 × 10−3 planet with Spitzer parallax", Monthly Notices of the Royal Astronomical
List of exoplanets discovered in 2020
List_of_exoplanets_discovered_in_2020
(2023), "Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey", The Astronomical Journal, 165
List of exoplanets discovered in 2022
List_of_exoplanets_discovered_in_2022
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