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Star in the constellation Perseus
32 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
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)
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
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
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
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
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
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
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 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 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
GRO J0422+32 is an X-ray nova and black hole candidate that was discovered by the BATSE instrument on the Compton Gamma Ray Observatory satellite on 5
GRO_J0422+32
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Persei (Mirfak). /ælˈdʒiːnᵻb/ Algieba γ1 Leonis A Leo Arabic From Arabic: الجبهة al-jabha ('the forehead' [of the lion]). /ælˈdʒiːbə/ Algol β Persei Aa1
List_of_proper_names_of_stars
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
– 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
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
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
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
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
Constellation in the northern celestial hemisphere
Cassiopeia showing the double cluster χ and h Persei as well as the clusters NGC 654, NGC 663, M103, NGC 457, NGC 225, NGC 7788, NGC 7790, NGC 7789 and
Cassiopeia_(constellation)
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
Poem by Hesiod
(including Doris, Electra, Callirhoe, Styx, Clymene, Metis, Eurynome, Perseis, and Idyia). From Hyperion and Theia came Helios (Sun), Selene (Moon),
Theogony
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
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
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
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
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
Stars with a supergiant luminosity class with a spectral type of K or M
Antares A Betelgeuse Epsilon Pegasi Zeta Cephei Lambda Velorum Eta Persei 31 and 32 Cygni Psi1 Aurigae 119 Tauri Mira was historically thought to be a
Red_supergiant
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
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
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
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
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
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
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
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
Southern 32 1.77 Alioth ε Ursae Majoris 0083 A1 III-IVp kB9 Northern 33 1.79 Dubhe α Ursae Majoris 0120 K0 III, F0 V Northern 34 1.82 Mirfak α Persei 0510
List_of_brightest_stars
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
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)
Classification of stars based on spectral properties
Real Starry Sky". Journal of the Royal Astronomical Society of Canada. 95: 32. Bibcode:2001JRASC..95...32L. "Spectral classification of stars (OBAFGKM)"
Stellar_classification
mission be affected?". Space. Retrieved 9 February 2026. "Starlink Group 17-32". Next Spaceflight. Retrieved 2 October 2025. "Kosmos". Next Spaceflight.
List of spaceflight launches in January–March 2026
List_of_spaceflight_launches_in_January–March_2026
Russian family of space launch vehicles
an Angara-1.2 and an Angara-A5 with a new booster, Persei. Only the launch of Angara-A5 with Persei upper stage ended up happening in 2021. The maiden
Angara_(rocket_family)
Persei Cluster Open cluster Perseus 02h 19m +57° 09′ 5.7 870 Galaxy Aries 02h 17m 09.2s +14° 31′ 22″ 16 871 Spiral galaxy Aries 02h 17m 10.8s +14° 32′ 53″
List_of_NGC_objects_(1–1000)
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
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
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
"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
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
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
Betelgeuse. RT Carinae 1,090 L/Teff UU Persei 1,079+9 −8 L/Teff LL Pegasi 1,070 L/Teff HD 126577 1,066+9 −32 L/Teff V766 Centauri Aa 1,060–1,160 ? V766
List_of_largest_stars
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)
[@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
Star in the constellation Perseus
40 Persei is a wide binary star system in the northern constellation of Perseus. It has the Bayer designation ο Persei, while 40 Persei is the Flamsteed
40_Persei
Heterogeneous class of stars with unusual spectra
and back to a WNL star is calculated to be around 20 M☉ in the Milky Way, 32 M☉ in the LMC, and over 50 M☉ in the SMC. The more evolved WNE and WC stages
Wolf–Rayet_star
members were identified. Among the group members he included β Hydri, ρ Persei, η Reticuli, φ1 Lupi, ζ Herculis and ε Octantis. He estimated the group
Zeta_Herculis_Moving_Group
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)
Star in the constellation Vulpecula
Strom, Stephen E.; et al. (2005), "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?", The Astronomical
17_Vulpeculae
F-type variable star
collision systems such as ASASSN-21qj, NGC 2547–ID8, HD 166191 and V488 Persei. Gaia-GIC-1 was initially discovered through the Gaia Photometric Science
Gaia20ehk
Lacertae A 138.6 ± 0.1 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″
List of star systems within 100–150 light-years
List_of_star_systems_within_100–150_light-years
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
Star in the constellation Taurus
S2CID 14878976 Eggen, Olin J. (October 1998), "The Pleiades and alpha Persei Clusters", The Astronomical Journal, 116 (4): 1810–1815, Bibcode:1998AJ
18_Tauri
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
Star in the constellation Camelopardalis
Strom, Stephen E.; et al. (2005), "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?", The Astronomical
42_Camelopardalis
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
Star in the constellation Ophiuchus
Taylor, A. R.; et al. (October 1987). "Radio detection of the Be star psi Persei". Monthly Notices of the Royal Astronomical Society. 228 (4): 811–817. Bibcode:1987MNRAS
Chi_Ophiuchi
"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
Astronomy catalogue
vdB 22 vdB 23 vdB 24 vdB 25 vdB 26 vdB 27 vdB 28 vdB 29 vdB 30 vdB 31 vdB 32 vdB 33 vdB 34 vdB 35 vdB 36 vdB 37 vdB 38 vdB 39 vdB 40 vdB 41 vdB 42 vdB
Van_den_Bergh_Catalog
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
Phenomenon wherein objects appear to move about their true positions in the sky
Its effect is much smaller than that of annual aberration, and is only 0.32 arcseconds in the case of an observer at the Equator, where the rotational
Aberration_(astronomy)
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
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
Upper bound to the mass of cold, nonrotating neutron stars
09617.x. S2CID 8393701. Gelino, D. M.; Harrison, T. E. (2003). "GRO J0422+32: The Lowest Mass Black Hole?". The Astrophysical Journal. 599 (2): 1254–1259
Tolman–Oppenheimer–Volkoff limit
Tolman–Oppenheimer–Volkoff_limit
Binary star in the Pleiades star cluster
South Africa, at the tip of the African continent, the star rises almost 32° above the horizon. Due to its declination of roughly +24°, Pleione is circumpolar
Pleione_(star)
Bronze tables containing inscriptions in Italic languages
grabouie, orer ose, persei ocre fisie pir orto est toteme iouine arsmor dersecor (27) subator sent, pusei neip heritu. dei crabouie persei tuer perscler uaseto
Iguvine_Tablets
of the 25 parsec White Dwarf Sample". The Astronomical Journal. 154 (1): 32. arXiv:1706.00709. Bibcode:2017AJ....154...32S. doi:10.3847/1538-3881/aa76e0
List of star systems within 30–35 light-years
List_of_star_systems_within_30–35_light-years
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 Pegasus
Tennessee, retrieved 2007-06-09 Harper, W. E. (1928), "The orbits of A Persei and HR 8210", Publications of the Dominion Astrophysical Observatory, 4:
IK_Pegasi
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
Star in the constellation Corvus
C.; Dror, David H. A. (2005). "B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?". The Astronomical
Zeta_Corvi
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
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
; 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
32 PERSEI
32 PERSEI
32 PERSEI
32 PERSEI
Surname or Lastname
English
English : possibly a variant of Lefridge, from the Middle English personal name Lefric, Old English Lēofrīc, a compound of lēof ‘dear’, ‘beloved’ + rīc ‘power’.
Girl/Female
Tamil
Generates harmony in dance and music
Male
French
French form of Hebrew Zekaryah, ZACHARIE means "whom Jehovah remembered."
Girl/Female
Hindu, Indian
A Smile; Beautiful; Very Special
Surname or Lastname
English (Suffolk)
English (Suffolk) : unexplained.
Male
Arthurian
, Lord of Belinus, or war-lord.
Boy/Male
Hindu
God
Girl/Female
Arabic, Bengali, French, Hawaiian, Hebrew, Hindu, Indian, Jewish, Kannada, Malayalam, Marathi, Muslim, Sanskrit, Sindhi, Telugu
Queen; Princess Blessed by God
Boy/Male
Bengali, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Telugu
Tall; Lord Vishnu
Boy/Male
Tamil
Parthipan | பரà¯à®¤à¯€à®ªà®£Â
Arjun
32 PERSEI
32 PERSEI
32 PERSEI
32 PERSEI
32 PERSEI
n.
An instrument used to illustrate the freezing of water by its own evaporation. The ordinary form consists of two glass bulbs, connected by a tube of the same material, and containing only a quantity of water and its vapor, devoid of air. The water is in one of the bulbs, and freezes when the other is cooled below 32¡ Fahr.
n.
A nonmetallic element occurring naturally in large quantities, either combined as in the sulphides (as pyrites) and sulphates (as gypsum), or native in volcanic regions, in vast beds mixed with gypsum and various earthy materials, from which it is melted out. Symbol S. Atomic weight 32. The specific gravity of ordinary octohedral sulphur is 2.05; of prismatic sulphur, 1.96.
n.
The fifth power of a number; as, a/ is the sursolid of a, or 32 that of 2.
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.
The fringe of teeth around the orifice of the capsule of mosses. It consists of 4, 8, 16, 32, or 64 teeth, and may be either single or double.
n.
A book composed of sheets so folded that each one makes thirty-two leaves; hence, indicating, more or less definitely, a size of book; -- usually written 32mo, or 32¡, and called thirty-twomo.