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meteoritic šaxâne-yi, šahâbsangi (#) Fr.: météoritique Of or pertaining to a → meteorite. |
meteoritic abundance farâvâni-ye šaxâne-yi, ~ šahânsangi Fr.: abondance météoritique The abundance of a chemical element as derived from meteorites. Meteoritic abundances measured from carbonaceous → CI chondrites are believed to represent → protosolar abundances. → meteoritic; → abundance. |
meteoritic impact barxord-e šaxâne-yi Fr.: impact météoritique A striking of a meteorite against another body, especially the solar system planets or satellites. → meteoritic; → impact. |
meteoritics šaxânik, šahâbsangšenâsi,
šahâbsangik Fr.: météoritiqu The science or study of meteorites. |
meteoroid šaxânevâr (#) Fr.: météoroïde A solid object in → interplanetary space before it reaches the Earth's atmosphere. Meteoroids are of → silicate and/or → metallic matter having a size from tiniest grains up to that of the smallest → asteroids. |
meteoroid stream râbeh-ye šaxânevâr Fr.: courants de météoroïdes The meteoroids distributed all along an → orbit and diffused somewhat around it. |
meteoroid swarm qang-e šaxânevâr Fr.: essaim de météoroïdes A relatively dense collection of meteoroids at certain spots along some → meteoroid streams. |
meteorological observation napâheš-e havâšenâxti Fr.: observation météorologique Evaluation or measurement of one or more meteorological elements. Meteorological, of or pertaining to → meteorology; → observation. |
meteorological observatory nepâhešgâh-e havâšenâxti Fr.: observatoire météorologique A scientific establishment dedicated to making precise and detailed meteorological observations and to studying and forecasting atmospheric phenomena by means of special equipments. Meteorological, of or pertaining to → meteorology; → observatory. |
meteorology havâšenâsi (#) Fr.: météorologie The study of the physics, chemistry, and dynamics of the Earth's atmosphere, including the related effects at the air-earth boundary over both land and the oceans. From Gk. meteorologia "discussion of celestial phenomena," from meteoron→ meteor + -logia, &rarr-logy. Havâšenâsi, from havâ "weather, air," → air. |
meter metr (#) Fr.: mètre The → SI unit of length; symbol m. It is defined by taking the fixed numerical value of the → speed of light in vacuum, c, to be 299 792 458 when expressed in the unit m/s, where the → second is defined in terms of ΔνCs. From Fr. mètre, from Gk. metron "measure," from PIE base *me- "to measure" (cf. O.Pers., Av. mā- "to measure;" Skt. mati "measures;" L. metri "to measure"). Metr, loan from Fr. |
methane metân (#) Fr.: méthane A colorless, odorless, inflammable gas gas of formula CH4; the simplest hydrocarbon. From meth- a combining form representing methyl + -ane a suffix used in names of hydrocarbons of the methane or paraffin series. |
methanol metânol (#) Fr.: méthanol, alcool méthylique Alcohol, also known as methyl alcohol, formula CH3OH, formed in small quantities in the oxidation of methane. → methanol maser. From → methane + -ol a suffix used in the names of chemical derivatives. |
methanol maser meyzer-e metânol Fr.: maser méthanol A maser source in which excited methanol molecules (CH3OH) produce → maser emission. Methanol masers are signposts of the early stages of star formation, many being associated with sources that have not developed an → H II region. There are more than 20 different methanol transitions that have been observed. They are divided into two categories: Class I, excited by collisions, and class II, excited by infrared radiation. The most important class I masers are at a frequency of 44.1 GHz, while he most important class II masers are at a frequency of 6.7 GHz. |
method raveš (#) Fr.: méthode A manner or mode of procedure, especially an orderly, logical, or systematic way of instruction, inquiry, investigation, experiment, and so on. From M.Fr. méthode, from L. methodus "way of teaching or going," from Gk. methodus "scientific inquiry, method of inquiry," originally "following after," from → meta- "after" + hodos "way." Raveš "mthod," originally "going, walking," from row "going," present stem of raftan "to go, walk;" Mid.Pers. raftan, raw-, Proto-Iranian *rab/f- "to go; to attack" + -eš a suffix of verbal nouns. |
method of least squares raveš-e kamtarin cârušhâ Fr.: méthode des moindres carrés A method of fitting a curve to data points so as to minimize the sum of the squares of the distances of the points from the curve. → method; → least squares. |
method of small perturbations raveš-e parturešhâ-ye kucak Fr.: méthode des petites perturbations The linearization of the appropriate equations governing a system by the assumption of a steady state, with departures from that steady state limited to small perturbations. Also called perturbation method. → method; → small; → perturbation. |
method of successive approximations raveš-e nazdinešhâ-ye payâpey Fr.: méthode d'approximations successives The solution of an equation or by proceeding from an initial approximation to a series of repeated trial solutions, each depending upon the immediately preceding approximation, in such a manner that the discrepancy between the newest estimated solution and the true solution is systematically reduced. → method; → successive; → approximation. |
Methuselah star setâre-ye Matušâleh Fr.: étoile Mathusalem → HD 140283. Name given to → HD 140283 by the popular press due to its very old age. Methuselah is a biblical patriarch supposed to have lived 969 years (Genesis 5:21-27). The name Methuselah, or the phrase "old as Methuselah," is commonly used to refer to any living thing reaching great age. |
methyl metil Fr.: méthyle A → methane molecule lacking one → hydrogen atom: CH3. → methyl chloride. Back formation from Fr. méthylène, → methylene. |
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