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Class of eclipsing binary stars
Algol variables or Algol-type binaries are a class of eclipsing binary stars that are similar to the prototype member of this class, β Persei (Beta Persei
Algol_variable
Eclipsing variable star in the constellation Perseus
constellation of Perseus and one of the first non-nova variable stars to be discovered. Algol is a three-star system, consisting of Beta Persei Aa1, Aa2
Algol
Programming language
to ALGOL 68. ALGOL 68 features include expression-based syntax, user-declared types and structures/tagged-unions, a reference model of variables and
ALGOL_68
Member of the ALGOL family of computer programming languages
ALGOL 60 (short for Algorithmic Language 1960) is a member of the ALGOL family of computer programming languages. It followed on from ALGOL 58 which had
ALGOL_60
Family of programming languages
ALGOL (/ˈælɡɒl, -ɡɔːl/; short for "Algorithmic Language") is a family of imperative computer programming languages originally developed in 1958. ALGOL
ALGOL
Star whose brightness fluctuates, as seen from Earth
first documented periodic variable was the eclipsing binary Algol. The periodic variable Omicron Ceti, later named Mira, was discovered in the 17th century
Variable_star
Svolopoulos, Sotirios (1988). "Spectral types of 80 early-type stars of variable radial velocity". Astronomical Society of the Pacific. 100: 828. Bibcode:1988PASP
List_of_stars_in_Cancer
Programming language
ALGOL 58, originally named IAL, is a member of the ALGOL family of computer programming languages. It was an early compromise design soon superseded by
ALGOL_58
Star system in the constellation Perseus
Lindemann Award from the Astronomische Gesellschaft. He classified it as an Algol variable and found a period of 13.196 days. Enebo refined the period to 13.1989
RW_Persei
Topics referred to by the same term
Look up Algol or ALGOL in Wiktionary, the free dictionary. Algol is a star system. Algol or ALGOL may also refer to: Algol variable or Algol-type binaries
Algol_(disambiguation)
Topics referred to by the same term
Gerard Kuiper, including: KUI 91AB, a variable star of Delta Cephei type KUI 93AB, an eclipsing binary of Algol variable type Kui (Chinese mythology) 夔, a
Kui
3.31 −1.84 349 M3III Propus, Praepes, Tejat Prior; semiregular and Algol variable, Vmax = 3.15m, Vmin = 3.9m, P = 232.9 d ξ Gem ξ 31 48737 32362 06h 45m
List_of_stars_in_Gemini
Binary star in the constellation Aquarius
to be an Algol-type eclipsing binary based on photometric observations made with the Hipparcos space observatory. It was assigned the variable-star designation
LL_Aquarii
Programming language dialect
The Interactive ALGOL 68 is a structured, imperative high-level computer programming language, a dialect of, and compiler for, ALGOL 68. It was made available
Interactive_ALGOL_68
Variable masking one with the same name
rules of the language. One of the first languages to introduce variable shadowing was ALGOL, which first introduced blocks to establish scopes. It was also
Variable_shadowing
Paradox in astronomy
much of its mass to its companion. Algol variable Pustylnik, I. (1998). "The Early History of Resolving the Algol Paradox". Astronomical and Astrophysical
Algol_paradox
2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. "Naming Stars". Retrieved 13 December
List_of_stars_in_Scorpius
Programming variable that persists for the lifetime of the program
allocated as required at run time. Static variables date at least to ALGOL 60 (1960), where they are known as own variables: A declaration may be marked with
Static_variable
Triple star system in constellation Draco
HD 139319 is a ternary system composed of the binary Algol variable star known as TW Draconis, and a main-sequence companion star at a separation of 3
HD_139319
Description of an algorithm that resembles a computer program
syntax sources include Fortran, Pascal, BASIC, C, C++, Java, Lisp, and ALGOL. Variable declarations are typically omitted. Function calls and blocks of code
Pseudocode
Open cluster in the Orion Nebula in the constellation Orion
37020, V1016 Orionis Algol variable B West X-ray source N/A COUP 766, MAX 97 B B1V 5 41 Orionis B, HD 37021, BM Orionis Algol variable B East X-ray source
Trapezium_Cluster
Star system in the constellation Sagittarius
et al. (April 2011), "Mass loss out of close binaries. The formation of Algol-type systems, completed with case B RLOF", Astronomy & Astrophysics, 528
V356_Sagittarii
Constellation in the northern celestial hemisphere
system is the prototype of a group of eclipsing binary stars named Algol variables, though it has a third member to make up what is actually a triple
Perseus_(constellation)
Quintuple star system in the constellation Ursa Major
The first pair of stars, J093010A, is a detached eclipsing binary (an Algol variable). The two stars within J093010A orbit with a period of about 1.3 days
1SWASP_J093010.78+533859.5
Algol variable in the constellation Chamaeleon
colleagues. Four years later, the system was found to be an Algol variable and was given the variable star designation RZ Chamaeleontis in 1974. J. Andersen
HD_93486
Catalogue of Variable Stars (GCVS4.2)". Retrieved 10 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Cassiopeia
Binary star system in the northern constellation of Auriga
system is believed to be a stream member of the Ursa Major Moving Group. Algol Capella Alsephina van Leeuwen, F. (November 2007), "Validation of the new
Beta_Aurigae
−00° 17′ 56.7″ 2.20 -5.8 916 B0III+O9V component of the Mintaka system; Algol variable, Vmax = 2.20m, Vmin = 2.32m, P = 5.73 d ι Ori ι 44 37043 26241 05h 35m
List_of_stars_in_Orion
Strasbourg. Retrieved 2007-01-04. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. E.B Knobel – On a catalogue of
List_of_stars_in_Lyra
Catalogue of Variable Stars (GCVS4.2)". Retrieved 4 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Canis_Major
Multiple star system in the constellation of Auriga
Light Changes of Epsilon Aurigae), where he suggested the star was an Algol variable and an eclipsing binary. The first hypothesis, set forth in 1937 by
Epsilon_Aurigae
Computer programming, a variable only usable in a portion of a program (the scope)
variables. On the other hand, many ALGOL-derived languages allow any number of nested levels of visibility, with private variables, functions, constants and types
Local_variable
Binary star system in the constellation Cetus
variable star discovered, with the possible exception of Algol. It is the prototype of the Mira variables. The system lies at a distance of 300 light-years (92
Mira
Type of variable star
Beta Cephei variables, also known as Beta Canis Majoris stars, are variable stars that exhibit small rapid variations in their brightness due to pulsations
Beta_Cephei_variable
Binary star in the constellation Capricornus
be from coronal activity in the secondary star. Delta Capricorni A is an Algol-type eclipsing binary star, with an orbital period of 1.022768 days and
Delta_Capricorni
Constellation split into two non-contiguous parts
IC 4756, is an Algol variable eclipsing binary with a 5.70 day period. The primary star in the system is also a Delta Scuti variable, undergoing multiple
Serpens
ALGOL 68C is an imperative computer programming language, a dialect of ALGOL 68, that was developed by Stephen R. Bourne and Michael Guy to program the
ALGOL_68C
Triple star system in constellation Hercules
HD 165590 is a quintuple system dominated by the binary Algol variable star known as V772 Herculis. The system lies in the constellation of Hercules about
HD_165590
Archived from the original on 2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Monoceros
Binary star in the constellation Cygnus
V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally
Y_Cygni
Triple star system in the constellation Scutum
astronomiques de Strasbourg. Retrieved 2025-09-04. "FR Scuti". International Variable Star Index. AAVSO. Retrieved 2025-10-07. Pantaleoni González, M.; Maíz
FR_Scuti
Constellation in the northern celestial hemisphere
days. Even further north is FL Lyrae, a much fainter 9th-magnitude Algol variable that drops by half a magnitude every 2.18 days during the primary eclipse
Lyra
Programming language
the ALGOL 60 language. Wirth was involved in the process to improve the language as part of the ALGOL X efforts and proposed a version named ALGOL W. This
Pascal_(programming_language)
System of two stars orbiting each other
Algol, a triple star system in the constellation Perseus, contains the best-known example of an eclipsing binary. Eclipsing binaries are variable stars
Binary_star
Catalogue of Variable Stars (GCVS4.2)". Retrieved 2012-07-12. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database
List_of_stars_in_Cepheus
Variable star in the constellation Cygnus
O. V.; Kireeva, N. N.; Pastukhova, E. N. (2017). "General catalogue of variable stars: Version GCVS 5.1". Astronomy Reports. 61 (1): 80. Bibcode:2017ARep
V380_Cygni
3.80 0.91 123 K0III variable ο1 Cyg ο1 31 V695 192577 99675 20h 13m 37.90s +46° 44′ 28.8″ 3.80 −4.29 1353 K2II+... Algol variable η Cyg η 21 188947 98110
List_of_stars_in_Cygnus
Programming language based on a proposal for ALGOL X
ALGOL W is a programming language. It is based on a proposal for ALGOL X by Niklaus Wirth and Tony Hoare as a successor to ALGOL 60. ALGOL W is a relatively
ALGOL_W
Binary star in the constellation Cepheus
the large cool primary star. The timing and duration of the eclipses is variable, although the exact onset is difficult to measure because it is gradual
VV_Cephei
Catalogue of Variable Stars (GCVS4.2)". Retrieved 2012-04-08. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database
List_of_stars_in_Carina
Variable star in the constellation Ursa Major
subdwarf O star, borderline white dwarf. It is classified as a detached Algol variable and ranges in brightness from an apparent visual magnitude of 14.8 down
BE_Ursae_Majoris
Programming language feature
supporting functions as result types (e.g. ALGOL 60, Pascal) or omitting nested functions and thus non-local variables (e.g. C). The early functional language
First-class_function
Demarcated group of source code statements that run in sequence
development of the first autocodes, and was formalized in the Algol 58 and Algol 60 reports. Algol 58 introduced the notion of the "compound statement", which
Block_(programming)
Main sequence star that is more luminous and bluer than expected
Blue straggler stars Star portal Algol variable – Class of eclipsing binary stars SX Phoenicis variable – Type of variable star Sandage, Allan (1953). "The
Blue_straggler
Part of a computer program where a given name binding is valid
of ALGOL 60. Representative language specifications follow: ALGOL 60 (1960) The following kinds of quantities are distinguished: simple variables, arrays
Scope_(computer_programming)
Type of variable stellar binary
regarded[by whom?] as a subtype of the Algol variables; however, their light curves differ (the eclipses of Algol variables are much more sharply defined). On
Beta_Lyrae_variable
110 U 156247 84500 17h 16m 31.72s +01° 12′ 38.1″ 5.89 −0.46 606 B5Vnn Algol variable 179 G. Oph 179 162774 87491 17h 52m 35.46s +01° 18′ 18.2″ 5.91 0.75
List_of_stars_in_Ophiuchus
Catalogue of Variable Stars (GCVS4.2)". Retrieved 30 July 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Triangulum
Catalogue of Variable Stars (GCVS4.2)". Retrieved 2012-04-03. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database
List_of_stars_in_Auriga
Variable star in the constellation Musca
GT Muscae, also known as 12 Muscae, is a variable star about 400 light years from the Earth, in the constellation Musca. It is a 5th magnitude star, so
GT_Muscae
Method in computer language design
– for example allowing a variable named if without clashing with the keyword if. Stropping is primarily associated with ALGOL and related languages in
Stropping_(syntax)
370 B3V + A Bibing, Sadr al Tauri, Pectus Tauri; eclipsing binary; Algol variable ε Tau ε 74 28305 20889 04h 28m 36.93s +19° 10′ 49.9″ 3.53 0.15 155 K0III
List_of_stars_in_Taurus
Sparse open cluster in the constellation of Lyra
through space, it may be associated with the Gould Belt. It includes an Algol variable star, BD+36° 3317, discovered in 2007 from Spain: this is a spectroscopic
Delta_Lyrae_cluster
Section of code that details a specific command
subroutines. assignment Fortran: variable = expression Pascal, Algol 60, Ada: variable := expression; C, C#, C++, PHP, Java: variable = expression; call Fortran:
Statement_(computer_science)
B4V Slowly pulsating B variable V397 Pup 195 V397 63786 38167 07h 49m 14.65s −35° 14′ 35.9″ 5.94 0.11 478 B9V Algol variable HR 2759 76 56410 35054 07h
List_of_stars_in_Puppis
N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 2007-01-03. Gould, B. A. "Uranometria Argentina"
List_of_stars_in_Crux
Gravitationally-binding region around a star in a binary system
contact, but they have changed substantially by the point this happens. Algol variables are the result of such situations. AE early overtaking Similar to AS
Roche_lobe
Star system in the constellation Perseus
velocity of about −12 km/s. In 1905 this system was found to be an Algol variable by Lidiya Tseraskaya. K. Graff determined a period of 0.84943 days.
RT_Persei
Eclipsing binary star of Algol type in the constellation Auriga
EO Aurigae is an eclipsing binary of Algol type in the northern constellation of Auriga. With a combined apparent magnitude of 7.71, it is too faint to
EO_Aurigae
2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. "Naming Stars". Retrieved 13 December
List_of_stars_in_Vela
Concept in programming language design
procedures in ALGOL: First and second class objects. In ALGOL, a real number may appear in an expression or be assigned to a variable, and either of
First-class_citizen
de Données astronomiques de Strasbourg. Retrieved 2007-01-03. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Leo_Minor
"Identification of a Constellation from a Position". Retrieved 2006-12-26. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Sagitta
Conditional operator in computer programming
conditional expressions with two, three, or more clauses. Languages following ALGOL-like syntax often support them with the same syntax as conditional statements
Ternary_conditional_operator
"Identification of a Constellation from a Position". Retrieved 2006-12-26. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Ursa_Minor
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
Blue dwarf star in the constellation Boötes
star in the northern constellation of Boötes. It has been identified as an Algol-type eclipsing binary, although subsequent observations do not confirm this
HD_126200
Formalism to describe programming languages
them "classes" in 1961 course materials. In the ALGOL 60 report, they were "metalinguistic variables," with other symbols defining the target language
Backus–Naur_form
Catalogue of Variable Stars (GCVS4.2)". Retrieved 2 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Ara
Type of star
the given magnitudes are in the V-band. Also a Beta Cephei variable Also an Algol variable Also a shell star Huang, L.; Guo, Z.; Hao, J.; Percy, J. R
Slowly_pulsating_B-type_star
Constellation in the northern hemisphere
1639. Over 200 variable stars are known in Coma Berenices, although many are obscure. Alpha Comae Berenices is a possible Algol variable. FK Comae Berenices
Coma_Berenices
379 A4IV VX Psc; δ Sct variable 35 Psc 35 70 1061 1196 00h 14m 58.78s +08° 49′ 15.7″ 6.02 1.50 261 F0IV UU Psc; Algol variable 73 Psc 73 105 6386 5074
List_of_stars_in_Pisces
2012-02-27. Retrieved 2010-07-16. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014. Star Name - R.H.Allen p. 246
List_of_stars_in_Indus
suspected variable δ Lib δ 19 132742 73473 15h 00m 58.39s −08° 31′ 08.2″ 4.91 0.06 304 B9.5V Zuben Elakribi or Mululizu; Algol variable, Vmax = 4.91m
List_of_stars_in_Libra
"Identification of a Constellation from a Position". Retrieved 2006-12-26. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List_of_stars_in_Vulpecula
Eclipsing binary
found from an examination of photographic plates, in 1951, that it was an Algol-type eclipsing binary system. The primary and secondary eclipses are of
ZZ_Boötis
Catalogue of Variable Stars (GCVS4.2)". Retrieved 8 April 2012. Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS
List_of_stars_in_Capricornus
Variable star system in constellation Andromeda
to the naked eye under good conditions. The primary pair consists of an Algol type eclipsing binary system of two B-type main-sequence stars both having
V348_Andromedae
Triple star system in the constellation Taurus
broad-band linear polarimetry of early-type binaries: II. Variable, phase-locked polarization in triple Algol-type system λ Tauri" (PDF), Astronomy & Astrophysics
Lambda_Tauri
−0.48 248 G4III... Algol variable 48 Per c 48 MX 25940 19343 04h 08m 39.67s +47° 42′ 45.3″ 3.96 −2.19 553 B3Ve MX Per; γ Cas variable ξ Per ξ 46 24912 18614
List_of_stars_in_Perseus
Star in the constellation Andromeda
Andromedae (TW And) is an eclipsing binary star, classified also as an Algol variable star, in the constellation Andromeda. Its brightness varies with a period
TW_Andromedae
Eclipsing binary star in the constellation Andromeda
drop to a magnitude of 13.07. This leads to its classification as an Algol variable star. The optical spectrum of QR Andromedae is not of a typical stellar
QR_Andromedae
Binary star in the constellation Aquarius
orbital plane of the two stars lies near the line of sight, so they form an Algol-type eclipsing binary. The first component of the system is an A-type main
29_Aquarii
Star in the constellation Perseus
V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally
1_Persei
"General Catalog of Variable Stars (GCVS database, version 2012Apr)". Retrieved 2013-03-24. "AAVSO Website". American Association of Variable Star Observers
List_of_stars_in_Chamaeleon
de Données astronomiques de Strasbourg. Retrieved 2007-01-02. "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
List of stars in Corona Borealis
List_of_stars_in_Corona_Borealis
Star in the constellation Orion
Theta1 Orionis A (θ1 Ori A) is a variable trinary star in the constellation Orion. Its apparent magnitude range is 6.72 to 7.65 with a period of 65.432
Theta1_Orionis_A
Polis; quintuple star; Algol variable ρ1 Sgr ρ1 44 174 181577 95168 19h 21m 40.38s −17° 50′ 50.1″ 3.92 1.06 122 F0III/IV δ Sct variable β1 Sgr β1 168 181454
List_of_stars_in_Sagittarius
Star in the constellation Perseus
binary pair forms a rotating ellipsoidal variable with a 1.53 day period. Star C forms an Algol-type variable system with the close binary, showing both
B_Persei
"Occultations from an Active Accretion Disk in a 72-day Detached Post-Algol System Detected by K2". The Astrophysical Journal. 854 (2): 109. arXiv:1801
List of transiting circumsecondary disks
List_of_transiting_circumsecondary_disks
ALGOL VARIABLE
ALGOL VARIABLE
Surname or Lastname
English
English : topographic name for someone living on (and farming) a hide of land, Old English hī(gi)d. This was a variable measure of land, differing from place to place and time to time, and seems from the etymology to have been originally fixed as the amount necessary to support one (extended) family (Old English hīgan, hīwan ‘household’). In some cases the surname is habitational, from any of the many minor places named with this word, as for example Hyde in Greater Manchester, Bedfordshire, and Hampshire.English : variant of Ide, with inorganic initial H-. Compare Herrick.Jewish (American) : Americanized spelling of Haid.
Boy/Male
Anglo, British, English
Variable
Boy/Male
Scandinavian
Surname.
Girl/Female
Biblical
According to variable songs or tunes.
Surname or Lastname
English
English : from the Middle English personal name Algod, Alegod, Halgod, of Scandinavian origin. Compare Old Danish Algot, from an unattested Alf-gautr ‘elf Goth’ or A{dh}al-gautr ‘noble Goth’.
Biblical
according to variable songs or tunes,
Surname or Lastname
English
English : from a medieval male personal name (from Latin Hilarius, a derivative of hilaris ‘cheerful’, ‘glad’, from Greek hilaros ‘propitious’, ‘joyful’). The Latin name was chosen by many early Christians to express their joy and hope of salvation, and was borne by several saints, including a 4th-century bishop of Poitiers noted for his vigorous resistance to the Arian heresy, and a 5th-century bishop of Arles. Largely due to veneration of the first of these, the name became popular in France in the forms Hilari and Hilaire, and was brought to England by the Norman conquerors.English : from the much rarer female personal name Eulalie (from Latin Eulalia, from Greek eulalos ‘eloquent’, literally well-speaking, chosen by early Christians as a reference to the gift of tongues), likewise introduced into England by the Normans. A St. Eulalia was crucified at Barcelona in the reign of the Emperor Diocletian and became the patron of that city. In England the name underwent dissimilation of the sequence -l-l- to -l-r- and the unfamiliar initial vowel was also mutilated, so that eventually the name was considered as no more than a feminine form of Hilary (of which the initial aspirate was in any case variable).
Girl/Female
Swedish
Pearl.
Surname or Lastname
English (of Norman origin)
English (of Norman origin) : habitational name from Saint-Hilaire-du-Harcouët in La Manche, which gets its name from the dedication of its church to St. Hilary, or alternatively from either of the places, in La Manche and Somme, called Saint-Lô. Both of the latter are named from a 6th-century St. Lauto, bishop of Coutances; his name is of variable form in the sources and uncertain etymology.North German : habitational name for someone from Sandel.Jewish (eastern Ashkenazic) : occupational name for a cobbler or shoemaker, Yiddish sandler (from Hebrew sandelar, from Late Latin sandalarius, an agent derivative of sandalium ‘shoe’).
Boy/Male
Anglo, Australian, British, English, French, Swedish
Variable; Brave with the Spear; Spear Rule
ALGOL VARIABLE
ALGOL VARIABLE
Boy/Male
Sikh
Heroic protector, Protector of the brave
Boy/Male
American, Australian, Chinese, Finnish, French, German, Greek, Latin, Portuguese, Spanish, Swedish
Manly; Warrior; Masculine; Brave; Similar to English Andrew
Boy/Male
American, Christian, Danish, Finnish, French, German, Hebrew, Hindu, Indian, Latin, Spanish, Swedish
God has Healed; Healer
Boy/Male
Irish
Girl/Female
Hindu, Indian, Sanskrit
Aware; Enlightened One
Boy/Male
Hindu, Indian
Lord Vishnu
Female
Russian
(Вера) Russian name, VERA means "faith; truth." Compare with another form of Vera.
Male
English
Faithful
Girl/Female
Hindu, Indian, Tamil
Special
Boy/Male
Hindu, Indian, Kannada, Oriya, Sanskrit, Telugu
Surrounded by Heroes; A Commander
ALGOL VARIABLE
ALGOL VARIABLE
ALGOL VARIABLE
ALGOL VARIABLE
ALGOL VARIABLE
a.
Having the capacity of varying or changing; capable of alternation in any manner; changeable; as, variable winds or seasons; a variable quantity.
n.
Those parts of the sea where a steady wind is not expected, especially the parts between the trade-wind belts.
a.
Liable to vary; too susceptible of change; mutable; fickle; unsteady; inconstant; as, the affections of men are variable; passions are variable.
n.
A shaking, shivering, or shuddering, as in the cold fit which precedes a fever; in old medical writings, a chill of less severity than a rigor, and more marked than an algor.
n.
A shifting wind, or one that varies in force.
a.
Pertaining to, or like, algae.
a.
Liable to be turned in opinion; changeable; variable; unsteady; inconstant; as versatile disposition.
n.
A reddish crust or sediment in wine casks, consisting essentially of crude cream of tartar, and used in marking pure cream of tartar, tartaric acid, potassium carbonate, black flux, etc., and, in dyeing, as a mordant for woolen goods; -- called also argol, wine stone, etc.
n.
The quality or state of being variable; variableness.
n.
A quantity which may increase or decrease; a quantity which admits of an infinite number of values in the same expression; a variable quantity; as, in the equation x2 - y2 = R2, x and y are variables.
n.
Crude tartar; an acidulous salt from which cream of tartar is prepared. It exists in the juice of grapes, and is deposited from wines on the sides of the casks.
n.
See Argol.
n.
A fixed star, in Medusa's head, in the constellation Perseus, remarkable for its periodic variation in brightness.
adv.
In a variable manner.
n.
Cold; chilliness.
n.
The quality or state of being variable; variability.
a.
Changeable; uncertain; inconstant; variable.
n.
That which is variable; that which varies, or is subject to change.
a.
Varying in from, character, or the like; variable; different; diverse.
n.
Crude tartar. See Argol.