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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
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
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 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
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
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
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 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 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
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 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
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 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
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
16th episode of the 7th season of Futurama
his way home. An invasion of Earth by Lrrr and his son Jrrr of Omicron Persei 8 ends with the Headless Clone of Agnew's death. A furious Richard Nixon's
T.:_The_Terrestrial
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
Species of butterfly
Euphaedra perseis, the Perseis mimic forester, is a butterfly in the family Nymphalidae. It is found in Guinea (Conakry), Sierra Leone, Liberia, Ivory
Euphaedra_perseis
City in ancient Macedon
Perseis (Ancient Greek: Περσηΐς) was a city of ancient Paeonia founded by Philip V of Macedon and named after Perseus. The city's exact location has not
Perseis_(Paeonia)
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
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
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
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
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
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
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
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
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
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 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
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
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
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
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
Cosmic matter (remnant)
observed with the spherical shell of Nova Persei 1901 or the energies remaining in the expanding bubbles like T Pyxidis. Most novae require a close binary
Nova_remnant
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
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
Open cluster in the constellation Perseus
which itself is part of the larger Double Cluster. The stars Gamma Persei and Eta Persei point in the general direction of the open cluster. Trumpler 2 -
NGC_957
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
30 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
30_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
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
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
Bibcode:2012ApJ...757...36K. doi:10.1088/0004-637x/757/1/36. S2CID 118452794. General Catalogue of Variable Stars, 3rd ed. (1971) Moscow[page needed] v t e v t e
GRO_J0422+32
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 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
Genus of gastropods
Oskars & Willassen, 2016 Spiniphiline kensleyi Gosliner, 1988 Spiniphiline persei Caballer & Ortea, 2015 Spiniphiline richardsoni Swinnen, 2021 Spiniphiline
Spiniphiline
English astronomer (1764–1786)
He is best known for his observations of the variable star Algol (Beta Persei) in 1782. John Goodricke, named after his great-grandfather Sir John Goodricke
John_Goodricke
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
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
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 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
Genus of plants
Dicranolepis incisa A.Robyns Dicranolepis laciniata Gilg Dicranolepis persei Cummins Dicranolepis polygaloides Gilg ex H.Pearson Dicranolepis pubescens
Dicranolepis
Variable star in the constellation Perseus
HR 1170, also known as HD 23728 and V376 Persei, is a star about 220 light years from the Earth, in the constellation Perseus. It is a 5th magnitude star
HR_1170
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 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
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
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
Balkom; Everitt, P. F.; Sadler, D. H.; Squadron-Leader May; Bennett, D. C. T.; Hinks, A. R.; Black, Archibald; Squadron-Leader Barnes; Comrie, L. J. (August
List_of_proper_names_of_stars
; Indebetouw, R.; Meade, M. R.; Meixner, M.; Misselt, K. A.; Robitaille, T. P.; Shiao, B.; Whitney, B. A. (2010). "Spitzer SAGE-SMC Infrared Photometry
List_of_brightest_stars
epic poet attached to the court of the kings of Pergamon, who wrote a Perseis in ten books and also poems about Eumenes and Attalus I. Chisholm, Hugh
Musaeus_of_Ephesus
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
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
F-type variable star
collision systems such as ASASSN-21qj, NGC 2547–ID8, HD 166191 and V488 Persei. Gaia-GIC-1 was initially discovered through the Gaia Photometric Science
Gaia20ehk
Classification of stars based on spectral properties
deviating mass have also been assigned letters: D for white dwarfs and L, T and Y for brown dwarfs (and exoplanets). In the MK system, a luminosity class
Stellar_classification
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
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
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
Reflection nebula in Perseus
star Epsilon Persei, which is also clearly visible to the naked eye. the cloud can be seen near a ninth magnitude star catalogued as XY Persei (A2II+B6)
VdB_24
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
supernovae Variable star A higher magnitude means a lower brightness. i.e. T Aurigae (+3.8) was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae"
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
Canadian voice actor (born 1958)
Hedonismbot, Morbo the news anchor, and Lrrr, ruler of the planet Omicron Persei 8, among numerous others. He has also done his Orson Welles impression on
Maurice_LaMarche
Chemical compound of hydrogen and oxygen
more than half of T Tauri stars such as AA Tauri as well as TW Hydrae, IRC +10216 and APM 08279+5255, VY Canis Majoris and S Persei. Liquid water is present
Water
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
.659.1536R. doi:10.1086/512672. S2CID 8913778. Haemmerlé, Lionel; Woods, T. E.; Klessen, Ralf S.; Heger, Alexander; Whalen, Daniel J. (2018). "The evolution
List_of_largest_stars
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
Brummelaar, T.; Ridgway, S. T.; Sturmann, J.; Sturmann, L.; Turner, N.; Farrington, C. (2015). "Spectral and spatial imaging of the Be+sdO binary ϕ Persei". Astronomy
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Poem by Hesiod
(including Doris, Electra, Callirhoe, Styx, Clymene, Metis, Eurynome, Perseis, and Idyia). From Hyperion and Theia came Helios (Sun), Selene (Moon),
Theogony
Ancient Greek god of the earth-encircling river, Oceanos
of Iapetus, and mother of Atlas, Menoetius, Prometheus, and Epimetheus; Perseis, wife of Helios and mother of Circe and Aeetes; Idyia, wife of Aeetes and
Oceanus
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
Stellar association
the blue supergiant 9 Persei. "Per OB1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2020-01-15. Sitnik, T. G. (May 2003). "The Line-of-Sight
Perseus_OB1
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
Constellation in the northern celestial hemisphere
M.; Pedretti, E.; Thureau, N.; Mérand, A.; ten Brummelaar, T.; McAlister, H.; Ridgway, S. T. (2011). "Colder and Hotter: Interferometric Imaging of β Cassiopeiae
Cassiopeia_(constellation)
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
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
Large Magellanic Cloud and possibly the largest known overall NML Cygni S Persei VY Canis Majoris - potentially the largest star known in the Milky Way VX
Hypergiant
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
"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
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
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
Type of star larger than main-sequence but smaller than a giant
scheme, including: B0: γ Cassiopeiae, δ Scorpii, B0.5: β Scorpii, ε Persei B1: ο Persei, β Cephei B2: γ Orionis, π Scorpii, θ Ophiuchi, λ Scorpii, ω Canis
Subgiant
Loose star cluster
Castor moving group AB Doradus moving group Zeta Herculis moving group Alpha Persei moving cluster Cameleopardis OB1 association OB star Moving groups Open
Stellar_association
Chris. "NASASpaceFlight.com". Clark, Stephen. "Spaceflight Now". Kelso, T.S. "Satellite Catalog (SATCAT)". CelesTrak. Krebs, Gunter. "Chronology of
List of spaceflight launches in January–March 2026
List_of_spaceflight_launches_in_January–March_2026
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
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
Class of high-mass X-ray binaries
as of 1996, only X Persei and LSI+61°303 have X-ray outbursts of much higher luminosity and harder spectrum (kT ≈ 10–20 keV) vs. (kT ≤ 1 keV). LSI+61°303
Be/X-ray_binary
Pattern of stars recognized on Earth's night sky
the Hyades, the Pleiades also in the Taurus constellation and the Alpha Persei Cluster (with Alcyone and Mirfak as the brightest stars). The northern Spring
Asterism_(astronomy)
Type of star that is massive and luminous
fainter than absolute magnitude −5, with some examples around −2 (e.g. 14 Persei). With bolometric corrections around zero, they may only be a few hundred
Supergiant
"Detection of the 128-day radial velocity variations in the supergiant α Persei. Rotational modulations, pulsations, or a planet?". Astronomy and Astrophysics
List_of_exoplanet_extremes
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
T PERSEI
T PERSEI
Female
Egyptian
, the mother of the priest Fai-iten-hemh-bai.
Male
Czechoslovakian
, living.
Surname or Lastname
English, French, German, Hungarian (Donát), Polish, and Czech (Donát)
English, French, German, Hungarian (Donát), Polish, and Czech (Donát) : from a medieval personal name (Latin Donatus, past participle of donare, frequentative of dare ‘to give’). The name was much favored by early Christians, either because the birth of a child was seen as a gift from God, or else because the child was in turn dedicated to God. The name was borne by various early saints, among them a 6th-century hermit of Sisteron and a 7th-century bishop of Besançon, all of whom contributed to the popularity of the baptismal name in the Middle Ages, which was not checked by the heresy of a 4th-century Carthaginian bishop who also bore it. Another bearer was a 4th-century gramMarian and commentator on Virgil, widely respected in the Middle Ages as a figure of great learning.
Female
Egyptian
, the goddess of time.
Female
Egyptian
, the daughter of King Snefru.
Male
Hungarian
Czech and Hungarian form of Latin Donatus, DONÃT means "given (by God)."
Female
Egyptian
, The Good Companion.
Female
Egyptian
, the wife of Toti.
Female
Norse
Old Norse name composed of the elements bjarga "to rescue" and ljótr "bright, light," hence "rescue light."Â
Female
Egyptian
, a daughter of Rameses II; & a wife of Rameses II.
Female
Icelandic
Icelandic form of Latin Margarita, MARGRÉT means "pearl."
Female
Egyptian
, the daughter of Osirtesen.
Male
Czechoslovakian
, earnest, serious.
Male
Czechoslovakian
, given.
Female
Egyptian
, the name of several Egyptian ladies.
Male
Hungarian
Hungarian form of Old High German Bernhard, BERNÃT means "bold as a bear."
Female
Egyptian
, The Most Powerful of Beings.
Female
Egyptian
, a sister of the prince Ra-hotep.
Female
Egyptian
, an Egyptian lady, the wife of Antefaker.
Female
Egyptian
, the goddess of darkness.
T PERSEI
T PERSEI
Boy/Male
Tamil
Manvik | மாஂநà¯à®µà®¿à®•
One who is consious/ intellegent, Kind hearted
Girl/Female
Muslim
Good news, Blessedness, Beatitude
Male
Egyptian
, the elder brother of Bata.
Girl/Female
Arabic
Very Beautiful
Male
Russian
(СавеÌлий) Russian name SAVELIY means "Sabine; a follower of another religion."
Male
Japanese
(修二) Japanese name SHUJI means "master/study second (son)."
Boy/Male
Bengali, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Oriya, Sanskrit, Sindhi, Telugu
Lustrous
Girl/Female
Afghan, African, Arabic, Australian, Danish, French, Swahili
Helper; From Kikuyu; Happy
Boy/Male
Indian
One who is without enmity, Hate
Surname or Lastname
English
English : variant spelling of Gain.
T PERSEI
T PERSEI
T PERSEI
T PERSEI
T PERSEI
v. t.
See Kiddy, v. t.
v. t.
See Jam, v. t.
v. t.
See Kittle, v. t.
v. t.
See Buttweld, v. t.
v. t.
See Feeze, v. t.
v. t.
See Bromate, v. t.
v. t.
See Forcarve, v. t.
v. t.
See Cob, v. t.
v. t.
See Agast, v. t.
v. t.
See Leach, v. t.
v. t.
See Entail, v. t.
v. t.
See Chivy, v. t.
v. t.
See Roust, v. t.
v. t.
See Reenforce, v. t.
v. t.
See Haze, v. t.