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melt godâxtan, godâzidan (#) Fr.: fondre (v.int.) To become liquefied by warmth or heat, as ice, snow, butter, or metal. (v.tr.) To reduce to a liquid state by warmth or heat; to fuse. M.E. melten, O.E. meltan "become liquid;" cf. O.N. melta "to digest;" Gk. meldein "to melt," L. mollis "soft, mild." Godâxtan, godâz- "to melt," from Mid.Pers. vitâxtan, vitâcitan "to melt," from Av. vi-taxti- "flowing away, melting," from vi- "apart, away from, out" (O.Pers. viy- "apart, away;" cf. Skt. vi- "apart, asunder, away, out;" L. vitare "to avoid, turn aside") + tak- "to run, to flow," taciāp- "flowing water," tacinti (3pl.pers.act.) "to flow," tacar- "course," tacan "current, streaming;" Mod.Pers. tâz-, tâxtan "to run; to hasten; to assault," tâzi "swift (greyhound)," tak "running, rush;" Mid.Pers. tâz-, tâxtan "to flow, to cause to walk," tc- "to flow, to walk," tag "running, attack," tâzig "swift, fast;" Khotanese ttajs- "to flow, to walk;" cf. Skt. tak- "to rush, to hurry," takti "runs;" O.Ir. tech- "to flow;" Lith. teketi "to walk, to flow;" O.C.S. tešti "to walk, to hurry;" Tokharian B cake "river;" PIE base *tekw- "to run; to flow." |
meltdown forugodâxt (#) Fr.: fusion du cœur de réacteur A severe accident in a nuclear reactor which is caused by a major failure in the reactor cooling circuit leading to the melting of the reactor core. Without coolant, the core would overheat so that the uranium fuel would melt. If the core continued to heat up, the steel walls of the core would also melt. If the molten core escaped from the containment housing of the reactor, large amounts of highly radioactive materials would be released into the atmosphere. The radioactive contamination of the air, water, and soil can have disastrous consequences for life. → melt; down, M.E. doun, from O.E. dune "downward," short for adune, ofdune, from a-, of "off, from" + dune "hill." Forugodâxt, from foru- "down, downward; below; beneath," as in forurixtan, forunešastan, foruraftan (Mid.Pers. frôt "down, downward;" O.Pers. fravata "forward, downward;" cf. Skt. pravát- "a sloping path, the slope of a mountain") + godâxt past stem of godâxtan, godazidan → melt. |
melting point noqte-ye godâz (#) Fr.: point de fusion The temperature at which a solid changes to a liquid. |
member hamvand (#) Fr.: membre A person or a thing that is part of a group body; e.g. a star which belongs to a cluster. From M.E., from O.Fr. membre, from L. membrum "limb, member of the body, part." Hamvand, literally "linked, joined together," from ham- "together, with; same, equally, even" (Mid.Pers. ham-, like L. com- and Gk. syn- with neither of which it is cognate. O.Pers./Av. ham-, Skt. sam-; also O.Pers./Av. hama- "one and the same," Skt. sama-, Gk. homos-; originally identical with PIE numeral *sam- "one," from *som-. The Av. ham- appears in various forms: han- (before gutturals, palatals, dentals) and also hem-, hen-) + vand "joined, tied," from bastan, vastan "to bind, shut" (O.Pers./Av. band- "to bind, fetter," banda- "band, tie" (cf. Skt. bandh- "to bind, tie, fasten;" PIE *bhendh- "to bind;" Ger. binden; E. bind). |
membership hamvandi (#) Fr.: adhésion The state of being a member. From → member + -ship a native E. suffix of nouns denoting condition, character, office, skill, etc., from M.E., O.E. -scipe; akin to shape. hamvandi, from hamvand, → member, + -i condition, character suffix. |
membership function karyâ-ye hamvandi Fr.: fonction d'adhésion One of several functions used in the → fuzzification and → defuzzification steps of a → fuzzy logic system to map the → nonfuzzy input values to → fuzzy linguistic terms and vice versa. A membership function is used to quantify a linguistic term. → membership; → function. |
memorize barmidan, az bar kardan Fr.: mémoriser To commit to memory, learn by heart. From memor-, → memory, + → -ize. Barmidan, from barm, → memory; az bar kardan, literally "to do from memory," from az preposition, bar, contraction of barm, kardan "to do, make," → -ize. |
memory barm Fr.: mémoire 1) The faculty of the mind to preserve and recall past sensations,
thoughts, knowledge, etc. M.E. memorie, from L. memoria, from memor "mindful, remembering;" cf. Gk. mermera "care," merimna "anxious thought, sorrow," martyr "witness;" Pers. šomârdan "to count;" Mid.Pers. ôšmârtan, ôšmurtan "to reckon, calculate, enumerate, account for;" from Av. base (š)mar- "to have in mind, remember, recall," pati-šmar- "to recall; to long for," hišmar-; Skt. smar- "to remember, become aware," smarati "he remembers." Barm "memory," variant bar (az bar kardan "to memorize"), bir, vir, from Mid.Pers. varm "memory," variants vir, vârom "mind, conscience;" from Av. vārəma, vārəm "according to one's wishes," from var- "to choose." |
memory capacity gonjâyeš-e barm Fr.: capacité de mémoire The amount of information which can be retained in a memory, usually expressed as the number of words which can be retained. For comparison of different memories this number is expressed in bits. |
Mendeleev's table jadval-e Mendeleev (#) Fr.: tableau de Mendeleïev See → periodic table. |
meniscus mâhak, kuž-kâv Fr.: ménisque A → lens with a crescent-shaped section; a → concavo-convex lens. Mod.L. meniscus, from Gk. meniskos "lunar crescent," diminutive of mene, → moon. Mâhak, diminutive of mâh, → moon. |
Menkalinan (Beta Aurigae) Mankeb-zel-enân, šâne-ye arâbe-rân Fr.: Menkalinan A multiple star of magnitude V = 1.90 which is situated in the → Auriga constellation at 81 → light-years away. Other main designations: HR 2088 and HD 40183. Although the third brightest star of the constellation, it bears "Beta" designation. Menkalinan is composed of two main components, which make up a → spectroscopic binary. The combined apparent magnitude varies over a period of 3.96 days between +1.89 and +1.94, as every 47.5 hours one of the stars partially eclipses the other. Both are metallic-lined → subgiant stars of spectral type A2 IV. Each is about 48 times more luminous than the Sun and has roughly the same mass and radius (2.6 times that of the Sun). There is a third component of magnitude 14.1, which is separated from the main pair by 13'', corresponding to a projected distance of 330 → astronomical units. From Ar. Al Mankib dhi'l 'Inan
( |
Menkent (Theta Centauri) Mankab Fr.: Menkent (θ Centauri) A → giant star of → apparent visual magnitude +2.06 located in the southern constellation → Centaurus. It has a → spectral type of K0 III and lies 61 → light-years away. Also called Haratan. Menkent, corruption of Ar. Mankib "shoulder," short for
Mankib al-Qanturis ( |
Mensa Mizkuh Fr.: Table The Table Mountain. A faint constellation near the south celestial pole, at 5h right ascension, 80° south declination. It contains part of the → Large Magellanic Cloud, and its brightest star is of magnitude 5.1. Abbreviation Men; genitive Mensae. First introduced by the French astronomer Nicolas Louis de Lacaille (1713-1762) under the name Mons Mensae, from L. mons "mountain" + mensa "table" to refer to Table Mountain in South Africa. Lacaille made important early observations of the southern sky from the Cape Town region. Mizkuh, from miz "table," originally "preparations for entertaining a guest; guest;" Mid.Pers. mêzd "offering, meal" + kuh→ mountain. |
mental menti, mentâl Fr.: mental Of or pertaining to the → mind. M.E., from M.Fr. mental, from L. mentalis "of the mind," from mens (genitive mentis) "mind," from PIE root *men- "to think." |
mentality mentigi Fr.: mentalité 1) Mental capacity or endowment. |
mention 1) ayât; 2) ayâtidan Fr.: 1) mentionner; 2) mention 1) To refer briefly to; name, specify, or speak of (Dictionary.com). M.E. mencioun, from O.Fr. mencion "mention, memory, speech," from L. mentionem "a calling to mind, a speaking of," from root of Old L. minisci "to think," related to mens "mind," from PIE root *men- "to think;" cf. Pers. man, mân "thought, to think," → mind. Ayât, from Mid.Pers. ayât, ayâd "remembrance, recollection, memory;" Mod.Pers. yâd. |
Merak (β Ursae Majoris) Merâq (#) Fr.: Merak A blue → dwarf star of → spectral type A1 with an → apparent magnitude of 2.37 in the constellation → Ursa Major. It lies 79 → light-years away and has a → luminosity almost 60 times solar, and a mass about triple that of the Sun. Although Merak ranks fifth in brightness in the → Big Dipper, it received the Beta designation from Bayer, who lettered the Dipper's stars from front to back. From Ar. al-Maraqq ( |
Mercator telescope teleskop-e Mercator Fr.: télescope de Mercator A 1.2 m semi-robotic telescope located at the Roque de los Muchachos Observatory on La Palma Island (Canary Islands, Spain). It is operated by the staff of the Institute of Astronomy, University of Leuven (Belgium). The telescope uses two modern instruments HERMES: a → high-resolution optical → spectrograph, and MAIA, a three-armed camera equipped with large → charge-coupled device (CCD)s and optimized for more specific rapid variability studies. The main science drivers of the research performed on the basis of Mercator data are related to a wide range of variable phenomena with a clear focus on stellar astrophysics, in particular the stellar internal structure by means of → asteroseismology. Named after the Flemish cartographer Gerardus Mercator (1512-1594), who studied and taught at the University of Leuven before moving to Duisburg (Germany) |
Mercury 1) Tir; 2) jivé, simâb Fr.: Mercure 1) The closest → planet to the
→ Sun and one of five planets visible with the
naked eye. The → greatest elongation
of Mercury is about 28°,
making it visible at most about 112 minutes after sunset or before sunrise.
It lies at a mean distance of about 0.39
→ astronomical units from the Sun.
Mercury is just 4,879 km in diameter, about 2.6 times smaller than
the Earth. Its → orbital period is 87.97 Earth days.
Mercury has a high → density, 5.4 g cm-3,
with only the Earth having a higher density among the planets. This is largely due to
Mercury being composed mainly of heavy metals and rock.
One → solar day on Mercury lasts the equivalent of 176
Earth days while the sidereal day (the time for 1 rotation in relation to
a fixed point) lasts 59 Earth days. Mercury is nearly
→ tidally locked to the Sun and over time
this has slowed the rotation of the planet to almost match
its orbit around the Sun. Mercury also has the highest orbital
→ eccentricity of all the planets with its distance
from the Sun ranging from 46 to 70 million km. Mercury has just 38% the
→ gravity of Earth, this is too little to maintain
an atmosphere against → solar winds, which blow it away.
The surface of Mercury which faces the Sun has
temperatures of up to 427°C, whilst on the alternate side this can be
as low as -173°C. Mercury's core has more iron than any other planet in the
→ solar system. This has to do with its formation and early
life. If the planet formed quickly, increasing temperatures of the
evolving Sun could have vaporized much of the existing surface,
leaving only a thin shell. From L. Mercurius "Mercury," the Roman god, originally a god of tradesmen and thieves, from merx "merchandise." 1) Mid.Pers. Tîr the name
of the planet Mercury, O.Pers. proper noun *Tira-dāta-
"given by Tir" (Hellenized Tiridates),
Mid.Pers. Tîr.dât the name of three Parthian Kings; Av.
Tīro.nakaθwa-. |
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