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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
29_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
Stellar classification distinguished by bright blue luminosity
Abt, & Tapscott (1978) further contributed the standards Acrab (B2 V), 29 Persei (B3 V), HD 36936 (B5 V), and HD 21071 (B7 V). Gray & Garrison (1994) contributed
B-type_main-sequence_star
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 in the constellation Perseus
GK Persei (also Nova Persei 1901) was a bright nova first observed on Earth in 1901. It was discovered by Thomas David Anderson, an Edinburgh clergyman
GK_Persei
Star system in the constellation Perseus
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
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
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
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
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
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
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 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 dwarf
V392_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
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
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
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
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
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 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
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
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
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
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
55 Persei is a single, blue-white hued star in the northern constellation Perseus. It is faintly visible to the naked eye under good seeing conditions
55_Persei
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
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
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
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
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
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
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
additions were done on 1 February 2017 (13 new star names), 30 June 2017 (29), 5 September 2017 (41), 17 November 2017 (3), 1 June 2018 (17), and on 10
List_of_proper_names_of_stars
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 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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
– 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
Classification of stars based on spectral properties
"Spectral Classification". Annual Review of Astronomy and Astrophysics. 11: 29–50. Bibcode:1973ARA&A..11...29M. doi:10.1146/annurev.aa.11.090173.000333.
Stellar_classification
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
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
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
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
"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
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
Retrieved 2022-08-29. "* Zet02UMa". simbad.u-strasbg.fr. Retrieved 2022-08-29. "VSX : Detail for bet And". www.aavso.org. Retrieved 2022-08-29. "VSX : Detail
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
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
52 Persei is a suspected triple star system in the northern constellation of Perseus. It has the Bayer designation f Persei, while 52 Persei is the Flamsteed
52_Persei
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)
Stellar association
Milky Way. The brightest member of the association is the blue supergiant 9 Persei. "Per OB1". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved
Perseus_OB1
O9.5Vn HD 73882 2,400 ± 100 1 O8.5IV 7.19 - 7.29 1 Camelopardalis A 2,580 ± 100 1 O9.7IIn 5.77 X Persei 2,600 ± 100 1 O9.5IIIe-B0Ve 6.778 NSVS 14256825
List_of_O-type_stars
Constellations recognized by the International Astronomical Union
constellations: Carina, Puppis, and Vela. The 88 constellations depict 42 animals, 29 inanimate objects, and 17 humans or mythological characters. Each IAU constellation
IAU_designated_constellations
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
"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
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
Russian heavy-lift launch vehicle
test flight. Orbital test flight No.2. 27 December 2021 19:00 Angara A5 / Persei 71753 Plesetsk, Site 35/1 Partial Failure IPN №1 (MGM №3) Geocentric supersynchronous
Angara_A5
Star in the constellation Perseus
4 Persei is a single star in the northern constellation of Perseus, located around 670 light years away from the Sun. It is visible to the naked eye as
4_Persei
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
arXiv:1507.05823. doi:10.1093/mnras/stv1809. Kilpatrick, Charles D.; et al. (29 June 2023). "EType II-P supernova progenitor star initial masses and SN 2020jfo:
List_of_largest_stars
descriptions of four new species". Zoosystematica Rossica. 29 (2): 301–315. doi:10.31610/zsr/2020.29.2.301. Kozur HW, Moix P, Ozsvárt, P (2007). "Stratigraphically
List of organisms named after famous people (born 1800–1899)
List_of_organisms_named_after_famous_people_(born_1800–1899)
Historical region of Georgia
Aeëtes Aeëtes, King of Colchis, son of the sun-god Helios and the Oceanid Perseis (a daughter of Oceanus), brother of Circe and Pasiphae, and father of Medea
Colchis
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 3.80 Delta Aquarii
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
Open cluster in Perseus
approximately 6m 42s east and 10′ 12″ south from the nearest visible star, γ Persei. NGC 1220 consists of approximately 26 stars with spectral types between
NGC_1220
Group of stars
clusters are the Pleiades and Hyades in Taurus. The Double Cluster of h+Chi Persei can also be prominent under dark skies. Open clusters are often dominated
Star_cluster
Phenomenon wherein objects appear to move about their true positions in the sky
as inertial. In the Earth's frame, the Sun moves, at a mean velocity v = 29.789 km/s, by a distance Δ x = v t {\displaystyle \Delta x=vt} ≈ 14,864.7 km
Aberration_(astronomy)
Russian family of space launch vehicles
booster, Persei. Only the launch of Angara-A5 with Persei upper stage ended up happening in 2021. The maiden flight of Angara 1.2 happened on 29 April 2022
Angara_(rocket_family)
Star whose brightness fluctuates, as seen from Earth
from a planetary nebula undergoes helium flash, becoming a supergiant. DY Persei variables are considered a subclass of cool R CrB variables. They are carbon-rich
Variable_star
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
+ 16.77 AC:K3 V + M7 V B:M3.5 V 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
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
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
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
Star in the constellation Canis Major
similar to other very late-type OH/IR red supergiants such as MY Cephei, S Persei, VX Sagittarii, and NML Cygni. Such stars were also referred to as "S Per
VY_Canis_Majoris
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
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 20 123000 – 186000 9.23 6 Cassiopeiae 8000
List_of_nearest_hypergiants
Ancient Greek mythological figure
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
Tethys_(mythology)
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
Scottish astronomer (1857–1911)
variable stars, and 10 novae. This includes the Horsehead Nebula and V Persei. In 1888, Fleming discovered the Horsehead Nebula on a telescope-photogrammetry
Williamina_Fleming
+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
Extinct Italic language of central Italy
daetom est tuer perscler uirseto auirseto uas est. di grabouie persei mersei esu bue (29) peracrei pihaclu pihafei. di.grabouie pihatu ocre fisei pihatu
Umbrian_language
; 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
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
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
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
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
Study of the movement of stars
Local Association (Pleiades moving group) AB Doradus moving group Alpha Persei moving cluster Beta Pictoris moving group Castor moving group Corona Australis
Stellar_kinematics
−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
Comparison of all orbital launch systems
December 2022. Retrieved 20 March 2023 – via Twitter. Percival, Claire (2022-05-29). "OFT-2 CST-100 Starliner (Uncrewed) | Atlas V N22". Everyday Astronaut.
Comparison of orbital launch systems
Comparison_of_orbital_launch_systems
29 PERSEI
29 PERSEI
Surname or Lastname
English, French, German, Dutch, Danish, and South Indian
English, French, German, Dutch, Danish, and South Indian : from the medieval personal name, of Biblical origin, from Aramaic t’Åm’a, a byname meaning ‘twin’. It was borne by one of the disciples of Christ, best known for his scepticism about Christ’s resurrection (John 20:24–29). The th- spelling is organic, the initial letter of the name in the Greek New Testament being a theta. The English pronunciation as t rather than th- is the result of French influence from an early date. In Britain the surname is widely distributed throughout the country, but especially common in Wales and Cornwall. The Ukrainian form is Choma.
Surname or Lastname
Americanized spelling of Jewish Leykin (from Belarus), a metronymic from Leyke, a pet form of the Yiddish female personal name Leye, from the Hebrew female personal name Lea, from which English Leah is derived (see Genesis 29
Americanized spelling of Jewish Leykin (from Belarus), a metronymic from Leyke, a pet form of the Yiddish female personal name Leye, from the Hebrew female personal name Lea, from which English Leah is derived (see Genesis 29 : 16) + the Slavic possessive suffix -in.English : from a medieval personal name, a diminutive of Lawrence. Compare Law 1 and Larkin.
29 PERSEI
29 PERSEI
Boy/Male
Hindu, Indian
A Friend
Surname or Lastname
English (Lancashire and Yorkshire)
English (Lancashire and Yorkshire) : habitational name from Burnley in Lancashire, so named with the Old English river name Brun (from brūn ‘brown’ or burna ‘stream’) + lēah ‘woodland clearing’.
Boy/Male
Tamil
The first Vedas, Lord Ganesh, Knower of the arthara Vedas
Surname or Lastname
English (West Yorkshire)
English (West Yorkshire) : apparently a habitational name, probably from any of various places called Normanton, notably the one in West Yorkshire, which are named with Old English Northman ‘Norseman’, ‘Viking’ + tūn ‘settlement’.
Girl/Female
Indian
Loud voice, Sound
Boy/Male
Tamil
Joy, Happiness
Boy/Male
Tamil
Charuvardhana | சாரà¯à®µà®°à¯à®¤à®¨à®¾
One who enhances beauty
Girl/Female
British, English
Bright Fame
Boy/Male
Indian, Sanskrit
Friend of the Earth; A Ruler
Boy/Male
American, British, English, French, Irish
Little Rock; Surname Derived from a Medieval Given Name; Nineteenth-century Irish Nationalist Charles Parnell
29 PERSEI
29 PERSEI
29 PERSEI
29 PERSEI
29 PERSEI
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.
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.
Inserted or introduced among others in the calendar; as, an intercalary month, day, etc.; -- now applied particularly to the odd day (Feb. 29) inserted in the calendar of leap year. See Bissextile, n.
n.
The period of a synodic revolution of the moon, or the time from one new moon to the next; varying in length, at different times, from about 29/ to 29/ days, the average length being 29 d., 12h., 44m., 2.9s.