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Stellar classification
An A-type main-sequence star is a main-sequence (core hydrogen burning) star of spectral type A. The spectral luminosity class is V. These stars have spectra
A-type_main-sequence_star
Stellar classification
An F-type main-sequence star is a main-sequence, core-hydrogen-fusing star of spectral type F. The spectral luminosity class is V. They have from around
F-type_main-sequence_star
Star in the stage when it has not yet reached the main sequence
A pre-main-sequence star (also known as a PMS star and PMS object) is a star in the stage when it has not yet reached the main sequence. Earlier in its
Pre-main-sequence_star
Stellar classification distinguished by bright blue luminosity
Hypergiants absolute magni- tude (MV) A B-type main-sequence star is a main-sequence (core hydrogen-burning) star of spectral type B. The spectral luminosity
B-type_main-sequence_star
Continuous band of stars that appears on plots of stellar color versus brightness
counters the star's collapse under gravity, maintaining the star in a state of hydrostatic equilibrium. The star's position on the main sequence is determined
Main_sequence
Stellar classification
A G-type main-sequence star is a main-sequence star of spectral type G. The spectral luminosity class is V. Such a star has about 0.9 to 1.1 solar masses
G-type_main-sequence_star
Stellar classification
A K-type main-sequence star (also called a "K-type dwarf" or "orange dwarf") is a main-sequence (core hydrogen-burning) star of spectral type K. The spectral
K-type_main-sequence_star
Topics referred to by the same term
White main-sequence star may refer to: A-type main-sequence star, main sequence stars ranging from 7,600 to 10,000 K F-type main-sequence star, main sequence
White_main-sequence_star
Classification of stars based on spectral properties
indicating a main-sequence star with a surface temperature around 5,800 K. Hertzsprung–Russell diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs
Stellar_classification
Main-sequence star of spectral type O
O-type main-sequence star is a main-sequence—core hydrogen-burning—star of spectral type O. The spectral luminosity class is V, although class O main sequence
O-type_main-sequence_star
Dim, low mass stars on the main sequence
least luminous, and coolest kind of star on the main sequence. Red dwarfs are by far the most common type of fusing star in the Milky Way, at least in the
Red_dwarf
Topics referred to by the same term
Blue main-sequence star may refer to: O-type main-sequence star, main sequence stars ranging above 30,000 K B-type main-sequence star, main sequence stars
Blue_main-sequence_star
Constellation in the northern celestial hemisphere
star in the night sky, as well as one of the closest. A yellow-white main-sequence star, it has a white dwarf companion. Gomeisa is a blue-white main-sequence
Canis_Minor
Point in stellar evolution
a star refers to the point on the Hertzsprung–Russell diagram where it leaves the main sequence after its main fuel is exhausted – the main sequence turnoff
Main_sequence_turnoff
Star of relatively small size and low luminosity
A dwarf star is a star of relatively small size and low luminosity. All main-sequence stars are dwarf stars. The meaning of the word "dwarf" has been
Dwarf_star
Changes to stars over their lifespans
state of equilibrium, becoming what is known as a main sequence star. Nuclear fusion powers a star for most of its existence. Initially the energy is
Stellar_evolution
Constellation in the northern celestial hemisphere
comprising an A-type main-sequence star and white dwarf in very close orbit; the latter a candidate for a future type Ia supernova as its main star runs out of
Pegasus_(constellation)
Constellation in the northern celestial hemisphere
fainter a yellow-white main sequence star. The third-brightest star is 21 Leonis Minoris, a rapidly rotating white main-sequence star of average magnitude 4
Leo_Minor
Brightest star in the constellation Leo
spectroscopic binary Regulus A consists of a blue-white main-sequence star and its companion, a pre-white dwarf. Regulus BC, also known as HD 87884, is separated
Regulus
Constellation in the southern celestial hemisphere
star is Alpha Pictoris, a white main-sequence star around 97 light-years away from Earth. Pictor also hosts RR Pictoris, a cataclysmic variable star system
Pictor
Constellation in the southern celestial hemisphere
star of spectral type K2III that has swollen to around 11 times the diameter of the Sun, having spent much of its life as a white main-sequence star.
Horologium_(constellation)
Large self-illuminated object in space
lose over half their total mass while on the main sequence. The time a star spends on the main sequence depends primarily on the amount of fuel it has
Star
Eclipsing binary star
U Cephei is an eclipsing binary star discovered in 1880. It consists of a blue-white main sequence star of spectral type B7/8V that is eclipsed every
U_Cephei
Constellation in the southern celestial hemisphere
faint constellation, with only one star brighter than fourth magnitude. Alpha Circini (Xami), a white main sequence star with an apparent magnitude of 3
Circinus
Constellation in the southern celestial hemisphere
magnitude of 1.16. Located 25.13 ± 0.09 light-years away, it is a white main-sequence star that is 1.92 ± 0.02 times as massive and 16.63 ± 0.48 as luminous
Piscis_Austrinus
Zodiac constellation in the northern hemisphere
B-type main sequence star before expanding and cooling to its current state as it spent its core hydrogen. The secondary is a white main sequence star of
Cancer_(constellation)
Constellation in the southern celestial hemisphere
Zeta2 Muscae is a white main sequence star of spectral type A5V around 330 light-years distant from Earth. It is part of a triple star system with faint
Musca
Constellation in the northern celestial hemisphere
member to make up what is actually a triple star system. The brightest component is a blue-white main-sequence star of spectral type B8V, which is 3.5 times
Perseus_(constellation)
Class of young variable stars
the pre-main-sequence phase of stellar evolution. It ends when a star of 0.5 M☉ or larger develops a radiative zone, or when a smaller star commences
T_Tauri_star
Constellation in the northern celestial hemisphere
by 0.1 magnitude with a period of 17.4 days. The primary is a white main-sequence star of spectral type A0V that is 2.91 times the mass of the Sun (M☉)
Corona_Borealis
Zodiac constellation straddling the celestial equator
Leonis, called Regulus, is a blue-white main-sequence star of magnitude 1.34, 77.5 light-years from Earth. It is a double star divisible in binoculars, with
Leo_(constellation)
Type of star, larger and brighter than the Sun
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Giant_star
Constellation in the Southern Celestial Hemisphere
now a yellow bright giant star of spectral type G5II. It likely spent most of its existence as a blue-white main sequence star of spectral type B7V. Bearing
Corvus_(constellation)
Binary star in the constellation Corona Borealis
component is a white main sequence star that has a stellar classification of A0V and 2.6 times the mass of the Sun. Estimates of the star's radius range
Alpha_Coronae_Borealis
Blue star with strong helium lines
helium main sequence, analogous to the main sequence formed by the more common hydrogen stars. Previously, a helium star was a synonym for a B-type star, but
Helium_star
Idealized physical body that absorbs all incident electromagnetic radiation
given B-V index measurement, the curves of both most common sequences of star (the main sequence and the supergiants) lie below the corresponding black-body
Black_body
Triple star system in the constellation Eridanus
List of IAU-approved Star Names. 40 Eridani A is a main-sequence dwarf of spectral type K0.5, 40 Eridani B is a 9th magnitude white dwarf of spectral type
40_Eridani
Constellation in the northern celestial hemisphere
Cepheid variable star visible from Earth. It is a triple star system, the supergiant primary star having two yellow-white main-sequence star companions that
Ursa_Minor
Stellar classification
main sequence. The coolest of them have initial masses of around 16 times the Sun. It is unclear what the upper limit to the mass of an O-type star would
O-type_star
Star in the constellation Puppis
HD 65810 is a class A2V (white main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.61 and it is approximately 241 light years
HD_65810
Stellar core remnant
around white dwarfs. It is expected that planets orbiting several AU from a star will survive the star's post-main-sequence transformation into a white dwarf
White_dwarf
Constellation in the Southern Celestial Hemisphere
is a yellow-white main sequence star of spectral type F9Ve and magnitude 9.6. Zeta Antliae is a wide optical double star. The brighter star—Zeta1 Antliae—is
Antlia
Former constellation
of Aries. The brightest star is now known as 41 Arietis (Bharani). At magnitude 3.63, it is a blue-white main sequence star of spectral type B8V around
Musca_Borealis
Star in the constellation Canis Minor
binary star system, Procyon consists of a white-hued main-sequence star of spectral type F5 IV–V, designated component A, in orbit with a faint white dwarf
Procyon
Star system in the constellation Carina
times as luminous as the Sun. Its partner A2 (or Aa2) is a blue-white main sequence star of spectral type B2V with around 9 times the Sun's mass and 3 times
QZ_Carinae
Type of star that is massive and luminous
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Supergiant
Binary star in the constellation Andromeda
is a double star in the northern constellation of Andromeda. The primary, with an apparent magnitude of 6.15, is a white main-sequence star of spectral
HD_1185
Star in the constellation Eridanus
139, e Eridani) is a star 19.7 light-years (6.0 parsecs) away from Earth in the constellation Eridanus. It is a main-sequence star with a stellar classification
82_G._Eridani
Former constellation
Andromedae is a blue-white main sequence star of spectral type B8V around 500 light-years distant from Earth. The IAU Working Group on Star Names approved the
Honores_Friderici
Zodiac constellation straddling the celestial equator
53 million years old. γ Aquarii, also called Sadachbia, is a white main sequence star of spectral type star of spectral type A0V that is between 158 and 315 million
Aquarius_(constellation)
Star in the constellation Orion
for "the endurer"), a name shared with Pi3 Orionis. It is a blue-white main sequence star of apparent magnitude 4.62 located over 1,300 light-years distant
Upsilon_Orionis
Star in the constellation Musca
luminous star around six times as massive as the Sun and 65.1 times the radius of the Sun. It is a binary star with a blue-white main sequence star companion
S_Muscae
Variable star in the constellation Corona Borealis
due to ejection of dust that obscured the star's light. Theta Coronae Borealis B is a white main sequence star of spectral type A2V that is around 2.5 times
Theta_Coronae_Borealis
Brightest star in Earth's night sky
next brightest star. Sirius is a binary star consisting of a main-sequence star of spectral type A0 or A1, termed Sirius A, and a faint white dwarf companion
Sirius
Brightest star in the constellation Lyra
the star. Vega's spectral class is A0V, making it a blue-tinged white main-sequence star that is fusing hydrogen to helium in its core. Since more massive
Vega
Binary star in the constellation Scorpius
moon and be visible in daytime. Antares B is a magnitude 5.5 blue-white main-sequence star of spectral type B2.5V; it also has numerous unusual spectral lines
Antares
Constellation in the southern celestial hemisphere
gravitationally bound to) the star HD 181327, which has its own debris disk. This latter star is a yellow-white main sequence star of spectral type F6V of magnitude
Telescopium
Star in the constellation Puppis
OU Puppis (OU Pup) is a chemically peculiar class A0 (white main-sequence) star in the constellation Puppis. Its apparent magnitude is about 4.9 and it
OU_Puppis
Constellation in the southern celestial hemisphere, containing the south celestial pole
which is a sunlike star with a massive planet with an orbital period of 1928 ± 46 days. HD 212301 is a yellow-white main sequence star with a hot jupiter
Octans
Constellation in the northern celestial hemisphere
that is around 4.01 times as massive as the Sun, and a yellow-white main sequence star of spectral type F8V that is around 3.73 times as massive as the
Lynx_(constellation)
Constellation in the northern celestial hemisphere
blue-white B9.5V main sequence star that is 2.9 times as massive as the Sun. The two orbit each other every ten years. Zeta Sagittae is a triple star system
Sagitta
Binary star in the constellation Hercules
temperature is 4,775 K. The Secondary component, 113 Herculis Ab, is a white main-sequence star of type A0 to A8. It is 2.18 times more massive than the Sun and
113_Herculis
Star in the constellation Horologium
times the diameter of the Sun, having spent much of its life as a white main sequence star. Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data
Alpha_Horologii
Star in the constellation Puppis
HD 70060 is a class A8V (white main-sequence) star in the constellation Puppis. Its apparent magnitude is 4.45 and it is approximately 93.4 light years
HD_70060
Star in the constellation Corvus
Zeta Corvi, Latinised from ζ Corvi, is a star in the constellation Corvus. It is a blue-white main-sequence star of apparent magnitude 5.21. Around 420
Zeta_Corvi
Star of luminosity class VI under the Yerkes spectral classification system
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Subdwarf
Multiple star system in the constellation Hydra
(WDS J10535-2008A) is a yellow-white main sequence star with the spectral type of F5V. The apparent magnitude of the star is +5.232. It has about 1.5 M☉
B3_Hydrae
Scatter plot of stars showing the relationship of luminosity to stellar classification
mass of large star systems Hayashi track – Luminosity–temperature relationship in stars Henyey track – Path taken by pre-main-sequence stars in the Hertzsprung–Russell
Hertzsprung–Russell_diagram
Star in the constellation of Corvus
Eta Corvi is an F-type main-sequence star, the sixth-brightest star in the constellation of Corvus. It is located 59.5 light-years (18.2 parsecs) from
Eta_Corvi
Puffy exoplanet in constellation Hydra
signal from the planet. The planet orbits a yellow-white main-sequence star named WASP-193. The star has a mass of 1.059+0.067 −0.068 M☉, a radius of 1
WASP-193b
Star in the constellation Pyxis
when it became clear that it is also a binary star system. The main star is a white main sequence star of spectral type A4V that is around 1.85±0.05 times
XX_Pyxidis
Constellation in the northern celestial hemisphere
expanded and cooled off the main sequence—likely to have lived most of its stellar life as a blue-white B-type main sequence star. Its common name comes from
Boötes
Star in the Pisces constellation
WASP-76, also known as BD+01 316, is a yellow-white main sequence star in the constellation of Pisces. A suspected stellar companion at a projected separation
WASP-76
Pattern of stars in the Northern Hemisphere
Astronomers have determined that if the star rotated 10% faster it would rip itself apart. Denebola is a white main sequence star in the constellation Leo. With
Spring_Triangle
Star in the constellation Andromeda
is a binary star located 44 light-years from Earth in the constellation of Andromeda. The system consists of an F-type main-sequence star (designated
Upsilon_Andromedae
Hot, giant star of early spectral type
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Blue_giant
Type of large cool star
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Red_giant
Variable star in the constellation Ara
is a blue-white main sequence star of spectral type B5V that is 5 times as massive as the Sun, while the secondary is a yellow-white star of spectral
R_Arae
Star in the constellation Cepheus
V Cephei is a white main sequence star in the constellation Cepheus. It only varies slightly by 0.03 of a magnitude. It was suspected of being variable
V_Cephei
Constellation in the northern celestial hemisphere
primary is a white star of spectral type A5IV with 3.5 times the mass of the Sun that is beginning to expand and evolve off the main sequence. The secondary
Triangulum
Minor constellation in the southern sky
ranges between magnitudes 5.90 and 5.94. Nu Phoenicis is a yellow-white main sequence star of spectral type F9V and magnitude 4.96. Lying some 49 light years
Phoenix_(constellation)
Binary pulsar system in the constellation Scorpius
AR Scorpii (AR Sco) is a binary star system that consists of a pulsar-like white dwarf and a red dwarf star. It is located close to the ecliptic plane
AR_Scorpii
Early stage in the process of star formation
infalling gas is depleted, leaving a pre-main-sequence star, which contracts to later become a main-sequence star at the onset of hydrogen fusion producing
Protostar
Brightest star in the constellation Aquila
α Aquilae and abbreviated Alpha Aql or α Aql. Altair is an A-type main-sequence star with an apparent visual magnitude of 0.77 and is one of the vertices
Altair
Hot, luminous star with a spectral type of A9 or earlier
diagram Spectral type O B A F G K M L T Brown dwarfs White dwarfs Red dwarfs Subdwarfs Main sequence ("dwarfs") Subgiants Giants Red giants Blue giants
Blue_supergiant
Star in the constellation Camelopardalis
Gliese 445 (Gl 445 or AC +79 3888) is an M-type main sequence star in the northern part of the northern circumpolar constellation of Camelopardalis. Gliese
Gliese_445
Constellation in the southern celestial hemisphere
apparent magnitude of 3.8. It spent much of its life as a blue-white (B-type) main sequence star before expanding, cooling and brightening as it used up its
Apus
Constellation in the southern celestial hemisphere
luminosity. Alpha Arae is a blue-white main sequence star of magnitude 2.95, that is 270 ± 20 light-years from Earth. This star is around 9.6 times as massive
Ara_(constellation)
Minor constellation in the southern celestial hemisphere
68—is the brightest star in the constellation. Having spent much of its 620-million-year lifespan as a blue-white main sequence star, it has swollen and
Microscopium
Constellation in the southern celestial hemisphere
other optical double, composed of Eta1 and Eta2. Eta1 is a blue-white main sequence star of spectral type B9V that was suspected of being variable, and
Hydrus
Red dwarf star in the constellation Ophiuchus
Barnard's Star is a small red dwarf star in the constellation of Ophiuchus. At a distance of 5.96 light-years (1.83 pc) from Earth, it is the fourth-nearest-known
Barnard's_Star
Quaternary star system in the constellation Libra
1093/mnras/staa282. Hillenbrand, Lynne A.; White, Russel J. (2004-04-01). "An Assessment of Dynamical Mass Constraints on Pre-Main-Sequence Evolutionary Tracks". The Astrophysical
Gliese_570
Star in the constellation Perseus
distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. In 1998 the star was named a candidate
50_Persei
Brightest star in the constellation of Carina
as a blue-white main sequence star of around 10 solar masses, before exhausting its core hydrogen and evolving away from the main sequence. The position
Canopus
Star in the constellation Pegasus
day. Its companion (IK Pegasi B) is a massive white dwarf—a star that has evolved past the main sequence and is no longer generating energy through nuclear
IK_Pegasi
Star system in the constellation Taurus
magnitude 6.28 A0 main-sequence star 117" away; C is V647 Tauri, a δ Sct variable star; and D is a magnitude 9.15 F3 main-sequence star. V647 Tau varies
Alcyone_(star)
Star in the constellation Musca
from ζ2 Muscae, is a star in the southern constellation of Musca. Its apparent magnitude is 5.16. This is a white main sequence star of spectral type A5V
Zeta2_Muscae
Triple star system
-9.93. The system is made up of two B-type main sequence stars in an eccentric 15-day orbit, with a white dwarf in a wider orbit. "HD 59635". SIMBAD.
HD_59635
Layer of a star's atmosphere
almost all luminous stars other than white dwarfs. They are most prominent and magnetically active on lower-main sequence stars, on brown dwarfs of F and later
Chromosphere
Nearest star to the Solar System
Proxima's relatively low energy-production rate, mean that it will be a main-sequence star for another four trillion years. Proxima Centauri has two known exoplanets
Proxima_Centauri
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
Boy/Male
Arabic, Hindu, Indian, Muslim, Sindhi
Cloud that Carries Rain; Prophet Name; Rain Clouds
Girl/Female
Indian
Proper name, Cloud that carries rain
Female
Swedish
Swedish contracted form of Latin Magdalena, MALIN means "of Magdala."
Surname or Lastname
English
English : occupational name for a watchman, Anglo-Norman French waite (of Germanic origin; compare Wachter), or from the same word in its original abstract/collective sense, ‘the watch’. There may also have been some late confusion with White.
Boy/Male
Indian, Sanskrit
Order; Sequence
Surname or Lastname
English
English : patronymic from White.
Boy/Male
Muslim/Islamic
Cloud that carries rain
Girl/Female
Bengali, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Sanskrit, Telugu
Sequence
Girl/Female
Tamil
Anuloma | அநà¯à®²à¯‹à®®à®¾
Sequence
Anuloma | அநà¯à®²à¯‹à®®à®¾
Girl/Female
British, English
Bright; Pure; Name of Colour
Boy/Male
Arabic, Muslim
Benefit
Boy/Male
Indian, Sikh
Music; In-sequence
Male
Hindi/Indian
(मणि) Hindi name MANI means "jewel." Compare with another form of Mani.
Boy/Male
British, English
White
Boy/Male
Native American
White man.
Male
German
German byname MANN means "a fierce strong man" or simply "man."
Surname or Lastname
English, Scottish, and Irish
English, Scottish, and Irish : from Middle English whit ‘white’, hence a nickname for someone with white hair or an unnaturally pale complexion. In some cases it represents a Middle English personal name, from an Old English byname, Hwīt(a), of this origin. As a Scottish and Irish surname it has been widely used as a translation of the many Gaelic names based on bán ‘white’ (see Bain 1) or fionn ‘fair’ (see Finn 1). There has also been some confusion with Wight.Translated form of cognate and equivalent names in other languages, such as German Weiss, French Blanc, Polish Białas (see Bialas), etc.Peregrine White (1620–1704), brother of Resolved, was born in Cape Cod harbor on board the Mayflower, thus becoming the first child of English descent to be born in New England. His father, William White, was the son of the rector of Barham, near Ipswich, Suffolk, England; he died in 1621 during the first winter at Plymouth Colony.
Boy/Male
Australian, Portuguese
White; Blond; Fair-one
Surname or Lastname
Scottish and northern English
Scottish and northern English : topographic name for a dweller at the chief farm (or home farm) on an estate, Scottish mains, or a habitational name from any of the various minor places named with this word (originally a shortened form of domain, later associated with the adjective main ‘principal’).English and Scottish : variant of Main 1–4.
Surname or Lastname
English, German, Dutch (De Mann), and Jewish (Ashkenazic)
English, German, Dutch (De Mann), and Jewish (Ashkenazic) : nickname for a fierce or strong man, or for a man contrasted with a boy, from Middle English, Middle High German, Middle Dutch man. In some cases it may have arisen as an occupational name for a servant, from the medieval use of the term to describe a person of inferior social status. The Jewish surname can be ornamental.English and German : from a Germanic personal name, found in Old English as Manna. This originated either as a byname or else as a short form of a compound name containing this element, such as Hermann.Jewish (Ashkenazic) : from the Yiddish male personal name Man (cognate with 1).Indian (Panjab) : Hindu (Jat) and Sikh name of unknown meaning.
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
Girl/Female
Australian, Greek, Swedish
Pearl; Diminutive Form of Margaret
Female
Spanish
Spanish name EMPERATRIZ means "empress."
Surname or Lastname
English
English : occupational name for an official who was responsible for protecting land or enclosed forest from damage by animals, poachers, or vandals, from Middle English hay ‘enclosure’ (see Hay 1) + ward ‘guardian’.
Boy/Male
English American
Friend; good friend.
Boy/Male
Arabic, Australian
Holding High
Boy/Male
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Telugu
Happy
Boy/Male
Welsh Celtic
Old.
Girl/Female
French, German, Latin, Spanish
Little and Womanly; Variant of Rosa; Beautiful
Boy/Male
Hindu, Indian, Kannada, Telugu
Lord Shiv; Shiv
Boy/Male
Hebrew Spanish
God is with us; god is among us.
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
WHITE MAIN-SEQUENCE-STAR
n.
All five cards, of a hand, in consecutive order as to value, but not necessarily of the same suit; when of one suit, it is called a sequence flush.
n.
A white pigment; as, Venice white.
n.
Something having the color of snow; something white, or nearly so; as, the white of the eye.
a.
As white as cream.
n.
A person with a white skin; a member of the white, or Caucasian, races of men.
n.
Simple succession, or the coming after in time, without asserting or implying causative energy; as, the reactions of chemical agents may be conceived as merely invariable sequences.
v. t.
To make white; to bleach; to blanch; to whitewash; as, to whiten a wall; to whiten cloth.
a.
White as snow; very white.
n.
That which follows as a result; a sequence.
v.
The chief or principal part; the main or most important thing.
a.
Very; extremely; as, main heavy.
n.
The state of being sequent; succession; order of following; arrangement.
v. i.
To grow white; to turn or become white or whiter; as, the hair whitens with age; the sea whitens with foam; the trees in spring whiten with blossoms.
n.
See White-face.
imp. & p. p.
of White
v. t.
To make white; to whiten; to whitewash; to bleach.
a.
Having a white front; as, the white-fronted lemur.
n.
A main-hamper.
conj.
During the time that; as long as; whilst; at the same time that; as, while I write, you sleep.
v. t.
To decree or announce as a sentence.