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Star in the constellation Cepheus
V Cephei is a white main sequence star in the constellation Cepheus. It only varies slightly by 0.03 of a magnitude. It was suspected of being variable
V_Cephei
Binary star in the constellation Cepheus
Gamma Cephei is a binary star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from γ Cephei, and abbreviated
Gamma_Cephei
Constellation in the northern celestial hemisphere
hypergiant, together with the red supergiants Mu Cephei, MY Cephei, VV Cephei, V381 Cephei, and V354 Cephei are among the largest stars known. In addition
Cepheus_(constellation)
Star in the constellation Cepheus
V354 Cephei is a red supergiant star located within the Milky Way. It is an irregular variable located over 13,000 light-years away from the Sun. It has
V354_Cephei
Red supergiant star in the constellation Cepheus
Mu Cephei is a red supergiant or hypergiant star in the northern constellation Cepheus. It is officially named the Garnet Star; Mu Cephei is its Bayer
Mu_Cephei
Star in the constellation Cepheus
Beta Cephei is a triple star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from β Cephei, and abbreviated
Beta_Cephei
Star in the constellation of Cepheus
asterism consisting of α Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Xi Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese
Alpha_Cephei
Binary star system in the constellation Cepheus
Cephei is a quadruple star system in the northern constellation of Cepheus, the King. Its name is a Bayer designation that is Latinized from δ Cephei
Delta_Cephei
Binary star in the constellation Cepheus
VV Cephei, also known as HD 208816, is an eclipsing binary star system located in the constellation Cepheus. It is both a B[e] star and shell star. As
VV_Cephei
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
Hypergiant star in the constellation Cepheus
RW Cephei is a K-type hypergiant and a semirregular variable star in the constellation Cepheus, at the edge of the Sharpless 132 H II region and close
RW_Cephei
Type of variable star
Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations
Beta_Cephei_variable
Labelled Omega Cephei (ω Cep/ω Cephei) by Bode in his Uranographia Designated by Burrett in his atlas Labelled Tau Cephei (τ Cep/τ Cephei) by Bode in his
List_of_stars_in_Cepheus
Star in the constellation Cepheus
Epsilon Cephei is a star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ε Cephei, and abbreviated Epsilon
Epsilon_Cephei
Topics referred to by the same term
airline v/v (volume by volume), the volume fraction VV Cephei, a star system Vorontsov-Vel'yaminov Interacting Galaxies, a catalogue of galaxies V//V, the
VV
Indian astronomer
Some sources also attribute the discovery of another variable star V Cephei or U Cephei to him but same has not been confirmed by the Madras Observatory
Chinthamani_Ragoonatha_Chary
Star in the constellation Cepheus
9 Cephei (9 Cep), also known as V337 Cephei, is a variable star in the constellation Cepheus. It is visible to the naked eye. In 1967, Graham Hill announced
9_Cephei
Variable star in the constellation Cepheus
W Cephei is a spectroscopic binary and variable star located in the constellation Cepheus. It is thought to be a member of the Cep OB1 stellar association
W_Cephei
Eclipsing binary star
U Cephei is an eclipsing binary star discovered in 1880. It consists of a blue-white main sequence star of spectral type B7/8V that is eclipsed every two
U_Cephei
Star in the constellation of Cepheus
ST Cephei (ST Cep), also known as BD+56°2793, is a red supergiant and a variable star located in the constellation Cepheus. It has a variable apparent
ST_Cephei
Variable star in the constellation Cepheus
S Cephei (S Cep), also designated as HD 206362, is a carbon star and Mira-type variable in the constellation Cepheus. Based on the measurement of its annual
S_Cephei
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 is
Lambda_Cephei
Triple star system in the constellation Cepheus
V381 Cephei (HR 8164) is a triple star system in the northern constellation of Cepheus. Its apparent magnitude is slightly variable between 5.5 and 5.7
V381_Cephei
Star in the constellation Scutum
hypergiant that may also challenge the Humphreys–Davidson limit UY Scuti MY Cephei Mistakenly referred to as RSGC1-01. Calculated, using the Stefan-Boltzmann
Stephenson_2_DFK_1
Red supergiant star in the constellation Orion
Tsuji, T. (2000). "Water on the early M supergiant stars α Orionis and μ Cephei". The Astrophysical Journal. 538 (2): 801–07. Bibcode:2000ApJ...538..801T
Betelgeuse
Vulpecula M1 III 4.40 V Cephei 291.6 ± 0.7 Cepheus A1V 6.57 Zeta Apodis 293 ± 3 Apus K2 III +4.78 HD 48265 (Nosaxa) 293 ± 6 G5IV/V 8.07 Sigma Octantis (Polaris
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Star in the constellation Cepheus
Zeta Cephei is a red supergiant star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ζ Cephei, and abbreviated
Zeta_Cephei
Star in the constellation Cepheus
consisting of η Cephei, 4 Cephei, HD 194298, θ Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for η Cephei itself
Eta_Cephei
Star in the constellation Cepheus
asterism consisting of Xi Cephei, 4 Cephei, HD 194298, Eta Cephei, Theta Cephei, Alpha Cephei, 26 Cephei, Iota Cephei and Omicron Cephei. Consequently, the Chinese
Xi_Cephei
Star in the constellation Cepheus
Nu Cephei is a blue-hued variable star in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from ν Cephei, and abbreviated
Nu_Cephei
Variable star in the constellation Cepheus
LZ Cephei, also known by its Flamsteed designation 14 Cephei, is a star about 3,600 light years from the Earth, in the constellation Cepheus. Its apparent
LZ_Cephei
Variable star in the constellation Cepheus
AR Cephei (AR Cep) is a variable star in the constellation Cepheus. It is classified as a semiregular star with a spectral type of M4III. Aernout de Sitter
AR_Cephei
Variable star in the constellation Cepheus
SS Cephei is a semiregular variable star in the constellation Cepheus. It is of spectral type M5III, and has an estimated temperature of about 3,700 K
SS_Cephei
Topics referred to by the same term
of the Pier Aeromar (former IATA code: VW), a former Mexican airline VW Cephei, a binary star system VW Hamme or VW Hamme, a Belgian association football
VW_(disambiguation)
Star in the constellation Virgo
their spectra. The primary is a blue giant and a variable star of the Beta Cephei type. Spica, along with Arcturus and Denebola—or Regulus, depending on the
Spica
Triple star system in the constellation Scorpius
two B-type stars and a pre-main-sequence star. The primary star is a Beta Cephei variable star with rapid brightness changes of about a hundredth of a magnitude
Lambda_Scorpii
Star in the constellation Cepheus
Pi Cephei is a trinary star system located in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from π Cephei, and
Pi_Cephei
Type of variable star
rise to maximum light followed by a slower fall to minimum (e.g. Delta Cephei). This is due to the phase difference between the radius and temperature
Classical_Cepheid_variable
Star in the constellation Cepheus
Iota Cephei is a star in the northern constellation Cepheus. Its name is a Bayer designation that is Latinized from ι Cephei, and abbreviated Iota Cep
Iota_Cephei
Star in the constellation Cepheus
T Cephei is a Mira variable star in the constellation Cepheus. Located approximately 600 light-years (180 parsecs) distant, it varies between magnitudes
T_Cephei
Main-sequence star of spectral type O
the O5 to 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
O-type_main-sequence_star
Red supergiant star in the constellation Cepheus
MY Cephei (abbreviated to MY Cep), also known as IRC +60375, is a red supergiant or hypergiant located in the open cluster NGC 7419 in the constellation
MY_Cephei
Reflection nebula in the constellation Cepheus
Tauri star PV Cephei. It is known for changing its shape dramatically on a timescale of months to years, as the brightness of PV Cephei changes. The nebula
Gyulbudaghian's_Nebula
Star in the constellation Cepheus
Rho1 Cephei is a double star located in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ1 Cephei, and abbreviated
Rho1_Cephei
Type of star
astronomy. Unless otherwise noted, the given magnitudes are in the V-band. Also a Beta Cephei variable Also an Algol variable Also a shell star Huang, L.; Guo
Slowly_pulsating_B-type_star
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
Star in the constellation Orion
1,300 light-years distant from the Solar System. It is a suspected Beta Cephei variable. Located south of Iota Orionis, Upsilon Orionis is one of two stars
Upsilon_Orionis
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
Scientific projections regarding the far future
S2CID 118403321. McClure, Bruce; Byrd, Deborah (22 September 2021). "Gamma Cephei, aka Errai, a future North Star". earthsky.org. Retrieved 25 December 2021
Timeline_of_the_far_future
Star in the constellation Cepheus
Rho2 Cephei is a solitary star in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ρ2 Cephei, or simply ρ
Rho2_Cephei
Star in the constellation Cepheus
consisting of 4 Cephei, HD 194298, η Cephei, α Cephei, ξ Cephei, 26 Cephei, ι Cephei and ο Cephei. Consequently, the Chinese name for θ Cephei itself is 天鈎三
Theta_Cephei
Star in the constellation Cepheus
V355 Cephei is a red supergiant located in the constellation of Cepheus. It has a radius between 770±154 and 790 solar radii, making it one of the largest
V355_Cephei
Variable star in the constellation Ophiuchus
naked eye of an observer far from city lights. V2052 Ophiuchi is a Beta Cephei variable (β Cep) star, varying slightly in brightness from magnitude 5.81
V2052_Ophiuchi
Star in the constellation Hercules
constellation Hercules, 139 parsecs (450 light-years) away. The brightest is a β Cephei variable, a pulsating star. Iota Herculis (Latinized from ι Herculis, abbreviated
Iota_Herculis
Type of variable star that pulsates radially
helium is doubly ionized. The term Cepheid originates from the star Delta Cephei in the constellation Cepheus, which was one of the early discoveries. On
Cepheid_variable
Star in the constellation Cepheus
24 Cephei is a single, yellow-hued star in the northern circumpolar constellation of Cepheus. With an apparent visual magnitude of 4.79, it is faintly
24_Cephei
Star in the constellation Puppis
as being a confirmed β Cephei variable, but with no explanation of when it was discovered. A 1971 thesis dedicated to β Cephei variables only mentions
HD_54893
Star in the constellation Cepheus
Cephei is a binary star system in the northern circumpolar constellation of Cepheus. Its name is a Bayer designation that is Latinized from κ Cephei,
Kappa_Cephei
Triple star system in the constellation Scutum
system located in the constellation of Scutum. It is classified as a VV Cephei-type system, which typically consists of a cool red supergiant and a hot
FR_Scuti
Star in the constellation Cepheus
19 Cephei is a supergiant star in the northern circumpolar constellation of Cepheus. It has a spectral class of O9 and is a member of Cep OB2, an OB association
19_Cephei
Star in the constellation Cepheus
V419 Cephei (BD+59°2342 or HIP 104719) is an irregular variable star in the constellation of Cepheus with an apparent magnitude that varies between 6.54
V419_Cephei
Triple star system in the constellation Centaurus
the detection of pulsations, the Aa component has been classified as a β Cephei variable. Beta Centauri is well known in the Southern Hemisphere as the
Beta_Centauri
Star in the constellation Canis Major
four largest galactic red supergiants per a survey, including Mu Cephei and V354 Cephei, along with later the extragalactic star, WOH G64 A, which used
VY_Canis_Majoris
Star in the constellation Musca
star. Alpha Muscae appears to be a Beta Cephei variable star. Telting and colleagues report it as a Beta Cephei with a high degree of confidence as they
Alpha_Muscae
Northern pole-star; brightest star in Ursa Minor
will move away from α UMi after the 21st century, passing close by Gamma Cephei by about the 41st century, moving towards Deneb by about the 91st century
Polaris
Star in the constellation Cepheus
11 Cephei is a single star in the northern constellation of Cepheus, located 179 light years away from the Sun. It is visible to the naked eye as a faint
11_Cephei
Binary star system in the constellation Cepheus
DH Cephei is a variable binary star system in the northern circumpolar constellation of Cepheus, positioned about two degrees to the east of the star system
DH_Cephei
B-type giant star in the constellation Pyxis
the naked eye. It has a stellar classification of B1.5III and is a Beta Cephei variable. This star has more than ten times the mass of the Sun and is more
Alpha_Pyxidis
Star system in the constellation Cepheus
VW Cephei (VW Cep) is a triple star in the constellation Cepheus, located roughly at 90.6 light years from the Sun. The two inner components form an eclipsing
VW_Cephei
Reflection nebula in the constellation Cepheus
located near the Mira-type variable star T Cephei, and near the bright magnitude +3.23 variable star Beta Cephei (Alfirk). The designation NGC 7023 refers
Iris_Nebula
Chinese alternative asset management firm
acquisitions. Cephei Capital was founded in 2006 with the support from CDH. Cephei focuses on investing in Chinese companies in the secondary market. Cephei now
CDH_Investments
OB Association in the constellation Cepheus
cool supergiants and hypergiants such as V509 Cassiopeiae (HR 8752) and RW Cephei. "Ass Cep OB 1". SIMBAD. Centre de données astronomiques de Strasbourg.
Cepheus_OB1
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
Binary star in the constellation Cepheus
Omicron Cephei is a binary star system in the northern constellation of Cepheus. Its name is a Bayer designation that is Latinized from ο Cephei, and abbreviated
Omicron_Cephei
"Analysis of far-infrared fine-structure emissions from the red supergiant μ Cephei". Astronomy & Astrophysics. doi:10.1051/0004-6361/202660113. ISSN 0004-6361
List_of_nearest_hypergiants
Catalogue, 5th Revised Ed. (Hoffleit+, 1991)". VizieR On-line Data Catalog: V/50. Originally Published in: 1964BS....C......0H. 5050. Bibcode:1995yCat.5050
List_of_proper_names_of_stars
Binary star in the constellation Cepheus
WZ Cephei is an eclipsing binary star of W Ursae Majoris-type in the constellation of Cepheus, located 976 light years away from the Sun. The stars orbit
WZ_Cephei
Variable Star in the constellation Cygnus
The system is a member of the young open cluster NGC 6871 and exhibits β Cephei type pulsations in its primary component, making it a key object for studying
V453_Cygni
all stars brighter than magnitude +2.50 in visible light, measured using a V-band filter in the UBV photometric system. Stars in binary systems (or other
List_of_brightest_stars
Comparison of a wide range of lengths
estimated diameter of VV Cephei A, a red hypergiant with a blue dwarf companion. 1.75 Tm – 11.7 au – estimated diameter of Mu Cephei, a red supergiant (possibly
Orders_of_magnitude_(length)
Binary star system in the constellation Cepheus
Krüger 60 (DO Cephei) is a binary star system located 13.1 light-years (4.0 parsecs) from Earth, being one of nearest stars. It is made up of a pair of
Krüger_60
Star in the constellation Crux
resulting in a rotational period of 13 to 17 days. β Crucis A is a known β Cephei variable, although with an effective temperature of about 27,000 K it is
Mimosa_(star)
Variable star in the constellation Hercules
Australis Past and future Northern Vega Tianbang Asuusiha Thuban Kochab Errai ι Cephei Alfirk Alderamin Deneb Fawaris Southern β Hydri γ Chamaeleontis I Carinae
Tau_Herculis
Star in the constellation Lupus
the blue-white glow of a B-type star. In 1956 it was identified as a Beta Cephei variable by Bernard Pagel and colleagues, which means it undergoes periodic
Alpha_Lupi
Chemical compound of hydrogen and oxygen
cooler stars and even detected in giant hot stars such as Betelgeuse, Mu Cephei, Antares and Arcturus. Circumstellar disks: including those of more than
Water
Star system in the constellation Perseus
star the blue-white hue that is typical of B-type stars. It is also a Beta Cephei variable star with a primary pulsation period of 0.1603 days, or 6.24 cycles
Epsilon_Persei
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
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
Class of variable star
eISSN 1538-4357. ISSN 0004-637X. S2CID 121391876. Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable
Rotating_ellipsoidal_variable
Astronomical principle
and a few months later by John Goodricke with the variability of Delta Cephei, the eponymous star for classical Cepheids. Most of the Cepheids were identified
Period-luminosity_relation
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
Cause of changes in luminosity in pulsating variable stars
variables, rapidly oscillating Ap stars (roAp) and ZZ Ceti variables. In Beta Cephei variables, stellar pulsations occur at a depth where the temperature reaches
Kappa–mechanism
& Laine, S. (8 June 2019). "Spectral Type of the Unusual Variable ASASSN-V J213939.3-702817.4". The Astronomer's Telegram. Retrieved 8 June 2019. Jayasinghe
List of stars that have unusual dimming periods
List_of_stars_that_have_unusual_dimming_periods
Multiple star system in the constellation of Scorpius
/ælˈnaɪjæt/, the traditional name for the entire star system) and a Beta Cephei variable) and Aa2; a third component (designated Sigma Scorpii Ab) at 0
Sigma_Scorpii
Star in the constellation Cepheus
Declination +87° 18′ 27.0304″ Apparent magnitude (V) 5.56 Characteristics Spectral type A8III or A7IV B−V color index 0.250±0.004 Astrometry Radial velocity
HD_221525
Variable star in the constellation Canis Major
with a stellar classification of B3 Ib. It has been classified as a Beta Cephei type variable star, but the supergiant spectral type and a period of over
Iota_Canis_Majoris
Star in the constellation Cepheus
PV Cephei is a variable star of Orion type located in the constellation of Cepheus at a distance of about 1,100 light-years from Earth. In visible light
PV_Cephei
Star in the constellation of Scorpius
or B3 star several times hotter than the Sun. HD 148703 is a candidate β Cephei variable and its variability was first noticed in 1983 by C. Sterken. Further
N_Scorpii
Nebula in the constellation Cepheus
rim being illuminated by HD 206267. The red supergiant or hypergiant Mu Cephei is located at the edge of the nebula. It is well known for being one of
IC_1396
Planet outside of the Solar System
radial-velocity observations suggested that a planet orbits the star Gamma Cephei. Partly because the observations were at the very limits of instrumental
Exoplanet
V CEPHEI
V CEPHEI
Boy/Male
Shakespearean American English German
King Henry V' Soldier in the King's army.
Boy/Male
English Shakespearean
From the Welsh Llewellyn. Famous bearer: Fluellen was a character in Shakespeare's 'Henry V'.
Boy/Male
Shakespearean
King Henry V' Duke of Bourbon.
Female
Egyptian
, the consort of Sebekhotep V.
Boy/Male
Shakespearean
King Henry V' Archbishop of Canterbury.
Boy/Male
Shakespearean English French
King Henry V' Soldier in the King's army.
Boy/Male
Shakespearean
King Henry V' Duke of Orleans.
Boy/Male
Shakespearean
King Henry V' Governor of Harfleur.
Male
Hungarian
Hungarian form of Latin Gustavus, GUSZTÃV means "meditation staff."
Boy/Male
Shakespearean
King Henry V' A French Lord.
Boy/Male
Shakespearean
King Henry V' Sir Thomas Erpingham, an officer in the King's army.
Boy/Male
Shakespearean
King Henry V' A French herald.
Boy/Male
Shakespearean
King Henry V' and 'King John' Arthur, Duke of Britaine.
Boy/Male
Hindu, Indian, Punjabi, Sikh
Meritorious; V Irtuous
Boy/Male
Shakespearean
King Henry V' A French Lord.
Boy/Male
Shakespearean
King Henry V' Earl of Cambridge, a conspirator against the King.
Boy/Male
Shakespearean
King Henry the Eighth' Ambassador from the Emperor Charles V.
Boy/Male
Shakespearean
King Henry V' Officer in the King's army.
Girl/Female
Shakespearean
King Henry V' Earl of Salisbury.
Boy/Male
Shakespearean
King Henry V' Officer in the King's army.
V CEPHEI
V CEPHEI
Male
Hebrew
(×ֵלִיָּה) Hebrew name ELIYAH means "the Lord is my God." In the bible, this is the name of several characters, including the prophet who lived during the reign of Ahab.
Surname or Lastname
English (Norfolk)
English (Norfolk) : habitational name from Mundford in Norfolk, so named from the Old English personal name Munda (from mund ‘protection’) + ford ‘ford’.
Male
Welsh
Welsh form of Irish Cailte, SCILTI means "the thin man." In Culhwch and Olwen, this was the name of a messenger of Arthur's.Â
Girl/Female
Muslim/Islamic
Beauty the planet venus
Girl/Female
Indian, Telugu
Happiness
Female
Irish
Variant spelling of Irish Béibhinn, BÉBINN means "fair lady."
Surname or Lastname
English
English : habitational name from a place in Lancashire, recorded in the early 13th century as D(e)ukesbiri, from the genitive case of the Old English personal name Deowuc or Duc(c) (both of uncertain origin) + Old English burh ‘fort’ (see Burke).
Female
Portuguese
Portuguese form of Greek Aikaterine, CATARINA means "pure."
Girl/Female
Japanese
Ball; circle.
Girl/Female
Tamil
Beautiful
V CEPHEI
V CEPHEI
V CEPHEI
V CEPHEI
V CEPHEI
v. t.
See Kittle, v. t.
v. i.
See Quob, v. i.
v. & n.
See Swoon, v. & n.
v. t.
See Leach, v. t.
v. t.
See Buttweld, v. t.
v. i.
See Poop, v. i.
v. t.
See Roust, v. t.
n. & v.
Murder, n. & v.
v. t.
See Kiddy, v. t.
v. t. & i.
See Avale, v.
v. i.
See Hollo, v. i.
v. t.
See Cob, v. t.
n. & v.
See Sward, n. & v.
v. i.
See Butt, v., and Abut, v.
v. i.
See Merrymake, v.
v. & n.
See Scent, v. & n.
v. i.
See Soul, v. i.