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Star in the constellation Perseus
5 Persei is a star in the northern constellation of Perseus located around 2,950 parsecs (9,600 ly) away from the Sun. It is part of the Perseus OB1 stellar
5_Persei
Brightest star in the constellation Perseus
consisting of α Persei, γ Persei, δ Persei, η Persei, μ Persei, ψ Persei, 48 Persei and HD 27084. Consequently, the Chinese name for α Persei itself is 天船三
Alpha_Persei
Eclipsing variable star in the constellation Perseus
Algol /ˈælɡɒl/, designated Beta Persei (β Persei, abbreviated Beta Per, β Per), known colloquially as the Demon Star, is a bright multiple star in the
Algol
Constellation in the northern celestial hemisphere
members of an open cluster known as the Alpha Persei Cluster. The best-known star, however, is Algol (Beta Persei), linked with ominous legends because of
Perseus_(constellation)
Open cluster in the constellation Perseus
The Alpha Persei Cluster, also known as Melotte 20 or Collinder 39, is an open cluster of stars in the northern constellation of Perseus. To the naked
Alpha_Persei_Cluster
Hot, luminous star with a spectral type of A9 or earlier
Orionis B-type supergiant, spectral type B2Ia 5 Persei, B-type supergiant, spectral type B5Ia 10 Persei, B-type supergiant, spectral type B2Ia Omicron²
Blue_supergiant
Triple star system in the constellation Perseus
Omicron Persei (ο Persei, abbreviated Omicron Per, ο Per) is a triple star system in the constellation of Perseus. From parallax measurements taken during
Omicron_Persei
Star in the constellation Perseus
GK Persei (also Nova Persei 1901) was a bright nova first observed on Earth in 1901. It was discovered by Thomas David Anderson, an Edinburgh clergyman
GK_Persei
Star system in the constellation Perseus
Epsilon Persei, Latinized from ε Persei, formally named Áldu, is a Triple star system kin the northern constellation of Perseus. It has a combined apparent
Epsilon_Persei
Star in the constellation Perseus
consisting of δ Persei, η Persei, α Persei, γ Persei, ψ Persei, 48 Persei, μ Persei and HD 27084. Consequently, the Chinese name for δ Persei itself is 天船五
Delta_Persei
Class of eclipsing binary stars
stars that are similar to the prototype member of this class, β Persei (Beta Persei, Algol). An Algol binary is a system where both stars are near-spherical
Algol_variable
Star in the constellation Perseus
S Persei is a red supergiant or hypergiant located near the Double Cluster in Perseus, north of the cluster NGC 869. It is a member of the Perseus OB1
S_Persei
Star in the constellation Perseus
48 Persei (also known as c Persei, 48 Per, HR 1273, HIP 19343, or HD 25940) is a Be star in the constellation Perseus, approximately the 500th brightest
48_Persei
Star system in the constellation Perseus
Eta Persei, Gamma Persei, Alpha Persei, Psi Persei, Delta Persei, 48 Persei, Mu Persei and HD 27084. Consequently, the Chinese name for Eta Persei itself
Eta_Persei
Star in the constellation Perseus
consisting of ψ Persei, η Persei, α Persei, γ Persei, δ Persei, 48 Persei, μ Persei and HD 27084. Consequently, the Chinese name for ψ Persei itself is 天船四
Psi_Persei
Subclass of R Coronae Borealis variables
DY Persei variables are a subclass of R Coronae Borealis (R CrB) variables. They are carbon-rich asymptotic giant branch (AGB) stars that exhibit pulsational
DY_Persei_variable
Star in the constellation Perseus
consisting of Xi Persei, Nu Persei, Epsilon Persei, Zeta Persei, Omicron Persei and 40 Persei. Consequently, the Chinese name for Xi Persei itself is 卷舌三
Xi_Persei
Variable star in the constellation Perseus
X Persei is a high-mass X-ray binary system located in the constellation Perseus, approximately 950 parsecs away. It is catalogued as 4U 0352+309 in the
X_Persei
Star in the constellation Perseus
consisting of ρ Persei, 9 Persei, τ Persei, ι Persei, κ Persei, β Persei, 16 Persei and 12 Persei. Consequently, the Chinese name for ρ Persei itself is 大陵六
Rho_Persei
Star in the constellation Perseus
Persei, 9 Persei, Tau Persei, Iota Persei, Beta Persei (Algol), Rho Persei, 16 Persei and 12 Persei. Consequently, the Chinese name for Kappa Persei itself
Kappa_Persei
Star in the constellation Perseus
Persei is a binary star system in the northern constellation Perseus. It is faintly visible to the naked eye with an apparent visual magnitude of 5.49
30_Persei
Star in the constellation Perseus
Phi Persei, Latinized from (Phi Per, φ Persei, φ Per) formally named Dajiangjunbei, is a class B2Vep fourth-magnitude star in the constellation Perseus
Phi_Persei
Star system in the constellation Perseus
RT Persei is a variable star system in the northern constellation of Perseus, abbreviated RT Per. It is an eclipsing binary system with an orbital period
RT_Persei
Chemical compound of hydrogen and oxygen
well as TW Hydrae, IRC +10216 and APM 08279+5255, VY Canis Majoris and S Persei. Liquid water is present on Earth, covering 71% of its surface. Liquid water
Water
Star in the constellation Perseus
31 Persei is a single star in the northern constellation of Perseus. It is visible to the naked eye as a dim, blue-white hued point of light with an apparent
31_Persei
Blue supergiant star in the constellation Perseus
9 Persei is a single variable star in the northern constellation Perseus, located around 4,300 light years away from the Sun. It has the Bayer designation
9_Persei
Yellow-white hued star in the constellation Perseus
ν Persei, Latinized as Nu Persei, is a single star and a suspected variable in the northern constellation of Perseus. It has a yellow-white hue and is
Nu_Persei
Red Supergiant star in the constellation Perseus
PR Persei (also known as HD 14404, HIP 10995, or BD+57 550) is a red supergiant star located in the constellation of Perseus in the northern celestial
PR_Persei
Star in the constellation Perseus
29 Persei is a single star in the northern constellation of Perseus, located approximately 640 light-years away from the Sun based on parallax. It is visible
29_Persei
Star in the constellation Perseus
SU Persei is a red supergiant star located in the constellation of Perseus. It is located within the Double Cluster, 7,250+470 −420 light-years away. It
SU_Persei
Binary star system in the constellation Perseus
34 Persei is a binary star system in the northern constellation of Perseus. It is visible to the naked eye as a faint, blue-white hued point of light with
34_Persei
Type of eruptive variable star
Goraya, P. S. (April 1988). "Scanner observations of shell stars Phi Persei and Psi Persei". Astrophysics and Space Science. 143 (1): 99–105. Bibcode:1988Ap&SS
Gamma_Cassiopeiae_variable
Type of star
A slowly pulsating B-type star (SPB), formerly known as a 53 Persei variable, is a type of pulsating variable star. They may also be termed a long-period
Slowly_pulsating_B-type_star
Star system in the constellation Perseus
RW Persei is a eclipsing binary star system in the northern constellation of Perseus. It has a peak apparent visual magnitude of 9.68, so this system is
RW_Persei
Star in the constellation Perseus
2 Persei is a binary star system in the northern constellation Perseus, located around 500 light years away from the Sun. It is visible to the naked eye
2_Persei
Emission nebula in the constellation Perseus
Hβ line in the nebula by the nearby prodigiously energetic O7 star, Xi Persei (also known as Menkib). The California Nebula was discovered by E. E. Barnard
California_Nebula
Variable star in the Alpha Persei Cluster
V488 Persei is a variable star in the constellation Perseus. The star was first identified as a variable in 1985 from data of a 0.9 m telescope at Kitt
V488_Persei
Star in the constellation Perseus
by the BATSE instrument on the Compton Gamma Ray Observatory satellite on 5 August 1992. During outburst, it was observed to be stronger than the Crab
GRO_J0422+32
Variable carbon star in the constellation Perseus
DY Persei is a variable star and carbon star in the Perseus constellation. At maximum it is 11th magnitude and at its faintest it drops to 16th magnitude
DY_Persei
Topics referred to by the same term
chemical element 1,4-Dioxane, a solvent DY Persei, a variable star in the Perseus constellation DY Persei variable, a subclass of R Coronae Borealis variables
Dy
Star in the constellation Perseus
variable star in the northern constellation of Perseus. Also known as V576 Persei, it is a sixth magnitude star that is dimly visible to the naked eye under
HD_21071
Star in the constellation Perseus
1 Persei (1 Per) is an eclipsing binary star in the constellation Perseus. Its uneclipsed apparent magnitude is 5.49. The binary star consists of two
1_Persei
lower brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae", pp. 1846-56, in Paul Murdin, ed. Encyclopedia of
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
Binary star system in the constellation Perseus
consisting of γ Persei, η Persei, α Persei, ψ Persei, δ Persei, 48 Persei, μ Persei and HD 27084. Consequently, the Chinese name for γ Persei itself is 天船二
Gamma_Persei
Star in the constellation Perseus
consisting of τ Persei, 9 Persei, ι Persei, κ Persei, β Persei, ρ Persei, 16 Persei and 12 Persei. Consequently, the Chinese name for τ Persei itself is 大陵二
Tau_Persei
Red giant star in the constellation Andromeda
into the greater form of Perseus envisioned by Johann Bayer as Upsilon Persei. Flamsteed oversaw its constellation reverting and the International Astronomical
51_Andromedae
Star in the constellation Perseus
55 Persei is a single, blue-white hued star in the northern constellation Perseus. It is faintly visible to the naked eye under good seeing conditions
55_Persei
Main sequence star in the constellation Perseus
consisting of ι Persei, 9 Persei, τ Persei, κ Persei, β Persei, ρ Persei, 16 Persei and 12 Persei. Consequently, the Chinese name for ι Persei itself is 大陵三
Iota_Persei
Nova event seen in 1887 in the constellation Perseus
V Persei, also known as Nova Persei 1887 was discovered by Williamina Fleming on a Harvard College Observatory objective-prism photograph taken on 3 November
V_Persei
Star in the constellation Perseus
20 Persei is a visual binary star in the northern constellation of Perseus, a few degrees from Pi Persei. It is visible to the naked eye as a dim, yellow-white
20_Persei
Star in the constellation Perseus
Zeta Persei (ζ Per, ζ Persei) is a star in the northern constellation of Perseus. With an apparent visual magnitude of 2.9, it can be readily seen with
Zeta_Persei
Star in the constellation Perseus
RY Persei is a variable star in the northern constellation of Perseus, abbreviated RY Per. It is an Algol variable with a period of 6.8635663 days, which
RY_Persei
Star in the constellation Perseus
Sigma Persei (Sigma Per, σ Persei, σ Per) is an orange K-type giant star with an apparent magnitude of +4.36. It is approximately 343 light-years from
Sigma_Persei
Star in the constellation Perseus
Omega Persei (ω Persei) is a solitary, orange-hued star in the northern constellation of Perseus. The star is faintly visible to the naked eye with an
Omega_Persei
Star in the constellation Andromeda
6 Persei is a binary star system in the northern constellation of Andromeda. It is faintly visible to the naked eye with an apparent visual magnitude of
6_Persei
Star in the constellation Perseus
asterism consisting of μ Persei, η Persei, γ Persei, α Persei, ψ Persei, δ Persei, 48 Persei and HD 27084. Consequently, μ Persei itself is known as 天船七
Mu_Persei
Rocket stage used on Soviet and later Russian expendable launch systems
engine. Blok D weighs 3.5 tons during liftoff, but some parts are jettisoned and the dry mass in space is 2.5 tons. It has 5.70 meters length and generates
Blok_D
Brightest star in the night sky
Magellanic Cloud, Milky Way, Carina Nebula, Hyades, Pleiades and the Alpha Persei Cluster (with Eta Carinae, Theta Tauri, Alcyone and Mirfak as the brightest
First-magnitude_star
Star in the constellation Perseus
16 Persei is a single, suspected variable star in the northern constellation of Perseus, located approximately 121 light years away based on parallax.
16_Persei
Star in the constellation Perseus
53 Persei is a single variable star in the northern constellation of Perseus. It has the Bayer designation d Persei, while 53 Persei is the Flamsteed
53_Persei
Star system in the constellation Perseus
Theta Persei (Theta Per, θ Persei, θ Per) is a star system 37 light years away from Earth, in the constellation Perseus. It is one of the closest naked-eye
Theta_Persei
American space and aeronautics agency
Observatory images Helix Nebula by Spitzer Space Telescope, 2007 1901 GK Persei supernova by Chandra X-ray Observatory, 2015 Carina Nebula by Hubble Space
NASA
Star in the constellation Perseus
T Persei is a red supergiant located in the constellation Perseus. It varies in brightness between magnitudes 8.3 and 9.7 and is considered to be a member
T_Persei
Binary star system
KS Persei is a binary system in the equatorial constellation of Perseus. It is sometimes known as Bidelman's Star, named after William P. Bidelman. The
KS_Persei
race from the planet Omicron Persei 8. Lrrr (/lɜːr/, voiced by Maurice LaMarche) is the ruler of the planet Omicron Persei 8, and always introduces himself
List_of_Futurama_characters
Star in the constellation Perseus
7 Persei is a star in the constellation Perseus, located 777 light years away from the Sun. While the star bears the Bayer designation Chi Persei, it
7_Persei
Cosmic matter (remnant)
progenitor stars via light echoes as observed with the spherical shell of Nova Persei 1901 or the energies remaining in the expanding bubbles like T Pyxidis.
Nova_remnant
Star in the constellation Perseus
52 Persei is a suspected triple star system in the northern constellation of Perseus. It has the Bayer designation f Persei, while 52 Persei is the Flamsteed
52_Persei
Binary star in the Pleiades star cluster
variable star, with brightness fluctuations that range between a 4.8 and 5.5 visual magnitude. It has a spectral classification of B8Vne, a hot main sequence
Pleione_(star)
Chinese constellation
天大將軍二 297 φ Persei 54 Andromedae* 51 Andromedae 3 天大將軍三 278 υ Persei 51 Andromedae 49 Andromedae 4 天大將軍四 258 ？ 49 Andromedae ω Andromedae 5 天大將軍五 282
Tian_Dajiangjun
Binary star system in the constellation Perseus
42 Persei is a binary star system in the northern constellation of Perseus. It has the Bayer designation n Persei, while 42 Persei is the Flamsteed designation
42_Persei
Star in the constellation Perseus
V718 Persei is a young star in the constellation of Perseus, located in the young open cluster IC 348. The star has several designations derived from the
V718_Persei
Star in the constellation Perseus
λ Persei, Latinized as Lambda Persei, is a star in the northern constellation of Perseus. It is visible to the naked eye as a faint, white-hued point of
Lambda_Persei
Type of large cool star
Cassiopeiae) δ Andromedae ρ Persei Mira (ο Ceti) χ Cygni Rasalgethi (α Herculis) The Sun will exit the main sequence in approximately 5 billion years and start
Red_giant
Apparent faster-than-light motion of distant astronomical objects
The apparent superluminal motion in the faint nebula surrounding Nova Persei was first observed in 1901 by Charles Dillon Perrine. "Mr. Perrine's photograph
Superluminal_motion
Open cluster in the constellation Coma Berenices
Melotte 111, but its proper motion and isochrone are inconsistent. Alpha Persei Cluster List of nearby stellar associations and moving groups "Cl Melotte
Coma_Star_Cluster
Star that has a supergiant luminosity class, with a spectral type of F or G
red supergiants; naked eye examples include Polaris, Alpha Leporis, Alpha Persei, Delta Canis Majoris and Iota¹ Scorpii. Many of them are variable stars
Yellow_supergiant
Spectroscopic binary star system in the constellation Perseus
43 Persei is a binary star system in the northern constellation Perseus. It is visible to the naked eye as a dim, yellow-white hued star with an apparent
43_Persei
Aging giant in the constellation Perseus
24 Persei is a star in the northern constellation of Perseus, located around 337 light years from the Sun. It is visible to the naked eye as a faint, orange-hued
24_Persei
Star in the constellation Perseus
4 Persei is a single star in the northern constellation of Perseus, located around 670 light years away from the Sun. It is visible to the naked eye as
4_Persei
Star in the constellation Perseus
8 Persei is a single star in the northern constellation of Perseus, located 416 light years away from the Sun. It is visible to the naked eye as a dim
8_Persei
Stars with a supergiant luminosity class with a spectral type of K or M
examples: Antares A Betelgeuse Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically thought to
Red_supergiant
Astronomical phenomenon caused by light reflected off surfaces distant from the source
assumed the possibility of expansion of the bright ring (nebula) around Nova Persei 1901 with a velocity exceeding that of light." He continues: "The comparison
Light_echo
Multiple-star system in the constellation of Perseus
Persei is a binary and possibly a triple star system in the northern constellation of Perseus. It has the Bayer designation e Persei, while 58 Persei
58_Persei
Star in the constellation Perseus
14 Persei is a single star in the northern constellation Perseus, located roughly 1,900 light years away from the Sun. It is visible to the naked eye as
14_Persei
Star in the constellation Perseus
54 Persei is a single star in the northern constellation of Perseus. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual
54_Persei
Star in the constellation Perseus
17 Persei is a single star in the northern constellation of Perseus, located about 420 light years away from the Sun. It is visible to the naked eye as
17_Persei
Greek goddess of magic and transitions
Hecate, Luna and Trivia. From her father Perses, Hecate is often called "Perseis" (meaning "daughter of Perses") which is also the name of one of the Oceanid
Hecate
stars from 0.29 to 0.395 R☉. Partial list containing stars from 0.395 to 0.5 R☉. Red dwarfs are considered the smallest stars known that are active fusion
List_of_smallest_known_stars
Daughter of King Aeëtes of Colchis in Greek mythology
Colchis. According to Hesiod (Theogony 956–962), Helios and the Oceanid Perseis produced two children, Circe and Aeëtes. Aeëtes then married the Oceanid
Medea
Binary star system in the constellation Perseus
binary star system in the constellation Perseus, located within the Alpha Persei Cluster. It has a blue-white hue and is visible to the naked eye with a
HD_21278
as per the formula: − 26.78 ≈ − 2.5 log 10 10 − 26.74 ⋅ − 0.4 ( 1 − 0.0167 ) 2 {\displaystyle -26.78\approx -2.5\log _{10}{\frac {10^{-26.74\cdot -0
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Star in the constellation Perseus
k Persei is a class G9.5III (yellow giant) star in the constellation Perseus. Its apparent magnitude is 4.77 and it is approximately 211 light years away
K_Persei
Variable star in the constellation Perseus
HD 21699, also known as HR 1063 and V396 Persei, is a star about 580 light years from the Earth, in the constellation Perseus. It is a 5th magnitude star
HD_21699
Constellation in the northern celestial hemisphere
borders, there are 157 stars brighter than or equal to apparent magnitude 6.5. The five brightest stars of Cassiopeia – Alpha, Beta, Gamma, Delta, and Epsilon
Cassiopeia_(constellation)
17th episode of the 4th season of Futurama
dealing monster" to Lrrr, ruler of the planet Omicron Persei 8. The three travel to Omicron Persei 8, where they learn Lrrr and his wife, Ndnd, are having
Spanish_Fry
Nova in the constellation Perseus
V392 Persei, also known as Nova Persei 2018, is a bright nova in the constellation Perseus discovered on April 29, 2018. It was previously known as a
V392_Persei
WGSN. Further batches of names were approved on 21 August, 12 September, 5 October, and 6 November 2016. These were listed in a table of 102 stars included
List_of_proper_names_of_stars
Star in the constellation Perseus
36 Persei is a solitary, variable star located 121 light years away from the Sun in the northern constellation of Perseus. It is visible to the naked eye
36_Persei
Star in the constellation Perseus
V520 Persei is a blue supergiant member of NGC 869, one of the Perseus Double Cluster open clusters. It is an irregular variable star. At a magnitude of
V520_Persei
5 PERSEI
5 PERSEI
Female
Japanese
(1-æ£, 2-é›…, 3-昌, 4-真, 5-政, 6-å°†) Unisex short form of Japanese names beginning with Masa-, MASA means 1) "correct, just," 2) "elegant," 3) "flourishing, prosperous" 4) "genuine, true," 5) "governing, political," 6) "military." Compare with strictly masculine Masa.
Surname or Lastname
English
English : variant spelling of Peak.Irish : variant of Peak 2.North German : metonymic occupational name for a spearmaker, from Middle Low German pēk ‘pike’. Compare Pike 4.Dutch : variant of Peck 4 and 5.
Boy/Male
Hindu, Indian, Tamil
5 Head of Snake
Surname or Lastname
German
German : diminutive of Summer 5.English (Bedfordshire) : unexplained.
Surname or Lastname
English
English : variant spelling of Kay 4 and 5.
Male
Japanese
(1-æš, 2-æ‚Ÿ, 3-è¡, 4-知, 5-覚, 6-è«, 7-了, 8-智) Japanese name SATORU means 1) "daybreak," 2) "enlightened," 3) "fast learner," 4) "knowledgeable," 5) "perceptive," 6) "persuasive," 7) "understanding," or 8) "wise."
Surname or Lastname
English
English : variant of Wall.Swedish : ornamental name composed of the elements wall, an old spelling of vall ‘grassy bank’ + man ‘man’.German (Wallmann) : variant of Wall 4 and 5.
Male
Japanese
(1-ç´€, 2-ä¿®, 3-ç†, 4-åŽ, 5-æ²», 6-çµ±) Japanese name OSAMU means 1) "chronicler," 2) "disciplined," 3) "logical," 4) "obtainer," 5) "to reign," 6) "ruler."
Surname or Lastname
English
English : patronymic from Kay 5.
Male
Japanese
(1-晋, 2-信, 3-紳, 4-心, 5-慎, 6-新, 7-進, 8-真) Japanese name SHIN means 1) "advancing," 2) "belief," 3) "gentleman," 4) "heart," 5) "humble," 6) "new," 7) "progressive," and 8) "true." Compare with another form of Shin.
Surname or Lastname
English (Yorkshire)
English (Yorkshire) : unexplained.French : from a diminutive of Bard 5.Hungarian (Bárdy) : habitational name for someone from a place called Bárd in Somogy county or in Máramaros, (now Maramures in Romania).
Boy/Male
Muslim
One who prays 5 times and fasts, Forever, Immortal
Female
Japanese
(1-æµå, 2-æ…¶å, 3-æ¡‚å, 4-敬å, 5-å•“å, 6-åœå, 7-景å) Japanese name KEIKO means 1) "blessed, lucky child," 2) "happy child," 3) "katsura tree child," 4) "respectful child," 5) "spring child," 6) "square jewel child," or 7) "sunny child."
Girl/Female
Assamese, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Telugu
A Garland of 5 Types of Flowers
Surname or Lastname
South German (Düll)
South German (Düll) : nickname for a stubborn man.German (Düll) : variant of Dill 5.English : unexplained.
Male
Japanese
(1-æ£, 2-é›…, 3-昌, 4-真, 5-政, 6-å°†) Unisex short form of Japanese names beginning with Masa-, MASA means 1) "correct, just," 2) "elegant, splendid" 3) "flourishing, prosperous" 4) "genuine, true," 5) "governing, political," 6) "military." Compare with another form of Masa.
Female
Japanese
(1-æµ, 2-æ…¶, 3-æ¡‚, 4-敬, 5-å•“, 6-åœ, 7-景) Japanese name KEI means 1) "blessed, lucky," 2) "happy," 3) "katsura tree," 4) "respectful," 5) "spring," 6) "square jewel," or "sunny."Â
Surname or Lastname
English
English : nickname from Middle English dull + -ard ‘dull or stupid person’. Compare Doll 5.Irish : either an importation to Ireland of the English name or, possibly, a reduced and altered form of de la Hyde (see Dollarhide).
Male
Japanese
(1-æµ, 2-ä½³, 3-敬, 4-åœ, 5-æ…§) Japanese name KEI means 1) "blessed, lucky," 2) "excellent," 3) "respect," 4) "square jewel," or 5) "wise."
Surname or Lastname
English
English : occupational name for a maker or seller of hoods, from Middle English hodestre, a feminine form of Hodder.German (also Höster) : habitational name for someone from either of two places called Host (see Host 5).
5 PERSEI
5 PERSEI
Girl/Female
Australian, British, Danish, English, French, German
Bright
Boy/Male
British, English, German
Ruler
Boy/Male
Arabic, Muslim, Parsi
Brave; Bold Man
Boy/Male
Muslim
Inhabitant
Girl/Female
Muslim/Islamic
Call
Boy/Male
Hindu, Indian
God Shiva
Boy/Male
Hebrew, Hindu, Indian
Joy; Delight; Shelter
Surname or Lastname
English
English : variant spelling of Metcalf.
Boy/Male
Tamil
Strong
Girl/Female
German
Defender; Industrious
5 PERSEI
5 PERSEI
5 PERSEI
5 PERSEI
5 PERSEI
n.
See 4th Trap, 5.
n.
Same as Gudgeon, 5.
n. & v.
See Prize, n., 5. Also Prize, v. t.
n.
Same as Reed, n., 5.
n.
See Relief, n., 5.
n.
See Flyer, n., 5.
n.
See Camp, n., 5.
n.
See Romance, 5.
n.
An umbilicus. See Umbilicus, 5 (b).
n.
See Closure, 5.
v.
See Affected, 5.
n.
Same as Placard, 4 & 5.
n.
A way for passage; a hall. See Passage, 5.
n.
The thorax of an insect. See Trunk, n., 5.
n.
Same as Relief, n., 5.
n.
See Tailing, n., 5.
a.
Affected with the vapors. See Vapor, n., 5.
n.
A morality play. See Morality, 5.
pref.
On; along; in traversing. Compare 5.
n.
See Tread, n., 5.