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Star in the constellation Cassiopeia
47 Cassiopeiae (also designated as or called 47 Cas, HR 581, HD 12230, and HIP 9727) is an F-type main-sequence star located about 108 light-years away
47_Cassiopeiae
Yellow hypergiant star in the constellation Cassiopeia
Rho Cassiopeiae is a yellow hypergiant star in the constellation Cassiopeia. Its name is a Bayer designation, pronounced /ˌroʊ kæsiəˈpiːaɪ, -sioʊ-, -iː/
Rho_Cassiopeiae
Star system in the constellation Cassiopeia
Gamma Cassiopeiae, Latinized from γ Cassiopeiae formally named Tiansi, is a multiple star system at the center of the distinctive "W" asterism in the
Gamma_Cassiopeiae
Former constellation
brightest star in the constellation was 50 Cassiopeiae. Other stars include 23 Cassiopeiae, 47 Cassiopeiae, 49 Cassiopeiae, and γ Camelopardalis. Bode also gave
Custos_Messium
Binary star system in the constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from η Cassiopeiae
Eta_Cassiopeiae
Star system in the constellation Cassiopeia
AR Cassiopeiae (AR Cas) is a variable star in the constellation of Cassiopeia. It is thought to be a member of a septuple star system, one of only two
AR_Cassiopeiae
B-type star in the constellation Cassiopeia
Nu Cassiopeiae is a solitary star in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ν Cassiopeiae, and
Nu_Cassiopeiae
Star in the constellation Cassiopeia
Upsilon2 Cassiopeiae is a solitary star in the constellation of Cassiopeia, a few degrees to the south of Gamma Cassiopeiae. It has the proper name Castula
Upsilon2_Cassiopeiae
Open star cluster in the constellation Cassiopeia
Dragonfly Cluster, E.T. Cluster, Owl Cluster, Kachina Doll Cluster or Phi Cassiopeiae Cluster. It was discovered by German-British astronomer William Herschel
NGC_457
Star in the constellation Cassiopeia
consisting of θ Cassiopeiae, ι Cassiopeiae, ε Cassiopeiae, δ Cassiopeiae, ν Cassiopeiae and ο Cassiopeiae. Consequently, θ Cassiopeiae itself is known
Theta_Cassiopeiae
Star in the constellation Cassiopeia
Upsilon1 Cassiopeiae is an astrometric binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized
Upsilon1_Cassiopeiae
Star in the constellation Cassiopeia
12 Cassiopeiae (12 Cas) is a white giant in the constellation Cassiopeia, about 860 light years away. It has an apparent magnitude of 5.4, so it faintly
12_Cassiopeiae
Star in the constellation Cassiopeia
Omicron Cassiopeiae is a triple star system in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from ο Cassiopeiae, and abbreviated
Omicron_Cassiopeiae
Variable star in the constellation Perseus
surrounded by a disk of expelled material. This qualifies it as a Gamma Cassiopeiae variable, and the visual range is magnitude 6 - 7. In 1989 and 1990,
X_Persei
Star in the constellation Cassiopeia
Chi Cassiopeiae is a solitary, yellow-hued star in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from χ Cassiopeiae, and
Chi_Cassiopeiae
Star in the constellation of Andromeda
π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae
Kappa_Andromedae
Nova seen in 1993
V705 Cassiopeiae, also known as Nova Cassiopeiae 1993 was a nova which erupted in the constellation Cassiopeia during 1993. The nova was discovered at
V705_Cassiopeiae
= 2.29m, P = 0.10 d γ Cas γ 27 5394 4427 00h 56m 42.50s +60° 43′ 00.3″ 2.47 −4.22 613 B0IV:evar Tiansi, Tsih, Navi; prototype γ Cas variable, Vmax = 1
List_of_stars_in_Cassiopeia
Variable star in the constellation Orion
Rotational velocity (v sin i) 179±4 km/s Age 43.6 Myr Other designations ω Ori, 47 Orionis, BD+04°1002, FK5 2423, HD 37490, HIP 26594, HR 1934, SAO 113001 Database
Omega_Orionis
Binary star in the constellation Cassiopeia
Xi Cassiopeiae is a blue-white hued binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized
Xi_Cassiopeiae
Triple star system in the constellation Eridanus
from a planet. The candidate planet would have had a minimum mass of 8.47±0.47 M🜨, and lie considerably interior to the habitable zone, receiving nine
40_Eridani
Star in the constellation Ophiuchus
inclination angle of its poles must be small; estimated as ~20°. It is a Gamma Cassiopeiae variable with an amplitude of 0.15 magnitude. The brightness has been
Chi_Ophiuchi
Che; et al. (2011). "Colder And Hotter: Interferometric Imaging Of Beta Cassiopeiae And Alpha Leonis". The Astrophysical Journal. 732 (2): 68. arXiv:1105
List of stars with resolved images
List_of_stars_with_resolved_images
Zodiac constellation in the southern celestial hemisphere
is a shell star of magnitude 4.9. Shell stars, like Pleione and Gamma Cassiopeiae, are stars with irregular variations caused by their abnormally high
Libra_(constellation)
Variable star in the constellation Canis Major
to the naked eye of an observer far from city lights. It is a Gamma Cassiopeiae variable star, whose brightness varies from magnitude 4.8 to 6.25. In
FY_Canis_Majoris
Star in the constellation Aquarius
also been applied to this star; though it shared that name with Delta Cassiopeiae. It is only one of two stars with ancient proper names to lie within
Alpha_Aquarii
Star in the constellation Centaurus
Cassiopeiae variable star with multiple periods of variability. The International Variable Star Index lists Eta Centauri as both a Gamma Cassiopeiae variable
Eta_Centauri
Star in the constellation Orion
Ross 47 is a variable star of spectral type M4 located in the constellation Orion. Based on parallax measurements, it lies 18.888 light-years (5.791 parsecs)
Ross_47
Variable star in the constellation Cassiopeiae
Iota Cassiopeiae, also named Huagai, is a multiple star system in the constellation Cassiopeia. Its name is a Bayer designation that is Latinized from
Iota_Cassiopeiae
"Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age". The Astrophysical Journal
List of nearest stars by spectral type
List_of_nearest_stars_by_spectral_type
Northern 89 2.46 Markeb κ Velorum 0540 B2 IV Southern 90 2.47 (1.6–3.0var) Tiansi γ Cassiopeiae 0610 B0.5 IVe Northern 91 2.48 Markab α Pegasi 0140 A0 IV
List_of_brightest_stars
Star in the constellation Cassiopeia
50 Cassiopeiae, also named Gang, is a white star in the northern constellation of Cassiopeia. In the past, it had been misidentified as a suspected nebula
50_Cassiopeiae
(River's end) /ˈeɪkərnɑːr/ Achird η Cassiopeiae A Cassiopeia Slovak (1950) Apparently first applied to η Cassiopeiae in the Skalnate Pleso Atlas of the
List_of_proper_names_of_stars
1 Andromeda 23h 09m 57.3642s +35° 32′ 55.658″ K2Ve 7.93 B K2Ve Delta Cassiopeiae (Rucbah)$ 99.4 ± 0.4 Cassiopeia 01h 25m 48.95147s +60° 14′ 07.0225″ A5
List of star systems within 95–100 light-years
List_of_star_systems_within_95–100_light-years
Star in the constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ψ Cassiopeiae
Psi_Cassiopeiae
Binary star system in the constellation Pisces
has a weak magnetic field with a strength of 0.4±0.2 G, and is a Gamma Cassiopeiae variable. The companion, component B, is a magnitude 7.51 star. van Leeuwen
Eta_Piscium
Type of star cluster
the cosmic distance scale: the Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae, A&A, 260 Quinn, Samuel N.; White, Russel J.; Latham, David
Open_cluster
Star system in the Centaurus constellation
With the placement of the Sun east of the magnitude 3.4 star Epsilon Cassiopeiae, nearly in front of the Heart Nebula, the "W" line of stars of Cassiopeia
Alpha_Centauri
Star in the constellation Apus
shows some peculiarity in the spectrum. It is classified as a Gamma Cassiopeiae type variable star and its brightness varies from magnitude +5.43 to
Kappa1_Apodis
K-type giant star in the constellation Cassiopeia
Tau Cassiopeiae is a solitary, orange hued star in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from τ
Tau_Cassiopeiae
Triple star system in the constellation Cassiopeia
include HR 5, ADS 61, as well as the variable-star designation V640 Cassiopeiae, which was given in 1985 after it was reported to fluctuate in brightness
HD_123
Binary star system in the constellation Centaurus
circumstellar disk of decreated gas. It is classified as a suspected Gamma Cassiopeiae type variable star with a visual magnitude varying from +4.30 down to
HD_102776
American astronaut (1926–1967)
(Ivan spelled backwards), is a seldom-used nickname for the star Gamma Cassiopeiae. Grissom used this name, plus two others for White and Chaffee, on his
Gus_Grissom
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
Thorne–Żytkow_object
Variable star in the constellation Lacerta
naked eye of an observer located far from city lights. It is a Gamma Cassiopeiae variable, varying in brightness from magnitude 5.22 to 5.48, over a period
EW_Lacertae
Constellations that are no longer widely recognised
is named Triminus from the former constellation Triangulum Minus. 49 Cassiopeiae A and 2 Ursae Minoris are named Rangifer and Tarandus, from the former
Former_constellations
Nova in the constellation Cassiopeia seen in 2021
Nova Cassiopeiae 2021, also known V1405 Cassiopeiae, was a nova in the constellation Cassiopeia. It reached a peak brightness of magnitude 5.449 on May
Nova_Cassiopeiae_2021
Binary star system in constellation Cassiopeia
Cassiopeiae is a binary star system in the northern constellation of Cassiopeia. Its name is a Bayer designation that is Latinized from ω Cassiopeiae
Omega_Cassiopeiae
M2.5 V 0.43 9.31 10.45 168.9965 ±0.0270 has two candidate planets Eta Cassiopeiae (Gliese 34) Achird (A)$ 19.3314 ±0.0025 Cas* 00h 49m 06.3s +57° 48′ 55″
List_of_nearest_stars
Comparison of a wide range of lengths
distance between Jupiter and the Sun 785 Gm (5.25 au) – diameter of Rho Cassiopeiae, a rare yellow hypergiant star 947 Gm (6.4 au) – diameter of Antares
Orders_of_magnitude_(length)
Star in the constellation Cassiopeia
Gliese 22, also catalogued V547 Cassiopeiae or ADS 440, is a hierarchical star system approximately 33 light-years (10.1 parsecs) away in the constellation
Gliese_22
Multiple star system in the constellation Cassiopeia
detached eclipsing binary and given the variable star designation V773 Cassiopeiae. The derived period of variability was 1.29 days, exactly half the orbital
ADS_1359
Constellations recognized by the International Astronomical Union
Argo Navis keel Canopus -0.74 494 Cassiopeia /ˌkæsioʊˈpiːə/ Cas Cass Cassiopeiae /ˌkæsioʊˈpiːiː/ ancient (Ptolemy) Cassiopeia (mythological character)
IAU_designated_constellations
Zodiac constellation straddling the celestial equator
(η Psc), 349 lightyears, class G7 IIIa, magnitude 3.62. It is a Gamma Cassiopeiae variable with a weak magnetic field. Torcular ("thread"), otherwise Omicron
Pisces_(constellation)
Star in the constellation Perseus
his catalogue, published in 1712. 48 Persei is classified as a Gamma Cassiopeiae variable, and it has been given the variable star designation MX Persei
48_Persei
Group of stars
the cosmic distance scale: The Cepheids U Sagittarii, CF Cassiopeiae, and CEab Cassiopeiae". Astronomy & Astrophysics. 560: A22. arXiv:1311.0865. Bibcode:2013A&A
Star_cluster
Process by which stars are named
into popular use, for example Sualocin for α Delphini and Navi for γ Cassiopeiae. The International Astronomical Union (IAU) has begun a process to select
Stellar designations and names
Stellar_designations_and_names
44 Eta Cassiopeiae Binary star system Suspected variable star 3.45 Lambda Ursae Majoris Star 3.45 Eta Ceti Star 3.466 Epsilon Gruis Star 3.47 3.41 Sigma
List of brightest natural objects in the sky
List_of_brightest_natural_objects_in_the_sky
Type of variable star
Leonis 4.4 11.3 310 71+5 −4 [5] S Carinae 4.5 9.9 149 497+22 −20 [6] R Cassiopeiae 4.7 13.5 430 187+9 −8 [7] R Horologii 4.7 14.3 408 313+40 −32 [8] U Orionis
Mira_variable
Star in the constellation Ara
indicating that it is a variable Be star but not obviously a Gamma Cassiopeiae variable. The International Variable Star Index defines it as GCAS +
Alpha_Arae
2024). "CHARA Near-Infrared Imaging of the Yellow Hypergiant Star ρ Cassiopeiae: Convection Cells and Circumstellar Envelope". The Astrophysical Journal
List_of_largest_stars
31m 28.99s +15° 20′ 45.0″ 3.62 −1.16 294 G8III Alpherg, Kullat-Nunu; γ Cassiopeiae variable Vmax = 3.59 m, Vmin = 3.65m γ Psc γ 6 21 219615 114971 23h 17m
List_of_stars_in_Pisces
Astrophysical phenomenon
supergiants Betelgeuse, Antares, and VV Cephei A; the yellow hypergiant Rho Cassiopeiae; the luminous blue variable Eta Carinae that has already produced a supernova
Supernova
Triple star system in the constellation Cassiopeia
48 Cassiopeiae is a triple star system in the northern constellation of Cassiopeia. It is visible to the naked eye with a combined apparent visual magnitude
48_Cassiopeiae
Open cluster in the constellation Cassiopeia
located almost exactly halfway between the bright stars Caph (β Cassiopeiae) and γ Cassiopeiae. It is large but not dense and can be observed by binoculars
NGC_129
Star in the constellation Cygnus
206267, Epsilon Cephei, Beta Lacertae, Sigma Cassiopeiae, Rho Cassiopeiae, Tau Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae
Pi1_Cygni
191939 174.4 ± 0.1 G9V 8.971 Has 7 exoplanets. Pi Cassiopeiae$ A 175 ± 1 Cassiopeia 00h 43m 28.070s +47° 01′ 28.36″ A5V 4.949# 18.6293±0.1142 B A5V Zeta
List of star systems within 150–200 light-years
List_of_star_systems_within_150–200_light-years
Variable star in the constellation Cassiopeia
Pi Cassiopeiae is a close binary star system in the constellation Cassiopeia, near the southern border with Andromeda. Its name is a Bayer designation
Pi_Cassiopeiae
Star in the constellation Cassiopeia
PZ Cassiopeiae is a red supergiant or hypergiant star located in the constellation of Cassiopeia, and a semi-regular variable star. PZ Cassiopeiae is
PZ_Cassiopeiae
Astronomy catalogue
vdB 37 vdB 38 vdB 39 vdB 40 vdB 41 vdB 42 vdB 43 vdB 44 vdB 45 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
Van_den_Bergh_Catalog
Star in the constellation Centaurus
varies from magnitude +2.51 to +2.65. It has been classified as a γ Cassiopeiae type variable. The energy from this star is being radiated at an effective
Delta_Centauri
Type of star larger than main-sequence but smaller than a giant
established the two-dimensional classification scheme, including: B0: γ Cassiopeiae, δ Scorpii, B0.5: β Scorpii, ε Persei B1: ο Persei, β Cephei B2: γ Orionis
Subgiant
Star in the constellation Carina
System". Monthly Notes of the Astronomical Society of South Africa. 18: 46–47. Bibcode:1959MNSSA..18...46C. Retrieved 9 January 2025. Kukarkin, B. V.; Kholopov
V345_Carinae
Star in the constellation Carina
a hypergiant), easily visible to the naked eye and brighter than Rho Cassiopeiae although not visible from much of the northern hemisphere. It is estimated
V382_Carinae
Star in the constellation Capricornus
variations showing a phase cycle of 1.03 days. It is classified as a Gamma Cassiopeiae variable with an amplitude of 0.16 in magnitude. Epsilon Capricorni Aa
Epsilon_Capricorni
Star whose brightness fluctuates, as seen from Earth
on an observable timescale. One of the best studied examples is Rho Cassiopeiae. R Coronae Borealis variables While classed as eruptive variables, these
Variable_star
Star that is particularly similar to the Sun
Tabetha S.; et al. (August 2008). "Angular Diameters of the G Subdwarf µ Cassiopeiae A and the K Dwarfs s Draconis and HR 511 from Interferometric Measurements
Solar_analog
from the Ma'der (eastern Anti-Atlas, Morocco)". Geologica Belgica. 28 (1–2): 47–71. Bibcode:2025GeolB..28...47C. doi:10.20341/gb.2025.003. Löser, H.; Cruz-Palma
2025_in_paleontology
Quadruple star system in the constellation Cassiopeia
under dark skies, although it lies only 21′ from the 2nd-magnitude γ Cassiopeiae and may be bound to it. The system is located approximately 540 light-years
HD_5408
DAZ9.5 HR 511 (V987 Cassiopeiae)$ 32.75 ± 0.01 Cassiopeia 01h 47m 44.83444s +63° 51′ 09.0110″ K0V 5.63 Gliese 22 (V547 Cassiopeiae) A 32.8 ± 0.7 Cassiopeia
List of star systems within 30–35 light-years
List_of_star_systems_within_30–35_light-years
Supernova remnant in the constellation of Cassiopeia
Cambridge Catalogue of Radio Sources. It is located 2° northeast of ε Cassiopeiae and is estimated to be 10,000 light-years away. Its rotation period is
3C_58
5.41 K0Ve 6 HD 400 Andromeda 6.21 F8 IV 7 CD-27 16 11.72 M0V 8 Beta Cassiopeiae (Caph) Cassiopeia 54.7 ± 0.3 +2.28 (2.25–2.31) F2 III 9 HD 469 G8III
List of Gliese and GJ objects (1-1000)
List_of_Gliese_and_GJ_objects_(1-1000)
Star in the constellation Puppis
irregularly between magnitude 4.6 and 4.9 and it is classified as a Gamma Cassiopeiae variable. It is approximately 930 light years away based on parallax
MX_Puppis
Sagittarius 19h 02m 36.73024s −29° 52′ 48.2279″ A2.5Va 2.59# B A3V 54 Cassiopeiae 88.12 ± 0.04 Cassiopeia 02h 09m 80.26080s +71° 33′ 07.2268″ F8V 6.587
List of star systems within 85–90 light-years
List_of_star_systems_within_85–90_light-years
Open cluster in the constellation Serpens
photometric observations of the selected Algol-type binaries - IV. V799 Cassiopeiae, BX Piscium and HD 172189". Monthly Notices of the Royal Astronomical
IC_4756
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
Lists_of_stars
Binary star in the Pleiades star cluster
small amount (~1/6 magnitude). Pleione is now classified as a Gamma Cassiopeiae type variable star, with brightness fluctuations that range between a
Pleione_(star)
Binary star system in the constellation Andromeda
Orbits of Bright Double-lined Spectroscopic Binaries. VII. 47 Andromedae, 38 Cassiopeiae, and HR 8467", The Astronomical Journal, 142 (3): 13, Bibcode:2011AJ
47_Andromedae
Classification of stars based on spectral properties
Kenneth J. H. (1995). Guide to the Sun. Cambridge University Press. pp. 47–53. ISBN 978-0-521-39788-9. Russell, Henry Norris (March 1914). "Relations
Stellar_classification
"Galactic clusters with associated Cepheid variables. II – NGC 129 and DL Cassiopeiae". Astronomical Journal. 104 (3): 1132–1143. Bibcode:1992AJ....104.1132T
List_of_open_clusters
Nebula
Sh 2-185 is an H II region centered on the massive star system Gamma Cassiopeiae (γ Cas) in the northern constellation of Cassiopeia. It was included
Sh_2-185
Star system in the constellation Vela
absorption lines) it is also dubbed the Spectral Gem of Southern Skies. Gamma Cassiopeiae, informally named Navi for astronaut Virgil Ivan "Gus" Grissom Iota Ursae
Gamma_Velorum
O5–5.5V((f))) 5.97 15 Sagittarii 4,200±650 1 O9.7 Iab or B0 Iab 5.37 AO Cassiopeiae (Pearce's Star) 4,300 ± 300 2 O8V((f)) + O9.2II 6.07-6.24 HD 149404 (V918
List_of_O-type_stars
Brightest star in the constellation Aquila
049 ly) G-type Alsafi (Sigma Draconis) (18.7993±0.0081 ly) Achird (Eta Cassiopeiae) (19.3314±0.0025 ly) K-type main-sequence star B e (82 G.) Eridani (19
Altair
Star in the constellation Cygnus
ṣadr "chest", the same word which gave rise to the star Schedar (Alpha Cassiopeiae). In 2016, the International Astronomical Union organized a Working Group
Gamma_Cygni
Open cluster in the constellation Cassiopeia
was a double star on Cassiopeia's knee, about 1° northeast of Delta Cassiopeiae, sometimes called as Ruchbah or Rukhbah. Messier 103 is an easy object
Messier_103
Constellation in the southern celestial hemisphere
this variation can be observed with the unaided eye. Classed as a Gamma Cassiopeiae variable or shell star, it is of spectral type B2II-IIIe and lies around
Pavo_(constellation)
Variable star in the constellation Hercules
main sequence. Omicron Herculis is an eruptive variable of the Gamma Cassiopeiae class, which are rapidly rotating B-class stars with mass outflow. It
Omicron_Herculis
Cluster of Orion complex 33 39,000 1,340 5.13 combined evolution SIMBAD κ Cassiopeiae Cassiopeia OB14 33 23,500 4,000 4.16 evolution SIMBAD μ Normae NGC 6169
List_of_most_massive_stars
Star in the constellation Cygnus
J2000 Constellation Cygnus Right ascension 20h 59m 49.55164s Declination +47° 31′ 15.3789″ Apparent magnitude (V) 4.74 Characteristics Spectral type B1
59_Cygni
47 CASSIOPEIAE
47 CASSIOPEIAE
47 CASSIOPEIAE
47 CASSIOPEIAE
Girl/Female
Arabic, Muslim
Winner; Achiever; A Boon; Gift; Acquirer
Female
German
Variant spelling of German Liese, LIES means "God is my oath."Â
Girl/Female
Indian, Punjabi, Sikh
Sunshine
Boy/Male
Hindu
Limitless, Infinite, Unbeaten
Girl/Female
Muslim/Islamic
A flower delicate, soft, slender
Boy/Male
Hindu
Girl/Female
Australian, German, Turkish
Lovable
Surname or Lastname
English
English : variant of the habitational name Beeston (see Beaston). The spelling reflects the local pronunciation of the Nottinghamshire place name, although this form is now quite widespread in England.
Girl/Female
Teutonic German
Armored battle maiden.
Male
English
Anglicized form of Hebrew Midyan, MIDIAN means "strife, war." In the bible, this is the name of a son of Abraham.
47 CASSIOPEIAE
47 CASSIOPEIAE
47 CASSIOPEIAE
47 CASSIOPEIAE
47 CASSIOPEIAE
n.
One opposed to the payment of rent; esp. one of those who in 1840-47 resisted the collection of rents claimed by the patroons from the settlers on certain manorial lands in the State of New York.