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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
V_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
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 in the constellation Perseus
S Persei is a red supergiant or hypergiant located near the Double Cluster in Perseus, north of the open cluster NGC 869. It is a member of the Perseus
S_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
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
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
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
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
Open cluster in the constellation Perseus
The Alpha Persei Cluster, also known as Melotte 20 or Collinder 39, is an open cluster of stars in the northern constellation of Perseus. To the naked
Alpha_Persei_Cluster
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 system in the constellation Perseus
Epsilon Persei, Latinized from ε Persei, formally named Áldu, is a Triple star system in 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
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
1877 AB Boötis +4.5 1887 V Persei +4.0 1891 T Aurigae +3.8 1898 V1059 Sagittarii +4.5 1899 V606 Aquilae +5.5 1901 GK Persei +0.2 1903 DM Geminorum +4
List of novae in the Milky Way galaxy
List_of_novae_in_the_Milky_Way_galaxy
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
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
Scottish astronomer (1857–1911)
310 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
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 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
Open clusters in the constellation Perseus
of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation
Double_Cluster
Star in the constellation Perseus
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
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
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
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)
Main sequence star in the constellation Perseus
consisting of ι Persei, 9 Persei, τ Persei, κ Persei, β Persei, ρ Persei, 16 Persei and 12 Persei. Consequently, the Chinese name for ι Persei itself is 大陵三
Iota_Persei
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
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
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
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
Star in the constellation Perseus
31 Persei is a single star in the northern constellation of Perseus. It is visible to the naked eye as a dim, blue-white hued point of light with an apparent
31_Persei
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
Open cluster in the constellation Perseus
NGC 869 (also known as h Persei) is an open cluster of stars located around 7,460 light years away in the constellation of Perseus. The cluster is around
NGC_869
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
Blue supergiant star in the constellation Perseus
9 Persei is a single variable star in the northern constellation Perseus, located around 4,300 light years away from the Sun. It has the Bayer designation
9_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 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
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
Cataclysmic variable star in the constellation Perseus
UV Persei (UV Per) is a cataclysmic variable star of the SU Ursae Majoris subclass of dwarf novae, located in the constellation Perseus. It is catalogued
UV_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
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
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
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 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
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
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
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
Sigma Persei (Sigma Per, σ Persei, σ Per) is an orange K-type giant star with an apparent magnitude of +4.36. It is approximately 343 light-years from
Sigma_Persei
Star in the constellation Perseus
50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.52, which is bright enough to be seen with the naked eye. Located around
50_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
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)
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
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
Star in the constellation Perseus
than the Crab Nebula gamma-ray source out to photon energies of about 500 keV. The mass of the black hole in GRO J0422+32 falls in the range 3.66 to 4.97
GRO_J0422+32
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
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
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
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
Stellar classification distinguished by bright blue luminosity
the standards Acrab (B2 V), 29 Persei (B3 V), HD 36936 (B5 V), and HD 21071 (B7 V). Gray & Garrison (1994) contributed two B9 V standards: Omega Fornacis
B-type_main-sequence_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
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
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
59 Persei is a suspected astrometric binary star system in the northern constellation of Perseus. It is visible to the naked eye as a dim, white-hued star
59_Persei
Star in the constellation Perseus
14 Persei is a single star in the northern constellation Perseus, located roughly 1,900 light years away from the Sun. It is visible to the naked eye as
14_Persei
Star in the constellation Perseus
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
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
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
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
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
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
54 Persei is a single star in the northern constellation of Perseus. It is visible to the naked eye as a faint, yellow-hued star with an apparent visual
54_Persei
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
Yellow-white hued star in the constellation Perseus
ν Persei, Latinized as Nu Persei, is a single star and a suspected variable in the northern constellation of Perseus. It has a yellow-white hue and is
Nu_Persei
Star in the constellation Perseus
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
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
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
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
17 Persei is a single star in the northern constellation of Perseus, located about 420 light years away from the Sun. It is visible to the naked eye as
17_Persei
Star in the constellation Perseus
49 Persei is a star in the northern constellation of Perseus. It is just visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude
49_Persei
Binary star system
KS Persei is a binary system in the equatorial constellation of Perseus. It is sometimes known as Bidelman's Star, named after William P. Bidelman. The
KS_Persei
Star in the constellation Perseus
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
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
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
Nova in the constellation Perseus
V392 Persei, also known as Nova Persei 2018, is a bright nova in the constellation Perseus discovered on April 29, 2018. It was previously known as a
V392_Persei
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
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
Star in the constellation Perseus
8 Persei is a single star in the northern constellation of Perseus, located 416 light years away from the Sun. It is visible to the naked eye as a dim
8_Persei
– 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
American space and aeronautics agency
New Horizons, 2015 Helix Nebula by Spitzer Space Telescope, 2007 1901 GK Persei supernova by Chandra X-ray Observatory, 2015 Carina Nebula by Hubble Space
NASA
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
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
Binary star in the Pleiades star cluster
in the IAU Catalog of Star Names. With an apparent magnitude of +5.05 in V, the star is rather difficult to make out with the naked eye, especially since
Pleione_(star)
Star in the constellation Perseus
57 Persei, or m Persei, is a suspected triple star system in the northern constellation of Perseus. It is at the lower limit of visibility to the naked
57_Persei
Open cluster in the constellation Perseus
NGC 884 (also known as χ Persei) is an open cluster of stars located 7,640 light years away in the constellation of Perseus. It is the east component of
NGC_884
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
Star in the constellation Perseus
Persei is a single star located 149 light years away from the Sun in the northern constellation of Perseus. It has the Bayer designation of l Persei,
32_Persei
Star in the constellation Perseus
also listed in the General Catalogue of Variable Stars as V1024 Persei. V1024 Persei was initially named as Ross 4 in 1925, on the basis of photographic
NSV_1436
Star in the constellation Perseus
11 Persei is a single star in the constellation of Perseus, located about 418 light years away from the Sun. It is visible to the naked eye as a dim, blue-white
11_Persei
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