AI & ChatGPT searches , social queries for 18 SCORPII
Search references for 18 SCORPII. Phrases containing 18 SCORPII
See searches and references containing 18 SCORPII!
Search references for 18 SCORPII. Phrases containing 18 SCORPII
See searches and references containing 18 SCORPII!18 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
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
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
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
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
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
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 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
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
Scorpii, Epsilon Scorpii, Zeta1 Scorpii and Zeta2 Scorpii, Eta Scorpii, Iota1 Scorpii and Iota2 Scorpii, Kappa Scorpii, Lambda Scorpii, Mu1 Scorpii and
Theta_Scorpii
American astronomer
the Allen Telescope Array (Beta Canum Venaticorum, HD 10307, HD 211415, 18 Scorpii, and 51 Pegasi). The second are her top candidates for the Terrestrial
Margaret_Turnbull
Star in the constellation Draco
Smith telescope at McDonald Observatory. Most other solar analogs such as 18 Scorpii are unlike the Sun in that they have several times the lithium abundance
HIP_56948
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
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 Ursa Major constellation
been proposed as a candidate solar twin. However, like the solar twin 18 Scorpii, HD 98618 has a lithium abundance significantly higher than that of the
HD_98618
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 Capricornus
The age of HD 197027, here annotated as HIP 102152, shown relative to the Sun, the younger solar twin 18 Scorpii and the formation of the Milky Way
HD_197027
"A Reduced Star Catalog Containing 537 Named Stars", Nov. 15 1971, page 18 (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網
List_of_stars_in_Scorpius
439″ F6V 3.85# The Closest Blue Straggler Star to Earth. Ba G7V Bb D 18 Scorpii 45.7 ± 0.6 Scorpius 16h 15m 37.27028s −08° 22′ 09.9821″ G2Va 5.503 Gliese
List of star systems within 45–50 light-years
List_of_star_systems_within_45–50_light-years
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
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
45.1 36 Ursae Majoris B K7Ve 8.77 8.06 10h 30m 25s +56° 00′ 00″ 45.2 18 Scorpii G1V 5.50 4.76 16h 15m 37s −08° 22′ 06″ 45.3 HD 23356 [nl] K2V 7.1 6.4
List_of_nearest_bright_stars
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
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 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
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
Star in the constellation Gemini
support a planet habitable by humans. 37 Geminorum is on the HabCat list. 18 Scorpii Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release
37_Geminorum
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
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
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
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
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
Nebula
nebula and reflection nebula in the constellation of Scorpius with Pi Scorpii at its center. It appears as a modest brightness making it one of the easier
Sh_2-1
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
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
Castor Sextenary star system Brightest sextuple star system 1.62 Lambda Scorpii (Shaula) Triple star system 1.64 1.59 Bellatrix Star 1.64 Gacrux Star 1
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Portugal, Brazil, and the Algarves. Flag of the independent Kingdom of Brazil (18 September – 1 December 1822) First flag of the Empire of Brazil with 19 stars
Flag_of_Brazil
"SIMBAD Astronomical Database". Strasbourg astronomical Data Center. Retrieved 18 August 2015. "HD 55". SIMBAD. Retrieved 1 March 2025. "HD 38A". SIMBAD. Retrieved
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
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
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
19th lunar mansion of Hindu astronomy
of stars in the tail of Scorpius: at least ε, μ, ζ, η, θ, ι, κ, and λ Scorpii. These stars are in the direction of the Galactic Center, the brightest
Mula_(nakshatra)
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
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
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
Lunar mansion in Hundu astrology
to 16°40'. It corresponds to the line of stars formed by β, δ, π and ρ Scorpii in the constellation Scorpius, which also form the Chinese lunar mansion
Anuradha_(nakshatra)
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
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 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
Stellar classification distinguished by bright blue luminosity
"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 (B8 V). The Revised
B-type_main-sequence_star
Astronomical X-ray source
variations of up to 1 magnitude in its intensity, with a period of around 18.9 hours. The source varies irregularly in optical wavelengths as well, but
Scorpius_X-1
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
Goldilocks super-Earth orbiting Gliese 667 C
closer to the "hot" inner edge of the habitable zone than Earth (254.3 K [−18.8 °C; −1.9 °F]). According to the Planetary Habitability Laboratory (PHL)
Gliese_667_Cc
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
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
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
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
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 Ophiuchus
24 Scorpii is a star that was originally placed by John Flamsteed within the constellation of Scorpius but in now placed within the southeastern constellation
24_Scorpii
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
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
molecular cloud. Nu Scorpii (Jabbah) A 470 Scorpius B3V 4.349 + 6.60 + 6.30 B B9III B B9III Winnecke 4B (M40) 470 ± 1 G0 V 10.11 Rho Scorpii (Iklil) 470 ± 10
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
B3-4Ia+ 264 110 1660000 11.702 V915 Scorpii 5600+570 −370 K0Ia-0 685.6 14.7 74100 – 185200 6.22 - 6.64 Zeta¹ Scorpii 6000 B1.5Ia+ 103 – 125.5 36 – 53 850000
List_of_nearest_hypergiants
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
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
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
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 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
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
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
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
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
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
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
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
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
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
Cygni V2140 Cygni V4030 Sagittarii Zeta¹ Scorpii In Galactic Center Region: Star 13, type O, LBV candidate Star 18, type O, LBV candidate In Westerlund 1:
Hypergiant
Astrophysical phenomenon
such systems that conveniently advertise themselves. One example is U Scorpii. Collapsar – Star that has undergone gravitational collapse Kilonova –
Supernova
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
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
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
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
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
Comparison of a wide range of lengths
000 Mm – total length of the mid-ocean ridges 12.000 Mm — diameter of AR Scorpii, largest pulsar ever discovered 12.000 Mm – diameter of Sirius B, a white
Orders_of_magnitude_(length)
Star in the constellation Canis Minor
coordinates at right ascension 19h 39m 18.11950s, declination −05° 13′ 29.9552″. It would be as bright as β Scorpii is in our sky. Procyon's closest neighboring
Procyon
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
Lunar mansion in Hindu astronomy
Tropical zodiac: 29° 20′ Scorpio – 12° 40′ Sagittarius 18 Jyeṣṭhā "The Eldest" α, σ, and τ Scorpii Astrological leader: Budha (Mercury) Symbol: circular
Nakshatra
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
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
Indra Anuvāka 18: Oblative mantras called Apri Anuvāka 19: Invocatory and oblative mantras for the sacrifice alluded to in Section [Anuvāka] 18 Anuvāka 20:
Taittirīya_Brāhmaṇa
State of Brazil
upper left corner symbolizes Maranhão itself, and is supposed to be Beta Scorpii, as the constellation Scorpius is also depicted on the national flag of
Maranhão
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
Star in the constellation Scorpius
HR 5907, also known as V1040 Scorpii and HD 142184, is a star about 470 light years from the Earth, in the constellation Scorpius. It is a 5th magnitude
HR_5907
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
2nd month of the Bengali calendar
astronomy and Vedic astrology associated with the string of the constellation Scorpii. It is the constellation visible on the meridian at midnight from the Indian
Joishtho
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
Constellation in the southern celestial hemisphere
into Scorpius and left unnamed by Francis Baily, before being named N Scorpii by Benjamin Apthorp Gould, who felt its brightness warranted recognition
Norma_(constellation)
(Pearce's Star) 4,300 ± 300 2 O8V((f)) + O9.2II 6.07-6.24 HD 149404 (V918 Scorpii) 4,300 ± 400 2 O7.5I(f) + ON9.7I 5.42 - 5.50 HD 150136 4,310 ± 390 3 O3
List_of_O-type_stars
Constellation in the southern celestial hemisphere
11th magnitude stars. Halfway between Theta Coronae Australis and Theta Scorpii is the dense globular cluster NGC 6541. Described as between magnitude
Corona_Australis
Lucky and Unlucky Days". Cambridge Archaeological Journal. 18 (3): 327–339. Bibcode:2008CArcJ..18..327P. doi:10.1017/S0959774308000395. S2CID 162969143. Jetsu
Stars_in_astrology
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII
18 SCORPII