An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 97
quark
  کو‌آرک   
kuârk (#)

Fr.: quark   

Any of the hypothetical particles with spin 1/2, baryon number 1/3, and electric charge 1/3 or -2/3 that, together with their antiparticles, are believed to constitute all the elementary particles classed as baryons and mesons. Quarks are distinguished by their flavors, designated as up (u), down (d), strange (s), charm (c), bottom or beauty (b), and top or truth (t), and their colors, red, green, and blue.

Quark, coined in 1963 by the American physicist Murray Gell-Mann (1929-), who took it from a nonsense word in James Joyce's novel Finnegans Wake (1939): Three quarks for Muster Mark! // Sure he has not got much of a bark // And sure any he has it's all beside the mark.

quark confinement
  پربست ِ کو‌آرک‌ها   
parbast-e kuârkhâ

Fr.: confinement des quarks   

The phenomenon wherein the → quarks are permanently bound together and can never be removed from the → hadrons they compose.

quark; → confinement.

quark star
  ستاره‌ی ِ کو‌آرکی   
setâre-ye kuârki

Fr.: étoile de quarks   

A hypothetical star so dense that it is composed of degenerate quarks, a matter denser than that of a neutron star.

quark; → star.

quark-hadron phase transition
  گذرش ِ فاز ِ کو‌آرک-هادرون   
gozareš-e fâz-e kuârk-hâdron

Fr.: transition de phase quark-hadron   

A phase transition, predicted by cosmological models, to have occurred at approximately 10-5 seconds after the Big Bang to convert a plasma of free quarks and gluons into hadron.

quark; → hadron; → phase; → transition.

quarter
  چارَک   
cârak (#)

Fr.: quartier   

A fourth of the Moon's period or monthly revolution around Earth. → first quarter; → last quarter.

from O.Fr. quartier, from L. quartarius "fourth part," from quartus "fourth," related to quattuor "four," cognate with Pers. câr, cahâr, as below.

Cârak "quarter," literally "fourth, a fourth part of one," from câr, contraction of cahâr, → four, + -ak, contraction of yak, yek "one." Yek "one, alone," from Mid.Pers. êwak (Proto-Iranian *aiua-ka-); O.Pers. aiva- "one, alone;" Av. aēuua- "one, alone;" cf. Skt. éka- "one, alone, single;" Gk. oios "alone, lonely;" L. unus "one;" E. one.

quarter-wave plate
  تیغه‌ی ِ چارک-موج   
tiqe-ye cârak-mowj

Fr.: lame quart d'onde   

A plate of doubly refracting material cut parallel to the optic axis of the crystal and of such a thickness that a phase difference of 90° is introduced between the ordinary and extraordinary rays for light of a particular wavelength. → half-wave plate.

quarter; → wave; → plate.

quartic equation
  هموگش ِ چارُمیک   
hamugeš-e câromik

Fr.: équation quartique   

An equation containing unknowns of the fourth power; the general form: ax4 + bx3 + cx2 + dx + e = 0.

From L. quart(us) "fourth" (→ quarter) + → -ic; → equation.

hamugeš, → equation; câromân, from cârom "fourth," from câr, cahâr "four" + -om "-th" + -ik, → -ic.

quartile
  چارکوار   
cârakvâr

Fr.: quartile   

In statistics, any of the four groups of a frequency distribution each containing 25% of the total number of individual observations.

From M.L. quartilis, from quart(us) "fouth" + -ilis "-ile" a suffix of adjectives expressing capability, susceptibility, liability, aptitude.

Cârakvâr, from cârak, → quarter, + -vâr suffix of similarity, size, aptitude.

quartz
  کو‌آرتز   
kuârtz (#)

Fr.: quartz   

One of the most abundant → minerals in the Earth's → crust. Quartz is made up of silicon dioxide (SiO2), or → silica. It has marked → piezoelectric properties and → dielectric strength.

From Ger. Quarz "rock crystal," from M.H.G. twarc.

quasar
  کو‌آسار، ستاره‌وَش   
kuâsâr (#), setârevaš (#)

Fr.: quasar   

An compact, extragalactic object which is highly luminous and looks like a star. Their redshifts can be large and their brightness varies. Quasars have an intrinsic luminosity which can reach some 100 times that of bright galaxies. They are thought to be active galactic nuclei with a size a little larger than the solar system. The first quasar to be identified as such, in 1963, was the radio source 3C 273 at a redshift of 0.158. With its 13th magnitude, it is the optically brightest quasar as observed from Earth. Some quasars are strong radio sources.

From quas(i) + (stell)ar (object).

Setârevaš, from setâré, → star, + -vaš, → quasi-.

quasi-
  چونان-، -وش   
cunân-, -vaš

Fr.: quasi-   

A prefix meaning "resembling, almost, having some, but not all of the features of."

From L. quasi "as if, as though," from qua(m)" as" + si "if."

Cunân "so, like that; just as if," from cun "how?," (Mid.Pers. cigôn "how?," cigônêh "nature, character," O.Pers/Av. ci- "what, any," collateral stem to ka- "who?, what?;" cf. Skt. ka-; Gk. po-; L. quo-; E. what, who; PIE *qwos/*qwes) + suffix ân. -vaš a suffix of similitude.

quasi-atom
  چونان-اتم، اتم‌وَش   
cunân-atom, atom-vaš

Fr.: quasi-atome   

A system in which the nuclei of two colliding atoms approach each other closely for a brief lapse of time so that their electrons are arranged in atomic orbitals characteristic of a single atom with combined atomic number.

quasi-; → atom.

quasi-closed subsystem
  زیر-راژمان ِ چونان‌بسته   
zir-râžmân-e cunân-basté

Fr.: sous-système quasi-fermé   

A subsystem if its intrinsic energy is large, on the average, with respect to the energy of its interaction with other portions of the → closed system.

quasi-; → closed; → subsystem.

quasi-linear theory
  نگره‌ی ِ چونان-خطی   
negare-ye cunân-xatti

Fr.: théorie quasi-linéaire   

In plasma physics, the theory that considers the interactions between waves and particles are of first order only. It ignores all terms of second order in the fluctuating quantities.

quasi-; → linear; → theory.

quasi-satellite
  چونان‌ماهواره، چونان‌بنده‌وار   
cunân-mâhvâré, cunân-bandevâr

Fr.: quasi-satellite   

An asteroid moving around the Sun having the same mean motion and mean → longitude as a planet, but a different → eccentricity. The asteroid remains near the planet much like a satellite even when its distance is large enough so that it is well outside the planet's → Hill sphere. The quasi-satellite motion is one class of possible → co-orbital motions of small bodies in 1:1 mean-motion → resonance with a planet. If the quasi-satellite orbit is coplanar with the planet, then the motion is stable in the → secular approximation. When the orbits are inclined enough, an asteroid can be trapped into such a motion for a finite period of time. Earth has several quasi-satellites (mainly 3753 Cruithne, 2002 AA29, 2003 YN107), also does Venus (the only one so far discovered, 2002 VE68). The possibility of such orbits was first suggested by J. Jackson (1913, MNRAS 74, 62).

The term quasi-satellite was first used by S. Mikkola & K. Innanen 1997, The Dynamical Behaviour of our Planetary System; Proceedings, p. 345); → quasi-; → satellite.

quasi-separatrix layer (QSL)
  لایه‌ی ِ چونان‌جداگر   
lâye-ye cunân-jodâgar

Fr.: couche quasi-séparatrice   

A region of the solar atmosphere where the gradient of the field line → linkage from one boundary to another is large so that the field lines can slip-run rapidly through the → plasma. The QSL results from → magnetic reconnection without → null point.

quasi-; → separatrix; → layer.

quasi-single-scattering approximation
  نزدینش ِ چونان-تک‌پراکنش   
nazdineš-e cunân-tak-parâkaneš

Fr.:   

A model of radiative transfer that ignores forward scattering of photons; assuming forward-scattered light as un-scattered.

quasi-; → single; → scattering; → approximation.

quasi-stellar object
  بر‌آخت ِ چونان‌ستاره‌ای   
barâxt-e cunân-setâre-yi

Fr.: objet quasi-stellaire   

Initial name of → quasars.

quasi-; → stellar; → object.

quasi-stellar radio source
  ر‌آدیو-خن ِ چونان‌ستاره، ~ ~ ِ ستاره‌وش   
râdio-xan-e cunân setâré, ~ ~ setâré-vaš

Fr.: radiosource quasi-stellaire   

A quasar with detectable radio emission.

quasi-; → stellar; → radio; → source.

quasicrystal
  چونان‌بلور   
cunân-bolur

Fr.: quasi-cristal   

A form of solid made up of ordered but non-repeating patterns of atoms, a symmetry that is forbidden for periodic crystals. In an ordinary crystal, only 1-, 2-, 3-, 4-, and 6-fold symmetries are possible, since these are the only symmetries that, when combined, can fill space. Prior to the discovery of quasicrystals, it was believed that 5-fold crystal symmetry could never occur. Quasicrystals are remarkable in that some of them display 5-fold or higher-fold forbidden symmetries. They are used as catalysts, in particular at high temperatures, to produce durable kinds of steel, like those used in objects such as razor blades and thin needles made specifically for eye surgery. The Nobel Prize in Chemistry 2011 was awarded to Daniel Schechtman for his discovery of quasicrystals in 1982.

quasi-; → crystal.

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