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Collection of matter whose mass varies with time
In mechanics, a variable-mass system is a collection of matter whose mass varies with time. It can be confusing to try to apply Newton's second law of
Variable-mass_system
Mass of a substance which passes per unit of time
law for variable mass systems by treating the mass in F = dP/dt = d(Mv) as a variable. [...] We can use F = dP/dt to analyze variable mass systems only if
Mass_flow_rate
Star whose brightness fluctuates, as seen from Earth
novae and supernovae. X-ray variables, close binary systems with a hot mass-accreting compact object. Extrinsic variable stars The variability is caused
Variable_star
System of two stars orbiting each other
considered to be a black hole. It is a high-mass X-ray binary, with the optical counterpart being a variable star. Sirius is another binary and the brightest
Binary_star
Binary star system in the constellation Cetus
or ο Cet. The system consists of a variable red giant (Mira A) along with a white dwarf companion (Mira B). Mira A is a pulsating variable star and was
Mira
Vehicle propelled by ejection of gases
Location used to launch and receive spacecraft Variable-mass system – Collection of matter whose mass varies with time Rocket propulsion Ammonium perchlorate
Rocket
Process of altering the timing of a valve lift event
emissions. It is increasingly being used in combination with variable valve lift systems. There are many ways in which this can be achieved, ranging from
Variable_valve_timing
Stars with irregular large fluctuations in brightness
stars in the sky. Cataclysmic variable stars are binary stars that consist of two components; a white-dwarf primary, and a mass-transferring secondary. The
Cataclysmic_variable_star
Parameter in physics problems
In a real spring–mass system, the spring has a non-negligible mass m {\displaystyle m} . Since not all of the spring's length moves at the same velocity
Effective mass (spring–mass system)
Effective_mass_(spring–mass_system)
Types of numerical variables in mathematics
distributions of discrete variables can be expressed in terms of probability mass functions. In discrete time dynamics, the variable time is treated as discrete
Continuous or discrete variable
Continuous_or_discrete_variable
Equations that describe the behavior of a physical system
on the mass and velocity, and Newton's second law requires some modification consistent with conservation of momentum; see variable-mass system. It may
Equations_of_motion
Heating or air-conditioning system
Variable air volume (VAV) is a type of heating, ventilating, and/or air-conditioning (HVAC) system. Unlike constant air volume (CAV) systems, which supply
Variable_air_volume
Type of variable stellar binary
A W Ursae Majoris variable, also known as a low mass contact binary, is a type of eclipsing binary variable star. These stars are close binaries of spectral
W_Ursae_Majoris_variable
Automotive transmission technology
A continuously variable transmission (CVT) is an automatic transmission that can change through a continuous range of gear ratios, typically resulting
Continuously variable transmission
Continuously_variable_transmission
Type of rigid buoyancy control device
A variable-buoyancy pressure vessel system is a type of rigid buoyancy control device for diving systems that retains a constant volume and varies its
Variable-buoyancy pressure vessel
Variable-buoyancy_pressure_vessel
Type of variable stellar binary
Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this
Beta_Lyrae_variable
Body of matter in a state of internal equilibrium
thermodynamic system at a given time is described by its state, which can be specified by the values of a set of thermodynamic state variables. A thermodynamic
Thermodynamic_system
Type of star that is luminous, blue, and variable in brightness
Luminous blue variables (LBVs) are rare, massive, evolved stars that show unpredictable and sometimes dramatic variations in their spectra and brightness
Luminous_blue_variable
Binary star in the constellation Cetus
component stars are both flare stars with the variable star designations BL Ceti and UV Ceti. The star system was discovered in 1948 by Willem Jacob Luyten
Gliese_65
Large self-illuminated object in space
variables, blue stragglers, and Type Ia supernovae. Mass transfer leads to cases such as the Algol paradox, where the most-evolved star in a system is
Star
Type of variable star that pulsates radially
A Cepheid variable (/ˈsɛfi.ɪd, ˈsiːfi-/) is a type of variable star that pulsates radially, varying in both diameter and temperature. It changes in brightness
Cepheid_variable
Reciprocating internal combustion engine
common rail injection system with a variable-geometry turbocharger. Most of those engine have the MIVEC variable valve timing system. The 4N14 2.3 L (2,268
Mitsubishi_4N1_engine
Properties independent of system size, and proportional to system size
such as the mass per volume (mass density) or volume per mass (specific volume), must remain the same in each half. The temperature of a system in thermal
Intensive and extensive properties
Intensive_and_extensive_properties
Class of young variable stars
T Tauri stars (TTS) are a class of variable stars that are less than about ten million years old. This class is named after the prototype, T Tauri, a young
T_Tauri_star
Stellar core remnant
puzzle. If a star is in a binary system, as is the case for Sirius B or 40 Eridani B, it is possible to estimate its mass from observations of the binary
White_dwarf
Star in the constellation Aquarius
LHS 68. It is a variable star showing flares as well as smaller brightness changes due to rotation. The aggregate mass of the system is 0.3262±0.0018
EZ_Aquarii
Symbol representing a mathematical object
that the variable represents or denotes the object, and that any valid candidate for the object is the value of the variable. The values a variable can take
Variable_(mathematics)
Variable representing a random phenomenon
A random variable (also called random quantity, aleatory variable, or stochastic variable) is a mathematical formalization of a quantity or object which
Random_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, and Ab
Algol
Star system in the constellation Carina
The apparent magnitude is variable from +6.16 to +6.49 with a period of 6 days. Hierarchy of components in the QZ Carinae system, omitting the distant J10444-6000
QZ_Carinae
Any analogy between electrical and mechanical systems, used for modelling
network diagrams for control systems. Mechanical–electrical analogies are developed by finding relationships between variables in one domain that have a
Mechanical–electrical analogies
Mechanical–electrical_analogies
Stellar system in the constellation Carina
Carinae system have an eccentric orbit with a period of 5.54 years. The primary is an extremely unusual star, similar to a luminous blue variable (LBV)
Eta_Carinae
Planetary system consisting of the Sun and objects orbiting it
orbiting bodies assembled. The Sun accounts for 99.86% of the Solar System's total mass. Inside the Sun's core, hydrogen is fused into helium, releasing
Solar_System
Linear regression model with a single explanatory variable
standard deviations of these variables. The intercept of the fitted line is such that the line passes through the center of mass (x, y) of the data points
Simple_linear_regression
Multiple star system in the constellation of Auriga
to study it in great detail. His work revealed that the system was an eclipsing binary variable, a star that dims when its partner obscures its light.
Epsilon_Aurigae
Star in the constellation Libra
which hosts a planetary system, 20.5 light-years (6.3 parsecs) away from Earth in the constellation Libra. Its estimated mass is about a third of that
Gliese_581
Early American intercontinental ballistic missile
2005, ISBN 0-517-56904-3, p. 11 Widnal Perair S., Lecture L14 - Variable Mass Systems The: Rocket Equation, 2008, MIT OpenCourseWar Sutton, George P,
HGM-25A_Titan_I
Japanese 2D fighting game/eroge series
Variable Geo (ヴァリアブル・ジオ, Variaburu Jio), also known as V.G., is a Japanese 2D fighting game and eroge series developed and published by TGL for consoles
Variable_Geo
Star at the centre of the Solar System
times that of Earth, making up about 99.86% of the total mass of the Solar System. The mass of the Sun's surface layer, its photosphere, consists mostly
Sun
Class of eclipsing binary stars
period to vary: in some Algol binaries, mass transfer between the closely spaced components of the variable may cause monotonic increases in period;
Algol_variable
Inline-3 engine
The patent for this system was bought by Koenigsegg's sister company Cargine Engineering in 2002. The variable displacement system allows fuel economy
Koenigsegg_TFG
Quintuple star system in the constellation Ursa Major
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 and
1SWASP_J093010.78+533859.5
Red giant star in the constellation Camelopardlis
of M0 III. It is a suspected variable star with a pulsation period of around 586 days. The star has 1.1 times the mass of the Sun and has expanded to
HD_36384
Rare star with tremendous luminosity and high rates of mass loss by stellar winds
luminosity, mass, size and mass loss because of its extreme stellar winds. The term hypergiant is defined as luminosity class 0 (zero) in the MKK system. However
Hypergiant
Eclipsing binary in the constellation Taurus
system was included in a 2003 study that featured GK Draconis and V1094 Tauri. The study suggested a mass of 1.10 M☉ for the primary star and a mass of
V1094_Tauri
Binary star system in the constellation Vulpecula
the primary star within the system. HD 189733 A is an orange dwarf star of the spectral type K1.5V. The star has a mass of 81 percent that of the Sun
HD_189733
Vapour density Variable-mass system Variable-sweep wing Variable Density Tunnel Variable mass hypothesis Variable speed of light Variables and some constants
Index_of_physics_articles_(V)
Eclipsing post-common envelope binary star system in the constellation Serpens
1550+131 was indeed a variable star. Reinhold Haefner discovered that the star is an eclipsing binary, in 1988. It was given its variable star designation
NN_Serpentis
Humorous system of units
(FFF) system is a humorous system of units based on unusual or impractical measurements. The length unit of the system is the furlong, the mass unit is
FFF_system
Star system in the constellation Andromeda
star system in the northern constellation of Andromeda, abbreviated IW And. It is the prototype of a class of variable stars known as IW And variables, which
IW_Andromedae
Mathematical function for the probability a given outcome occurs in an experiment
between discrete and continuous random variables. In the discrete case, it is sufficient to specify a probability mass function p {\displaystyle p} assigning
Probability_distribution
Physical system that responds to a restoring force proportional to displacement
x {\displaystyle x} of the mass and a constant k {\displaystyle k} . Balance of forces (Newton's second law) for the system is F = m a = m d 2 x d t 2
Harmonic_oscillator
Variable stars of late spectral types
sequence. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to
BY_Draconis_variable
Star in the constellation Virgo
the Sun. It is a spectroscopic binary star and rotating ellipsoidal variable; a system whose two stars are so close together they are egg-shaped rather than
Spica
Device that helps steer vehicles by augmenting steering effort of the steering wheel
electric power variable gear ratio steering (VGS) system. In 2002, Toyota introduced the "Variable Gear Ratio Steering" (VGRS) system on the Lexus LX
Power_steering
Physical phenomenon of stars
the system rapidly develops into a Type-Ia supernova. Another alternate scenario for the same system is the formation of a cataclysmic variable or a
Stellar_mass_loss
Star system in the constellation Taurus
one of the first discovered extremely low-mass white dwarfs (ELM WDs). The primary component of the system was identified in 2009 by astronomers A. Kawka
NLTT_11748
Mechanical device for storing rotational energy
the flywheel's moment of inertia is constant (i.e., a flywheel with fixed mass and second moment of area revolving about some fixed axis) then the stored
Flywheel
Brightest star in the constellation Orion
mass of the star. Rigel varies slightly in brightness, its apparent magnitude ranging from 0.05 to 0.18. It is classified as an Alpha Cygni variable due
Rigel
Graphical representation of energy flows in physical systems
use the concept of analogous power conjugate variables whose product is energy flow, or power; these variable pairs are called effort and flow and, for example
Bond_graph
Small number of stars that orbit each other
transfer of mass between stars – the two stars will trace out a stable elliptical orbit around the barycenter of the system. Examples of binary systems are Sirius
Star_system
Main sequence star in the constellation Draco
the star, the star is classified as a planetary transit variable and has received the variable star designation V581 Draconis. In 2008 a study was undertaken
TrES-2A
Star in the constellation Pegasus
of Pegasus. It has roughly 1.4 times the Sun's mass and 5 times its luminosity. It is part of a system that also contains a debris disk and at least four
HR_8799
Star in the constellation Libra
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
HN_Librae
Slow irregular eruptive variable stars
its original luminosity. Variables of this type are double star systems with one red giant, which probably is a Mira variable, and one a hot compact object
Symbiotic_nova
Dim, low mass stars on the main sequence
discovered orbiting within the Gliese 581 planetary system between 2005 and 2010. One planet has about the mass of Neptune, or 16 Earth masses (M🜨). It orbits
Red_dwarf
Type of star that is massive and luminous
and post-AGB stars, highly expanded and unstable low-mass stars such as the RV Tauri variables. The majority of AGB stars are assigned giant or bright
Supergiant
Variable star in the constellation Leo
R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo. The apparent magnitude of R Leonis
R_Leonis
Measure of energy in a thermodynamic system
a closed homogeneous system is its energy function H(S, p), with its entropy S[p] and its pressure p as natural state variables which provide a differential
Enthalpy
Five-star system in the constellation Orion
being photometrically variable in 1977, and formally classified as a variable star in 1979. In 1996, a large number of low-mass pre-main sequence stars
Sigma_Orionis
Star in the constellation Gemini
small amplitude radial velocity variations, but is not photometrically variable. Since 1993 scientists have suspected an exoplanet orbiting Pollux, from
Pollux_(star)
Star in the constellation Ursa Major
W Ursae Majoris (W UMa) is the variable star designation for a binary star system in the northern constellation of Ursa Major. It has an apparent visual
W_Ursae_Majoris
Type of variable star
SW Sextantis variable stars are a kind of cataclysmic variable star; they are double-star systems in which there is mass transfer from a red dwarf to
SW_Sextantis_variable
Class of variable star
Rotating ellipsoidal variables are a class of close binary variable star systems whose components are ellipsoidal. They are not eclipsing, but fluctuations
Rotating_ellipsoidal_variable
G-type star in the constellation Virgo
classified as a planetary transit variable and has received the variable star designation V732 Virginis. This was one of the systems selected to be named in the
WASP-39
Type of variable star
low mass, Population II stars, in common with W Virginis and BL Herculis variables, the type II Cepheids. Classical Cepheid variables are higher mass population
RR_Lyrae_variable
Highly magnetic type of cataclysmic variable binary star system
astronomy, a polar is a highly magnetic type of cataclysmic variable (CV) binary star system, originally known as an AM Herculis star after the prototype
Polar_(star)
Star in the constellation Aquarius
AE Aquarii is a cataclysmic variable binary star of the DQ Herculis type. Based upon parallax measurements, the system is located at a distance of about
AE_Aquarii
Multiple star system in the constellation Hercules
is a triple star system. The primary (brightest) of the three stars, designated α1 Herculis or α Herculis A, is a pulsating variable star on the asymptotic
Alpha_Herculis
Variables that are Fourier transform duals
conjugate variables, depending on the type of work a certain system is doing (or is being subjected to). Examples of canonically conjugate variables include
Conjugate_variables
Binary star in the constellation Ophiuchus
X Ophiuchi is a binary star system in the equatorial constellation of Ophiuchus, abbreviated X Oph. It is a Mira variable that ranges in brightness from
X_Ophiuchi
Space of all possible states that a system can take
model system in classical mechanics, the phase-space coordinates of the system at any given time are composed of all of the system's dynamic variables. Because
Phase_space
Variable star in the constellation Orion
FU Orionis is a variable and binary star system in the constellation of Orion, that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has
FU_Orionis
Binary star system in the constellation Cepheus
prototype of the Cepheid variable stars that undergo periodic changes in luminosity. Delta Cephei was discovered to be variable by John Goodricke during
Delta_Cephei
Binary star in the constellation Scorpius
If placed at the center of the Solar System, it would extend out to somewhere in the asteroid belt. Its mass is calculated to be 13 or 15 to 16 times
Antares
Multiple star system in the constellation Orion
this suggests that the binary system was created through a capture, rather than by being formed together and undergoing a mass transfer. This capture may
Iota_Orionis
Meanings of mass in special relativity
invariant mass. For example, photons have zero rest mass but contribute to the inertia (and weight in a gravitational field) of any system containing
Mass_in_special_relativity
Star system in the constellation of Telescopium
constellation, near Pavo to the south and Ara to the west. The system appears as a variable star that is dimly visible to the naked eye with an apparent
HR_6819
Star in the constellation Scutum
900 light-years away in the constellation Scutum. It is also a pulsating variable star, with a maximum brightness of magnitude 8.29 and a minimum of magnitude
UY_Scuti
Star system in the constellation Cassiopeia
emission lines. It is now considered a Be star. Gamma Cassiopeiae is a variable star system. Based upon parallax measurements made by the Hipparcos satellite
Gamma_Cassiopeiae
amount. Its products include thermal mass flow controllers/meters, Coriolis mass flow controllers/meters, variable area meters (aka rotameters), level
Brooks_Instrument
Binary star in the constellation Leo
evolution models. The secondary component, γ Leonis B, has been found to be a variable star by data taken during the Hipparcos mission. The combined magnitude
Gamma_Leonis
Variable star in Monoceros
Monoceros. It is an ellipsoidal variable about 1,500 light-years distant, too faint to be seen to the naked eye, with a variable apparent magnitude between
V723_Monocerotis
Integral of a comparatively larger force over a short time interval
the time interval begins. The application of Newton's second law for variable mass allows impulse and momentum to be used as analysis tools for jet- or
Impulse_(physics)
Star in the constellation Canis Major
supergiant (O-rich RHG or RSG) and pulsating variable star 1.2 kiloparsecs (3,900 light-years) from the Solar System in the slightly southern constellation
VY_Canis_Majoris
Chain gun
operation system. It works with an electric motor as on the Bushmaster gun produced by ATK. The Profense PF 50 features a digital, programmable, variable rate
Profense_PF_50
Double stars that show a significant interaction between their components
accretion disk may form. The physical conditions in such a system can be complex and highly variable, and they are common sources of cataclysmic outbursts
Interacting_binary_star
Binary star system in the constellation of Tucana
star system 144 light years away in the constellation of Tucana. It has an apparent visual magnitude of 8.5, and is a RS Canum Venaticorum variable. The
DS_Tucanae
Relation of types of systems with corresponding dynamics
the effort variable and entropy flow rate as the flow variable. Many applications of dynamical models convert all energy domains in the system into an electrical
Analogical_models
Computer that adjusts electronics in an internal combustion propulsion system
spark advance or the electronic throttle system) Variable valve timing and/or variable valve lift systems The sensors used by the ECU include: accelerator
Engine_control_unit
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
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.
Boy/Male
Anglo, British, English
Variable
Surname or Lastname
English
English : status name denoting a serf, Middle English, Old French vass(e), from Late Latin vassus, of Celtic origin. Compare Welsh gwas ‘boy’, Gaelic foss ‘servant’.English : variant of Vause.Swedish : variant of Wass.South German : variant of Fass.Hungarian : from vas ‘iron’, hence a metonymic occupational name for a blacksmith, or a nickname for a resilient, tough man.
Surname or Lastname
English
English : patronymic from the personal name May (see May).
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.
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.
Female
English
English short form of Latin Cassandra, CASS means "she who entangles men."Â
Surname or Lastname
English
English : from Old French bas(se) ‘low’, ‘short’ (Latin bassus ‘thickset’; see Basso), either a descriptive nickname for a short person or a status name meaning ‘of humble origin’, not necessarily with derogatory connotations.English : in some instances, from Middle English bace ‘bass’ (the fish), hence a nickname for a person supposedly resembling this fish, or a metonymic occupational name for a fish seller or fisherman.Scottish : habitational name from a place in Aberdeenshire, of uncertain origin.Jewish (Ashkenazic) : metonymic occupational name for a maker or player of bass viols, from Polish, Ukrainian, and Yiddish bas ‘bass viol’.German : see Basse.
Male
Hebrew
(מַשָׂ×) Variant spelling of Hebrew Massa, MASA means "burden." Compare with another form of Masa.
Surname or Lastname
English
English : from a pet form of the medieval personal name Pascal, which was brought to England from France.German : topographic name from Pass ‘pass’, ‘passage’ (from Middle Low German pas ‘pace’, ‘passage way’, ‘water gauge’).Jewish (Ashkenazic) : metonymic occupational name or nickname from Yiddish and Polish pas ‘belt’, ‘girdle’.
Male
Swedish
Norwegian and Swedish form of Greek Mattathias, MATS means "gift of God."
Surname or Lastname
English
English : variant of Marsh.French : habitational name from places so named in Ardèche, Ardennes, Gard, Loire, Nièvre, and Meurthe-et-Moselle, from the Latin personal name Marcius, used adjectivally.French : from the personal name Meard, Mard, Mart, vernacular forms of the saint’s name Médard. Morlet notes that there are a number of places called Saint-Mars, formerly recorded in Latin as Sanctus Medardus.French : from the name of the month, mars ‘ March’, denoting seed sown in March, and hence a metonymic name for an arable grower.French (De Mars) : habitational name from Mars in the Ardennes.Dutch : from a short form of the personal name Marsilius.
Male
Hebrew
(מַשָׂ×) Hebrew name MASSA means "burden." In the bible, this is the name of a son of Ishmael.
Surname or Lastname
English and Welsh
English and Welsh : from the personal name Moss, a Middle English vernacular form of the Biblical name Moses.English and Scottish : topographic name for someone who lived by a peat bog, Middle English, Old English mos, or a habitational name from a place named with this word. (It was not until later that the vocabulary word came to denote the class of plants characteristic of a peat-bog habitat, under the influence of the related Old Norse word mosi.)Americanized form of Moses or some other like-sounding Jewish surname.Irish (Ulster) : part translation of Gaelic Ó Maolmhóna ‘descendant of Maolmhóna’, a personal name composed of the elements maol ‘servant’, ‘tonsured one’, ‘devotee’ + a second element which was assumed to be móin (genitive móna) ‘moorland’, ‘peat bog’.
Boy/Male
Arabic, Muslim, Pashtun
Gul - Flowers; Mast - Excitement
Surname or Lastname
English
English : from the feminine personal name Mirabel, equated in medieval records with Latin mirabilis ‘marvellous’, ‘wonderful’ (in the sense ‘extraordinary’).
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
Hebrew
 Medieval Jewish form of Hebrew Moshe, MOSS means "drawn out." Compare with another form of Moss.
Male
Italian
Short form of Italian Tommaso, MASO means "twin."
Surname or Lastname
English
English : from the medieval female personal name Cass, a short form of Cassandra. This was the name (of uncertain, possibly non-Greek, origin) of an ill-fated Trojan prophetess of classical legend, condemned to foretell the future but never be believed; her story was well known and widely popular in medieval England.
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
Girl/Female
Australian, French
Darling; Similar to Cherie Dear One
Boy/Male
Hindu, Indian
Lord Krishna
Boy/Male
Hindu
A herb
Boy/Male
Tamil
Sinkam
Boy/Male
American, Anglo, Australian, British, Christian, Danish, Dutch, English, French, German, Jamaican, Latin
Pierces; Pierced Valley
Boy/Male
Tamil
Vishtrit | விஷதà¯à®°à®¿à®¤
Boy/Male
Arthurian Legend
Lord of the Isle of Glass.
Boy/Male
Biblical
A rejoicing; our proud lord.
Surname or Lastname
English
English : unexplained.
Boy/Male
Hindu
Expected
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
VARIABLE MASS-SYSTEM
n.
A state of confusion or disorder; -- prob. variant of mess, but influenced by muss, a scramble.
n.
An invariable quantity; a constant.
a.
Worthy; estimable; deserving esteem; as, a valuable friend; a valuable companion.
v. t.
To represent by parable.
a.
Invariable.
a.
Having the capacity of varying or changing; capable of alternation in any manner; changeable; as, variable winds or seasons; a variable quantity.
v. t.
To furnish with a mast or masts; to put the masts of in position; as, to mast a ship.
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 mass; a heap.
a.
Having value or worth; possessing qualities which are useful and esteemed; precious; costly; as, a valuable horse; valuable land; a valuable cargo.
a.
Friendly; kindly; sweet; gracious; as, an amiable temper or mood; amiable ideas.
n.
Mass; church service.
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.
Arable land; plow land.
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.
a.
Liable to vary; too susceptible of change; mutable; fickle; unsteady; inconstant; as, the affections of men are variable; passions are variable.
adv.
In a variable manner.
v. i.
To celebrate Mass.
n.
That which is variable; that which varies, or is subject to change.
a.
Arable; tillable.