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microwave background radiation tâbeš-e paszamine-ye rizmowj Fr.: rayonnement micro-onde du fond cosmique Thermal radiation with a temperature of 2.73 K that is apparently uniformly distributed in the Universe. It is believed to be a redshifted remnant of the hot radiation that was in thermal equilibrium with matter during the first hundred thousand years after the Big Bang. Same as → cosmic microwave background (CMB) radiation. → microwave; → background; → radiation. |
microwave radiation tâbeš-e rizmowj (#) Fr.: rayonnement micro-onde Electromagnetic radiation carried by → microwaves. |
migration mužeš, kuc (#) Fr.: migration 1) The process or act of migrating; a migratory movement. → migrate; → -tion. Kuc "the act of moving from a dwelling, a place to another, decamping, migration." |
million milyon (#) Fr.: million A thousand thousand (106). O.Fr. million, from It. millione, literally "a great thousand," augmentative of mille "thousand," from L. mille. Milyon, Loan from Fr. |
Milne-Eddington approximation nazdineš-e Milne-Eddington Fr.: approximation de Milne-Eddington The approximation of a stellar atmosphere with a plane parallel grey atmosphere in radiative equilibrium. It is assumed that a spectral is formed in such a way that the ratio of the line absorption coefficient to the continuous absorption coefficient is constant with depth. → Milne Universe; Arthur Stanley Eddington (1882-1944), prominent British astrophysicist; → approximation. |
minimum deviation kažraft-e kaminé Fr.: déviation minimale Same as → angle of minimum deviation. |
minimum orbit intersection distance (MOID) durâ-ye kamine-ye andarsekanj-e madâr Fr.: distance minimale d'intersection d'une orbite The minimum distance between the paths of two orbiting objects around a → primary. Such distance between an object and Earth is called Earth MOID. → minimum; → orbit; → intersection; → distance. |
Mintaka (δ Orionis) Mantaqé (#) Fr.: Mintaka The faintest and the westernmost of the three stars which appear in a row and make up the → Orion's Belt. It is a blue star of magnitude 2.23 lying 915 light-years away. Mintaka is in fact an → eclipsing binary with a period of 5.7 days. The main star has a → spectral type of O9.5 and radiates near 90,000 times the → solar luminosity. Mintaka is remarkable as regards the discovery of the → interstellar medium. The ISM was discovered by the German astronomer Johannes Hartmann (1855-1936) through the study of δ Orionis. He remarked that the calcium line at 3934 Å did not share in the periodic displacements of the lines caused by the orbital motion of the star. This suggested that the calcium line was not from the stars but from an intervening interstellar absorbing cloud. Mintaka, from al-Mintaqah "the belt," from al-Mintaqah al-Jauzâ'
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mission gosilân Fr.: mission An operation designed to carry out the goals of a specific program, such as a a space flight or voyage. Mission, from L. missionem (nominative missio) "act of sending," from mittere "to send," of unknown origin. Gosilân, from gosil, variant gosi "sending away, dismission;" Mid.Pers. wisé "to despatch" (Parthian Mid.Pers. wsys- "to despatch;" Buddhist Mid.Pers. wsydy "to despatch;" Sogdian 'ns'yd- "to exhort"), from Proto-Iranian *vi-sid- "to despatch, send off," from prefix vi- "apart, away, out," + *sid- "to call" + -ân nuance suffix. |
modernization novineš (#) Fr.: modernisation 1) The act of modernizing; the state of being modernized; something modernized. |
modification vâtarz, vâtarzeš Fr.: modification An act or instance of modifying; the state of being modified; partial alteration. Verbal noun of → modify. |
modulation degarâhangeš (#) Fr.: modulation General: The modification of some property of a phenomenon by
another distinct phenomenon. Verbal noun of → modulate. |
modulation transfer function (MTF) karyâ-ye tarâvaž-e degarâhangeš Fr.: fonction de transfert de modulation A measure of the ability of an optical system to reproduce (transfer) various levels of detail from the object to the image, as shown by the degree of contrast (modulation) in the image. → optical transfer function. → modulation; → transfer; → function. |
molar concentration dabzeš-e moli Fr.: concentration molaire Of a gas included in the composition of a → gas mixture, the ratio of the number of moles of this gas to the total number of moles of all the gases in the mixture. Same as mole fraction and mole-fraction concentration. → molar; → concentration. |
molar heat of vaporization garmâ-ye boxâreš-e moli Fr.: chaleur de vaporisation molaire The amount of heat energy required to vaporize 1 mole of a liquid at its → boiling point, usually expressed in kJ/mol. → molar; → heat; → vaporization. |
molecular diffusion paxš-e molekuli Fr.: diffusion moléculaire A mixing process in a → fluid caused by the → random relative motions due to → Brownian motion of the individual particles. See also → eddy diffusion. |
molecular emission gosil-e molekuli Fr.: émission moléculaire An → electromagnetic radiation emitted by → interstellar molecules through → transitions between → energy states of → molecules. |
molecular proposition gozâre-ye molekuli Fr.: proposition moléculaire In → propositional logic, a → sentence containing at least one → connectives. See also → atomic proposition. → atomic; → proposition. |
molecular vibration šiveš-e molekuli Fr.: vibration moléculaire The dynamical motion of chemically bound atoms which constantly change their position with each other. The vibration of molecules is treated within → quantum theory. Therefore, the energy of molecular vibration can only take → discrete values. To a first approximation, molecular vibrations can be approximated as → simple harmonic oscillator assigned to each mode. |
Moon formation diseš-e Mâng Fr.: formation de la Lune Any of several theories about how the → Moon originated, among which: → fission theory, → capture theory, → co-formation theory, and → giant impact hypothesis. The model that is best supported by all the available data is the giant impact hypothesis. See also → canonical model. |
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