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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
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
Open cluster in the constellation Perseus
supergiant Mirfak, also known as Alpha Persei. Bright members also include Delta, Sigma, Psi, 29, 30, 34, and 48 Persei. The Hipparcos satellite and infrared
Alpha_Persei_Cluster
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 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 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 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
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
37 B A4 IV BL Crucis 480 ± 10 Crux M4-5III 5.38 48 Persei 480 ± 10 B3Ve 4.03 Member of Alpha Persei Cluster. PP Carinae 480 ± 30 Carina B4 Vne 3.22 -
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
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
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
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
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
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
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
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 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
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
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
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
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
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
Publications of the Astronomical Society of the Pacific. 48 (283). San Francisco, CA: 139. Bibcode:1936PASP...48..139R. doi:10.1086/124681. Davis, George A. Jr
List_of_proper_names_of_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
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
Constellation in the northern celestial hemisphere
mythology, who boasted about her unrivaled beauty. Cassiopeia was one of the 48 constellations listed by the 2nd-century Greek astronomer Ptolemy, and it
Cassiopeia_(constellation)
– On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket Persei, on the constellation boundary between Andromeda with Perseus RU And, database
List_of_stars_in_Andromeda
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
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
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
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
Moon −12.7 mag Venus −4.92 mag Jupiter −2.94 mag Mars −2.94 mag Mercury −2.48 mag Saturn −0.55 mag Any exact order of the visual brightness of stars is
List_of_brightest_stars
"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
17-31". Next Spaceflight. Retrieved 19 February 2026. "Starlink Group 10-48". Next Spaceflight. Retrieved 14 March 2026. "CASC/Unknown Payload". Next
List of spaceflight launches in January–March 2026
List_of_spaceflight_launches_in_January–March_2026
Derriopos. According to Livy, Philip V of Macedon founded the city of Perseis in Derriopos, named after his eldest son, Perseus. After the defeat in
Derriopos
Constellations recognized by the International Astronomical Union
most notable of these is Argo Navis, which was one of Ptolemy's original 48 constellations. In the 1750s, the French astronomer Nicolas Louis de Lacaille
IAU_designated_constellations
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
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)
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
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
Open cluster in the constellation Perseus
northern constellation of Perseus, positioned 2° SSE of the faint star Lambda Persei. The same telescope field contains the clusters NGC 1528 and NGC 1545. NGC
NGC_1513
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
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
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
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
NASA space telescope launched in 1999
International Year of Light 2015 Cluster of newly formed stars in Orion Nebula GK Persei: Nova of 1901 X-ray light rings from a neutron star in Circinus X-1 Cygnus
Chandra_X-ray_Observatory
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
Type of star cluster
number of open clusters, such as the Pleiades, the Hyades and the Alpha Persei Cluster, are visible with the naked eye. Some others, such as the Double
Open_cluster
Constellation in the northern celestial hemisphere
was assigned by Johann Bayer to Perseus, where he designated it "Upsilon Persei (υ Per)", but it was moved to Andromeda by the International Astronomical
Andromeda_(constellation)
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
supergiant and OH/IR star. RSGC1-F06 (FMR2006 6) 1,382+298 −384 L/Teff S Persei 1,364±6 AD Oxygen-rich red supergiant. Also called a hypergiant. Stephenson
List_of_largest_stars
Gruis Star 1.77 1.75 Alioth Star 1.77 Alnitak Triple star system 1.79 Alpha Persei Star 1.79 Dubhe Binary star system 1.84 Delta Canis Majoris Star 1.85 Epsilon
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Lenticular galaxy in the constellation Perseus
1193 1220 1245 1342 1348 1444 1513 1528 1545 1582 1605 1624 Other Alpha Persei Cluster IC 348 Perseus OB1 Trumpler 2 Nebulae NGC 650 (Little Dumbbell Nebula)
IC_310
Binary star in the Pleiades star cluster
Publications of the Astronomical Society of Japan. 48 (2): 317–334. Bibcode:1996PASJ...48..317K. doi:10.1093/pasj/48.2.317. Mason, B. D.; et al. (1996). "Pleione"
Pleione_(star)
Nymph daughters of Oceanus
and the mother of Iris and the Harpies. Other notable Oceanids include: Perseis, wife of the Titan sun god Helios and mother of Circe, and Aeetes the king
Oceanids
Extinct Italic language of central Italy
grabouie orer ose persei ocre fisie pir orto est (26) toteme iouine arsmor dersecor subator sent pusei neip heritu. (27) dei crabouie persei tuer perscler
Umbrian_language
Hypothetical hybrid star type
star V595 Cassiopeiae 01h 43m 02.72s +56° 30′ 46.02″ Cassiopeia 2002 IO Persei 03h 06m 47.27s +55° 43′ 59.35″ Perseus 2002 KN Cassiopeiae 00h 09m 36.37s
Thorne–Żytkow_object
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
7 ± 0.7 Pegasus 22h 50m 00.19307s +24° 36′ 05.6926″ G8 III 3.514 Kappa Persei (Misam) 112.7 ± 0.8 Perseus 03h 09m 29.77156s +44° 51′ 27.1463″ G9.5 IIIb
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
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
Application in medieval astrology
designation Longitude (2020) Planet Gemstone Plant Symbol Algol Caput Larvæ Beta Persei 26 Taurus 26 Saturn & Jupiter diamond black hellebore Alcyone (or Pleiades)
Behenian_fixed_star
Farrington, C. (2015). "Spectral and spatial imaging of the Be+sdO binary ϕ Persei". Astronomy & Astrophysics. 577: A51. arXiv:1503.03423. Bibcode:2015A&A
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
The following nearest bright stars are found within 15.0 parsecs (48.9 ly) of the closest star, the Sun, and have an absolute magnitude of +8.5 or brighter
List_of_nearest_bright_stars
Hungarian astronomer, mathematician (1869–1932)
Harkányi B.: A Nova Persei (3.1901) photometrikus megfigyelése. Ógyallai Kis. Kiadv. 1. (1901) Harkányi B., A Nova (3.1901) Persei photometriai megfigyelése
Béla_Harkányi
trigonometry: radius = distance × sin( diameter_angle / 2 ) = 17,600 × sin(19′/2) = 48.6 ly. Nayak, P. K.; et al. (September 2018). "Star clusters in the Magellanic
List_of_largest_star_clusters
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
; et al. (February 2006). "The new orbital elements and properties of ɛ Persei". Astronomy and Astrophysics. 446 (2): 583–589. Bibcode:2006A&A...446..583L
List_of_most_massive_stars
Comparison of all orbital launch systems
500 3,700 to GEO Expendable 1 Plesetsk, Vostochny 2024 2024 Angara A5 / Persei Russia Khrunichev 54.9 m N/A 6,500 3,700 to GEO Expendable 1 Plesetsk,
Comparison of orbital launch systems
Comparison_of_orbital_launch_systems
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
Main sequence star
discovered in the past, such as around NGC 2547–ID8, HD 166191 and V488 Persei. List of extrasolar planetary collisions BD+20°307 Brown, A. G. A.; et al
ASASSN-21qj
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
Heterogeneous class of stars with unusual spectra
The only other Wolf–Rayet star brighter than magnitude 6 is θ Muscae (WR 48), a triple star with two O class companions. Both are WC stars. The "ex" WR
Wolf–Rayet_star
1999). "The Mass and Age of Very Low Mass Members of the Open Cluster alpha Persei". The Astrophysical Journal. 510 (1): 266–273. arXiv:astro-ph/9807145. Bibcode:1999ApJ
List_of_open_clusters
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
Chalcidoidea)" (PDF). Bulletin of the British Museum (Natural History) Entomology. 48: 131–395. Archived (PDF) from the original on 3 June 2021. Retrieved 1 May
List of organisms named after famous people (born 1800–1899)
List_of_organisms_named_after_famous_people_(born_1800–1899)
Phenomenon wherein objects appear to move about their true positions in the sky
unpublished version". The British Journal for the History of Science. 43 (1): 19–48. doi:10.1017/S0007087409990379. JSTOR 40731002. PMID 28974287. Media related
Aberration_(astronomy)
± 0.3 Leo Minor 09h 35m 39.50219s +35° 48′ 36.4770″ G8V 4.80/12.50 B M5V WISE 0325+0831 36.5 T7 Theta Persei$ A 36.6 ± 0.3 Perseus 02h 44m 11.98704s
List of star systems within 35–40 light-years
List_of_star_systems_within_35–40_light-years
+25° 42′ 37.392″ K1V 6.27 has 1 known planet Gliese 122 69.5 ± 2.1 MV 50 Persei 69.6 ± 1.2 Perseus 04h 08m 36.61660s +38° 02′ 23.0488″ F7V 5.52 HR 5070
List of star systems within 65–70 light-years
List_of_star_systems_within_65–70_light-years
Constellation in the northern celestial hemisphere
slow nova, similar to DQ Herculis. Like DQ Herculis, WZ Sagittae, Nova Persei 1901 and Nova Aquilae 1918, it is a very close binary with a very short
Auriga
Polyatomic ion (H3, charge +1)
in many other diffuse cloud sightlines, such as GCS 3–2, GC IRS 3, and ζ Persei. To approximate the path length of H+3 in these clouds, Oka used the steady-state
Trihydrogen_cation
Type of binary star system with a white dwarf and main-sequence star
magnitude at minimum: the prototype DQ Herculis, and the unusual slow nova, GK Persei. In intermediate polar systems, material stripped from a red dwarf secondary
Intermediate_polar
[@RussianSpaceWeb] (22 December 2023). "Roskosmos says "Orion" space tug (a.k.a. Persei/Block DM-03) was shipped to Vostochny spaceport for the first launch of
List of spaceflight launches in January–June 2024
List_of_spaceflight_launches_in_January–June_2024
Plexaura, Galaxaura, Dione, Melobosis, Thoe, Polydora, Cerceis, Pluto, Perseis, Ianeira, Acaste, Xanthe, Petraea, Menestho, Europa, Metis, Eurynome, Telesto
List_of_Oceanids
binary Algol type (EA/SD) (prototype) The Demon Star DY Persei R Coronae Borealis / DY Persei / (prototype) φ Per (Dajiangjunbei) 3m.96 4m.11 0.15 19
List_of_variable_stars
Ancient region and kingdom in the Balkans
Philip V of Macedon conquered the rest by capturing Bylazora; after this Perseis and Astraion were founded. The citizens of Paeonian cities were not Macedonians
Paeonia_(kingdom)
+01° 14′ 39″ 14.2 868 Spiral galaxy Cetus 02h 15m 58.4s −00° 42′ 48″ 15.6 869 h Persei Cluster Open cluster Perseus 02h 19m +57° 09′ 5.7 870 Galaxy Aries
List_of_NGC_objects_(1–1000)
Dark nebula in the constellation Camelopardalis
(α Persei), the brightest star in the constellation of Perseus, located at the center of a bright association of blue stars known as the Alpha Persei Cluster
Camelopardalis_dark_region
Fourth stage on the Angara rockets
Structural weight reduction. In 2014 RSC Energia designated two versions: 14S48 Persei (Perseus) and 14S49, which incorporated most features of the proposed 11S861-03
Blok_DM-03
S 40° 3.2 8 Menkar α Ceti nose (of the whale) 315 N 04° 2.5 9 Mirfak α Persei elbow of the Pleiades 309 N 50° 1.82 10 Aldebaran α Tauri follower (of the
List_of_stars_for_navigation
French dynasty
23 August 1240 Barony of Sully [fr] Alix de Brienne 1177 four children? Perseis d'Aschères no children Margaret no children 23 August 1240 Sully-sur-Loire
House_of_Blois
Messier marathon
Binoculars 88 NGC 288 Globular cluster Scl Telescope - Binoculars 89 Alpha Persei Cluster Open cluster Per Binoculars 90 NGC 1342 Open cluster Per Telescope
Sufi_Observing_Competition
0821-669‡ 34.44 ± 0.20 DA9.8 2MASS J00501994−3322402§ 34.5 ± 0.9 T7 Iota Persei$ 34.50 ± 0.05 Perseus 03h 09m 04.019s +49° 36′ 47.80″ G0V 4.05# L 98-59
List of star systems within 30–35 light-years
List_of_star_systems_within_30–35_light-years
Type of eruptive variable star
atmospheric hydrogen deficiencies, and obviously the intermittent fadings. The DY Persei variables have been considered a sub-class of R CrB variable, although they
R_Coronae_Borealis_variable
Binary star system in the constellation Carina
Landsman, Wayne; et al. (March 1996), "The White-Dwarf Companions of 56 Persei and HR 3643", Publications of the Astronomical Society of the Pacific, 108:
HR_3643
−64° 52′ 16.53″ A5-7 IV-V 4.77 34.7355 ± 0.1575 planetary collision Algol (Beta Persei/Demon Star) A$ 94 ± 2 Perseus 03h 08m 10.13245s +40° 57′ 20.3280″ B8 V 2
List of star systems within 90–95 light-years
List_of_star_systems_within_90–95_light-years
arXiv:2012.05220. Bibcode:2021AJ....161..147B. doi:10.3847/1538-3881/abd806. SU Persei's database entry at VizieR. Anugu, Narsireddy; Baron, Fabien; et al. (October
List of stars with resolved images
List_of_stars_with_resolved_images
Astronomical event where one body is hidden by another
2007-05-01. Price, Aaron (January 1999). "Variable Star Of The Month: Beta Persei (Algol)". AAVSO. Archived from the original on 2007-04-05. Retrieved 2007-05-01
Eclipse
Heap of Corpses Pi Persei Gorgonea Secunda Perseus A single-star asterism in the Stomach mansion. 積水 Jī Shuǐ Stored Water Lambda Persei 天讒 Tiān Chán Celestial
List_of_Chinese_star_names
White dwarf
1193 1220 1245 1342 1348 1444 1513 1528 1545 1582 1605 1624 Other Alpha Persei Cluster IC 348 Perseus OB1 Trumpler 2 Nebulae NGC 650 (Little Dumbbell Nebula)
ZTF_J0139+5245
48 PERSEI
48 PERSEI
Surname or Lastname
English
English : perhaps a variant of Babb. In the British Isles it is now most common in mid-Wales and in the border county of Shropshire, where it is recorded from the 16th century.William Bebb (1802–73), Governor of OH 1846–48, was a descendant of an immigrant from Montgomeryshire, Wales.
Surname or Lastname
English
English : habitational name from Bagby in North Yorkshire, recorded in Domesday Book as Baghebi, from the Old Norse personal name Baggi + Old Norse býr ‘farmstead’, ‘village’.Scottish : possibly from Begbie in East Lothian.James Bagby, a Scot, arrived in Jamestown, VA, in about 1628. One of his descendants, Arthur Pendleton Bagby (1794–1858), was governor of Alabama (1837–1841) and a U.S. senator (1841–48).
Surname or Lastname
English
English : from the Middle English female personal name Mau(l)d, a reduced form of the Norman name Mathilde, Matilda, composed of the Germanic elements maht ‘might’, ‘strength’ + hild ‘strife’, ‘battle’. The learned form Matilda was much less common in the Middle Ages than the vernacular forms Mahalt, Maud and the reduced pet form Till. The name was borne by the daughter of Henry I of England, who disputed the throne of England with her cousin Stephen for a number of years (1137–48). In Germany the popularity of the name in the Middle Ages was augmented by its being borne by a 10th-century saint, wife of Henry the Fowler and mother of Otto the Great.
48 PERSEI
48 PERSEI
Surname or Lastname
English
English : topographic name for someone who lived near an ash tree, or a habitational name from a place named with the Old English word æsc (see Ash). The Anglo-Norman French preposition de ‘of’, ‘from’ has become fused to the name.Americanized spelling of German Dasch.Indian : variant of Das.
Boy/Male
Muslim
Eagle
Girl/Female
Muslim
Righteous
Boy/Male
Australian, Biblical
Twin
Girl/Female
American, Australian, British, English, Scottish
Young Fighter; Female Version of Evan; Right Handed; Young Warrior
Girl/Female
Hindu, Indian, Malayalam, Marathi, Sanskrit
Achieving
Boy/Male
Hindu, Indian, Punjabi, Sikh
King; King of Kings
Boy/Male
Hindu
Female
English
 Medieval Latin name ROSA means "rose." Compare with another form of Rosa.
Boy/Male
Tamil
48 PERSEI
48 PERSEI
48 PERSEI
48 PERSEI
48 PERSEI
n.
A silver coin of Florence, first struck in the twelfth century, and noted for its beauty. The name is given to different coins in different countries. The florin of England, first minted in 1849, is worth two shillings, or about 48 cents; the florin of the Netherlands, about 40 cents; of Austria, about 36 cents.
n.
One of a group of shooting stars which appear yearly about the 10th of August, and cross the heavens in paths apparently radiating from the constellation Perseus. They are beleived to be fragments once connected with a comet visible in 1862.
a.
Having the characteristics of Circe, daughter of Sol and Perseis, a mythological enchantress, who first charmed her victims and then changed them to the forms of beasts; pleasing, but noxious; as, a Circean draught.
n.
Leap year; every fourth year, in which a day is added to the month of February on account of the excess of the tropical year (365 d. 5 h. 48 m. 46 s.) above 365 days. But one day added every four years is equivalent to six hours each year, which is 11 m. 14 s. more than the excess of the real year. Hence, it is necessary to suppress the bissextile day at the end of every century which is not divisible by 400, while it is retained at the end of those which are divisible by 400.
n.
The principles of a political party in England (1838-48), which contended for universal suffrage, the vote by ballot, annual parliaments, equal electoral districts, and other radical reforms, as set forth in a document called the People's Charter.