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Star in the constellation Cassiopeia
4 Cassiopeiae is a red giant in the northern constellation of Cassiopeia, located approximately 790 light-years away from the Sun. It is visible to the
4_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)
Star system in the constellation Cassiopeia
Gamma Cassiopeiae, Latinized from γ Cassiopeiae formally named Tiansi, is a multiple star system at the center of the distinctive "W" asterism in the
Gamma_Cassiopeiae
Yellow hypergiant star in the constellation Cassiopeia
Rho Cassiopeiae is a yellow hypergiant star in the constellation Cassiopeia. Its name is a Bayer designation, pronounced /ˌroʊ kæsiəˈpiːaɪ, -sioʊ-, -iː/
Rho_Cassiopeiae
Star in constellation of Cassiopeia
from δ Cassiopeiae, and abbreviated Delta Cas or δ Cas. Based on parallax measurements taken during the Hipparcos mission, it is approximately 99.4 light-years
Delta_Cassiopeiae
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
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
Star in the constellation Cassiopeia
Alpha Cassiopeiae is a star in the northern constellation of Cassiopeia. It has the proper name Schedar, pronounced /ˈʃɛdɑːr/); Alpha Cassiopeiae is its
Alpha_Cassiopeiae
Red supergiant star in the constellation Cassiopeia
V762 Cassiopeiae is a star in the constellation of Cassiopeia. Its apparent magnitude vary between 5.82 and 5.95, which makes it faintly visible to the
V762_Cassiopeiae
Star in the constellation Cassiopeia
designation, which is Latinized from ε Cassiopeiae and abbreviated Epsilon Cas or ε Cas. With an apparent visual magnitude of 3.4, this is one of the brightest
Epsilon_Cassiopeiae
Star in the constellation Cassiopeia
Zeta Cassiopeiae is a variable star in the constellation of Cassiopeia. It has the proper name Fulu, pronounced /ˈfuːluː/; Zeta Cassiopeiae is its Bayer
Zeta_Cassiopeiae
Star in the constellation Cassiopeia
Omicron Cassiopeiae is a triple star system in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from ο Cassiopeiae, and abbreviated
Omicron_Cassiopeiae
Star in the constellation Cassiopeia
12 Cassiopeiae (12 Cas) is a white giant in the constellation Cassiopeia, about 860 light years away. It has an apparent magnitude of 5.4, so it faintly
12_Cassiopeiae
Star in the constellation Cassiopeia
S Cassiopeiae (S Cas, HD 7769) is a Mira variable and S-type star in the constellation Cassiopeia. It is an unusually cool star, rapidly losing mass and
S_Cassiopeiae
Star in the constellation Cassiopeia
designation that is Latinized from φ Cassiopeiae, and abbreviated Phi Cas or φ Cas. With a combined apparent magnitude of +4.95, it is visible to the naked
Phi_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
Supernova in the constellation Cassiopeia
SN 1572 (also Tycho's Star, Tycho's Nova, or Tycho's Supernova), or B Cassiopeiae (B Cas), was a supernova of Type Ia in the constellation Cassiopeia,
SN_1572
Supernova remnant in the constellation Cassiopeia
although it is possible that it was recorded as a sixth magnitude star 3 Cassiopeiae by John Flamsteed in 1680. Possible explanations lean toward the idea
Cassiopeia_A
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
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
HR 511 (also designated V987 Cassiopeiae and Gliese 75 among others) is an orange dwarf of spectral type K0V in the constellation Cassiopeia. With an
HR_511
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
Triple star system in the constellation Andromeda
α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae,
Psi_Andromedae
Star in the constellation Cassiopeia
10 Cassiopeiae (10 Cas) is a blue-white giant star in the constellation Cassiopeia, about 960 light years away. 10 Cassiopeiae is a B9 giant star. It
10_Cassiopeiae
Star in the constellation Circinus
visual magnitude, mass, and classification. The system behaves as a Gamma Cassiopeiae variable showing occasional outbursts of up to 0.27 in magnitude. "Hipparcos
Theta_Circini
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
K-type giant star in the constellation Cassiopeia
τ Cassiopeiae, and abbreviated Tau Cas or τ Cas. This star is bright enough to be seen with the naked eye, having an apparent visual magnitude of +4.86
Tau_Cassiopeiae
Star in the constellation Cassiopeia
consisting of σ Cassiopeiae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae
Sigma_Cassiopeiae
Star in the constellation Cassiopeia
R Cassiopeiae is a variable star in the northern constellation of Cassiopeia. It is located approximately 570 light years distant from the Sun, but is
R_Cassiopeiae
Variable star in the constellation Canis Major
observer far from city lights. It is a Gamma Cassiopeiae variable star, whose brightness varies from magnitude 4.8 to 6.25. In 1967, Alejandro Feinstein detected
FY_Canis_Majoris
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
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
Star in the constellation Cassiopeia
V509 Cassiopeiae (V509 Cas or HR 8752) is one of two yellow hypergiant stars found in the constellation Cassiopeia, which also contains Rho Cassiopeiae. HR
V509_Cassiopeiae
Topics referred to by the same term
engineer Cè, a Chinese star name which can refer to either: Gamma Cassiopeiae Kappa Cassiopeiae Copy editing, improving the formatting, style, and accuracy
CE
Star in the constellation Ophiuchus
~20°. It is a Gamma Cassiopeiae variable with an amplitude of 0.15 magnitude. The brightness has been measured varying from magnitude 4.18 down to 5.0. Chi Ophiuchi
Chi_Ophiuchi
Star in the constellation Pavo
a gas disk around it. It is a γ Cassiopeiae variable or shell star which has occasionally brightened to magnitude 4.0. The stellar classification of
Lambda_Pavonis
Variable star in the constellation Cassiopeiae
that is Latinized from ι Cassiopeiae, and abbreviated Iota Cas or ι Cas. The system has a combined apparent magnitude of about 4.5, making it visible to
Iota_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
Star system in the Centaurus constellation
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
Alpha_Centauri
Star in the constellation Cassiopeia
strong radio variability. It was given the variable star designation V615 Cassiopeiae. LS I +61 303 emits HE and VHE (High Energy and Very High Energy) gamma
LS_I_+61_303
Star in the constellation Canis Minor
been suspected of variability, and in 1977 it was classified as a γ Cassiopeiae variable in the General Catalogue of Variable Stars. A number of studies
Beta_Canis_Minoris
Star in the constellation Cassiopeia
Latinized from υ1 Cassiopeiae, and abbreviated Upsilon1 Cas or υ1 Cas. This system visible to the naked eye with an apparent visual magnitude of 4.82. Based upon
Upsilon1_Cassiopeiae
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
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
Star in the constellation Apus
Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to +5.61. This is a runaway star with a peculiar velocity of 69.8±4.7 km/s
Kappa1_Apodis
Star in the constellation Cassiopeia
PZ Cassiopeiae is a red supergiant or hypergiant star located in the constellation of Cassiopeia, and a semi-regular variable star. PZ Cassiopeiae is
PZ_Cassiopeiae
Star system in the constellation Cassiopeia
AO Cassiopeiae, also known as Pearce's Star, is a binary system composed of an O8 main sequence star and an O9.2 bright giant that respectively weigh
AO_Cassiopeiae
Star in the constellation Cassiopeia
WZ Cassiopeiae (WZ Cas) is a deep red hued star in the northern constellation of Cassiopeia. It is a variable star with a magnitude that ranges from 6
WZ_Cassiopeiae
Binary star system in the constellation Scorpius
space anywhere in the main ring system." Delta Scorpii A is a Gamma Cassiopeiae variable star. This type of star shows irregular slow brightness variations
Delta_Scorpii
+62° 55′ 54.4″ 4.17 −6.34 4127 B1Ia Cexing, α Cyg variable, Vmax = 4.12m, Vmin = 4.21m, P = 2.65 d θ Cas θ 33 6961 5542 01h 11m 05.93s +55° 08′ 59.8″ 4.34 1
List_of_stars_in_Cassiopeia
Triple star system in the constellation Eridanus
named Keid, is easily visible to the naked eye, with an apparent magnitude of 4.43. It is orbited by a binary pair whose two components are designated 40
40_Eridani
planet) approved on 1 March 2020. An additional two star names were approved on 4 April 2022. In June 2023, an additional 20 names were approved in the NameExoWorlds
List_of_proper_names_of_stars
Star system in the constellation Cassiopeia
Adams. It is a double-lined spectroscopic binary with an orbital period of 13.4 days and an eccentricity of 0.13. The system was found to be variable in 1958
V373_Cassiopeiae
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
Star in the constellation Cepheus
Cephei, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae
Epsilon_Cephei
Nova seen in 1993
V705 Cassiopeiae, also known as Nova Cassiopeiae 1993 was a nova which erupted in the constellation Cassiopeia during 1993. The nova was discovered at
V705_Cassiopeiae
Binary star system in the constellation Centaurus
classified as a suspected Gamma Cassiopeiae type variable star with a visual magnitude varying from +4.30 down to +4.39. Anderson, E.; Francis, Ch. (2012)
HD_102776
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
186000 9.23 6 Cassiopeiae 8000 A2.5Ia+ 193 22.0 200000 5.34-5.45 Rho Cassiopeiae 8150±1630 G2 0 (F8pIa-K0pIa-0) 700 40 300000 – 530000 4.1 to 6.2 BP Crucis
List_of_nearest_hypergiants
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
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
Star in the constellation Camelopardalis
Samus et al. (2017) classify it as a Be variable, rather than a Gamma Cassiopeiae type, and it ranges from a peak Hipparcos magnitude of 5.10 down to 5
11_Camelopardalis
Star in the constellation Cassiopeia
1 Cassiopeiae is a single star in the northern constellation of Cassiopeia, located around 1,130 light years from the Sun. It is visible to the naked
1_Cassiopeiae
2024). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The Astrophysical Journal
List_of_largest_stars
Planned United States spaceflight (1967)
after themselves and introduced them into NASA documentation. Gamma Cassiopeiae became Navi – Ivan (Gus Grissom's middle name) spelled backwards. Iota
Apollo_1
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
dwarfs, as well as 4 sub-brown dwarfs. The closest system is Alpha Centauri, with Proxima Centauri as the closest star in that system, at 4.2465 light-years
List_of_nearest_stars
Star in the constellation Lacerta
α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae,
Alpha_Lacertae
Binary star system in the constellation Canis Major
classified as a Gamma Cassiopeiae type variable star. Due to its variable nature, the brightness of the system varies from magnitude +4.42 to +4.82. van Leeuwen
27_Canis_Majoris
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
log 10 ( 10 − 0.4 ⋅ 1.81 + 10 − 0.4 ⋅ 4.173 ) {\displaystyle 1.69\approx -2.5\log _{10}\left(10^{-0.4\cdot 1.81}+10^{-0.4\cdot 4.173}\right)} Combined
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
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
Variable star in the constellation Perseus
surrounded by a disk of expelled material. This qualifies it as a Gamma Cassiopeiae variable, and the visual range is magnitude 6 - 7. In 1989 and 1990,
X_Persei
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 of Andromeda
α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae,
Kappa_Andromedae
Triple star system in the constellation Cassiopeia
YZ Cassiopeiae (21 Cas) is a star system 103.8 parsecs (339 ly) away from Earth, in the constellation Cassiopeia. It comprises three stars: an eclipsing
YZ_Cassiopeiae
Comparison of a wide range of lengths
(5.25 au) – diameter of Rho Cassiopeiae, a rare yellow hypergiant star 947 Gm (6.4 au) – diameter of Antares A 965 Gm (6.4 au) – maximum distance between
Orders_of_magnitude_(length)
Star in the constellation Canis Major
the Southern Hemisphere, Omega Canis Majoris is classified as a Gamma Cassiopeiae-type variable star. Both the luminosity and the radial velocity vary
Omega_Canis_Majoris
Star in the constellation of Andromeda
α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae,
Iota_Andromedae
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
Star in the constellation Sagittarius
designation, V4024 Sagittarri, in 1978. It is classified as an eruptive Gamma Cassiopeiae variable and has been measured ranging in brightness from visual magnitude
V4024_Sagittarii
Star in the constellation Cassiopeia
Cassiopeia. Visually, it is located 106 arcminutes north of the bright star γ Cassiopeiae. With an apparent visual magnitude of 9.56, it is not observable with
Gliese_49
Variable star in the constellation Centaurus
experience transient periodicities. Mu Centauri is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +2.92 to
Mu_Centauri
Star whose brightness fluctuates, as seen from Earth
Cassiopeiae (γ Cas) variables are non-supergiant fast-rotating B class emission line-type stars that fluctuate irregularly by up to 1.5 magnitudes (4
Variable_star
Binary star system in the constellation Pisces
G7 IIIa. It 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
Eta_Piscium
Zodiac constellation in the southern celestial hemisphere
maximum magnitude is 4.9. FX Librae, designated 48 Librae, is a shell star of magnitude 4.9. Shell stars, like Pleione and Gamma Cassiopeiae, are stars with
Libra_(constellation)
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
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
Classification of stars based on spectral properties
Bibcode:1981A&AS...46..193H. – Luminosities are derived from Mbol figures, using Mbol(☉)=4.75. Weidner, Carsten; Vink, Jorick S. (December 2010). "The masses, and the
Stellar_classification
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
Figure on a compass, map, nautical chart
allowing bearings to be given such as "two points off the starboard bow". A 4-point compass rose An 8-point compass rose A 16-point compass rose A 32-point
Compass_rose
Star in the constellation Crux
(2017) have tentatively classified it as a Gamma Cassiopeiae variable with a brightness range of 4.88–5.7 mag in the Johnson B band. CH Crucis has 5
CH_Crucis
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
Constellation in the southern celestial hemisphere
each other as viewed from Earth, they are unrelated. Kappa is a Gamma Cassiopeiae variable of spectral type B2Vne, which brightened by 50% between 1963
Canis_Major
Star in the constellation Canis Major
the star. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +3.4 to +3.97. The star became 50% brighter
Kappa_Canis_Majoris
4 CASSIOPEIAE
4 CASSIOPEIAE
Surname or Lastname
English (mainly Yorkshire)
English (mainly Yorkshire) : patronymic from Seller 1–4.
Surname or Lastname
English
English : variant spelling of Ray 1–4.
Surname or Lastname
English
English : variant of Lyon 3.Irish : variant of Lyon 4.
Surname or Lastname
English
English : variant of Hearn 4. This is predominantly a MD name.
Surname or Lastname
English
English : variant of Hearn 4.
Female
Japanese
(1-亮, 2-é¼, 3-è«’, 4-涼) Japanese unisex name RYO means 1) "brightness," 2) "distant," 3) "reality," 4) "refreshing."
Surname or Lastname
English
English : patronymic from Seal 4.
Female
Japanese
(1-æ, 2- 京, 3- å”, 4- 郷) Variant spelling of Japanese unisex Kyou, KYO means 1) "apricot," 2) "capital," 3) "cooperation," or 4) "village."Â
Surname or Lastname
English
English : variant of Hearn 2 and 4.
Female
Japanese
(1-æ, 2- 京, 3- å”, 4- 郷) Japanese unisex name KYOU means 1) "apricot," 2) "capital," 3) "cooperation," or 4) "village."Â
Boy/Male
Sikh
Who is always victorious, Winner from 4 directions, Perfectly victorious
Female
Japanese
(1-儀, 2-典, 3-則, 4-法) Japanese unisex name NORI means 1) "ceremony, regalia," 2) "code, precedent," 3) "model, rule, standard," 4) "law, rule."
Surname or Lastname
English and Welsh
English and Welsh : variant of Bach 3 and 4.
Surname or Lastname
English
English : patronymic from Seal 4.
Surname or Lastname
English
English : variant spelling of Rock.German (Röcke) : variant of Rock 4.
Boy/Male
Sikh
Who is always victorious, Winner from 4 directions, Perfectly victorious
Surname or Lastname
English
English : variant spelling of Hearn 4.
Surname or Lastname
English
English : variant spelling of Kay 4 and 5.
Surname or Lastname
English
English : variant of Cave 1 or 4.
Female
Japanese
(1-鈴, 2-零, 3-麗, 4-霊) Japanese name REI means 1) "bell," 2) "nothing, zero" or 3) "lovely," 4) "spirit."
4 CASSIOPEIAE
4 CASSIOPEIAE
Girl/Female
Hindu, Indian, Marathi
Content; Satisfaction
Boy/Male
Hindu
Morality, Superior
Boy/Male
Danish, German, Swedish
God is Good
Female
Italian
Italian form of Hebrew No'omiy, NOEMI means "my delight, my pleasantness."
Girl/Female
Hindu, Indian, Malayalam
Beautiful
Boy/Male
French Latin
To rise again.
Boy/Male
German
From the Linden Tree Mountain
Girl/Female
Tamil
Smiling
Girl/Female
Indian
A lamp
Male
Ukrainian
, a stone.
4 CASSIOPEIAE
4 CASSIOPEIAE
4 CASSIOPEIAE
4 CASSIOPEIAE
4 CASSIOPEIAE
n.
See Tierce, 4.
n.
See Flyer, n., 4.
n.
See Slime, 4.
n.
See Gad, n., 4.
n.
Same as Presbytery, 4.
n.
See Umber, 4.
n.
See Waft, n., 4.
n.
Same as Wale, n., 4.
n.
See Galley, n., 4.
n.
See Rose, n., 4.
n.
See Grit, n., 4.
n.
Offset, n., 4.
n.
Same as Cribbing, 4.
n.
Same as Tailing, 4.
n.
See Assessment, 4.
n.
See 1st Hag, 4.
p. p. & a.
Same as Relative, 4.
n.
See Mule, 4.
n.
Same as Indentation, 4.
n.
Sympathy. See Sympathy, 4.