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Radio astronomy observatory in New Mexico, US
The Karl G. Jansky Very Large Array (VLA) is a centimeter-wavelength radio astronomy observatory in the southwestern United States built in the 1970s.
Very_Large_Array
66-telescope radio observatory in Chile
The Atacama Large Millimeter/submillimeter Array (ALMA) is an astronomical interferometer of 66 radio telescopes in the Atacama Desert of northern Chile
Atacama Large Millimeter Array
Atacama_Large_Millimeter_Array
Telescope in the Atacama Desert, Chile
generally used separately but can be combined to achieve a very high angular resolution. The VLT array is also complemented by four movable Auxiliary Telescopes
Very_Large_Telescope
System of ten radio telescopes
The Very Long Baseline Array (VLBA) is a system of ten radio telescopes which are operated remotely from their Array Operations Center located in Socorro
Very_Long_Baseline_Array
1997 film by Robert Zemeckis
Bassett, Rob Lowe, Jake Busey, and David Morse co-star. It features the Very Large Array in New Mexico, the Arecibo Observatory in Puerto Rico, the Mir space
Contact_(1997_American_film)
Array used for astronomical observations
leading to the development of large instruments such as the Very Large Array and the Atacama Large Millimeter Array. Optical/infrared interferometry
Astronomical_interferometer
American nonprofit organization
the Karl G. Jansky Very Large Array (VLA), the North American share of the international Atacama Large Millimeter/submillimeter Array (ALMA), and NRAO's
Associated_Universities,_Inc.
Subfield of astronomy that studies celestial objects at radio frequencies
are required in order to get a good quality image. For example, the Very Large Array has 27 telescopes giving 351 independent baselines at once. Beginning
Radio_astronomy
Hypothetical black hole formed soon after the Big Bang
signals related to the existence of PBHs. ngVLA – the next generation Very Large Array will be able to improve GW bounds by an order of magnitude over the
Primordial_black_hole
Radio telescope in the Canary Islands
The Very Small Array (VSA) was a 14-element interferometric radio telescope operating between 26 and 36 GHz that is used to study the cosmic microwave
Very_Small_Array
1977 narrowband radio signal from SETI
sensitive Very Large Array did not detect the signal, and the probability that a signal below the detection threshold of the Very Large Array could be
Wow!_signal
Directional radio antenna used in radio astronomy
seen from the radio source, is called a baseline. For example, the Very Large Array (VLA) near Socorro, New Mexico has 27 telescopes with 351 independent
Radio_telescope
Federally funded research and development center for radio astronomy
Domenici Array Operations Center (AOC). Located on the New Mexico Tech university campus, the AOC serves as the headquarters for the Very Large Array (VLA)
National Radio Astronomy Observatory
National_Radio_Astronomy_Observatory
American physicist and radio engineer (1905–1950)
the NRAO renamed the Very Large Array (VLA) radio telescope in Magdalena, New Mexico, as the Karl G. Jansky Very Large Array in honor of Jansky's contribution
Karl_Guthe_Jansky
International radio telescope project
telescope's collecting area, not to the extent of the entire telescope array, which is far larger. Conceived in the 1990s, and further developed and designed by
Square_Kilometre_Array
Reionization-Limited HI Cloud near to the spiral galaxy M94
confirmation of the H I detection came from follow-up observations with the Very Large Array (VLA) and the Robert C. Byrd Green Bank Telescope (GBT). CDG-2 "Cloud
Cloud-9_(RELHIC)
Barred spiral galaxy in the Local Group
Burst Mission and Chandra X-Ray Observatory, the Very Large Array, and the Very Long Baseline Array. The microquasar was the first observed within the
Andromeda_Galaxy
Radio source at center of the Milky Way
plausible candidate for the location of this supermassive black hole. The Very Large Telescope at Chile and Keck Telescope at Hawaii have detected stars orbiting
Sagittarius_A
Set of multiple antennas which work together
Turnstile antenna array used for satellite communication Flat microstrip array antenna for satellite TV reception. The Very Large Array, a radio telescope
Antenna_array
Radio telescope array in California
which can be instantaneously imaged is 17 times that obtainable by the Very Large Array telescope. The instantaneous frequency coverage of more than four octaves
Allen_Telescope_Array
Effort to find civilizations not from Earth
"Allen Telescope Array" (ATA) after the project's benefactor, Paul Allen. Its sensitivity is designed to be equivalent to a single large dish more than
Search for extraterrestrial intelligence
Search_for_extraterrestrial_intelligence
2025-02-28. "About the Next-Generation Very Large Array". NRAO. Retrieved 2026-03-01. "Largest Telescope Array in North America Under Development by NRAO"
List_of_radio_telescopes
County in New Mexico, United States
Technology, the National Radio Astronomy Observatory and its associated Very Large Array, the Magdalena Ridge Observatory, and the Langmuir Laboratory for Atmospheric
Socorro_County,_New_Mexico
Unincorporated community in New Mexico, United States
of the Gila National Forest and not very far west of the Plains of San Agustin, the location of the Very Large Array radio telescope, which is also located
Pie_Town,_New_Mexico
1982 studio album by Night Ranger
Entertainment Co. The cover art of the album features dishes of the Very Large Array in central New Mexico. During the recording of the album, the band
Dawn_Patrol_(album)
American medical physicist and astronaut (born 1983)
Laboratory in Washington, D.C., where he studied supernovae using the Very Large Array radio telescope. He also volunteered as an emergency medical technician
Christopher Williams (astronaut)
Christopher_Williams_(astronaut)
Red supergiant star in the constellation Orion
of roughly 152±20 pc or 500±65 ly. In 2008, measurements using the Very Large Array (VLA) produced a radio solution of 5.07±1.10 mas, equaling a distance
Betelgeuse
from the Milky Way. SN 1986J was discovered August 21, 1986 using the Very Large Array radio telescope, about three years after the initial explosion. On
SN_1986J
Neutron star in the Scutum constellation
telescope archives, including the Giant Metrewave Radio Telescope and the Very Large Array, which revealed evidence of the object dating back to 1988. The signature
GPM_J1839−10
1993 live album by Dire Straits
"Money for Nothing". The cover art of the album features dishes of the Very Large Array in central New Mexico. In November 2023, On the Night was included
On_the_Night
Radio telescope in Green Bank, WV, US
vital complement to the Atacama Large Millimeter Array, the Expanded Very Large Array, the Very Long Baseline Array, and other high-angular-resolution
Green_Bank_Telescope
Network of radio communication facilities run by NASA
such as the Parkes Observatory, the Green Bank Telescope, and the Very Large Array, are sometimes used to supplement the antennas of the DSN. The antennas
NASA_Deep_Space_Network
Radio telescope network located mainly in the Netherlands
The Low-Frequency Array (LOFAR) is a large radio telescope, with an antenna network located mainly in the Netherlands, and spreading across 7 other European
Low-Frequency_Array
Former radio telescope in Puerto Rico, United States
the karst regions of Puerto Rico that offered perfect cavities for a very large dish. Originally, a fixed parabolic reflector was envisioned, pointing
Arecibo_Telescope
Radio telescope array
historically required cooling to very low temperatures, which made each antenna too expensive to build such a large array. Therefore the second enabling
Deep_Synoptic_Array
Gamma-ray burst detected on May 8, 1997
astronomer Dale Frail at the National Radio Astronomy Observatory's Very Large Array. Frail began making observations at a wavelength of 20 centimeters
GRB_970508
Phenomenon resulting from the superposition of two waves
consist either of arrays of parabolic dishes or two-dimensional arrays of omni-directional antennas. All of the telescopes in the array are widely separated
Wave_interference
Astronomy organization
pulsars to create a pulsar timing array. They use data from the Green Bank Telescope, Arecibo Observatory, the Very Large Array, and the Canadian Hydrogen Intensity
North American Nanohertz Observatory for Gravitational Waves
North_American_Nanohertz_Observatory_for_Gravitational_Waves
Radio galaxy in the constellation Centaurus
infrared images of Centaurus A in 2006. Evidence of gamma emissions with very high energy (more than 100 GeV) was detected by the H.E.S.S Observatory in
Centaurus_A
Constellation in the southern hemisphere
in data of the United States National Radio Astronomy Observatory's Very Large Array Sky Survey. There is some speculation that the void may be due to quantum
Eridanus_(constellation)
Low redshift quasar in the constellation Boötes
48 shows a similar [O II]/Hβ ratio. Follow-up observations with the Very Large Array showed two 10-12 kpc bubbles, one "eastern bubble", consistent with
Teacup_galaxy
Scientific study of celestial objects
of active galaxies, and at a larger scale, the groups and clusters of galaxies. These assist the understanding of the large-scale structure of the cosmos
Astronomy
American astronomer
was also heavily involved in the development of the Very Large Array and the Very Long Baseline Array. Clark earned a BS in 1959 and a PhD in 1964, both
Barry_G._Clark
English astrophysicist (born 1984)
POSSUM survey with the Australian Square Kilometre Array Pathfinder, on the Board of the Very Large Array Survey Science Group and co-chair of the Extragalactic
Jamie_Farnes
Topics referred to by the same term
Sky at Twenty-Centimeters, an astronomical survey carried out by the Very Large Array Far Infrared and Sub-millimetre Telescope, of the Herschel Space Observatory
First
Observatory
Detail from below Plaque inside the building Historical control electronics Array of brushes. The brushes allowed the mirror to move continuously in the military
Stockert_Radio_Telescope
1995 single by Dave Matthews Band
Matthews used to do. The cover art of the album features dishes of the Very Large Array in central New Mexico. Mika has recorded a version of this song as
Satellite (Dave Matthews Band song)
Satellite_(Dave_Matthews_Band_song)
Physics research center
(>1 GHz) and gain comparable to photomultiplier tubes, while also producing very low noise, and significantly reducing false positives. Its field-of-view
Berkeley_SETI_Research_Center
2002 studio album by Bon Jovi
Its cover art, a stylized image of a radio telescope dish at the Very Large Array, was photographed by Kevin Westenberg and produced by Kevin Reagan
Bounce_(Bon_Jovi_album)
Census-designated place in New Mexico, United States
State Road 12, Datil is on the edge of the Cibola National Forest. The Very Large Array is also nearby. Datil is named after the nearby Datil Mountains. The
Datil,_New_Mexico
Substellar object
magnetic fields. Observing programs at the Arecibo Observatory and the Very Large Array have detected over a dozen such objects, which are also called ultracool
Brown_dwarf
1982 science fiction novel by Arthur C. Clarke
telescope; the film approximates this opening scene, instead using the Very Large Array as its setting. Victor Millson: Floyd's bureaucratic successor, rival
2010:_Odyssey_Two
Nebula around the Pistol Star
thousand years ago. The nebula was first observed in radio light by the Very Large Array in the early 1980s. It was named for its shape as seen in low resolution
Pistol_Nebula
Ongoing NASA interstellar program
Telescope was brought into the array in time for the fly-by of Neptune in 1989. In the United States, the Very Large Array in New Mexico was brought into
Voyager_program
1990s astrophysics experiment in Utah
Shower Array (CASA) was a significant ultra high high-energy astrophysics experiment operating in the 1990s. It consisted of a very large array of scintillation
Chicago_Air_Shower_Array
Region in the southwestern U.S. state of New Mexico
the Very Large Array, a radio astronomy observatory. The plains were chosen for the observatory because of their isolated location away from large population
Plains_of_San_Agustin
Observatory in northern California, USA
the Western United States. The observatory is home to the Allen Telescope Array and one of the three CHIME FRB outriggers, as well a number of other smaller
Hat_Creek_Radio_Observatory
Village in the United States
astronomers and astro-photographers together under its very dark skies. The Very Large Array lies 24 miles (39 km) due west of the community. The Magdalena
Magdalena,_New_Mexico
Radio telescope at Jodrell Bank Observatory, Cheshire, England
1988. The telescope forms part of the MERLIN and European VLBI Network arrays of radio telescopes. Both Bernard Lovell and Charles Husband were knighted
Lovell_Telescope
Galaxy in the constellation Hydra
from Australia on 3 July 1983. On 6 July, it was observed with the Very Large Array and became the first Type I supernova to have a radio emission detected
Messier_83
Astronomical observatory in Cheshire, England
ran from the 1980s to 2000, and the amplifiers and cryostats for the Very Small Array. It has also constructed the front-end modules of the 30 and 44 GHz
Jodrell_Bank_Observatory
Hubble Space Telescope Treasury Project
incorporates commitments from observatories around the world, such as the Very Large Array radio observatory, the European Space Agency's XMM-Newton satellite
Cosmic_Evolution_Survey
Tidal disruption event
radio emission from AT2018hyz using the Very Large Array (VLA), MeerKAT, and the Australia Telescope Compact Array (ATCA), despite no radio emission detected
AT_2018hyz
Microwave radio frequency band from 8–12 GHz
which work in the X-band including the Green Bank Telescope and the Very Large Array. Radio Astronomy has a Frequency Allocation for (quiet) bands at 10
X_band
Pair of colliding ring galaxies
COSMOS-Web field from the Chandra X-ray Observatory (CXO) and the Very Large Array (VLA) and new Keck/LRIS spectra confirmed the presence of an active
Infinity_Galaxy
BATSE-triggers from the same direction. Follow-up radio observations with the Very Large Array by Dale Frail did not find an afterglow at the derived position from
History of gamma-ray burst research
History_of_gamma-ray_burst_research
Stars with a supergiant luminosity class with a spectral type of K or M
"Distance and Kinematics of the Red Hypergiant VY CMa: Very Long Baseline Array and Very Large Array Astrometry". The Astrophysical Journal. 744 (1): 23
Red_supergiant
Multiple exposure image of deep space in the constellation Ursa Major
telescopes, the Kitt Peak National Observatory telescopes, and the Very Large Array (VLA) could conduct follow-up observations. Twenty fields satisfying
Hubble_Deep_Field
electrodynamics, quantum mechanics, and electrochemistry; and so is studied by a very large array of different professional researchers. The fields they reside in include
Quantum_electrochemistry
Elliptical globular cluster in the constellation Sagittarius
of between 10 and 20 solar masses (M☉) each were unearthed with the Very Large Array radio telescope in New Mexico and corroborated by the Chandra X-ray
Messier_22
Stream of ionized matter flowing away from a rotating astronomical object
the relativistic jet The M87 jet seen by the Very Large Array in radio frequency (the viewing field is larger and rotated with respect to the above image
Astrophysical_jet
Galaxy in the constellation Serpens
Observatory, Hubble Space Telescope, Spitzer Space Telescope, the Very Large Array, and the Multi-Element Radio Linked Interferometer Network. "Search
3C_321
Canadian astronomer
NRAO's Assistant Director for the Karl G. Jansky Very Large Array and the Very Long Baseline Array, and site director for New Mexico operations. In 2016
Dale_Frail
Disc galaxy in the constellation Cancer
observations made with the Atacama Large Millimeter Array (ALMA), it was studied with the Karl G. Jansky Very Large Array (JVLA) observatory and the Hubble
DLA0817g
Astronomical object appearing as a bright blob, discovered by Hanny van Arkel
optical images, and a "western bubble", only seen in radio images by the Very Large Array. The Chandra observations revealed a loop in x-ray emission, consistent
Hanny's_Voorwerp
Radio waves produced by the Sun
observations include the Very Large Array, Atacama Large Millimeter Array, Murchison Widefield Array, and Low-Frequency Array. The collage above shows
Solar_radio_emission
Passive sound reflection device
which has a sculpture made of limestone called the Listening Vessels Very Large Array – Socorro County, New Mexico Visitor Center has a 'whispering gallery'
Acoustic_mirror
Galaxy in the constellation Cetus
was first measured at radio wavelengths by the Very Long Baseline Array (VLBA) and the Very Large Array (VLA). The hot dust around the nucleus was subsequently
Messier_77
Indian astrophysicist and radio astronomer
University of Bombay. It was an exciting period in radio astronomy when the Very Large Array in New Mexico came into operation producing high-quality radio images
D._J._Saikia
Binary systems of planetary-mass objects
were found in the archives of observations of the Karl G. Jansky Very Large Array (VLA) of the National Radio Astronomy Observatory (NRAO) over three
Jupiter-mass_binary_object
Brown dwarf in the constellation Draco
emission that it exhibited in the past. Radio observations with the Very Large Array detected the brown dwarf. The strong detection is due to weakly circularly
2MASS_1237+6526
U.S. region
National Monument. Southwestern New Mexico is also home to both the Very Large Array and White Sands Missile Range containing the Trinity Site. The geology
Southwestern_New_Mexico
Canadian radio telescope
Intensity and Real-time Analysis eXperiment (HIRAX), a proposed radio telescope array in South Africa in the same frequency band as CHIME Canadian Hydrogen Observatory
Canadian Hydrogen Intensity Mapping Experiment
Canadian_Hydrogen_Intensity_Mapping_Experiment
Protoplanetary Nebula in the constellation of Cygnus
was discovered by Rudolph Minkowski in 1946. It was imaged by the Very Large Array (VLA) in 1983 and by Hubble Space Telescope in 1996. The object is
M1-92
Computer architecture bit width
Machine. By using a 1-bit architecture for the individual processors a very large array (e.g. the Connection Machine had 65,536 processors) could be constructed
1-bit_computing
Quasar in the constellation Auriga
1.2 ± 0.4 c. 3C 147 is one of four primary calibrators used by the Very Large Array (along with 3C 48, 3C 138, and 3C 286). Visibilities of all other sources
3C_147
Film making technique
(1989). The Bat Cave in Batman Returns (1992). The Karl G. Jansky Very Large Array in Contact (1997). The bunkhouse of the Furious Five and its surrounding
Matte_painting
Quasar discovered in 1960
same redshift. 3C 48 is one of four primary calibrators used by the Very Large Array (along with 3C 138 and 3C 147, and 3C 286). Visibilities of all other
3C_48
Location used for observing terrestrial or celestial events
shielding. Some of the world's major radio observatories include the Very Large Array in New Mexico, United States, Jodrell Bank in the UK, Arecibo in Puerto
Observatory
Star in the constellation Perseus
orbit. Later the object was also detected as a radio source with the Very Large Array (VLA) and named JVLA 1. Researchers observed unprecedented variations
LRLL_54361
Astronomical survey
astronomical survey of the Northern Hemisphere carried out by the Very Large Array (VLA) of the National Radio Astronomy Observatory (NRAO), resulting
NRAO_VLA_Sky_Survey
Class-M stars with a temperature below 2,700 K
astrophysicists began observation campaigns at the Arecibo Observatory and the Very Large Array to search for additional objects emitting radio waves. To date hundreds
Ultra-cool_dwarf
Astronomical object with two images
frequency images. In mid-1979, a team led by David Roberts at the Very Large Array (VLA) near Socorro, New Mexico, discovered a relativistic jet emerging
Twin_Quasar
Type of antenna
A passive electronically scanned array (PESA), also known as passive phased array, is an antenna in which the beam of radio waves can be electronically
Passive electronically scanned array
Passive_electronically_scanned_array
Brightest cluster galaxy of Abell 2390
redshift of (z) 0.230. It was first discovered by astronomers in the Very Large Array (VLA) survey in 1993. Abell 2390 BCG is known to host a complex radio
Abell_2390_BCG
Diffuse nebula in the constellation Orion
being ionized from the outside by M42. Later observations with the Very Large Array showed solar-system-sized condensations associated with these sources
Orion_Nebula
Astronomical observatory in Chile
kilometers from the main peak. It consists of an array of twelve 0.2-meter robotic telescopes with a very large field of view of 96 square degrees or several
Paranal_Observatory
University of Tasmania; the 22m dish of Mopra, part of the Long Baseline Array, operated by CSIRO; the 25m dish of Sheshan near Shanghai, operated by the
Joint Institute for Very Long Baseline Interferometry European Research Infrastructure Consortium
Joint_Institute_for_Very_Long_Baseline_Interferometry_European_Research_Infrastructure_Consortium
Quasar often used for calibration
detected by Fermi-LAT. High resolution images made at 8.4 GHz with the Very Large Array show that 3C 286 has a jet about 2.6 arc seconds long extending west-south-west
3C_286
American poet
of Literary Magazines and Presses (CLMP). In 2023, Osman released A Very Large Array: Selected Poems (DABA), a collection of work published in various out-of-print
Jena_Osman
VERY LARGE-ARRAY
VERY LARGE-ARRAY
Girl/Female
Persian American
Child of light. Famous Bearer: Margaret Thatcher, former Prime Minister of the United Kingdom.
Boy/Male
Arabic, Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Muslim, Parsi, Pashtun, Telugu, Ukrainian
Large; Very Tall; Decoration; Unknown; Brave Fighter
Female
Russian
(Вера) Russian name, VERA means "faith; truth." Compare with another form of Vera.
Male
Portuguese
Portuguese form of Roman Latin Verissimus, VERÃSSIMO means "very true."
Boy/Male
Indian
Large, Very tall (, Son of sohrab)
Surname or Lastname
English
English : variant of Sark.German : unexplained.
Female
English
English surname transferred to unisex forename use, derived from the Middle English personal name Alfred, AVERY means "elf counsel."
Girl/Female
English
Lark.
Surname or Lastname
English and French
English and French : nickname (literal or ironic) meaning ‘generous’, from Middle English, Old French large ‘generous’, ‘free’ (Latin largus ‘abundant’). The English word came to acquire its modern sense only gradually during the Middle Ages; it is used to mean ‘ample in quantity’ in the 13th century, and the sense ‘broad’ first occurs in the 14th. This use is probably too late for the surname to have originated as a nickname for a fat man.
Surname or Lastname
English (mainly Norfolk)
English (mainly Norfolk) : variant of Lark 1.
Male
English
Short form of English Vernon, VERN means "place of alder trees."
Surname or Lastname
English
English : nickname from Old French verai ‘true’.The widow Bridget Very settled with her children in Salem, MA, in about 1634. She had many prominent descendants, including the poet Jones Very (1813–1880).
Boy/Male
French
The red-haired one.
Male
English
English surname transferred to forename use, from a Norman baronial name VERE means "alder."
Boy/Male
Dutch Anglo Saxon
Tall.
Boy/Male
Muslim
Large, Very tall (, Son of sohrab)
Female
English
Short form of English Margaret, MARGE means "pearl."
Male
English
English surname transferred to unisex forename use, originally a Norman French form of Middle English Alfred, AVERY means "elf counsel."
Surname or Lastname
English and Scottish (of Norman origin)
English and Scottish (of Norman origin) : habitational name from any of numerous places named in France named Vert or Le Vert.
Surname or Lastname
English and French
English and French : metonymic occupational name for a boatman, from Middle English, Old French barge ‘boat’, ‘barge’.Dutch : variant of Berg.
VERY LARGE-ARRAY
VERY LARGE-ARRAY
Boy/Male
Hebrew
Uncle.
Surname or Lastname
English, French, German, Dutch, Spanish (Simón), Czech and Slovak (Šimon), Slovenian, Hungarian, and Jewish (Ashkenazic)
English, French, German, Dutch, Spanish (Simón), Czech and Slovak (Å imon), Slovenian, Hungarian, and Jewish (Ashkenazic) : from the personal name, Hebrew Shim‘on, which is probably derived from the verb sham‘a ‘to hearken’. In the Vulgate and in many vernacular versions of the Old Testament, this is usually rendered Simeon. In the Greek New Testament, however, the name occurs as SimÅn, as a result of assimilation to the pre-existing Greek byname SÄ«mÅn (from sÄ«mos ‘snub-nosed’). Both Simon and Simeon were in use as personal names in western Europe from the Middle Ages onward. In Christendom the former was always more popular, at least in part because of its associations with the apostle Simon Peter, the brother of Andrew. In Britain there was also confusion from an early date with Anglo-Scandinavian forms of Sigmund (see Siegmund), a name whose popularity was reinforced at the Conquest by the Norman form Simund.The earliest documented bearer of the surname Simon in New France came from the Saintonge region of France and was in Montreal by 1655. Another, from Paris, is recorded in Quebec City in 1659 with the secondary surname Lapointe.
Girl/Female
Arabic, Indian, Irish, Muslim, Tamil
Rainy Cloud
Girl/Female
Indian
Daughter
Boy/Male
Bengali, Indian
Upstream of a River
Female
English
Latin form of Macedonian Greek Berenike, BERENICE means "bringer of victory." In the bible, this is the name of the eldest daughter of Herod Agrippa.
Girl/Female
American, Arabic, Buddhist, Danish, Gujarati, Hebrew, Hindu, Indian, Kannada, Marathi, Muslim, Punjabi, Sanskrit, Sikh, Tamil
A Star; Action; Fate; Destiny
Boy/Male
Hindu, Indian, Tamil
Warrior Arjuna
Surname or Lastname
English (Yorkshire)
English (Yorkshire) : variant of Farley.
Male
Scottish
Scottish Gaelic form of German Wilhelm, UILLEAM means "will-helmet."
VERY LARGE-ARRAY
VERY LARGE-ARRAY
VERY LARGE-ARRAY
VERY LARGE-ARRAY
VERY LARGE-ARRAY
v. i.
To disagree; to be at variance or in dissension; as, men vary in opinion.
a.
Very large; monstrous; astonishing; as, a whapping story.
n.
Anything very large, forcible, or astonishing.
n.
A movement or piece in largo time.
v. t.
To change the aspect of; to alter in form, appearance, substance, position, or the like; to make different by a partial change; to modify; as, to vary the properties, proportions, or nature of a thing; to vary a posture or an attitude; to vary one's dress or opinions.
a.
Very large; monstrous; big.
a.
Very large; whapping.
n.
A large omnibus used for excursions.
n.
A very great number; an indefinitely large number.
adv.
In a high degree; to no small extent; exceedingly; excessively; extremely; as, a very great mountain; a very bright sum; a very cold day; the river flows very rapidly; he was very much hurt.
a. & a. pron.
Every one. Cf.
n.
A large boat used by flag officers.
a.
Having a large or generous heart or disposition; noble; liberal.
n.
Anything very large or extraordinary.
a.
Huge; very large.
a.
Having large hands, Fig.: Taking, or giving, in large quantities; rapacious or bountiful.
superl.
Abundant; ample; as, a large supply of provisions.
n.
A large, roomy boat for the conveyance of passengers or goods; as, a ship's barge; a charcoal barge.
superl.
Exceeding most other things of like kind in bulk, capacity, quantity, superficial dimensions, or number of constituent units; big; great; capacious; extensive; -- opposed to small; as, a large horse; a large house or room; a large lake or pool; a large jug or spoon; a large vineyard; a large army; a large city.
n.
Something very large, or larger than common; a whopper, as a stout or tall person.