An Etymological Dictionary of Astronomy and Astrophysics

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory



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Number of Results: 693

Fr.: mascon   

A region on the surface of the → Moon where the → gravitational attraction is slightly higher than normal due to the presence of dense rock.

Short for mass concentration; → mass; → concentration.

narin (#)

Fr.: masculin   

1) Having qualities appropriate to or usually associated with a man.
2) Of, relating to, or constituting the gender that ordinarily includes most words or grammatical forms referring to males (

M.E. masculin, from O.Fr. masculin "of the male sex," from L. masculinus "male, of masculine gender," from masculus "male, masculine; worthy of a man," diminutive of mas "male person, male," of unknown origin.

Narin, from nar "male," from Mid.Pers. nar, "male, manly;" Av. nar- "male, man," nairya- "male, manly;" cf. Skt nara- "male, man."

meyzer (#)

Fr.: maser   

1) A source of very intense, narrow-band, coherent microwave radiation involving → stimulated emission, as in the → laser.
2) A device that generates such radiation.
3) In astronomy, maser emission detected from a number of molecules and associated with several environments: the vicinity of newly forming stars and → H II regions (OH, water, SiO, and methanol masers); the circumstellar shells of evolved stars, i.e. red giants and supergiants (OH, water, and SiO masers); the shocked regions where supernova remnants are expanding into an adjacent molecular cloud (OH masers); and the nuclei and jets of active galaxies (OH and water masers). The hydroxyl radical (OH) was the first interstellar maser detected (Weinreb et al. 1963).

Maser stands for Microwave Amplification by Stimulated Emission of Radiation; → laser.

maser emission
  گسیل ِ میزری   
gosil-e meyzeri (#)

Fr.: émission maser   

An emission arising from the → maser process.

maser; → emission.

  ۱) ماسک؛ ۲) ماسک زدن   
1) mâsk (#); 2) mâsk zadan (#)

Fr.: 1) masque; 2) masquer   

1) Something that serves to cover or conceal.
Electronics: A pattern used to control the configuration of conducting material deposited or etched onto a semiconductor chip.
2) Electronics: To override one signal with a stronger one.

From M.Fr. masque "covering to hide or guard the face," from It. maschera, from M.L. masca "mask, specter, nightmare," of uncertain origin.

1) Mâsk, loan from Fr., as above; 2) with verb zadan "to make, to do," originally "to strike, beat; to do; to play an instrument" (Mid.Pers. zatan, žatan; O.Pers./Av. jan-, gan- "to strike, hit, smite, kill" (jantar- "smiter"); cf. Skt. han- "to strike, beat" (hantar- "smiter, killer"); Gk. theinein "to strike;" L. fendere "to strike, push;" Gmc. *gundjo "war, battle;" PIE *gwhen- "to strike, kill").


Fr.: masque, masquage   

1) A method of improving → spatial resolution of images. → pupil masking; → unsharp masking.
2) Computers: The process of specifying a number of values that allow extracting desired information from a set of characters or bits while suppressing the undesired information.

Verbal noun of → mask.

  ۱) جرم، غند؛ ۲) توده، انبوه   
1) jerm (#), qond (#); 2) tudé (#), anbuh (#)

Fr.: masse   

1) A measure of the amount of material in an object, defined either by the inertial properties of the object or by its gravitational influence on other bodies. See also → inertial mass, → gravitational mass.
2) A considerable assemblage, number, or quantity.

From O.Fr. masse "lump," from L. massa "kneaded dough, lump," from Gk. maza "barley cake, lump, mass, ball," related to massein "to knead."

Jerm, from Ar. jirm.
Qond "assembled, collected; a crowd," related to gondé "coarse, thick; big;" Mid.Pers. gund "troop, group, gathering;" loaned into Arm. gund and Ar. jund.
Tudé "heap, stack, tumulus;" cf. Kurd. tavda "all, total;" Tati tâya "heap, mass;" Sogd. tuδē "heap, mass." Perhaps related to PIE *teuta- "people, tribe;" cf. Lith. tauta, Oscan touto, O.Irish tuath, Goth. þiuda, O.E. þeod "people, folk, race."
Anbuh "numerous, abundant," from Proto-Iranian *ham-buH- "to come together," from ham- "together," → com- + *buH- "to be , become," Av. ham.bauu- "to come together, unite," from ham- as above + bauu-, bu- "to be, become," O.Pers. bav- "to be, become," Mod.Pers. budan "to be," Skt. bhavati "becomes, happens," PIE base *bheu-, *bhu- "to grow, become;" cf. Gk. phu- "become," P.Gmc. *beo-, *beu-, E. be.

mass absorption coefficient
  همگر ِ درشم ِ جرمی   
hamgar-e daršm-e jermi

Fr.: coefficient d'absorption de masse   

A measure of the rate of absorption of radiation, expressed as the linear absorption coefficient divided by the density of the medium through which radiation is passing.

mass; → absorption; → coefficient.

mass defect
  کاست ِ جرم   
kâst-e jerm

Fr.: défaut de masse   

The difference between the rest mass of an atomic nucleus (made up of protons and neutrons) and the sum of the masses of its individual protons and neutrons. The mass difference is equal to the released binding energy. Also called mass deficiency

mass; → defect.

mass density
  چگالی ِ جرمی   
cagâli-ye jermi

Fr.: densité massique   

The mass per unit area of the ring material, integrated through the thickness of the ring. Sometimes called → surface density (Ellis et al., 2007, Planetary Ring Systems, Springer).

mass; → density.

mass discrepancy
  ناهم‌خوانی ِ جرم   
nâhamxâni-ye jerm

Fr.: écart de masse   

1) For → massive stars and → supergiants, the difference between the → spectroscopic mass and the → evolutionary mass. Early studies found that the spectroscopic mass was systematically less than the evolutionary mass by as much as a factor of 2 for supergiants. Improvements in the stellar atmosphere models (taking into account → line blanketing) have decreased or eliminated the size of the discrepancy for Galactic stars. There is still a mass discrepancy for the hottest → O stars in the → Magellanic Clouds (See, e.g. Massey et al. 2009, ApJ 692, 618).
2) For a → cluster of galaxies, the apparent difference between the mass of the cluster obtained by using the → virial theorem, and the mass inferred from the total luminosities of the member galaxies.

mass; → discrepancy.

mass energy
  کاروژ ِ جرم   
kâruž-e jerm

Fr.: énergie de masse   

The energy (E) associated with a mass (m), as specified by the → mass-energy equivalence  E = mc2, where c is the → speed of light. For a moving body the total energy of the particle is expressed by: E2 = m2c4 + p2c2, where m is → rest mass and p → momentum.

mass; → energy.

mass extinction
  خاموشی ِ انبوه   
xâmuši-ye anbuh

Fr.: extinction en masse   

An event in the history of life on Earth in which large numbers of species (sometimes more than 90% of some species) vanish in a relatively short period of time. In spite of controversy, it is generally recognized that there have been at least six major mass extinctions. These occurred in the late Cambrian (500 million years ago), in the late Ordovician (440 million years ago), in the late Devonian (365 million years ago), at the end of the Permian (245 million years ago), in the late Triassic (208 million years ago), and at the end of the Cretaceous (65 million years ago).

mass; → extinction.

mass flow
  تچان ِ جرم   
tacân-e jerm

Fr.: écoulement de masse   

The mass of a fluid that passes a specified unit area in a unit amount of time.

mass; → flow.

mass formula
  دیسول ِ جرم   
disul-e jerm

Fr.: formule de masse   

An → equation expressing the → atomic mass of a → nuclide as a function of its → mass number and the → atomic mass unit.

mass; → formula.

mass fraction
  برخه‌ی ِ جرم   
barxe-ye jerm

Fr.: fraction de masse   

The fractional amount (by mass) of a given element or nuclide in a given composition.

mass; → fraction.

mass function
  کریای ِ جرم   
karyâ-ye jerm

Fr.: fonction de masse   

1) The number of a class of objects as a function of their mass. → initial mass function (IMF); → present-day mass function (PDMF).
2) A numerical relation between the masses of the two components of a → spectroscopic binary that provides information on the relative masses of the two stars when the spectral lines of only one component can be seen. If Mp is the mass of primary (whose spectrum is known), Ms is the mass of secondary, and i the → angle of inclination of the orbit, the mass function is given by: (Ms3. sin3i) / (Mp + Ms)2.

mass; → function.

mass loss
  دسترفت ِ جرم   
dastraft-e jerm

Fr.: perte de masse   

The outpouring of particles and gas from a star, occurring at varying rates and by a variety of processes throughout a star's lifetime. → Bipolar flows are believed to be due to mass loss by forming → protostars, while → massive stars lose their mass through powerful → stellar winds.

mass; → loss.

mass loss rate
  نرخ ِ دسترفت ِ جرم   
nerx-e dastraft-e jerm

Fr.: taux de perte de masse   

The rate with which the → mass loss process takes place, usually expressed in → solar mass per year. → radiation-driven mass loss. The mass loss rate and the → terminal velocity are anti-correlated, since the → wind momentum is constant, → bi-stability jump.

mass loss; → rate.

mass number
  عدد ِ جرمی   
adad-e jermi (#)

Fr.: nombre de masse   

The total number of → protons and → neutrons in the → atomic nucleus (symbol A). The mass number is written either after the → chemical element name or as a superscript to the left of an element's symbol. For example, the most common isotope of oxygen is oxygen-16, or 16O, which has 8 protons and 8 neutrons.

mass; → number.

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