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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
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
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
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
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)
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
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 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
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
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
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
Open clusters in the constellation Perseus
of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation
Double_Cluster
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
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
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
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
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
Oceanid nymph and wife of Helios in Greek mythology
(Ancient Greek: Πέρση, romanized: Pérsē, lit. 'destroyer') or Perseis (Περσηίς, Persēís) is one of the 3,000 Oceanids, fresh water-nymph daughters of
Perse_(mythology)
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
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 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
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
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
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
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
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
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
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
Open cluster in the constellation Perseus
NGC 869 (also known as h Persei) is an open cluster located around 7,460 light years away in the constellation of Perseus. The cluster is around 14 million
NGC_869
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
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
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
Persei, it is a sixth magnitude star that is dimly visible to the naked eye under good viewing conditions, having an apparent visual magnitude of 6.09
HD_21071
Type of eruptive variable star
8 (6): 6. Bibcode:2008PZP.....8....6T. ISSN 0373-7683. Tur, N. S.; Goraya, P. S. (April 1988). "Scanner observations of shell stars Phi Persei and Psi
Gamma_Cassiopeiae_variable
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
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
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
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 Perseus
XX Persei (IRC +50052 / HIP 9582 / BD+54°444) is a semiregular variable red supergiant star in the constellation Perseus, between the Double Cluster and
XX_Persei
Star in the constellation Perseus
clusters. It is an irregular variable star. At a magnitude of about 6.6, V520 Persei is the brightest member in either NGC 869 or NGC 884, although the
V520_Persei
Star in the constellation Perseus
12 Persei (12 Per) is a double-lined spectroscopic binary star system in the northern constellation Perseus. Its combined apparent magnitude is 4.94, which
12_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
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
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
Blue supergiant star in the constellation Perseus
10 Persei is a blue supergiant star in the constellation Perseus. Its apparent magnitude is 6.26 although it is slightly variable. 10 Persei is located
10_Persei
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 B2
1_Persei
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
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
Type of large cool star
Geminorum) Capella Aa (α Aurigae) Schedar (α Cassiopeiae) δ Andromedae ρ Persei Mira (ο Ceti) χ Cygni Rasalgethi (α Herculis) The Sun will exit the main
Red_giant
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
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
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
Open cluster in the constellation Perseus
NGC 884 (also known as χ Persei) is an open cluster located 7640 light years away in the constellation of Perseus. It is the east component of the Double
NGC_884
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 Lacerta
Strom, Stephen E.; et al. (2005), "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?", The Astronomical
6_Lacertae
Star in the constellation Perseus
RS Persei is a red supergiant variable star located in the Double Cluster in Perseus. The star's apparent magnitude varies from 7.82 to 10.0, meaning it
RS_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
Chinese constellation
『中西対照恒星図表』科学出版社.(in Chinese) 陳遵媯 (1982): 「中西星名対照表」『中国天文史』 vol.3, 上海人民出版社, app. 6.(in Chinese) 渡辺敏夫 (1963): 「保井春海星図考」『東京商船大学研究報告』No. 14.(in Japanese) Allen
Tian_Dajiangjun
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
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
Star in the constellation Perseus
57 Persei, or m Persei, is a suspected triple star system in the northern constellation of Perseus. It is at the lower limit of visibility to the naked
57_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
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
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
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 in the WGSN's
List_of_proper_names_of_stars
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
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
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
Poem by Hesiod
(including Doris, Electra, Callirhoe, Styx, Clymene, Metis, Eurynome, Perseis, and Idyia). From Hyperion and Theia came Helios (Sun), Selene (Moon),
Theogony
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
12th episode of the 1st season of Futurama
by Brian Sheesley. The episode features an attack by aliens from Omicron Persei 8, when their leader, Lrrr, is outraged when the final episode of the series
When_Aliens_Attack
11th episode of the 6th season of Futurama
August 26, 2010. In the episode, the Omicronian ruler of the planet Omicron Persei 8, Lrrr, experiences marriage trouble with his queen, Ndnd. He departs for
Lrrreconcilable Ndndifferences
Lrrreconcilable_Ndndifferences
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
1.79 Dubhe α Ursae Majoris 0120 K0 III, F0 V Northern 34 1.82 Mirfak α Persei 0510 F5 Ib Northern 35 1.82 Wezen δ Canis Majoris 1,800 F8 Ia Southern 36
List_of_brightest_stars
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
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
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
Mystery religion in the Roman Empire
horns. The context is a prayer to the god Phoebus. The cave is described as persei, which in this context is usually translated Persian. According to the translator
Mithraism
Retrieved 3 October 2021. "Starlink Group 6-88". Next Spaceflight. Retrieved 2 October 2025. "Starlink Group 6-96". Next Spaceflight. Retrieved 9 January
List of spaceflight launches in January–March 2026
List_of_spaceflight_launches_in_January–March_2026
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
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
Country in Southeast Europe
and ten years after Philip V of Macedon captured Bylazora; after this Perseis and Astraion were founded. The Romans established the province of Macedonia
North_Macedonia
"Periodic Low-amplitude Radial Velocity Variations in the Supergiant α Persei", The Astrophysical Journal, 985 (2): 176, Bibcode:2025ApJ...985..176B,
List_of_nearest_supergiants
Brightest star in the constellation of Carina
same behaviour has been measured in other F-class supergiants such as α Persei and is now believed to be a normal property of such stars. The spectrum
Canopus
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
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
Star in the constellation Perseus
b Persei (also known as HD 26961) is a spectroscopic triple star in the constellation Perseus. Its apparent magnitude is 4.60, making it visible to the
B_Persei
Classification of stars based on spectral properties
class M0V, with magnitude 6.7 (the limiting magnitude for typical naked-eye visibility under good conditions being typically quoted as 6.5), and it is extremely
Stellar_classification
Nuclear explosion in a white dwarf star
Verro, K.; Kolka, I. (2014). "A Dynamical Study of the Nova Remnant of GK Persei / Stella Novae: Past and Future Decades.". Stellar Novae: Past and Future
Nova
Star in the constellation Scutum
hypergiant, it has been compared to another pulsating but cooler supergiant, S Persei, and is also found to be a maser source of H 2O, SiO, and OH masers. However
UY_Scuti
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
American astronomer
dissertation on "Proper motions and parallaxes of 359 stars in the cluster h Persei." Following her graduation from Swarthmore College, Pettit worked as an
Hannah_Steele_Pettit
Fifteenth letter of the Greek alphabet
Such stars include Omicron Andromedae, Omicron Ceti (Mira), and Omicron Persei. In Claudius Ptolemy's (c. 100–170) Almagest, tables of sexagesimal numbers
Omicron
Star in the constellation Perseus
49 Persei is a star in the northern constellation of Perseus. It is just visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude
49_Persei
Class of high-mass X-ray binaries
spectroscopy are used to accurately identify these optical counterparts. X Persei is a binary system containing a γ Cassiopeiae variable and a pulsar. It
Be/X-ray_binary
Star in the constellation Perseus
3 Persei is a single, orange-hued star in the northern constellation of Perseus. It is dimly visible to the naked eye under good viewing conditions, having
3_Persei
125823). Named after William P. Bidelman. Bidelman's peculiar star is KS Persei (HD 30353), a PV Telescopii variable. Bidelman's high-latitude Be star is
Stars_named_after_people
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
Star in the constellation Perseus
π Persei, Latinized as Pi Persei, is a single star in the northern constellation of Perseus. It has the traditional name Gorgonea Secunda /ɡɔːrɡəˈniːə
Pi_Persei
Andromedae (α And) Now included in the constellation Andromeda Bayer's Chi Persei is NGC 884, the eastern cluster of the Double Cluster – Wagman, Morton (2003)
Table of stars with Bayer designations
Table_of_stars_with_Bayer_designations
6 PERSEI
6 PERSEI
Male
Hebrew
(שָׂרָף) Hebrew name SARAPH means "burning one" or "serpent." In the bible, this is the name of a son of Shelah. It is also the name of a species of venomous serpents mentioned in Numbers 21:6, and the name of an order of six-winged angels mentioned by Isaiah who attend upon God.
Boy/Male
Hindu, Indian, Tamil
Lord Muruga; Lord Vishnu; God with 6 Faces (Subrahmanyeswara Swamy)
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 (very common in England, especially in the south Midlands, and in Wales) and German (especially northwestern Germany)
English (very common in England, especially in the south Midlands,
and in Wales) and German (especially northwestern Germany) : patronymic
from the personal name Adam. In the U.S. this form has absorbed
many patronymics and other derivatives of Adam in languages
other than English. (For forms, see Hanks and Hodges 1988.)This American family name was borne by two early presidents of the
United States, father and son. They were descended from Henry Adams,
who settled in Braintree, MA, in 1635/6, from Barton St. David,
Somerset, England. The younger of the two presidents, John Quincy
Adams (1767–1848) derived his middle name from his maternal
grandmother’s family name (see
Surname or Lastname
English and Irish (of Norman origin)
English and Irish (of Norman origin) : from the Old French personal name Picot, Pigot, a pet form of Pic (see Pike 6).
Surname or Lastname
English (Norman) and French
English (Norman) and French : nickname from Old French druerie ‘love’, ‘friendship’, a derivative of dru ‘lover’, ‘friend’ (see Drew 3). In Middle English the word also had the concrete meanings ‘love affair’, ‘love token’, ‘sweetheart’.English (Norman) and French : from a Germanic personal name composed of Old High German triuwa ‘truth’, ‘trust’ + rīc ‘power(ful)’.Irish (County Roscommon) : English name adopted by bearers of Gaelic Mac an Druaidh ‘son of the druid’. Compare Drew 6.
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-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."
Surname or Lastname
English
English : from a pet form of the personal name William.Benjamin Wilmot and his wife, with their 6-year-old son William, emigrated from England to New Haven, CT, in or before 1640.
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 : unexplained; perhaps a variant of Tongs, itself a variant of Tong 6.Possibly an altered spelling of German Dungs, a variant of Dung.
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.
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
English : possibly from Middle English Old French personal name Pic (see Pike 6) + the diminutive suffix -in.
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."
Female
Greek
(Θεοφάνια) Feminine form of Greek Theophanes, THEOPHANIA means "manifestation of God." This name used to be given to girls born on the Epiphany (January 6)--also called the 12th day of Christmas--which commemorates the visit of the three wise men (the Magi) to the infant Jesus.
Surname or Lastname
English
English : unexplained; possibly a respelling of Kay 6, a shortened form of Scottish and Irish McKay.Korean : There is only one Chinese character and one clan for the Kye family name. According to the Kye family genealogy, the clan was founded by a Ming Dynasty government official named Kye SÅk-son who migrated to KoryÅ and settled in today’s Suan County of Hwanghae Province. The majority of bearers of the Kye family name today live in North Korea.
Surname or Lastname
English
English : from the Middle English, Old French personal name Picot, Pigot, a pet form of Pic (see Pike 6). In Middle English, the form Piket (Old French Picquet) was also common.
Surname or Lastname
English (East Anglia, chiefly Norfolk)
English (East Anglia, chiefly Norfolk) : occupational name for someone who mowed pasture lands to provide hay, from an agent derivative of Middle English mow(en) ‘mow’ (Old English mÄwen).Welsh : nickname from mawr ‘big’ (see Moore 6).German (Möwer) : nickname from an agent derivative of Middle High German mÅven ‘to torment, trouble, or burden’.
Surname or Lastname
English
English : variant spelling of Hain 1–3.German : variant spelling of Hain 4.Jewish : variant spelling of Hain 6.
6 PERSEI
6 PERSEI
Girl/Female
Indian
Independent, Supportive, One who is loved by everyone
Girl/Female
American, Anglo, Australian, British, Chinese, Christian, Danish, English, French, German, Gothic, Greek, Gujarati, Hindu, Indian, Irish, Jamaican, Kannada, Malayalam, Welsh
Pearl; Strong and Capable; Strong; Great; Diminutive of Margaret; Margaret
Boy/Male
Muslim
Sea
Girl/Female
Hindu
Winner, Victor
Boy/Male
Tamil
Vasa Spring season, Happy
Boy/Male
Hindu
Arva means fastest motion wind
Girl/Female
Muslim
Act of kindness. Benefaction. Bestowal.
Boy/Male
Australian, Chinese
Happy
Boy/Male
Muslim
The place where earth & Sky Meet
Boy/Male
Hindu, Indian
Son; Stories of Budhdha's Previous Incarnations
6 PERSEI
6 PERSEI
6 PERSEI
6 PERSEI
6 PERSEI
n.
See Race, n., 6.
n.
A parasite; a sponger. See def. 6, above.
n.
Same as List, n., 6.
n. pl.
See Doublet, 6 and 7.
n.
The fly of a flag: See Fly, n., 6.
n.
See Siren, 6.
n.
See Fellowship, n., 6.
n.
See Jig, 6.
n.
The condition of being of equal in intensity; -- applied to relations; as, 3:6 and 6:12 are relations of cointension.
v. t.
To surpass in singing. See Breast, n., 6.
n.
See Kite, n., 6.
n.
Same as Center, n., 6.
n.
The space between two axes. See Axis, 6.
n.
A cradle, as for a broken limb. See Cradle, 6.
n. pl.
See Fluxion, 6(b).
n.
See Drag, n., 6, and Drag sail, under Drag, n.
n.
A disease in vegetables. See Brand, n., 6.
n.
A genus of lizards. See Dragon, 6.
n.
A stigma. See Stigma, n., 6 (a) & (b).
n.
A symbol representing six units, as 6, vi., or VI.