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Binary systems of planetary-mass objects
Jupiter-mass binary objects (JuMBOs) are a hypothetical class of celestial objects, defined as a planetary-mass objects orbiting a common center of mass
Jupiter-mass_binary_object
Unit of mass equal to the total mass of the planet Jupiter
The Jupiter mass, also called Jovian mass, is the unit of mass equal to the total mass of the planet Jupiter. This value may refer to the mass of the planet
Jupiter_mass
Planet not gravitationally bound to a star
mass objects with decreasing mass. It was also predicted that the binary fraction decreases with mass. These binaries were named Jupiter-mass Binary Objects
Rogue_planet
Size-based definition of celestial objects
loss. The shrinking star can then become a planetary-mass object. An example is a Jupiter-mass object orbiting the pulsar PSR J1719−1438. These shrunken
Planetary-mass_object
Two astronomical bodies which orbit each other
center of mass to be located outside of either object. (See animated examples.) The most common kinds of binary system are binary stars and binary asteroids
Binary_system
lists can be sorted according to an object's radius and mass and, for the most massive objects, volume, density, and surface gravity, if these values are
List of Solar System objects by size
List_of_Solar_System_objects_by_size
Diffuse nebula in the constellation Orion
of pairs of rogue planets, similar in mass to the planet Jupiter, and called JuMBOs (Jupiter Mass Binary Objects). In July 2025, observations of the Orion
Orion_Nebula
Substellar object
substellar objects that have more mass than the biggest gas giant planets, but less than the least massive main-sequence stars. Their mass is approximately
Brown_dwarf
Center of mass of multiple bodies orbiting each other
(kéntron) 'center') is the center of mass around which two or more bodies orbit. A barycenter is a dynamical point, not a physical object. It is an important concept
Barycenter_(astronomy)
List of largest planets by size
(2013-05-01). "Direct-imaging discovery of a 12-14 Jupiter-mass object orbiting a young binary system of very low-mass stars". Astronomy and Astrophysics. 553:
List_of_largest_exoplanets
possibilities as to why Jupiter-like orbits are rare, including that data is lacking or the grand tack hypothesis.) Do Jupiter-mass Binary Objects (JuMBOs) exist
List of unsolved problems in astronomy
List_of_unsolved_problems_in_astronomy
Fifth planet from the Sun
Jupiter is the fifth planet from the Sun, and the largest in the Solar System. This is a gas giant with a mass nearly 2.5 times that of all the other planets
Jupiter
2023 film
(2025) Capotauro (2025) Little red dots The Cliff CAPERS-LRD-z9 Jupiter-mass binary objects (JuMBOs) Institutions NASA Goddard Space Flight Center Space
Deep_Sky
Binary system where two planetary-mass objects share an orbital axis external to both
a double planet (also binary planet) is a binary satellite system where both objects are planets, or planetary-mass objects, and whose barycenter is
Double_planet
Natural physical entity in space
An astronomical object, celestial object, stellar object or heavenly object is a naturally occurring physical entity, association, or structure that exists
Astronomical_object
Small Solar System body that is composed of two bodies
The term is also used for stellar contact binaries. An example of a contact binary is the Kuiper belt object 486958 Arrokoth, which was imaged by the New
Contact binary (small Solar System body)
Contact_binary_(small_Solar_System_body)
Equilibrium points near two orbiting bodies
Lagrangian points or libration points, are points of equilibrium for small-mass objects under the gravitational influence of two massive orbiting bodies. Mathematically
Lagrange_point
Area of the Solar System beyond the planets, comprising small bodies
brighter, has a larger fraction of binary objects, has a different size distribution, and lacks very large objects. The mass of the dynamically cold population
Kuiper_belt
Asteroid sharing the orbit of Jupiter
for the objects brighter than absolute magnitude 9.0.[needs update] The total mass of the Jupiter trojans is estimated at 0.0001 of the mass of Earth
Jupiter_trojan
Astronomical object without the mass to sustain hydrogen fusion
decreasing mass until, at the mass of Jupiter, a substellar object has a central density less than 10 g/cm3. The density decrease balances the mass decrease
Substellar_object
Astronomic function
In astronomy, the binary mass function or simply mass function is a function that constrains the mass of the unseen component (typically a star or exoplanet)
Binary_mass_function
Binary brown dwarf system in the constellation Eridanus
J0336−0143 or W0336, is a binary system comprising two planetary-mass Y-type brown dwarfs tightly orbiting around their common center of mass. The system is located
WISE_J0336−0143
High-mass planet orbiting close to a star
periods, spanning 0.36–11.8 Jupiter masses and 1.3–111 Earth days. The mass cannot be greater than approximately 13.6 Jupiter masses because then the pressure
Hot_Jupiter
Astronomical object not gravitationally bound to a star
may be a former interstellar object, captured some 4.5 billion years ago, as evidenced by its co-orbital motion with Jupiter and its retrograde orbit around
Interstellar_object
Standard unit of mass in astronomy
000092)×1030 kg. The solar mass is about 333000 times the mass of Earth (M🜨), or 1047 times the mass of Jupiter (MJ). The value of the gravitational constant was
Solar_mass
Long-period exoplanet orbiting b Centauri
binary star system b Centauri, located in the southern constellation Centaurus. The planet is a super-Jupiter, with a mass 10.9 times that of Jupiter
B_Centauri_b
Topics referred to by the same term
payload Jumbo, a muscadine cultivar JuMBO, abbreviation for "Jupiter-mass Binary Objects" in the Orion Nebula Jumbo, Lyndon B. Johnson's nickname for
Jumbo_(disambiguation)
Lowest possible mass of the celestial object
minimum mass is the lower-bound calculated mass of observed objects such as planets, stars, binary systems, nebulae, and black holes. Minimum mass is a widely
Minimum_mass
Scenario of giant planet migration
jumping-Jupiter scenario specifies an evolution of giant-planet migration described by the Nice model, in which an ice giant (an additional Neptune-mass planet)
Jumping-Jupiter_scenario
Super-Earth ice exoplanet
380 million mi), or an orbit that would fall between the orbits of Mars and Jupiter in the Solar System (This range of distances is the range of error in measurement
OGLE-2005-BLG-390Lb
Planetary mass binary in the constellation Crater
planetary mass binary located 86±23 light-years from the Earth in the constellation Crater. The components of 2MASS J1119–1137 are each roughly four Jupiter masses
2MASS_J11193254−1137466
Planetary system consisting of the Sun and objects orbiting it
Solar System objects, see List of minor-planet groups and Comet § Classification. The mass of the Solar System excluding the Sun, Jupiter and Saturn can
Solar_System
Trans-Neptunian object
174567 Varda (provisional designation 2003 MW12) is a large binary trans-Neptunian object in the hot classical population of the Kuiper belt, located
174567_Varda
Planetary-mass bodies that are also natural satellites
planetary-mass moon is a planetary-mass object that is a natural satellite of another non-stellar celestial object. Because of their mass, these moons
Planetary-mass_moon
Open cluster in the constellation Cancer
small nebulous object to the naked eye, and has been known since ancient times. Classical astronomer Ptolemy described it as a "nebulous mass in the breast
Beehive_Cluster
Small planetary-mass object
dwarf planets and dates of discovery A dwarf planet is a small planetary-mass object that is in direct orbit around the Sun, massive enough to be gravitationally
Dwarf_planet
Circumbinary planetary-mass object orbiting ROXs 42B
of Texas at Austin & University of Toronto. The object has a best estimated mass around 9 to 10 Jupiter masses, depending on the age of the star, similar
ROXs_42Bb
Brown dwarf in the constellation Hydra
37 °F). It has an estimated mass between 3 and 10 Jupiter masses, which makes it a planetary-mass object below the 13-Jupiter-mass rough limit for deuterium
WISE_0855−0714
Astronomical objects colder than red dwarfs
An object with the spectral type L (also called L-dwarf) can be either a low-mass star, a brown dwarf or a young free-floating planetary-mass object. If
L_dwarf
Galactic X-ray source in the constellation Cygnus that is very likely a black hole
occasional X-ray bursts lasting only for about 1 ms. Cygnus X-1 is a high-mass X-ray binary system located about 7,000 light-years away, that includes a blue
Cygnus_X-1
Accumulation of matter around a star
of circumplanetary objects (as seen in the eclipsing binary TY CrA). For disks orbiting a low secondary-to-primary mass ratio binary, a tilted circumbinary
Circumstellar_disc
(Jupiter and Saturn) and two ice giants (Uranus and Neptune). When excluding the Sun, the four giant planets account for more than 99% of the mass of
List of gravitationally rounded objects of the Solar System
List_of_gravitationally_rounded_objects_of_the_Solar_System
gravitationally rounded objects of the Solar System. This also includes a list of the eight planets according to the IAU definition. For a list of objects in the Solar
Lists_of_planets
Brown dwarf binary in the constellation Scorpius
Jupiter masses, which would have made the smaller object a planetary-mass object, or planemo. The system was announced as the first reported binary system
Oph_162225-240515
Large, round non-stellar astronomical object
follows: Objects with true masses below the limiting mass for thermonuclear fusion of deuterium (currently calculated to be 13 Jupiter masses for objects of
Planet
Distant body in the outer Solar System
perturbations of a Jupiter-mass (MJ) object at 5,000 AU (or less), a Neptune-mass object at 2,000 AU, or even an Earth-mass object at 1,000 AU. Computer
Sedna_(dwarf_planet)
Brown dwarf or planet colder than 500 Kelvin
An object with a spectral type Y (also called Y dwarf) is either a brown dwarf or a free-floating planetary-mass object. They have temperatures below around
Y_dwarf
Hypothetical bodies around the Solar System
System had a former binary star system by the Sun, which merged and broke into two due to rotational instability, forming Jupiter and Saturn. Fred Hoyle's
List of hypothetical Solar System objects
List_of_hypothetical_Solar_System_objects
Large self-illuminated object in space
The mass, radius, surface gravity, and rotation period can then be estimated based on stellar models. (Mass can be calculated for stars in binary systems
Star
Planetary object disrupted by other body
planetary-mass object, planetesimal, moon, exomoon or asteroid that has been disrupted or destroyed by a nearby or passing astronomical body or object such
Disrupted_planet
Mass transferring brown dwarf binary
recognized as a binary brown dwarf until 2026. The ZTF J1239+8347 system consists of two L-type brown dwarfs, each with masses between 60 and 80 Jupiter masses
ZTF_J1239+8347
Constellation in the southern hemisphere
similar to Jupiter. It is an orange-hued main-sequence star of magnitude 3.7, 10.5 light-years from Earth. Its one planet, with an approximate mass of one
Eridanus_(constellation)
Types of planet by chemical mass
types by their mass, radius, orbit, physical and chemical composition, or by another classification. Hypothetical astronomical object § Hypothetical planet
List_of_planet_types
Coming together of two stars
dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms not
Stellar_collision
Hypothetical Solar System planet
suggestion that they were a binary object disrupted near aphelion during an encounter with a distant object. The disruption of a binary would require a relatively
Planet_Nine
Distant planetesimals in the Solar System
stellar perturbations alone, and that the most likely cause would be a Jupiter-mass object in a distant orbit. This hypothetical gas giant was nicknamed Tyche
Oort_cloud
Jupiter trojan asteroid
largest Jupiter trojans, with a diameter on the order of 150 km. However, in 2001 it was discovered to be a binary asteroid of two similarly sized objects. The
617_Patroclus
Astronomical object orbiting Kappa Andromedae
constellation, about 170 light-years away. The companion's mass is roughly 17 times the mass of Jupiter. As early history on Kappa And b is filled with debate
Kappa_Andromedae_b
known 133 objects are bound in 95 stellar systems. Of those, 103 are main sequence stars: 78 red dwarfs and 25 "typical" stars having greater mass. Additionally
List_of_nearest_stars
Citizen science project to find exoplanets
phases of mass transfer in the future, and likely end up as a double neutron star gravitational wave progenitor or an exotic Thorne-Zytkow object. Astronomy
Planet_Hunters
Time an astronomical object takes to complete one orbit around another object
stars, or binary stars. It may also refer to the time it takes a satellite orbiting a planet or moon to complete one orbit. For celestial objects in general
Orbital_period
Possible dwarf planet
confirmed doubly synchronous binary in the trans-Neptunian region, joining Pluto–Charon and Eris–Dysnomia. In 2025, the total mass of the Salacia–Actaea system
120347_Salacia
Set of gravitationally bound objects in orbit
commonly by the name of their primary (e.g. "Jupiter system"). Where only one satellite is known, or it is a binary with a common centre of gravity, it may
Satellite_system_(astronomy)
Binary star system in the Cygnus constellation
Kamp narrowed his uncertainties, claiming that the object had a mass of eight times that of Jupiter, a calculated orbital period of 4.8 years, and a semi-major
61_Cygni
Union's definition of a planet in the Solar System Object is in orbit around the Sun Object has sufficient mass for its self-gravity to overcome rigid body forces
Definition_of_planet
Millisecond pulsar in the constellation Sagitta
The Black Widow pulsar (PSR B1957+20) is an eclipsing binary millisecond pulsar in the Milky Way. Discovered in 1988, it is located roughly 6,500 light-years
Black_Widow_pulsar
Accumulation of matter around a planet
disk-bearing object is 2MASS J11151597+1937266, which is only 45 parsec distant. It could be a planetary-mass object or a low-mass brown dwarf. These objects with
Circumplanetary_disk
certain object: Lacc - accretion luminosity Lbol - bolometric luminosity Mass comparison: ME, M🜨 - mass of Earth MJ, M♃ - mass of Jupiter MS, M☉ - mass of
List of common astronomy symbols
List_of_common_astronomy_symbols
Stellar core remnant
double-degenerate model, two carbon–oxygen white dwarfs in a binary system merge, creating an object with mass greater than the Chandrasekhar limit in which carbon
White_dwarf
Astronomical phenomenon due to the gravitational lens effect
gravitational lens effect. It can be used to detect objects that range from the mass of a planet to the mass of a star, regardless of the light they emit. Typically
Gravitational_microlensing
and M.F. Doyle (1998). "Detectability of Jupiter-to-brown-dwarf-mass companions around small eclipsing binary systems". Brown Dwarfs and Extrasolar Planets
Methods of detecting exoplanets
Methods_of_detecting_exoplanets
Star observed by the Kepler space telescope that is suspected to have a transiting planet
guarantee of a transiting planet, because other astronomical objects—such as an eclipsing binary in the background—can mimic a transit signal. For this reason
Kepler_object_of_interest
Star in the constellation Cetus
annually. The star is over 5 billion years old and has only about 18% the mass of the Sun and 21% of its radius. LHS 1140's rotational period is 130 days
LHS_1140
produced. 2012 — It has been surmised that J1407b, a possibly planetary-mass object that eclipsed the star V1400 Centauri (aka. J1407) in 2007, may have
List_of_exomoon_candidates
Planet that is outside the Milky Way galaxy
a smaller companion, PA-99-N2, weighing just around 6.34 times the mass of Jupiter. This suspected planet is the first announced in the Andromeda Galaxy
Extragalactic_planet
Binary star system
that the object is a real member of the association, showing signs of low gravity and youth, and estimated a mass of 60 times the mass of Jupiter (MJ), an
UScoCTIO_108
Binary star system in the constellation Cetus
leaving behind a white dwarf. This binary star system consists of a red giant (Mira, designated Mira A) undergoing mass loss and a high-temperature white
Mira
Globular cluster in Scorpius
been found to be a binary star with a pulsar companion, PSR B1620−26 and a planet orbiting it with a mass of 2.5 times that of Jupiter (MJ). One star in
Messier_4
Constellation straddling the celestial equator
Discovered in 1785 by William Herschel, it has earned the nickname "Ghost of Jupiter" because of its striking resemblance to the giant planet. Its blue-green
Hydra_(constellation)
Planet that orbits two stars instead of one
(2013-05-01). "Direct-imaging discovery of a 12-14 Jupiter-mass object orbiting a young binary system of very low-mass stars". Astronomy and Astrophysics. 553:
Circumbinary_planet
Moon of Orcus
trans-Neptunian object. Vanth is massive enough that it shifts the barycenter of the Orcus–Vanth system outside of Orcus, forming a binary system in which
Vanth_(moon)
Constellation in the northern celestial hemisphere
subsequently showed it instead to be a low-mass star somewhere between 100 and 200 times the mass of Jupiter. Possible stable planetary orbits in the habitable
Corona_Borealis
Spectrograph on the James Webb Space Telescope
instrument is a multi-object spectrograph and is capable of simultaneously measuring the near-infrared spectrum of up to 100 objects like stars or galaxies
NIRSpec
Class of young variable stars
years. Most T Tauri stars are in binary star systems. In various stages of their life, they are called young stellar object (YSOs). It is thought that the
T_Tauri_star
NASA/ESA/CSA space telescope launched in 2021
BOTS mode: the Jupiter-sized planet HAT-P-14b NIRISS aperture masking interferometry (AMI): A precise detection of the very low-mass companion star AB
James_Webb_Space_Telescope
Exoplanet in the constellation Draco, known for being the "Darkest Exoplanet"
temperature. The planet's mass and radius indicate that it is a gas giant with a bulk composition similar to that of Jupiter. Unlike Jupiter, but similar to many
TrES-2b
European space mission to measure gravitational waves
by small compact objects, known as extreme mass ratio inspirals, binaries of compact stars, substellar objects orbiting such binaries, and possibly other
Laser Interferometer Space Antenna
Laser_Interferometer_Space_Antenna
Zodiac constellation in the northern hemisphere
largest known, with a mass of 18 billion solar masses, more than six times the value calculated for the previous largest object. Cancer was first recorded
Cancer_(constellation)
Celestial object in the constellation Aquarius
a two- to three-billion-year-old brown dwarf with mass between 2 and 40 Jupiter masses. The object shows signs of low gravity (brighter K band in the
CFBDSIR_2149−0403
Star system in the Centaurus constellation
Centauri AB are the nearest binary stars to the Sun at a distance of 4.344 ly (1.33 pc). Rigil Kentaurus has 1.1 times the mass (M☉) and 1.5 times the luminosity
Alpha_Centauri
Extrasolar planet
discovered had been gas giants many times the mass of Jupiter. 51 Eridani b is a gas giant more massive than Jupiter. Predictions of substellar evolution models
51_Eridani_b
Space navigation technique
typical mass for an interplanetary space probe whereas Jupiter has a mass of almost 2 × 1024 metric tons. Therefore, a one-ton spacecraft passing Jupiter will
Gravity_assist
Binary Kuiper belt object
1998 WW31 is a non-resonant trans-Neptunian object and binary system from the Kuiper belt located in the outermost region of the Solar System, approximately
1998_WW31
Hypothetical star orbiting the Sun, supposedly responsible for extinction events
separated from this binary system over four billion years ago, meaning it could not be responsible for the more recent cycles of mass extinctions. More
Nemesis_(hypothetical_star)
Scenario for the dynamical evolution of the Solar System
such as the Kuiper belt, the Neptune and Jupiter trojans, and the numerous resonant trans-Neptunian objects dominated by Neptune. The original core of
Nice_model
Astronomical object
stars and brown dwarfs. The object is notable because its estimate mass, 6±1 times the mass of Jupiter, places it in the mass range for rogue planets. As
WISE_J1147−2040
Exoplanets confirmed or discovered from direct imaging
directly imaged planets and imaged planetary-mass companions (objects that orbit a star but formed through a binary-star-formation process, not a planet-formation
List of directly imaged exoplanets
List_of_directly_imaged_exoplanets
March 2008. "Jupiter's Moon Lysithea". www.iki.rssi.ru. Retrieved 24 January 2025. Nicholson, S. B. (1951). "An unidentified object near Jupiter, probably
List_of_natural_satellites
Transient x-ray binary system
categorize the system as either a high mass (above 10 solar masses) or low mass (less than 1 solar mass) X-ray binary, abbreviated as LMXB and HMXB, respectively
X-ray_transient
Astronomical objects of planetary size that did not form in orbit around a star
A sub-brown dwarf or planetary-mass brown dwarf is an astronomical object that formed in the same manner as stars and brown dwarfs (i.e. through the collapse
Sub-brown_dwarf
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
Boy/Male
American, Australian, French, German, Greek, Latin, Polish, Swedish
Cheerful; Happy; Joyful; Similar to Hilary
Boy/Male
Arabic, Muslim, Pashtun
Gul - Flowers; Mast - Excitement
Male
Hebrew
(מַשָׂ×) Variant spelling of Hebrew Massa, MASA means "burden." Compare with another form of Masa.
Male
Hebrew
 Medieval Jewish form of Hebrew Moshe, MOSS means "drawn out." Compare with another form of Moss.
Boy/Male
Indian, Sikh
Cute Feisty Powerful Strong and Answers with Sass and Class
Female
Turkish
Turkish name PINAR means "spring."
Male
Italian
Short form of Italian Tommaso, MASO means "twin."
Male
Scandinavian
Scandinavian form of Old Norse Einarr, EINAR means "lone warrior."
Male
English
 English surname transferred to forename use, derived from medieval Jewish Moss (2), MOSS means "drawn out." Compare with another form of Moss.
Male
Hindi/Indian
Variant spelling of Hindi Vijay, BIJAY means "victory."
Male
Hebrew
(מַשָׂ×) Hebrew name MASSA means "burden." In the bible, this is the name of a son of Ishmael.
Female
Hebrew
Variant spelling of Hebrew Bina, BINAH means "intelligence, wisdom."Â
Male
Swedish
Norwegian and Swedish form of Greek Mattathias, MATS means "gift of God."
Boy/Male
Latin Biblical
Supreme god.
Female
English
English short form of Latin Cassandra, CASS means "she who entangles men."Â
Female
Portuguese
Portuguese form of Hebrew Yehuwdiyth, JUDITE means "Jewess" or "praised."
Female
Japanese
(1-æ£, 2-é›…, 3-昌, 4-真, 5-政, 6-å°†) Unisex short form of Japanese names beginning with Masa-, MASA means 1) "correct, just," 2) "elegant," 3) "flourishing, prosperous" 4) "genuine, true," 5) "governing, political," 6) "military." Compare with strictly masculine Masa.
Male
Japanese
(1-æ£, 2-é›…, 3-昌, 4-真, 5-政, 6-å°†) Unisex short form of Japanese names beginning with Masa-, MASA means 1) "correct, just," 2) "elegant, splendid" 3) "flourishing, prosperous" 4) "genuine, true," 5) "governing, political," 6) "military." Compare with another form of Masa.
Male
Hindi/Indian
(विनय) Hindi name VINAY means "leading asunder."
Surname or Lastname
English
English : variant of Mace 1.French (Picardy) : metonymic occupational name from masse ‘mace’, ‘hammer’.French : habitational name from places called Masse (Allier and Cô-d’Or), or La Masse (Eure, Lot, Puy-de-Dôme, Saône-et-Loire).French (Massé) : habitational name from a place called Massé in Maine-et-Loire, so named from Gallo-Roman Macciacum (from the personal name Maccius + the locative suffix -acum).Dutch : from Middle Dutch masse ‘clog’; ‘cudgel’, perhaps a metonymic occupational name for someone who wielded a club.Dutch : possibly a variant of Maas 1, or a patronymic from Mas.
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
Boy/Male
Gujarati, Hindu, Indian
Lord Shiva
Boy/Male
British, English, Indian, Tamil
Master; Dennis' Son
Girl/Female
Australian, Swedish
Yew
Surname or Lastname
English
English : unexplained.Possibly a shortened form of any of several German compound surnames formed with Full- or Füll-.
Boy/Male
American, Australian, British, Chinese, Christian, English, French, German, Indian, Latin, Spanish, Swedish
Hairy; Long Haired; Variant of Caesar; Hirsute; With Abundant Hai
Girl/Female
Tamil
Like a fairy, Beautiful, Like a An Angel
Girl/Female
Arabic, Muslim
Prayer; Supplication
Boy/Male
Tamil
Rustom | à®°à¯à®¸à¯à®¤à¯‹à®®
Warrior
Girl/Female
Biblical
Who reckons or is counted.
Female
Babylonian
, Chaos; a primaeval goddess.
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
JUPITER MASS-BINARY-OBJECT
n.
A mass; a heap.
a.
Of a pale yellowish color; as, Canary stone.
superl.
Compacted into, or consisting of, a mass; having bulk and weight ot substance; ponderous; bulky and heavy; weight; heavy; as, a massy shield; a massy rock.
n.
A pale yellow color, like that of a canary bird.
v. t.
To form or collect into a mass; to form into a collective body; to bring together into masses; to assemble.
n.
Species of Serranus, the sea bass and rock bass. See Sea bass.
a.
Of or pertaining to the urine; as, the urinary bladder; urinary excretions.
n.
A medicinal substance made into a cohesive, homogeneous lump, of consistency suitable for making pills; as, blue mass.
n.
Mass; church service.
v. t.
To collect into a mass or heap; to gather a great quantity of; to accumulate; as, to amass a treasure or a fortune; to amass words or phrases.
v. i.
To celebrate Mass.
a.
Relating or belonging to bile; conveying bile; as, biliary acids; biliary ducts.
n.
Wine made in the Canary Islands; sack.
n.
See Finery.
a.
Of or pertaining to the Canary Islands; as, canary wine; canary birds.
n.
A state of confusion or disorder; -- prob. variant of mess, but influenced by muss, a scramble.
v. i.
To perform the canary dance; to move nimbly; to caper.
n.
A canary bird.
pl.
of Bass
v. t.
To furnish with a mast or masts; to put the masts of in position; as, to mast a ship.