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Star in the constellation Cepheus
Kappa 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
Cause of changes in luminosity in pulsating variable stars
The kappa opacity mechanism is the driving mechanism behind the changes in luminosity of many types of pulsating variable stars. The term Eddington valve
Kappa–mechanism
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
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
List of star systems within 300–350 light-years
List_of_star_systems_within_300–350_light-years
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 Scorpius
Kappa Scorpii, Latinized from κ Scorpii, is a binary star system in the southern constellation of Scorpius. With an apparent visual magnitude of 2.4,
Kappa_Scorpii
Study of oscillations in stars
excited by the kappa mechanism. Beta Cephei variables are slightly hotter (and thus more massive), also have modes excited by the kappa mechanism and additionally
Asteroseismology
Type of variable star that pulsates radially
Beta Doradus, RT Aurigae, Polaris, as well as Delta Cephei. Type II Cepheids include: W Virginis, Kappa Pavonis and BL Herculis. Anomalous Cepheids include:
Cepheid_variable
Star in the constellation of Andromeda
Kappa Andromedae, Latinized from κ Andromedae, also named Kaffalmusalsala, is a star in the northern constellation of Andromeda. It is visible to the
Kappa_Andromedae
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
Open cluster in the constellation Crux
The Jewel Box (also known as the Kappa Crucis cluster, NGC 4755, or Caldwell 94) is an open cluster in the constellation Crux, originally discovered by
Jewel_Box_(star_cluster)
Non-periodic comet
it was a magnitude 8.0 object about 3 degrees southeast of the star Kappa Cephei. The subsequent two nights were clear, which helped Candy and G. E. Taylor
C/1960_Y1_(Candy)
Puppis by Lacaille, reassigned to Carina as A Carinae by Gould Upsilon Cephei was designated to the star HR 7955 that appeared in Burritt's star atlas
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
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
Variable binary star system in the constellation Centaurus
Kappa Centauri is a triple star system in the southern constellation of Centaurus. Its name is a Bayer designation that is Latinized from κ Centauri,
Kappa_Centauri
system 2.45 2.38 Eta Canis Majoris Star 2.46 Alpha Cephei Star Suspected variable star 2.473 Kappa Velorum Binary star system 2.48 Alpha Pegasi Star 2
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
American astronomer (1868–1921)
radiated by the star in the visible spectrum). Henrietta found that Delta Cephei was the "standard candle" that had long been sought by astronomers. A similar
Henrietta_Swan_Leavitt
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
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
(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
Cambridge University Press. p. 170. ISBN 0-521-44921-9. Kaler, James B. "Saiph (Kappa Orionis)". Stars. University of Illinois. Archived from the original on
List_of_proper_names_of_stars
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)
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
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
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
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
Astrophysical limit on radiation from stars
{\displaystyle L={\frac {c}{\kappa }}\int _{S}\nabla \Phi \cdot dS={\frac {c}{\kappa }}\int _{V}\nabla ^{2}\Phi \,dV={\frac {4\pi Gc}{\kappa }}\int _{V}\rho \,dV={\frac
Eddington_luminosity
Series of disputed celestial events (1977)
Gamma Cephei, Psi Draconis, 16 Draconis, Psi Herculis, Kappa Coronae Borealis and Delta Coronae Borealis. The object stopped near Gamma Cephei at an azimuth
Petrozavodsk_phenomenon
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
Star in the constellation Orion
amplitude. This star has unusual variable spectral lines and lies with the β Cephei variable instability strip. However, it is now thought that the variable
Eta_Orionis
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
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
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
Star in the constellation of Draco
Forbidden Enclosure, refers to an asterism consisting of Alpha Draconis, Kappa Draconis, Lambda Draconis, 24 Ursae Majoris, 43 Camelopardalis, Alpha Camelopardalis
Thuban
J2339–0424 291 ± 2 DABZ Alpha Vulpeculae (Anser) 291 ± 3 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
List of star systems within 250–300 light-years
List_of_star_systems_within_250–300_light-years
Constellation in the northern celestial hemisphere
stars. Markab has an apparent magnitude of 2.48, while Algenib is a Beta Cephei variable that varies between magnitudes 2.82 and 2.86 every 3 hours 38 minutes
Pegasus_(constellation)
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)
Type of eruptive variable star
5m.50 0.50 Zeta Ophiuchi 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
Gamma_Cassiopeiae_variable
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
also known as 2M1207b. Iota Aquarii 211 ± 3 Aquarius B8 V 4.279 Omicron Cephei A 211 ± 7 Cepheus G8III 4.86+7.13 B F6V Gamma Gruis (Aldhanab) 211 ± 9 Grus
List of star systems within 200–250 light-years
List_of_star_systems_within_200–250_light-years
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 Mu
List_of_O-type_stars
(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
Constellation in the southern celestial hemisphere
M, Morel T, Ilyin I (April 2009). "New magnetic field measurements of β Cephei stars and slowly pulsating B stars". Astronomische Nachrichten. 330 (4):
Telescopium
(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
Subclass of pulsating star
to the swelling and shrinking of the star through the Eddington Valve or Kappa-mechanism. The stars have a helium rich atmosphere. As helium is compressed
Delta_Scuti_variable
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)
; 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
Astronomical phenomena viewed from the planet Mars
celestial pole of Mars. The pole is about halfway between Deneb and Alpha Cephei, less than 10° from the former, a bit more than the apparent distance between
Astronomy_on_Mars
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)
1.91 4970 FU Tauri b 16.0 800 2375 imaging 2008 456.63 0.05 2838 Gamma Cephei Ab 1.85 903.3 2.05 radial vel. 2003 44.16 1.4 4744 Proper name Tadmor Gamma
List of exoplanets discovered between 2000–2009
List_of_exoplanets_discovered_between_2000–2009
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
Extraterrestrial view of outer space
Cephei; it is more accurate to state that the top two stars of the Northern Cross, Sadr and Deneb, point to the north Celestial pole of Mars. Kappa Velorum
Extraterrestrial_sky
Fluctuations in stellar radius
{\begin{aligned}{\frac {dA_{1}}{dt}}&=\kappa _{1}A_{1}+\left(Q_{11}A_{1}^{2}+Q_{12}A_{2}^{2}\right)A_{1}\\[1ex]{\frac {dA_{2}}{dt}}&=\kappa _{2}A_{2}+\left(Q_{21}A_
Stellar_pulsation
KAPPA CEPHEI
KAPPA CEPHEI
Girl/Female
Gujarati, Hindu, Indian
Thought; Able; Fit
Boy/Male
Tamil
Attitude
Boy/Male
Indian, Sanskrit
Universal Father
Boy/Male
Hindu, Indian, Tamil, Telugu
Of Vishnu and Shiva; Ayya means Vishnu and Appa means Shiva
Boy/Male
Hindu, Indian, Kannada, Marathi, Sanskrit, Telugu
Able; Fit
Surname or Lastname
English
English : unexplained; perhaps from either of two medicinal and edible plants commonly known by this name (Arctium lappa and A. minus). However, the word is not recorded in OED before 1597, rather too late for surname formation.
Girl/Female
Hindu, Indian
Father; Daddy
Boy/Male
Tamil
Able, Fit
Girl/Female
Gujarati, Indian
Meaningful
Surname or Lastname
English
English : topographic name for someone who lived by a maple tree, Middle English mapel (Old English mapul).French : from Latin mapula, a diminutive of mappa ‘piece of cloth’, ‘napkin’, presumably a metonymic occupational name for a cloth merchant or a weaver.
Surname or Lastname
English
English : from Middle English cappe ‘cap’, ‘hat’ (Old English cæppe), hence a metonymic occupational name for a maker of caps and hats, or a nickname for someone who wore distinctive headgear. Compare Capper.Americanized spelling of German Kapp.
Surname or Lastname
English
English : variant spelling of Chappell.French : from a diminutive of Old French chape ‘hooded cloak’, ‘cape’, ‘hood’, or ‘hat’ (from Late Latin cappa, capa), hence a metonymic occupational name for a maker of cloaks or hats, or a nickname for a habitual wearer of a distinctive cloak or hat.
Boy/Male
Hindu, Indian
Attitude
KAPPA CEPHEI
KAPPA CEPHEI
Girl/Female
Hindu, Indian
Princess of Heart
Girl/Female
Gujarati, Hindu, Indian, Kannada, Marathi, Sindhi, Tamil, Telugu
Fish-like Beautiful Eyes
Girl/Female
American, Anglo, Australian, British, Christian, English, Hindu, Indian
Chalk Port; Landing Place; Port
Female
English
English occupational surname for a "dyer" or "seller of fabrics," transferred to forename use, derived from Old French escarlate, SCARLETT means "scarlet cloth."Â
Boy/Male
Tamil
Prathamesh | பà¯à®°à®¤à®®à¯‡à®·
Lord God, Lord Ganesh, Lord of the best
Boy/Male
Hindu, Indian
Man with Long-life
Girl/Female
Indian, Sanskrit
Wish
Girl/Female
Tamil
Samanvita | ஸமாஂநà¯à®µà®¿à®¤à®¾
Name of Goddess Durga
Boy/Male
Muslim/Islamic
Slave of the Self-Subsistent
Biblical
shaken or beaten by the waves
KAPPA CEPHEI
KAPPA CEPHEI
KAPPA CEPHEI
KAPPA CEPHEI
KAPPA CEPHEI
n.
A genus of coarse biennial herbs (Lappa), bearing small burs which adhere tenaciously to clothes, or to the fur or wool of animals.
n.
The fossil resin of the kauri tree of New Zealand.
n.
A kind of cloth prepared by the Polynesians from the inner bark of the paper mulberry; -- sometimes called also kapa.
n.
One of the Brahmanic eons, a period of 4,320,000,000 years. At the end of each Kalpa the world is annihilated.