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Star in the constellation Cepheus
Lambda Cephei is a blue supergiant star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from λ Cephei, and
Lambda_Cephei
Triple star system in the constellation Scorpius
Lambda Scorpii is a triple star system and the second-brightest object in the constellation of Scorpius. It is formally named Shaula; Lambda Scorpii is
Lambda_Scorpii
Hot, luminous star with a spectral type of A9 or earlier
B2Ia Omicron² Canis Majoris, B-type supergiant, spectral type B3Ia Lambda Cephei, O-type supergiant, spectral type O6.5I(n)fp Mu Sagittarii, B-type supergiant
Blue_supergiant
Tauri. Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements can be inconsistent
List_of_largest_stars
NSVS 14256825 A 2,700 ± 100 2 sdOB 13.2 Has a M-type companion star. Lambda Cephei 3,098.5 1 O6.5If(n)p +5.050 HD 193322 3,100 2 O9Vnn + O8.5 III +5.958
List_of_O-type_stars
Visible star that is nearly aligned with Earth's axis of rotation
Cephei ("Errai") by 3000 AD, with Errai reaching its closest alignment with the northern celestial pole around 4200 AD. Iota Cephei and Beta Cephei will
Pole_star
Open cluster in the constellation Cepheus
as supernovae. Mu Cephei, Nu Cephei, and NGC 7160 may have been companions of those stars. It has been suggested that Lambda Cephei and 68 Cygni are runaway
NGC_7160
41 3.37 Lambda Tauri Triple star system 3.41 3.39 Gamma Phoenicis Binary star system 3.41 Zeta Pegasi Star 3.41 Zeta Lupi Star 3.41 Eta Cephei Star 3.41
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Star in the constellation Cygnus
runaway stars known in the Milky Way (along with the O-type supergiants Lambda Cephei and Zeta Puppis). Initially it was suggested a supernova explosion of
BD+43_3654
Type of variable star
non-GCAS Be star variables. λ Eridani itself is incorrectly listed as a Beta Cephei variable. The AAVSO International Variable Star Index defines a LERI type
Lambda_Eridani_variable
Star that has a supergiant luminosity class, with a spectral type of F or G
Scorpii. Many of them are variable stars, mostly pulsating Cepheids such as δ Cephei itself. Hertzsprung–Russell diagram Spectral type O B A F G K M L T Brown
Yellow_supergiant
Binary star system in the constellation of Andromeda
λ Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae
Lambda_Andromedae
Stars with a supergiant luminosity class with a spectral type of K or M
well-known naked-eye examples: Antares A Betelgeuse Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically
Red_supergiant
Star in the constellation Crux
Crucis is listed in the General Catalogue of Variable Stars as a possible β Cephei-type variable. Its brightness varies with an amplitude of 0m.02 over a period
Lambda_Crucis
l-Yamīn the Right Arm (of Cepheus) الذراع اليمين الذّراع اليَمِين Alpha Cephei Aldhibah ʼaḍ-Ḍibaāʽ [Adh-Dhibaaʽ], ʼaḍ-Ḍibāʽ [Adh-Dhibaaʽe] the Hyenas الضباع
List_of_Arabic_star_names
Astrophysical limit on radiation from stars
LGGS J013350.62+303230.3 309,000 3,800 HV 888 302,000 3,442–3,500 M4Ia RW Cephei 300,000 4,400 K2Ia-0 A K-type yellow hypergiant. LGGS J013358.54+303419
Eddington_luminosity
(2023-07-01). "Solar-like oscillations in γ Cephei A as seen through SONG and TESS - A seismic study of γ Cephei A". Astronomy & Astrophysics. 675: A197.
List_of_nearest_giant_stars
Constellation in the southern celestial hemisphere
star of magnitude 1.3, and lies 353 light-years from Earth. It is a Beta Cephei-type variable star with a variation of less than 0.1 magnitudes. γ Crucis
Crux
Variable star in the constellation Eridanus
Eri is classified in the General Catalogue of Variable Stars as a Beta Cephei variable. The AAVSO International Variable Star Index defines a LERI type
Lambda_Eridani
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
yellow hypergiant that is one of the brightest to the naked eye; and Mu Cephei (Garnet Star), one of the largest and brightest stars known. In 1956, the
Hypergiant
Type of star larger than main-sequence but smaller than a giant
G8: β Aquilae, δ Pavonis, λ Andromedae K0: η Cephei, κ Coronae Borealis, δ Eridani, 55 Cancri A K1: γ Cephei, π Hydrae, φ Serpentis, δ Leporis Later analysis
Subgiant
Constellation in the southern celestial hemisphere
B1.5 III that is 460 ± 10 light-years distant from Earth. It is a Beta Cephei variable, pulsating in brightness by 0.03 of a magnitude every 7 hours and
Lupus_(constellation)
Large self-illuminated object in space
Size comparison of some well-known supergiant and hypergiant stars, featuring Cygnus OB2-12, V382 Carinae, Betelgeuse, VV Cephei, and VY Canis Majoris
Star
Star in the constellation Octans
hemisphere for the 1908 Revised Harvard Photometry catalogue. The Pole Star and Lambda Ursae Minoris were used for the northern hemisphere. It was then noted that
Sigma_Octantis
Alfirk β Cephei Aa Cepheus Arabic From Arabic: الفرق al-firq ('the flock'). Name given by Ulugh Beg to the asterism consisting of α, β and η Cephei. /ˈælfərk/
List_of_proper_names_of_stars
Constellation in the southern celestial hemisphere
Canis Majoris. Also called Mirzam or Murzim, Beta is a blue-white Beta Cephei variable star of magnitude 2.0, which varies by a few hundredths of a magnitude
Canis_Major
Star in the constellation Scorpius
The primary component of the pair, κ Sco A, is a variable star of Beta Cephei type. It is undergoing radial pulsations with a dominant frequency of five
Kappa_Scorpii
Classification of stars based on spectral properties
standards: B0V – Upsilon Orionis B0Ia – Alnilam B2Ia – Chi2 Orionis B2Ib – 9 Cephei B3V – Alkaid B3V – Haedus B3Ia – Omicron2 Canis Majoris B5Ia – Aludra B8Ia
Stellar_classification
87 2.45 Aludra η Canis Majoris 2,000 B5 Ia Southern 88 2.46 Alderamin α Cephei 49 A8Vn Northern 89 2.46 Markeb κ Velorum 0540 B2 IV Southern 90 2.47 (1
List_of_brightest_stars
Space Telescope: A Parallax of the Fundamental Distance Calibrator delta Cephei". The Astronomical Journal. 124 (3): 1695–1705. arXiv:astro-ph/0206214.
List_of_nearest_supergiants
Constellation in the southern celestial hemisphere
times as luminous and 8 times as massive as the Sun. The star is a Beta Cephei variable with about 4.7 times the Sun's diameter, and pulsates every 2.2 hours
Musca
examples of stars in this mass range include Antares, Spica, Gamma Velorum, Mu Cephei, and members of the Quintuplet Cluster. Type Ia supernova progenitors are
List_of_supernova_candidates
Zhao; et al. (2009). "Imaging And Modeling Rapidly Rotating Stars: Alpha Cephei And Alpha Ophiuchi". The Astrophysical Journal. 701 (1): 209–224. arXiv:0906
List of stars with resolved images
List_of_stars_with_resolved_images
Type of star that is massive and luminous
in Cygnus; and Delta Cephei (itself the prototype) and Polaris are Cepheid variables and yellow supergiants. Antares and VV Cephei A are red supergiants
Supergiant
59.5s +57° 41′ 45″ M3.0V 0.271 9.79 11.76 249.5 ±0.1 B flare star B (DO Cephei) M4.0V 0.176 11.41 13.38 DENIS J1048−3956 13.1932 ±0.0027 Ant* 10h 48m 14
List_of_nearest_stars
Brightest star in the constellation Lyra
uncertain. This group contains about 16 stars, including Alpha Librae, Alpha Cephei, Castor, Fomalhaut and Vega. All members of the group are moving in nearly
Vega
Study of oscillations in stars
understood to be high-order gravity modes excited by the kappa mechanism. Beta Cephei variables are slightly hotter (and thus more massive), also have modes excited
Asteroseismology
Stage of stellar evolution
during a blue loop from the red-giant branch, are thought to make up the δ Cephei variables. Both types of star have luminous and unstable photospheres at
Blue_loop
Small number of stars that orbit each other
might comprise a physical binary and an optical companion (such as Beta Cephei) or, in rare cases, a purely optical triple star (such as Gamma Serpentis)
Star_system
Star whose brightness fluctuates, as seen from Earth
ten variable stars were known. John Goodricke himself discovered Delta Cephei and Beta Lyrae. Since 1850, the number of known variable stars has increased
Variable_star
Astrophysical phenomenon
Spica, Rigel and Deneb, the red supergiants Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta
Supernova
Star in the constellation Cygnus
of Pi1 Cygni, Alpha Lacertae, 4 Lacertae, Pi2 Cygni, HD 206267, Epsilon Cephei, Beta Lacertae, Sigma Cassiopeiae, Rho Cassiopeiae, Tau Cassiopeiae, AR
Pi1_Cygni
Wide-band photometric system used in astronomy
UBVRI light curves of the prototype Cepheid variable, Delta Cephei
UBV_photometric_system
(Edasich) 101.2 ± 0.3 Draco 15h 24m 55.77463s +58° 57′ 57.8344″ K2III 3.290 Xi Cephei (Kurhah) Ba 101.34 ± 0.06 Cepheus 22h 03m 47.440s +64° 37′ 40.70″ A3Vm 4
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Type of variable star
oscillating Ap SX Phoenicis Blue-white with early spectra Alpha Cygni Beta Cephei Slowly pulsating B-type PV Telescopii Blue large-amplitude pulsator Long-period
Rapidly_oscillating_Ap_star
Main-sequence star of spectral type O
O8 types, and listed 5 O9 V standards (HD 46202, HD 52266, HD 57682, 14 Cephei, 10 Lacertae) and 3 O9.5 V standards (HD 34078, Sigma Orionis, Zeta Ophiuchi)
O-type_main-sequence_star
Star in the constellation Canis Major
magnitude) variability in the brightness of HR 2501 during their search for beta Cephei variable stars in the southern sky. Christoffel Waelkens et al. confirmed
HR_2501
Type of chemically peculiar star
α Geminorum Ba 2.96 α Volantis 4.00 Acubens A α Cancri A 4.26 Kurhah ξ Cephei 4.29 θ1 Crucis 4.30 π Virginis 4.64 μ Aurigae 4.88 2 Ursae Majoris 5.46
Am_star
Spectroscopic binary system in the constellation of Orion
brightness variability has led to the star being classified as a pulsating Beta Cephei variable, but no evidence has been found of pulsations superimposed on the
Psi2_Orionis
Constellation in the northern celestial hemisphere
Delta (Sarvvis) Psi (4.3), and 48 Persei (4.0);, the 2.9 magnitude Beta Cephei variable Epsilon Persei (Áldu) and the stars 29 (5.2), 30 (5.5), 31 (5.0)
Perseus_(constellation)
Region of an astronomical diagram
the long period variable AGB stars. At hotter temperatures are the Beta Cephei and PV Telescopii variables. Right at the edge of the instability strip
Instability_strip
unconfirmed exoplanets. SSSPM J1549-3544 313.2 ± 0.6 Lupus sdK5 14.78 Kappa Cephei 314 Cepheus B9III TOI-3493 315.59±0.65 G0 Has one known exoplanet. HD 108501
List of star systems within 300–350 light-years
List_of_star_systems_within_300–350_light-years
Type of eruptive variable star
Ophiuchus 2m.56 2m.58 0.02 O9.5V Also a Beta Cephei variable Pleione Taurus 4m.77 5m.5 0.77 B8Vne Lambda Pavonis Pavo 4m.00 4m.26 0.26 B2II-IIIe Phi
Gamma_Cassiopeiae_variable
Continuous band of stars that appears on plots of stellar color versus brightness
difficult to detect. Other classes of unstable main-sequence stars, like Beta Cephei variables, are unrelated to this instability strip. The total amount of
Main_sequence
; et al. (August 2009), "Imaging and Modeling Rapidly Rotating Stars: α Cephei and α Ophiuchi", The Astrophysical Journal, 701 (1): 209–224, arXiv:0906
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
(zēng yī, 1st added star), 增二 (zēng èr, 2nd added star) etc. For example, γ Cephei is referred to as 少衛增八 (Shào Wèi Zēng Bā, 8th Added Star of Second Imperial
List_of_Chinese_star_names
Star in the constellation of Draco
Enclosure, refers to an asterism consisting of Alpha Draconis, Kappa Draconis, Lambda Draconis, 24 Ursae Majoris, 43 Camelopardalis, Alpha Camelopardalis and
Thuban
Binary star system in the constellation Andromeda
et al. (2015). "The 2003–2004 multisite photometric campaign for the β Cephei and eclipsing star 16 (EN) Lacertae with an appendix on 2 Andromedae, the
2_Andromedae
List of largest planets by size
(July 2023). "Solar-like oscillations in γ Cephei A as seen through SONG and TESS: A seismic study of γ Cephei A". Astronomy & Astrophysics. 675: A197.
List_of_largest_exoplanets
Class of massive star with a spectral type of A to K
bound, yellow hypergiants and red supergiants are not clearly separated; RW Cephei (roughly 4,000 K (3,730 °C; 6,740 °F), 295,000 L☉) is an example of a star
Yellow_hypergiant
Stellar classification
planets have been found around evolved K-giant stars including Pollux, Gamma Cephei and Iota Draconis. Doppler surveys around a wide variety of stars indicate
A-type_main-sequence_star
German-British astronomer and composer (1738–1822)
Uranus () features the capital initial letter of Herschel's surname. Mu Cephei is also known as Herschel's Garnet Star Herschel, a crater on the Moon Herschel
William_Herschel
Constellation in the northern celestial hemisphere
Musalsalah in Arabic. It has also been called Persea ("Perseus's wife") or Cepheis ("Cepheus's daughter"), all names that refer to Andromeda's role in the
Andromeda_(constellation)
Constellation split into two non-contiguous parts
one study, it could be one of the first discovered hybrids between Beta Cephei variables and slowly pulsating B stars. Although not visible to the naked
Serpens
Overview of the scientific field of astronomy
Scuti variable SX Phoenicis variable Blue-white with early spectra Beta Cephei variable PV Telescopii variable Long Period and Semiregular Mira variable
Outline_of_astronomy
−60° 43′ 44″ 44.9 ι Piscium F7V 4.06 3.36 23h 39m 57s +05° 37′ 38″ 45.0 γ Cephei A K1IV 2.94 2.24 23h 39m 21s +77° 37′ 56″ 45.0 Gliese 615 K0V 7.36 6.66
List_of_nearest_bright_stars
Desmet, M.; Aerts, C. (November 2006). "An asteroseismic study of the β Cephei star β Canis Majoris". Astronomy and Astrophysics. 459 (2): 589–596.
List_of_most_massive_stars
Star in the constellation Gemini
Evidence Supporting Cluster Membership for the Keystone Calibrator Delta Cephei", Astrophysical Journal, 747 (2): 145, arXiv:1201.0993, Bibcode:2012ApJ
Zeta_Geminorum
Stars sorted by absolute magnitude
99J Hubrig, S.; et al. (June 2006), "Discovery of magnetic fields in the βCephei star ξ1 CMa and in several slowly pulsating B stars*", Monthly Notices of
List_of_most_luminous_stars
processing BCEP – (celestial object) Beta CEPhei, a class of pulsating variable stars for which Beta Cephei is the archetypal object also BCE BCG – (celestial
List_of_astronomy_acronyms
System of two stars orbiting each other
white dwarf-pulsar binary PSR B1620-26, the subgiant-red dwarf binary Gamma Cephei, and the white dwarf-red dwarf binary NN Serpentis, among others. A study
Binary_star
M3-4 + M5-6 b 902 HD 222237 Tucana 37.329 ± 0.008 7.09 K3+V b 903 Gamma Cephei (Errai) Cepheus 44.98 ± 0.09 3.21 K1III-IV CN1 + M4V Ab (Tadmor) 904 Iota
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Portion of the giant branch before helium ignition
difficult to measure directly. The current mass of Cepheid variables such as δ Cephei can be measured accurately because there are either binaries or pulsating
Red-giant_branch
Type of star
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 05280−6910
OH/IR_star
star is a supergiant. List of nearest supergiants Nearest hypergiant μ Cephei (Garnet Star) 3,060 light-years (940 pc) Nearest carbon star CW Leonis 310
List_of_star_extremes
American astronomer
blue variable (LBV). This is the star Zeta puppis. The red supergiant VV Cephei stars were defined as a class by Bidelman in 1954. In this artist's conception
William_P._Bidelman
LAMBDA CEPHEI
LAMBDA CEPHEI
Boy/Male
Indian
Jaws.
Surname or Lastname
English
English : habitational name from Lambden in Berwickshire.
Girl/Female
Muslim
Soft to touch
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.
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’.
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.
Girl/Female
Indian
Praiseworthy, Praiser of Allah
Female
Italian
Italian form of English Amber, AMBRA means "amber."
Girl/Female
Indian
Flame
Boy/Male
Hindu
Lord Ganesh, The huge bellied Lord
Girl/Female
Indian
Soft to touch
Girl/Female
Muslim
Praiseworthy, Praiser of Allah
Girl/Female
Arabic, Indian, Muslim, Pashtun, Sanskrit
Flame; Large; Spacious; Tall; Another Name for Durga and Lakshmi
Girl/Female
Indian
Ambitious
Girl/Female
Muslim
Dark lipped
Girl/Female
Muslim
Flame
Female
Native American
Native American Indian name ALAMEDA means "grove of cottonwood."
Girl/Female
Muslim
Ambitious
Female
Spanish
Feminine form of Spanish Amado, AMADA means "beloved."
Girl/Female
Indian
Dark lipped
LAMBDA CEPHEI
LAMBDA CEPHEI
Girl/Female
Arabic, Australian, Islamic, Muslim, Pakistani, Urdu
Beautiful; Pure; Kind
Boy/Male
Tamil
Konark | கோநாரà¯à®•
The Sun
Girl/Female
Tamil
One who tends to the weak and heals
Boy/Male
American, Australian, British, English, French
Raven; Raven-haired
Boy/Male
Hindu, Indian, Malayalam, Marathi
Father of the Pandavas; Character of Mahabharata
Girl/Female
Indian, Punjabi, Sikh
Supreme Longing of Beloved
Female
French
Medieval French form of Teutonic Helewidis, HELEWISE means "hale-wide; very healthy and sound."
Girl/Female
Indian
Honour, Pride
Boy/Male
Hindu
Victorious, Conquering, Defeating
Boy/Male
Irish
Relic.
LAMBDA CEPHEI
LAMBDA CEPHEI
LAMBDA CEPHEI
LAMBDA CEPHEI
LAMBDA CEPHEI
pl.
of Lamina
n.
The lamb's-quarters (Chenopodium album).
n.
The blade of a leaf; the broad, expanded portion of a petal or sepal of a flower.
n.
Any person who is as innocent or gentle as a lamb.
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.
p. pr. & vb. n.
of Lamb
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.
The name of the Greek letter /, /, corresponding with the English letter L, l.
a.
Shaped like the Greek letter lambda (/); as, the lambdoid suture between the occipital and parietal bones of the skull.
n.
A thin plate or scale; specif., one of the thin, flat processes composing the vane of a feather.
n.
A thin plate or lamina.
v. i.
To bring forth a lamb or lambs, as sheep.
n.
The point of junction of the sagittal and lambdoid sutures of the skull.
n.
A lamp or candlestick.
n.
A lamb.
pl.
of Lamina
imp. & p. p.
of Lamb
a.
Lamed; lame; disabled; impeded.
n.
A lamb.
n.
A viola da gamba.