AI & ChatGPT searches , social queriess for 54 CASSIOPEIAE
Search references for 54 CASSIOPEIAE. Phrases containing 54 CASSIOPEIAE
See searches and references containing 54 CASSIOPEIAE!
Search references for 54 CASSIOPEIAE. Phrases containing 54 CASSIOPEIAE
See searches and references containing 54 CASSIOPEIAE!54 CASSIOPEIAE
Star in the constellation Cassiopeia
54 Cassiopeiae is a star in the northern constellation Cassiopeia. Located 88 ly (27 pc) from Earth, it has an apparent magnitude of 6.59, which makes
54_Cassiopeiae
Constellation in the northern celestial hemisphere
known, including the yellow hypergiants Rho Cassiopeiae and V509 Cassiopeiae and white hypergiant 6 Cassiopeiae. In 1572, Tycho Brahe's supernova flared
Cassiopeia_(constellation)
Sagittarius 19h 02m 36.73024s −29° 52′ 48.2279″ A2.5Va 2.59# B A3V 54 Cassiopeiae 88.12 ± 0.04 Cassiopeia 02h 09m 80.26080s +71° 33′ 07.2268″ F8V 6.587
List of star systems within 85–90 light-years
List_of_star_systems_within_85–90_light-years
Binary star system in the constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from η Cassiopeiae
Eta_Cassiopeiae
Star system in the constellation Cassiopeia
AR Cassiopeiae (AR Cas) is a variable star in the constellation of Cassiopeia. It is thought to be a member of a septuple star system, one of only two
AR_Cassiopeiae
Second-brightest star in the constellation Cassiopeia
originally γ Cassiopeiae, η Cassiopeiae, α Cassiopeiae and ζ Cassiopeiae, but were later identified as κ Cassiopeiae, η Cassiopeiae, α Cassiopeiae and λ Cassiopeiae
Beta_Cassiopeiae
Star in the constellation Cassiopeia
Kappa Cassiopeiae, also named Cexing, is a star in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from κ Cassiopeiae, and
Kappa_Cassiopeiae
B-type star in the constellation Cassiopeia
Nu Cassiopeiae is a solitary star in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ν Cassiopeiae, and
Nu_Cassiopeiae
Star in the constellation Cassiopeia
variations in its brightness, between magnitudes 5.54 and 5.59. At an age of 218 million years, 10 Cassiopeiae has expanded away from the main sequence after
10_Cassiopeiae
Binary star system
Mu Cassiopeiae is a binary star system in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from μ Cassiopeiae, and abbreviated
Mu_Cassiopeiae
Star in the constellation Cassiopeia
consisting of θ Cassiopeiae, ι Cassiopeiae, ε Cassiopeiae, δ Cassiopeiae, ν Cassiopeiae and ο Cassiopeiae. Consequently, θ Cassiopeiae itself is known
Theta_Cassiopeiae
Open star cluster in the constellation Cassiopeia
Dragonfly Cluster, E.T. Cluster, Owl Cluster, Kachina Doll Cluster or Phi Cassiopeiae Cluster. It was discovered by German-British astronomer William Herschel
NGC_457
Star in the constellation Cassiopeia
Upsilon2 Cassiopeiae is a solitary star in the constellation of Cassiopeia, a few degrees to the south of Gamma Cassiopeiae. It has the proper name Castula
Upsilon2_Cassiopeiae
Star in the constellation Cassiopeia
is a variable star. It was given its variable star designation, V863 Cassiopeiae, in 2001. The total amplitude of the variations is only 0.09 magnitudes
WR_1
Star in the constellation Perseus
match any particular orbital phase. The variations are classified as γ Cassiopeiae-type, shell stars with eruptions and irregular fading. Roman, Nancy G
Phi_Persei
K-type giant star in the constellation Cassiopeia
Tau Cassiopeiae is a solitary, orange hued star in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from τ
Tau_Cassiopeiae
Star in the constellation Cassiopeia
Upsilon1 Cassiopeiae is an astrometric binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized
Upsilon1_Cassiopeiae
Binary star system in constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ω Cassiopeiae
Omega_Cassiopeiae
Star in the constellation Cassiopeia
50 Cassiopeiae, also named Gang, is a white star in the northern constellation of Cassiopeia. In the past, it had been misidentified as a suspected nebula
50_Cassiopeiae
K0II-IIIvar Schedar β Cas β 11 432 746 00h 09m 10.09s +59° 09′ 00.8″ 2.28 1.17 54 F2III-IV Caph; δ Sct variable, Vmax = 2.25m, Vmin = 2.29m, P = 0.10 d γ Cas
List_of_stars_in_Cassiopeia
Star system in Cassiopeia
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
Variable star in the constellation Lacerta
naked eye of an observer located far from city lights. It is a Gamma Cassiopeiae variable, varying in brightness from magnitude 5.22 to 5.48, over a period
EW_Lacertae
Binary star system in the constellation Cassiopeia
49 Cassiopeiae, also named Rangifer, is a binary star system in the northern circumpolar constellation of Cassiopeia. It is visible to the naked eye as
49_Cassiopeiae
Triple star system in the constellation Eridanus
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
40_Eridani
Star in the constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from σ Cassiopeiae
Sigma_Cassiopeiae
Binary star system in the constellation Draco
rapid variations" (PDF), Acta Universitatis Carolinae, Mathematica et Physica, 21 (2): 33–54, Bibcode:1980AcMPh..21...33K, retrieved 15 February 2023.
CX_Draconis
Multiple star system in the constellation Cassiopeia
detached eclipsing binary and given the variable star designation V773 Cassiopeiae. The derived period of variability was 1.29 days, exactly half the orbital
ADS_1359
Open cluster in the constellation Cassiopeia
located almost exactly halfway between the bright stars Caph (β Cassiopeiae) and γ Cassiopeiae. It is large but not dense and can be observed by binoculars
NGC_129
(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
Triple star system in the constellation Cassiopeia
48 Cassiopeiae is a triple star system in the northern constellation of Cassiopeia. It is visible to the naked eye with a combined apparent visual magnitude
48_Cassiopeiae
Star in the constellation Cassiopeia
Chi Cassiopeiae is a solitary, yellow-hued star in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from χ Cassiopeiae, and
Chi_Cassiopeiae
Binary star in the constellation Cassiopeia
Xi Cassiopeiae is a blue-white hued binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized
Xi_Cassiopeiae
Variable star in the constellation Cassiopeia
Pi Cassiopeiae is a close binary star system in the constellation Cassiopeia, near the southern border with Andromeda. Its name is a Bayer designation
Pi_Cassiopeiae
Star in the constellation Cassiopeia
TZ Cassiopeiae (TZ Cas, HIP 117763, SAO 20912) is a variable star in the constellation Cassiopeia with an apparent magnitude of around +9 to +10. It is
TZ_Cassiopeiae
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 in the constellation Cassiopeia
Gliese 22, also catalogued V547 Cassiopeiae or ADS 440, is a hierarchical star system approximately 33 light-years (10.1 parsecs) away in the constellation
Gliese_22
Variable star in the constellation of Andromeda
component B was a close spectroscopic binary. Omicron Andromedae is a Gamma Cassiopeiae type variable star and the system's brightness varies from magnitude
Omicron_Andromedae
American astronaut (1926–1967)
(Ivan spelled backwards), is a seldom-used nickname for the star Gamma Cassiopeiae. Grissom used this name, plus two others for White and Chaffee, on his
Gus_Grissom
Star in the constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ψ Cassiopeiae
Psi_Cassiopeiae
"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
2024). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The Astrophysical Journal
List_of_largest_stars
significance is tied to the presence of a pre-main-sequence star known as V633 Cassiopeiae (or HBC 3 or LkHα 198), first identified in 1960. Its spectrum has been
Star-forming regions of Cassiopeia
Star-forming_regions_of_Cassiopeia
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
Variable star in the constellation Cassiopeia
HD 224355, also known as V1022 Cassiopeiae, HR 9059 and (in early publications) Boss 6148, is an eclipsing binary star in the constellation Cassiopeia
HD_224355
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
Binary star system in the constellation Canis Major
The magnitude 5.39 secondary, component B, is classified as a Gamma Cassiopeiae type variable star. Due to its variable nature, the brightness of the
27_Canis_Majoris
Nebula
Sh 2-185 is an H II region centered on the massive star system Gamma Cassiopeiae (γ Cas) in the northern constellation of Cassiopeia. It was included
Sh_2-185
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
Binary star system in the constellation Pisces
has a weak magnetic field with a strength of 0.4±0.2 G, and is a Gamma Cassiopeiae variable. The companion, component B, is a magnitude 7.51 star. van Leeuwen
Eta_Piscium
Type of variable star
843+43 −39 [51] T Cassiopeiae 6.9 13.0 445 374+37 −31 [52] R Pegasi 6.9 13.8 378 353+35 −29 [53] V Cassiopeiae 6.9 13.4 229 298+15 −14 [54] T Pavonis 7.0
Mira_variable
O-type main sequence star in the constellation Ophiuchus
If the star's luminosity were not obscured, it would shine at magnitude 1.54, becoming the brightest of the constellation and the twenty-third brightest
Zeta_Ophiuchi
Triple star system in the constellation Cassiopeia
(340 parsecs) from Earth. It has the variable-star designation V746 Cassiopeiae (abbreviated to V746 Cas). The system is faintly visible to the naked
HD_1976
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
Quadruple star system in the constellation Cassiopeia
under dark skies, although it lies only 21′ from the 2nd-magnitude γ Cassiopeiae and may be bound to it. The system is located approximately 540 light-years
HD_5408
Comparison of a wide range of lengths
distance between Jupiter and the Sun 785 Gm (5.25 au) – diameter of Rho Cassiopeiae, a rare yellow hypergiant star 947 Gm (6.4 au) – diameter of Antares
Orders_of_magnitude_(length)
"Authigenic clays shaped Ediacara-style exceptional fossilization". Geology. 54 (3): 210–214. doi:10.1130/G53967.1. Gougeon, R.; Mángano, M. G.; Buatois,
2025_in_paleontology
Astronomy catalogue
vdB 44 vdB 45 vdB 46 vdB 47 vdB 48 vdB 49 vdB 50 vdB 51 vdB 52 vdB 53 vdB 54 vdB 55 vdB 56 vdB 57 vdB 58 vdB 59 vdB 60 vdB 61 vdB 62 vdB 63 vdB 64 vdB
Van_den_Bergh_Catalog
Velorum Star 2.23 Gamma Cygni Star Suspected variable star 2.23 Alpha Cassiopeiae Star 2.230 Gamma Draconis Star 2.24 2.21 Alpha Coronae Borealis Binary
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
Lists_of_stars
Open cluster in the constellation Cassiopeia
was a double star on Cassiopeia's knee, about 1° northeast of Delta Cassiopeiae, sometimes called as Ruchbah or Rukhbah. Messier 103 is an easy object
Messier_103
How large a sphere or circle appears
(2024-08-05). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star $\rho$ Cassiopeiae: Convection Cells and Circumstellar Envelope". arXiv:2408.02756v2 [astro-ph
Angular_diameter
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
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
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
Open star cluster in the constellation Cassiopeia
NGC 637, and the bright magnitude +2.2 irregular variable star Gamma Cassiopeiae. The cluster is 7 arcmins across. It was discovered by William Herschel
NGC_559
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 + A/F 9.1 K0III
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
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
Supernova remnant in the constellation of Cassiopeia
Cambridge Catalogue of Radio Sources. It is located 2° northeast of ε Cassiopeiae and is estimated to be 10,000 light-years away. Its rotation period is
3C_58
Brightest star in the constellation Aquila
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
Altair
Star in the constellation Cassiopeia
star in the northern constellation of Cassiopeia, positioned near Zeta Cassiopeiae. This object has a blue-white hue and is dimly visible to the naked eye
HD_3240
List of stars with high proper motion
RM LP 40-365 "high" +498 PM; RM Luyten's Star 3.738 17.35 PM; RM Mu Cassiopeiae Al Marfik 3.777 -98 Name; PM; RM Omicron Columbae "high" PM Proxima Centauri
List of stars with large proper motion
List_of_stars_with_large_proper_motion
31m 28.99s +15° 20′ 45.0″ 3.62 −1.16 294 G8III Alpherg, Kullat-Nunu; γ Cassiopeiae variable Vmax = 3.59 m, Vmin = 3.65m γ Psc γ 6 21 219615 114971 23h 17m
List_of_stars_in_Pisces
Star that is particularly similar to the Sun
Tabetha S.; et al. (August 2008). "Angular Diameters of the G Subdwarf µ Cassiopeiae A and the K Dwarfs s Draconis and HR 511 from Interferometric Measurements
Solar_analog
54.36 ± 1.92 M4.5V WISE 1804+3117 54.4 +12.2 −8.4 T9.5 WISE 0148-7202 54.4 +19.8 −11.4 T9.5 Gliese 633 54.47 ± 0.98 M2.5V Beta Cassiopeiae (Caph)$ 54
List of star systems within 50–55 light-years
List_of_star_systems_within_50–55_light-years
Star in the constellation Cygnus
ṣadr "chest", the same word which gave rise to the star Schedar (Alpha Cassiopeiae). In 2016, the International Astronomical Union organized a Working Group
Gamma_Cygni
Open star cluster in the constellation Cassiopeia
observed by binoculars. It is located 2,5° northeast of the star Delta Cassiopeiae. In the same low power field can also be seen the open clusters NGC 663
NGC_654
Star in the constellation Cepheus
2025, and it is now so entered in the IAU Catalog of Star Names. 49 Cassiopeiae A was given the proper name Rangifer. Anderson, E.; Francis, Ch. (2012)
2_Ursae_Minoris
Star in the constellation Canis Minor
4071. Bibcode:2014ApJ...791...54G. doi:10.1088/0004-637X/791/1/54. S2CID 118744016. 54. Newton, Elisabeth R.; et al. (January 2017). "The Hα Emission
YZ_Canis_Minoris
"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
Eclipsing binary star system in the constellation of Ursa Major
1997), "Search for dust shells in W Ser binaries and similar object: RX Cassiopeiae and TX Ursae Majoris", Astronomy Letters, 23 (6): 698–703, Bibcode:1997AstL
TX_Ursae_Majoris
Open cluster in the constellation Cassiopeia
one of which is a suspected cluster member. The eclipsing binary OX Cassiopeiae was once thought to be a member, but is now known to be a background
NGC_381
Star in the constellation Camelopardalis
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
Gliese_445
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
Open cluster in the constellation Serpens
photometric observations of the selected Algol-type binaries - IV. V799 Cassiopeiae, BX Piscium and HD 172189". Monthly Notices of the Royal Astronomical
IC_4756
Planetary-mass object in the constellation Pisces
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
SIMP_J013656.5+093347
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
Navigation (PDF). Bethesda, MD: National Imagery and Mapping Agency. ISBN 0-939837-54-4. Retrieved 2016-09-20. Strasbourg Astronomical Data Center (CDS) (2010)
List_of_stars_for_navigation
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 in the constellation Carina
It is classified as a slow irregular variable whose prototype is TZ Cassiopeiae. List of largest known stars Vallenari, A.; et al. (Gaia collaboration)
V528_Carinae
Stars sorted by absolute magnitude
SIMBAD μ Normae (in NGC 6169) 339,000 -9.085 3,260 4.91 28,000 SIMBAD κ Cassiopeiae (in Cassiopeia OB14) 302,000 -8.96 4,000 4.16 23,500 SIMBAD τ Canis Majoris
List_of_most_luminous_stars
Star in the constellation Eridanus
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
82_G._Eridani
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
Mira variable (M) γ Cas (Tiansi) Cassiopeia 1m.6 3m.0 1.4 Gamma Cassiopeiae (GCAS) R Cas 4m.7 13m.5 8.9 430 d Mira variable (M) S Cas 7m
List_of_variable_stars
Open star cluster in the constellation Cassiopeia
of Cassiopeia, positioned about 1.5° to the WNW of the star Epsilon Cassiopeiae. The cluster was discovered on 9 November 1787 by German-born English
NGC_637
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 5.07 6.18 17h 15m 20
List_of_nearest_bright_stars
Red dwarf star in the constellation Cetus
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
GJ_1002
Binary star system in the Cygnus constellation
measurements, along with two other possibilities, Delta Eridani and Mu Cassiopeiae. A number of astronomers soon took up the task, including attempts by
61_Cygni
Star in the constellation Canis Major
the Hipparcos Catalogue of 1997 gives a purely notional parallax of 1.78±3.54 milliarcseconds (mas), and Gaia DR2 gives a purely notional parallax of −5
VY_Canis_Majoris
−37° 04′ 51″ M3.5 11.80 130.4186±0.0534 Mu Cassiopeiae (Gliese 53) A$ 25.033±0.084 Cassiopeia 01h 08m 16.4s +54° 55′ 13″ G5VIp 5.14# 130.2881±0.4348 B M5V
List of star systems within 25–30 light-years
List_of_star_systems_within_25–30_light-years
Open cluster in the constellation Cassiopeia
locate in the sky, being half a degree away from the bright star Kappa Cassiopeiae. However, spotting the cluster itself is difficult because of its low
NGC_146
54 CASSIOPEIAE
54 CASSIOPEIAE
Surname or Lastname
English (Shropshire)
English (Shropshire) : from the Welsh personal name Einws, a diminutive of Einion (of uncertain origin, popularly associated with einion ‘anvil’).English : patronymic from the medieval personal name Hain 2.English : habitational name from Haynes in Bedfordshire. This name first appears in Domesday Book as Hagenes, which Mills derives from the plural of Old English hægen, hagen ‘enclosure’.Irish : variant of Hines.John Haynes (?1594–1653) had emigrated from Essex, England, where his father was lord of the manor of Copford Hall near Colchester, to MA, where he was governor in 1635. He moved to CT, and was the colony's first governor (1639–53/54).
Surname or Lastname
English
English : habitational name for someone from Dunster in Somerset, recorded in 1138 as Dunestore ‘craggy pinnacle (Old English torr) of a man named Dun(n)’.Henry Dunster emigrated to MA in 1640 from Bury, Lancashire, England, and was made the first president of Harvard College (1640–54) almost immediately upon arrival in MA.
Surname or Lastname
English
English : nickname for someone with gray hair or a gray beard, from Old English græg ‘gray’. In Scotland and Ireland it has been used as a translation of various Gaelic surnames derived from riabhach ‘brindled’, ‘gray’ (see Reavey). In North America this name has assimilated names with similar meaning from other European languages.English and Scottish (of Norman origin) : habitational name from Graye in Calvados, France, named from the Gallo-Roman personal name Gratus, meaning ‘welcome’, ‘pleasing’ + the locative suffix -acum.French and Swiss French : habitational name from Gray in Haute-Saône and Le Gray in Seine-Maritime, both in France, or from Gray-la-ville in Switzerland, or a regional name from the Swiss canton of Graubünden.A leading English family called Grey, holders of the earldom of Stamford, can be traced to Henry de Grey, who was granted lands at Thurrock, Essex, by Richard I (1189–99). They once held great power, and Henry Grey, Duke of Suffolk (1517–54), married a granddaughter of Henry VII. Because of this he felt entitled to claim the throne for his daughter, Lady Jane Grey (1537–54), after the death of Henry VIII. For this, and for his part in Wyatt’s rebellion, both he and his daughter were beheaded.
Surname or Lastname
English (Devon)
English (Devon) : topographic name for someone who lived ‘at the end of the cottages’, from Middle English, Old English ende ‘end’ + cot ‘cottage’. One locality so named is Endicott in Cadbury, Devon; another is now called Youngcott, in Milton Abbot.John Endecott (1588–1665) was a prominent figure in the early history of MA, being one of the founding fathers of Salem, MA, in 1638. He served as governor of Massachusetts Bay Colony (1629–30), and worked harmoniously with his successor, John Winthrop, despite differences on points of religious doctrine. He served as governor again in 1644–45, 1649–50, 1651–54, and 1655–64, and as deputy governor in many of the intervening years. He is buried in the King’s Chapel Burying Ground in Boston.
Female
Welsh
Welsh form of French Guinevere, the Arthurian legend name of Gwenhwyvach's sister, possibly composed of the elements gwen "fair, holy, white" and hwyfar "smooth, soft,"Â hence "white and smooth." There are other possibilities. It may come from Proto-Celtic *vindo-siabraid, GWENGWYVAR means "white phantom." Or, the names of the sisters may mean "Gwenhwy the Great" (Gwenhwy-vawr) and "Gwenhwy the Less" (Gwenhwy-vach). Gwenhwyvach and Gwenhwyvar did not get along well together; Triad 84 of the Culhwch states that the Battle of Camlann was caused by the enmity between the two sisters. Triad 53 lists the slap that Gwenhwyvach gave Gwenhwyvar as one of the "Three Harmful Blows of the Island of Britain." And Triad 54 describes how Mordred raided Arthur's court and threw Gwenhwyvar to the ground and beat her.Â
54 CASSIOPEIAE
54 CASSIOPEIAE
Boy/Male
Hindu, Indian, Marathi
Strong; Robust
Boy/Male
Muslim
One of the main angels of Allah
Boy/Male
Hindu, Indian, Marathi
Sun; Moon
Boy/Male
Hindu
Lord Krishna, Beloved of Radha
Girl/Female
Celtic
A mythical queen.
Female
English
English name derived from the Taino word zabana, SAVANNAH means "savannah."
Boy/Male
Indian
Wealth and Success
Female
English
Variant spelling of English Gena, JENA means "well born."
Girl/Female
American, British, Christian, English, Hebrew, Latin
Beautiful Seacoast; Light; Golden; Prayerful; Breeze
Boy/Male
Hindu
Peace
54 CASSIOPEIAE
54 CASSIOPEIAE
54 CASSIOPEIAE
54 CASSIOPEIAE
54 CASSIOPEIAE