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Star system in Cassiopeia
Lambda Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from λ Cassiopeiae
Lambda_Cassiopeiae
Star in the constellation Cassiopeia
consists of Alpha, Beta, Kappa, Eta and Lambda Cassiopeiae. Consequently, the Chinese name for Alpha Cassiopeiae itself is 王良四 (Wáng Liáng sì, English:
Alpha_Cassiopeiae
Binary star system in the constellation Cassiopeia
Beta Cassiopeiae (Caph), Kappa Cassiopeiae, Alpha Cassiopeiae (Schedar) and Lambda Cassiopeiae. Consequently, the Chinese name for Eta Cassiopeiae itself
Eta_Cassiopeiae
Constellation in the northern celestial hemisphere
was the Camel. Its head was composed of Lambda, Kappa, Iota, and Phi Andromedae; its hump was Beta Cassiopeiae; its body was the rest of Cassiopeia, and
Cassiopeia_(constellation)
Type of eruptive variable star
A Gamma Cassiopeiae variable (γ Cassiopeiae variable) is a type of variable star, named for its prototype γ Cassiopeiae. The General Catalogue of Variable
Gamma_Cassiopeiae_variable
Binary star system in the constellation of Andromeda
π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae
Lambda_Andromedae
Star in the constellation Cassiopeia
9 Cassiopeiae (9 Cas) is a white giant star in the constellation Cassiopeia, about 2,370 light years away. 9 Cassiopeiae is classified as an A1 type giant
9_Cassiopeiae
Star in the constellation Canis Major
HR 2501, also known as HD 49131 and HP Canis Majoris, is a star about 2,000 light years from the Earth, in the constellation Canis Major. It is a 5th magnitude
HR_2501
Star in the constellation Ophiuchus
inclination angle of its poles must be small; estimated as ~20°. It is a Gamma Cassiopeiae variable with an amplitude of 0.15 magnitude. The brightness has been
Chi_Ophiuchi
Type of variable star
Stars does not have a type for λ Eridani variables, only GCAS for Gamma Cassiopeiae variables and BE for non-GCAS Be star variables. λ Eridani itself is
Lambda_Eridani_variable
Star in the constellation Centaurus
Cassiopeiae variable star with multiple periods of variability. The International Variable Star Index lists Eta Centauri as both a Gamma Cassiopeiae variable
Eta_Centauri
B-type star with emission lines
are also included. The first star recognized as a Be star was Gamma Cassiopeiae, observed 1866 by Angelo Secchi, the first star ever observed with emission
Be_star
Hypothetical hybrid star type
star V595 Cassiopeiae 01h 43m 02.72s +56° 30′ 46.02″ Cassiopeia 2002 IO Persei 03h 06m 47.27s +55° 43′ 59.35″ Perseus 2002 KN Cassiopeiae 00h 09m 36
Thorne–Żytkow_object
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
to the Galactic Center and one of the most luminous stars known; Rho Cassiopeiae, a yellow hypergiant that is one of the brightest to the naked eye; and
Hypergiant
Centauri Binary star system 2.21 2.14 Lambda Velorum Star 2.23 Gamma Cygni Star Suspected variable star 2.23 Alpha Cassiopeiae Star 2.230 Gamma Draconis Star
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Type of star
the disappearance of, the "shell" are called Gamma Cassiopeiae variables. Pleione and Gamma Cassiopeiae itself are both variable stars that have intermittent
Shell_star
Star in the constellation Cygnus
Lacertae, Sigma Cassiopeiae, Rho Cassiopeiae, Tau Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, Lambda Andromedae, Kappa
Pi1_Cygni
Star in the constellation Ara
indicating that it is a variable Be star but not obviously a Gamma Cassiopeiae variable. The International Variable Star Index defines it as GCAS +
Alpha_Arae
Class of massive star with a spectral type of A to K
mass-losing hot stars, but was not applied to cooler stars. In 1991, Rho Cassiopeiae was the first to be described as a yellow hypergiant, likely becoming
Yellow_hypergiant
Northern 69 2.23 Eltanin γ Draconis 0150 K5 III Northern 70 2.24 Schedar α Cassiopeiae 0230 K0 IIIa Northern 71 2.25 Naos ζ Puppis 1,080 O4 If(n)p Southern
List_of_brightest_stars
Star in the constellation Pavo
rotating hot blue star which has developed a gas disk around it. It is a γ Cassiopeiae variable or shell star which has occasionally brightened to magnitude
Lambda_Pavonis
Stars with a supergiant luminosity class with a spectral type of K or M
(1992). "Photometry of yellow semiregular variables – HR 8752 (= V509 Cassiopeiae)". Astronomy and Astrophysics. 263: 123. Bibcode:1992A&A...263..123P
Red_supergiant
the Raised (tail of the scorpion) الشولة Lambda Scorpii Schedar aṣ-Ṣadr the Breast الصدر Alpha Cassiopeiae Sheliak ash-Shiliyāq Lyra الشلياق Beta Lyrae
List_of_Arabic_star_names
Multiple star system in the constellation Scorpius
system. It is one of only two such known systems, the other being AR Cassiopeiae.[citation needed] Higher-multiplicity star systems are uncommon because
Nu_Scorpii
Type of large cool star
Gacrux (γ Crucis) Pollux (β Geminorum) Capella Aa (α Aurigae) Schedar (α Cassiopeiae) δ Andromedae ρ Persei Mira (ο Ceti) χ Cygni Rasalgethi (α Herculis)
Red_giant
(River's end) /ˈeɪkərnɑːr/ Achird η Cassiopeiae A Cassiopeia Slovak (1950) Apparently first applied to η Cassiopeiae in the Skalnate Pleso Atlas of the
List_of_proper_names_of_stars
Variable star in the constellation Hercules
main sequence. Omicron Herculis is an eruptive variable of the Gamma Cassiopeiae class, which are rapidly rotating B-class stars with mass outflow. It
Omicron_Herculis
Che; et al. (2011). "Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And Alpha Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105
List of stars with resolved images
List_of_stars_with_resolved_images
Star system in the Centaurus constellation
With the placement of the Sun east of the magnitude 3.4 star Epsilon Cassiopeiae, nearly in front of the Heart Nebula, the "W" line of stars of Cassiopeia
Alpha_Centauri
Small number of stars that orbit each other
the system can be considered a sextuple. Jabbah AR Cassiopeiae V871 Centauri Acrux Gamma Cassiopeiae QZ Carinae Astronomy portal Outer space portal Science
Star_system
A1 V 4.52 B A1 V HD 191939 174.4 ± 0.1 G9V 8.971 Has 7 exoplanets. Pi Cassiopeiae$ A 175 ± 1 Cassiopeia 00h 43m 28.070s +47° 01′ 28.36″ A5V 4.949# 18.6293±0
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
1 Andromeda 23h 09m 57.3642s +35° 32′ 55.658″ K2Ve 7.93 B K2Ve Delta Cassiopeiae (Rucbah)$ 99.4 ± 0.4 Cassiopeia 01h 25m 48.95147s +60° 14′ 07.0225″ A5
List of star systems within 95–100 light-years
List_of_star_systems_within_95–100_light-years
M2.5 V 0.43 9.31 10.45 168.9965 ±0.0270 has two candidate planets Eta Cassiopeiae (Gliese 34) Achird (A)$ 19.3314 ±0.0025 Cas* 00h 49m 06.3s +57° 48′ 55″
List_of_nearest_stars
Classification of stars based on spectral properties
Leporis – G5II III normal giants Arcturus – K0III IV subgiants Gamma Cassiopeiae – B0.5IVpe V main-sequence stars (dwarfs) Achernar – B6Vpe sd (prefix)
Stellar_classification
Constellation in the southern celestial hemisphere
and Lambda Canis Majoris. Although of similar spectra and nearby each other as viewed from Earth, they are unrelated. Kappa is a Gamma Cassiopeiae variable
Canis_Major
(2011-05-10). "Colder and Hotter: Interferometric imaging of {\beta} Cassiopeiae and {\alpha} Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105
List_of_nearest_giant_stars
Boschi, F.; Munari, U. (August 2003). "High resolution spectroscopy over lambda lambda 8500-8750 Å for GAIA. IV. Extending the cool MK stars sample". Astronomy
List of star systems within 30–35 light-years
List_of_star_systems_within_30–35_light-years
G0 V 10.11 Rho Scorpii (Iklil) 470 ± 10 Scorpius B2 IV 3.86 Epsilon Cassiopeiae (Segin) 470 ± 10 Cassiopeia B3 V 3.37 Gamma Pegasi (Algenib) 470 ± 30
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
Grouping of evolved cool luminous stars
masers are typically found in oxygen-rich M-type AGB stars such as R Cassiopeiae and U Orionis, while HCN and SiS masers are generally found in carbon
Asymptotic_giant_branch
Double binary star system in the constellation Ursa Major
Velorum, informally named Regor for astronaut Roger B. Chaffee Gamma Cassiopeiae, informally named Navi for astronaut Virgil Ivan "Gus" Grissom van Leeuwen
Iota_Ursae_Majoris
Type of variable star
periodic FS Canis Majoris RS Canum Venaticorum Other Flare Gamma Cassiopeiae Lambda Eridani Wolf–Rayet Cataclysmic AM Canum Venaticorum Dwarf nova Luminous
Rapidly_oscillating_Ap_star
Type of variable star
spectral types having amplitudes of about 1 mag in V The M2 supergiant TZ Cassiopeiae is given as a representative example. (visual magnitude, unless marked
Slow_irregular_variable
2024). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The Astrophysical Journal
List_of_largest_stars
Brightest star in the constellation Leo
Sturmann, L. (2011-04-18). "Colder and Hotter: Interferometric imaging of β Cassiopeiae and α Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105.0740
Regulus
"Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age". The Astrophysical Journal
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Astrophysical phenomenon
supergiants Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta Carinae that has already produced a supernova
Supernova
CN CH White dwarf Chemically peculiar Am Ap/Bp CEMP HgMn He-weak Barium Lambda Boötis Lead Technetium Be Shell B[e] Helium Extreme Blue straggler Remnants
Lists_of_stars
Type of star
QX Puppis V669 Cassiopeiae W43A HV 2112 S Persei VX Sagittarii V1804 Sagittarii VY Canis Majoris AH Scorpii MY Cephei PZ Cassiopeiae IRC −30308 NML Cygni
OH/IR_star
Type of star larger than main-sequence but smaller than a giant
established the two-dimensional classification scheme, including: B0: γ Cassiopeiae, δ Scorpii, B0.5: β Scorpii, ε Persei B1: ο Persei, β Cephei B2: γ Orionis
Subgiant
Star of luminosity class VI under the Yerkes spectral classification system
44.9 MJ, making it a brown dwarf. Kapteyn's Star Groombridge 1830 Mu Cassiopeiae 2MASS J05325346+8246465, a possible halo brown dwarf and the first substellar
Subdwarf
Binary star in the constellation of Andromeda
that mark the prime meridian of the heavens, the other two being Beta Cassiopeiae and Gamma Pegasi. It was believed to bless those born under its influence
Alpheratz
O5–5.5V((f))) 5.97 15 Sagittarii 4,200±650 1 O9.7 Iab or B0 Iab 5.37 AO Cassiopeiae (Pearce's Star) 4,300 ± 300 2 O8V((f)) + O9.2II 6.07-6.24 HD 149404 (V918
List_of_O-type_stars
Process by which stars are named
into popular use, for example Sualocin for α Delphini and Navi for γ Cassiopeiae. The International Astronomical Union (IAU) has begun a process to select
Stellar designations and names
Stellar_designations_and_names
Constellation in the northern celestial hemisphere
variations are slight, Gomeisa is classified as a shell star (Gamma Cassiopeiae variable), with a maximum magnitude of 2.84 and a minimum magnitude of
Canis_Minor
Variable star in the constellation Orion
HD 290327 b Star clusters NGC 1662 1980 1981 2169 2175 2194 2202 Other Lambda Orionis Orion OB1 Trapezium (θ1) Nebulae NGC 1788 1990 1999 2022 2023 2064
Omega_Orionis
Constellation in the northern celestial hemisphere
(1982). "A Comparison of the X-ray Properties of X Persei and Gamma Cassiopeiae". The Astrophysical Journal. 263 (1): 277–88. Bibcode:1982ApJ...263.
Perseus_(constellation)
Constellation in the southern celestial hemisphere
this variation can be observed with the unaided eye. Classed as a Gamma Cassiopeiae variable or shell star, it is of spectral type B2II-IIIe and lies around
Pavo_(constellation)
"Galactic clusters with associated Cepheid variables. II – NGC 129 and DL Cassiopeiae". Astronomical Journal. 104 (3): 1132–1143. Bibcode:1992AJ....104.1132T
List_of_open_clusters
570 (in Libra) A K5Ve 5.72 6.86 14h 57m 28.00s −21° 24′ 55.7″ 19.2 η Cassiopeiae A G3V 3.46 4.59 00h 49m 06.29s +57° 48′ 54.7″ 19.3 36 Ophiuchi A K1Ve
List_of_nearest_bright_stars
System of two stars orbiting each other
binary white dwarf system with an orbital period of about 5.4 minutes Eta Cassiopeiae, a nearby visual binary star system in the constellation Cassiopeia Kepler-14
Binary_star
Star types predicted by theory
came to be, proposed by Matthieu Gounelle and Georges Meynet in 2012 3 Cassiopeiae A star recorded by astronomer John Flamsteed, but never seen again 34
Hypothetical_star
Constellation split into two non-contiguous parts
photometric observations of the selected Algol-type binaries - IV. V799 Cassiopeiae, BX Piscium and HD 172189". Monthly Notices of the Royal Astronomical
Serpens
supergiant II-P Gamma Cassiopeiae (Tiansi) 00h 56m 42.50108s +60° 43′ 00.2984″ Cassiopeia 550 ± 10 B0.5IVe Main-sequence II Lambda Scorpii (Shaula) 17h
List_of_supernova_candidates
5.41 K0Ve 6 HD 400 Andromeda 6.21 F8 IV 7 CD-27 16 11.72 M0V 8 Beta Cassiopeiae (Caph) Cassiopeia 54.7 ± 0.3 +2.28 (2.25–2.31) F2 III 9 HD 469 G8III
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Star whose brightness fluctuates, as seen from Earth
on an observable timescale. One of the best studied examples is Rho Cassiopeiae. R Coronae Borealis variables While classed as eruptive variables, these
Variable_star
Overview of the scientific field of astronomy
star Flare star Giants and supergiants Luminous blue variable Gamma Cassiopeiae variable R Coronae Borealis variable Eruptive binary RS Canum Venaticorum
Outline_of_astronomy
Rén Old Man Alpha Carinae Canopus Carina 附路 Fù Lù Auxiliary Road Zeta Cassiopeiae Fulu Cassiopeia A single-star asterism in the Legs mansion. Fù Lù became
List_of_Chinese_star_names
Star name Temperature (K) Spectral type Distance (light years) Notes S Cassiopeiae 1,800 S3,4–S5,8 3,100±300 LL Pegasi 1,800 C 4,200 RW Leonis Minoris 1
List_of_coolest_stars
Stars sorted by absolute magnitude
ISSN 0004-6361. S2CID 15874925. Murdin, P.; Penston, M. V. (1977-12-01). "The Lambda Orionis association". Monthly Notices of the Royal Astronomical Society
List_of_most_luminous_stars
Type of star that is massive and luminous
stars visible to the naked eye and one of the largest in the galaxy. Rho Cassiopeiae, a variable yellow hypergiant, is one of the most luminous naked-eye
Supergiant
Cluster of Orion complex 33 39,000 1,340 5.13 combined evolution SIMBAD κ Cassiopeiae Cassiopeia OB14 33 23,500 4,000 4.16 evolution SIMBAD μ Normae NGC 6169
List_of_most_massive_stars
Clustering of stars in astronomy diagram
star. Other well-known examples include: Capella Aa ε Tauri β Ceti α Cassiopeiae δ Andromedae Arcturus has sometimes been thought to be a clump giant
Red_clump
Norbert S. (December 2024). "A Time-dependent Spectral Analysis of γ Cassiopeiae". The Astrophysical Journal. 978 (1): 105. doi:10.3847/1538-4357/ad944e
List_of_smallest_known_stars
cluster GCAS – (celestial object) Gamma CASsiopeiae, a class of eruptive variable stars named after Gamma Cassiopeiae, the archetype for the class GCMS –
List_of_astronomy_acronyms
Observatory in Urbana, Illinois, U.S.
papers in the Astrophysical Journal on eclipsing binaries Lambda Tauri, Algol, 1H Cassiopeiae (HR 8926), ellipsoidal variables π5 Orionis, and b Persei
Astronomical Observatory (University of Illinois Urbana-Champaign)
Astronomical_Observatory_(University_of_Illinois_Urbana-Champaign)
star WR 102 T= 200,000 K (200,000 °C; 360,000 °F) List of hottest stars Coolest star S Cassiopeiae T= 1,800 K (1,530 °C; 2,780 °F) List of coolest stars
List_of_star_extremes
American astronomer
acquainted with the celebrate carbon star 280 Schjellerup, better known as WZ Cassiopeiae, which was recognized about 100 years ago as an unusual member of a group
William_P._Bidelman
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
Girl/Female
Indian
Praiseworthy, Praiser of Allah
Female
Italian
Italian form of English Amber, AMBRA means "amber."
Girl/Female
Indian
Ambitious
Girl/Female
Muslim
Dark lipped
Girl/Female
Muslim
Flame
Girl/Female
Arabic, Indian, Muslim, Pashtun, Sanskrit
Flame; Large; Spacious; Tall; Another Name for Durga and Lakshmi
Surname or Lastname
English
English : from Middle English lamb, a nickname for a meek and inoffensive person, or a metonymic occupational name for a keeper of lambs. See also Lamm.English : from a short form of the personal name Lambert.Irish : reduced Anglicized form of Gaelic Ó Luain (see Lane 3). MacLysaght comments: ‘The form Lamb(e), which results from a more than usually absurd pseudo-translation (uan ‘lamb’), is now much more numerous than O’Loan itself.’Possibly also a translation of French agneau.
Female
Native American
Native American Indian name ALAMEDA means "grove of cottonwood."
Female
Greek
(Λαμία) Greek myth name of an evil spirit who abducts and devours children, LAMIA means "large shark." The name means "vampire" in Latin and "fiend" in Arabic.
Surname or Lastname
English
English : habitational name from Lambden in Berwickshire.
Boy/Male
Hindu
Lord Ganesh, The huge bellied Lord
Boy/Male
Indian
Jaws.
Girl/Female
Muslim
Praiseworthy, Praiser of Allah
Girl/Female
Indian
Soft to touch
Girl/Female
Muslim
Ambitious
Girl/Female
Muslim
Soft to touch
Female
Spanish
Feminine form of Spanish Amado, AMADA means "beloved."
Surname or Lastname
English
English : from a pet form of Lamb 1 and 2.English : from an Old Norse personal name Lambi, from lamb ‘lamb’.
Girl/Female
Indian
Flame
Girl/Female
Indian
Dark lipped
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
Boy/Male
Tamil
Ritveek | ரிதà¯à®µà®¿à®•
Boy/Male
Gujarati, Hindu, Indian, Marathi
Unbeatable
Girl/Female
Spanish
Blooming.
Girl/Female
Assamese, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Sindhi, Telugu
River
Male
Chinese
may the state govern, or may the kingdom heal.
Female
French
French feminine form of Roman Latin Faustinus, FAUSTINE means "lucky."
Boy/Male
Arabic
Strong
Female
English
From a French word used as a term of endearment, BIBI means "bauble, toy."
Boy/Male
Hindu, Indian
Impress
Boy/Male
British, English
From the Red Ford
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
LAMBDA CASSIOPEIAE
n.
A viola da gamba.
n.
Any person who is as innocent or gentle as a lamb.
pl.
of Lamina
imp. & p. p.
of Lamb
n.
A thin plate or lamina.
n.
The point of junction of the sagittal and lambdoid sutures of the skull.
pl.
of Lamina
n.
A lamp or candlestick.
n.
A monster capable of assuming a woman's form, who was said to devour human beings or suck their blood; a vampire; a sorceress; a witch.
n.
A thin plate or scale; specif., one of the thin, flat processes composing the vane of a feather.
p. pr. & vb. n.
of Lamb
a.
Shaped like the Greek letter lambda (/); as, the lambdoid suture between the occipital and parietal bones of the skull.
n.
The lamb's-quarters (Chenopodium album).
n.
A thin plate or scale; a layer or coat lying over another; -- said of thin plates or platelike substances, as of bone or minerals.
a.
Lamed; lame; disabled; impeded.
n.
A lamb.
n.
The name of the Greek letter /, /, corresponding with the English letter L, l.
v. i.
To bring forth a lamb or lambs, as sheep.
n.
The blade of a leaf; the broad, expanded portion of a petal or sepal of a flower.
n.
A lamb.