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Triple star or quadruple star system in the constellation Perseus
56 Persei is at least a triple star and possibly a quadruple star system in the northern constellation of Perseus. It is visible to the naked eye as a
56_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
1 Lacerta 22h 08m 40.818s +45° 44′ 32.11″ K0IVe 6.080 B G2IV C DA(?) 56 Persei A 138.7 ± 0.5 Perseus 04h 24m 37.46102s +33° 57′ 35.2908″ F4V 5.77 B DA3
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
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 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
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 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
HR_3643
Red giant star in the constellation Andromeda
51 Andromedae, Gamma Andromedae, Phi Persei, 49 Andromedae, Chi Andromedae, Upsilon Andromedae, Tau Andromedae, 56 Andromedae, Beta Trianguli, Gamma Trianguli
51_Andromedae
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
884, χ Persei, one half of the famous Double Cluster. In March of 1904, Lidiya Tseraskaya discovered that the star, then referred to as BD+56°583, is
RS_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
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
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
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
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
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
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
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
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
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
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
Chinese constellation
Andromedae γ Andromedae 54 Andromedae* 2 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
Tian_Dajiangjun
"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
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
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
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
Observatory
succeeded in obtaining further photographic evidence of the nebula at ξ Persei (now called the "California Nebula"). After building the giant telescope
Archenhold_Observatory
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
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
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
Star in the constellation Perseus
21 Persei is a single, variable star in the northern constellation of Perseus, located about 331 light years away from the Sun. It is visible to the naked
21_Persei
Mythology of the Night Sky. Patrick Moore's Practical Astronomy Series. pp. 19–56. doi:10.1007/978-1-4614-0137-7_3. ISBN 978-1-4614-0136-0. S2CID 115168457
List_of_proper_names_of_stars
– 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
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
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)
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
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
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)
Volantis 720 L/Teff V1111 Ophiuchi (IRC +10365) 720 – 900 L/Teff XX Persei 718+80 −56 AD RX Telescopii 716 L/Teff V Camelopardalis 716±185 AD CD–61°3575
List_of_largest_stars
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
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
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
Configuration. Future launches using DM-03 upper stage will fly on Angara A5 as Persei/Orion Upper stage from Plesetsk and Vostochny and is the last time the upper
List of spaceflight launches in January–March 2026
List_of_spaceflight_launches_in_January–March_2026
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
Constellations recognized by the International Astronomical Union
(mythological winged horse) Enif 2.40 1121 Perseus /ˈpɜːrsiəs/ Per Pers Persei /ˈpɜːrsiaɪ/ ancient (Ptolemy) Perseus (mythological character) Mirfak 1
IAU_designated_constellations
+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 02h 17m
List_of_NGC_objects_(1–1000)
American television sitcom (1955–1956)
of these days, Ndnd, bang! zoom! straight to the third moon of Omicron Persei 8!!" The Moonlighting episode "A Trip to the Moon" contains a lengthy parody
The_Honeymooners
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
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
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
and the easiest to see in the night sky. RSGC2 (Stephenson 2) 26.1 Alpha Persei cluster 22.8 Jewel Box 20 Hyades 17.6 Nearest open cluster Beehive Cluster
List_of_largest_star_clusters
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
Classification of stars based on spectral properties
Annals of the Astronomical Observatory of Harvard College. 56 (5): 115. Bibcode:1912AnHar..56..115C. Hearnshaw (1986) pp. 121–122 "Annie Jump Cannon". www
Stellar_classification
"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
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
[@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
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 - 3
List of star systems within 450–500 light-years
List_of_star_systems_within_450–500_light-years
Heterogeneous class of stars with unusual spectra
"Classification and temperatures of Wolf–Rayet stars". The Observatory. 56: 196–197. Bibcode:1933Obs....56..196B. Swings, P. (1942). "The spectra of Wolf–Rayet stars
Wolf–Rayet_star
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
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 in the constellation Andromeda
Great General, together with γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, θ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli, γ Trianguli and
Chi_Andromedae
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
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
Carinae 6000 G0-4-Ia+ 485 ± 56 24±5.1 212000±12300 3.83 V602 Carinae 7000 M3 Ia-Iab 1015 17.7 – 20 126000 8.39 S Persei 7900±300 M3 Iae–M7 1298+64 −57
List_of_nearest_hypergiants
Binary star in the constellation Triangulum
consisting of δ Trianguli, γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli and γ Trianguli
Delta_Trianguli
Medieval instruction manual on the astrolabe by Geoffrey Chaucer
25–27. Robinson 1983, Prologue lines 30-36. Robinson 1983, Prologue lines 56–57. Skeat 1900, Introduction, sections 2-4. Skeat 1900, Introduction section
A_Treatise_on_the_Astrolabe
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 Andromeda
Upsilon Andromedae, Gamma Andromedae, Phi Persei, 51 Andromedae, 49 Andromedae, Chi Andromedae, Tau Andromedae, 56 Andromedae, Beta Trianguli, Gamma Trianguli
Upsilon_Andromedae
was a brighter nova than HR Lyrae (+6.5) Prialnik, Dina. "Novae", pp. 1846-56, in Paul Murdin, ed. Encyclopedia of Astronomy and Astrophysics. London: Institute
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
and references Zeta Ophiuchi 440 ± 40 1 O9.5 V 2.56 – 2.58 The closest O-type star to Earth. Phi Persei B 720 ± 30 1 sdO 4.06 Has a B-type companion star
List_of_O-type_stars
Astronomy catalogue
vdB 46 vdB 47 vdB 48 vdB 49 vdB 50 vdB 51 vdB 52 vdB 53 vdB 54 vdB 55 vdB 56 vdB 57 vdB 58 vdB 59 vdB 60 vdB 61 vdB 62 vdB 63 vdB 64 vdB 65 vdB 66 vdB
Van_den_Bergh_Catalog
; 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
Melis, Carl; Gáspár, András (2021-09-01). "Extreme Variability of the V488 Persei Debris Disk". The Astrophysical Journal. 918 (2): 71. arXiv:2108.02901.
List of extrasolar planetary collisions
List_of_extrasolar_planetary_collisions
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
Star in the constellation of Leo Minor
orbits from photoelectric radial velocities - Paper 200: Kappa Persei, Beta Leonis Minoris, 56 Ursae Majoris, HR 4593, and 39 Cygni". The Observatory. 128:
Beta_Leonis_Minoris
+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
Star in the constellation Cygnus
mentioned in the paper. 6 Geminorum BI Cygni NR Vulpeculae RS Persei RW Cygni S Persei SU Persei TV Geminorum V424 Lacertae List of largest stars "ASAS-SN
AZ_Cygni
Parameters of Our Sample of M and K Dwarfs". The Astronomical Journal. 158 (2): 56. arXiv:1905.07921. Bibcode:2019AJ....158...56H. doi:10.3847/1538-3881/ab23fe
List_of_smallest_known_stars
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
8998-760-1) 307.3 ± 0.3 K3IV 11.19 Has two confirmed exoplanet (YSES-1b & c). Rho Persei (Gorgonea Tertia) 308 ± 7 Perseus M4 II +1.65 HD 224693 (Axólotl) 308.3
List of star systems within 300–350 light-years
List_of_star_systems_within_300–350_light-years
Star in the constellation Andromeda
asterism consisting of γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli, γ Trianguli
Gamma_Andromedae
Hypothetical hybrid star type
unlikely super-AGB 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
Thorne–Żytkow_object
Binary star in the constellation Triangulum
consisting of β Trianguli, γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, τ Andromedae, 56 Andromedae, γ Trianguli and δ Trianguli
Beta_Trianguli
Stars sorted by absolute magnitude
Scorpius OB2) 38,000 -6.71 440 2.307 (combined) 27,400 SIMBAD ε Persei A (in α Persei Cluster) 28,300 -6.391 640 2.88 (combined) 26,500 SIMBAD θ Carinae
List_of_most_luminous_stars
Catalogue of 245 star clusters compiled By British astronomer Philibert Jacques Melotte
cluster Andromeda 5.7 Mel 13 NGC 869 h Persei of Double Cluster Open cluster Perseus 3.7 Mel 14 NGC 884 χ Persei of Double Cluster Open cluster Perseus
Melotte_catalogue
Binary near-Earth asteroid
pair of asteroids of approximately equal size and mass, each about 0.9 km (0.56 mi) in diameter. Classified as a near-Earth asteroid and potentially hazardous
2017_YE5
Latin Catholic diocese in Hungary
1562–1563 András Dudich 1563–1572 Gergely V Bornemissza 1572–1582 Boldizsár Persei Melegh 1582–1587 István III Mathisy 1587–1597 Pál III Szegedy 1598–1608
Diocese_of_Szeged–Csanád
−38° 52′ 56.6″ 36.3 HD 85512 K5V 7.67 7.43 09h 51m 06.31s −43° 30′ 10.0″ 36.4 11 Leonis Minoris A G8V 5.40 5.16 09h 35m 39.50s +35° 48′ 36.5″ 36.5 θ Persei A
List_of_nearest_bright_stars
Star in the constellation Triangulum
consisting of γ Trianguli, γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli, and δ Trianguli
Gamma_Trianguli
105.6 12 Persei Perseus 78.9 ± 0.8 4.94 F9 V 107 Theta Persei Perseus 36.29 ± 0.09 4.11 / 9.987 F8 V + M1.5 V 108 Iota Horologii Horologium 56.61 ± 0.04
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
20h 44m 02.33404s −51° 55′ 15.4970″ A9IV 4.52 Wolf 1106 78.84 sdM1.5 12 Persei A 78.9 ± 0.8 Perseus 02h 42m 14.91569s +40° 11′ 38.1898″ F9V B F 2MASSW
List of star systems within 75–80 light-years
List_of_star_systems_within_75–80_light-years
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 +49° 13′ 42.4111″ F7V 4.12/10# B
List of star systems within 35–40 light-years
List_of_star_systems_within_35–40_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
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
(2010). "ICE Breakers" (PDF). American Entomologist. 56 (3): 132–133+ 185. doi:10.1093/ae/56.3.132. Archived (PDF) from the original on 2016-08-20.
List of organisms named after famous people (born 1800–1899)
List_of_organisms_named_after_famous_people_(born_1800–1899)
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
−34° 40′ 04.6″ 5.29 0.06 363 B9/B9.5V 53 Persei variable HD 46815 106 46815 31299 06h 33m 49.49s −36° 13′ 56.2″ 5.42 −0.06 406 K3III HD 37811 39 37811
List_of_stars_in_Columba
Star in the constellation Cygnus
orbits from photoelectric radial velocities - Paper 200: Kappa Persei, Beta Leonis Minoris, 56 Ursae Majoris, HR 4593, and 39 Cygni", The Observatory, 128:
39_Cygni
56 PERSEI
56 PERSEI
56 PERSEI
56 PERSEI
Surname or Lastname
English
English : unexplained; possibly from the legal term bailor ‘one who delivers goods’.
Boy/Male
Tamil
Harivansh | ஹரிவஂஷ
Belonging to the family of Hari
Girl/Female
Bengali, Indian
To do Something
Girl/Female
Tamil
Dhrushma | தà¯à®°à¯à®·à®®à®¾à®‚
Doshima
Boy/Male
Tamil
Decent, Beautiful
Girl/Female
Arabic, Australian, French, Muslim
Right Guidance; Variant of Huda
Boy/Male
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Punjabi, Sikh, Telugu
Leader; God; Master
Girl/Female
Arabic, Muslim
Glorious; Powerful
Girl/Female
Tamil
Excellent, Highest social standing, Tall, Towering
Girl/Female
American, Australian, British, English, German
Little and Womanly; Feminine Variant of Charles
56 PERSEI
56 PERSEI
56 PERSEI
56 PERSEI
56 PERSEI
v. t.
To add (any given number or quantity) to itself a certain number of times; to find the product of by multiplication; thus 7 multiplied by 8 produces the number 56; to multiply two numbers. See the Note under Multiplication.
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.
The arc or portion of the equator intersected between the meridian of a given place and the meridian of some other place from which longitude is reckoned, as from Greenwich, England, or sometimes from the capital of a country, as from Washington or Paris. The longitude of a place is expressed either in degrees or in time; as, that of New York is 74¡ or 4 h. 56 min. west of Greenwich.
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.
n.
A number or quality which is contained in another an exact number of times, or is an aliquot part of it; thus, 7 is the submultiple of 56, being contained in it eight times.