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covalence ham-arzâyi Fr.: covalence Chemistry: The number of covalent bonds which an atom can from. The sharing of electrons to form chemical bonds. → equivalence. From → co- + valence, from L. valentia "strength, worth," valere "to be worth; be strong." Ham-arzâyi, from ham-→ co- + arzâyi, from arzidan "to be worth," arzân "worthy; of small value, cheap," arj "esteem, honour, price, worth," Mid.Pers. arz "value, worth," arzidan "be worth," arzân "valuable;" Av. arəjaiti "is worth," arəja- "valuable," arəg- "to be worth;" cf. Skt. arh- "to be worth, to earn," árhant- "worthy person;" Gk. alphanein "to bring in as profit," alphein "to ear, obtain;" Lith. algà "salary, pay;" PIE base *algwh- "to earn; price, value." |
covalent bond band-e ham-arzâ Fr.: lien covalent A chemical bond between two atoms of the same or different elements, in which each atom contributes one electron to be shared in a pair. |
covariance hamvartâyi Fr.: covariance In statistics, a measure of linear dependence. For two random variables X and Y with expectations mx and my, the covariance is E{(X - mx)(Y - my)}. |
covariant hamvartâ Fr.: covariant In physics, having the property of remaining invariant in form under a Lorentz transformation. |
covariant tensor tânsor-e hamvartâ Fr.: tenseur covariant A tensor whose components are distinguished by → subscript indices. |
cover pušidan; pušeš (#) Fr.: couvrir; couverture 1) To spread over an area or surface. From M.E., from O.Fr. covrir, from L. cooperire "to cover over, overwhelm, bury," from the intensive prefix → com- + operire "to close, cover." Pušidan "to cover; to put on," → envelope; pušeš, verbal noun of pušidan. |
coverage pušeš (#) Fr.: couverture 1) General: The extent to which something is covered. From → cover + -age a suffix forming abstract nouns. → cover. |
cow gâv (#) Fr.: vache The female of bovine animals. M.E. cou, cognate with Pers. Gâv, as below. Mid.Pers. "bull, cow;" Av. gao-, gāvuš; cf. Skt. go-, gáus; Gk. bous ";" L. bos "ox, bull, cow;" O.E. cu "cow;" Ger. Kuh "cow;" PIE *gwows "cow." |
Cowling model model-e Cowling Fr.: modèle de Cowling A model of the internal structure of → massive stars in which a → convective core is surrounded by a large → radiative envelope. However, recent studies point to the presence of a thin → convection zone in the outer envelope of hot massive stars, beneath the → photosphere, which is caused by opacity peaks associated with iron and helium ionization. See also → iron convection zone. After Thomas Cowling (1906-1990), a British astronomer, who put forward the model; → model. |
CP star setâre-ye CP Fr.: étoile CP |
CP-symmetry hamâmuni-ye bâr-hamâli Fr.: symétrie charge-parité Same as → charge-parity symmetry. |
crab xarcang (#) Fr.: crabe 1) Any decapod crustacean of the suborder Brachyura, having the eyes
on short stalks and a short, broad, more or less flattened body, the
abdomen being small and folded under the thorax.
→ Cancer; → Crab nebula;
→ Crab pulsar. M.E. crabbe; O.E. crabba, from Germanic *krab(b)- (cf. Low Ger. krabben "to scratch, claw"); PIE base *gerbh- "to scratch;" cf. Gk. graphein "to write." Xarcang "crab," from Mid.Pers. karcang, cf. Lori qerženg from kar-, qer- + cang, ženg "claw." The meaning of the first component, xar/qer, is not clear. It may be related to Av. xruta-, xraoždva- "hard," as in xruždisma- "hard ground" (from xruždi- + zam-), and to the PIE *qarq- "to be hard." In that case, the Pers. term for crab would literally mean "hard claw." |
Crab nebula (M1, NGC 1952) miq-e xarcang Fr.: Nébuleuse du Crabe An expanding cloud of debris from the explosion of a → Type I supernova in the → constellation → Taurus. Its light reached Earth in 1054 and was visible to the naked eye even in the daytime. Lying about 6,300 → light-years away, the Crab nebula is an intense → radio source (Tau A), and also a source of X-rays and gamma-rays. The diameter of the → supernova remnant is about 6 light-years; it is expanding at velocity of 1000 km/sec. |
Crab pulsar pulsâr-e xarcang (#), tapâr-e ~ (#) Fr.: pulsar du Crabe A → pulsar discovered in the center of the → Crab nebula in 1969. It is a highly magnetized → neutron star with a radius of 10-15 km that spins 30 times a second. |
cradle gahvâré (#) Fr.: berceau 1) A bed for a baby that is usually designed to rock back and forth when pushed gently.
→ Newton's cradle. M.E. cradel, from O.E cradol akin to O.H.G. kratto "basket," Ger. Krätze "basket carried on the back;" Pers. gereh "knot;" Skt. granth- "to tie a knot" (Cheung 2007). Gahvâré "cradle," variants gâhvâré, gowvâré, govâré, from Mid.Pers. gâhwârag "cot, cradle." |
craft nâv (#) Fr.: petit bateau A ship or other vessel. M.E., from O.E. cræft "strength, skill;" cf. Ger. Kraft, D. kracht, O.N. kraptr. The "ship" meaning comes from the expression "vessel of small craft (trade)." Nâv "ship;" O.Pers./Av. *nāv-, O.Pers. nāviyā- "fleet;" cf. Skt. nau-, nava- "ship, boat;" Gk. naus. |
crater 1, 2) lâvak, kandâl; 3) Jâm Fr.: 1, 2) cratère; 3) Coupe 1) A bowl-like depression on the rigid surface of a planet, satellite, or asteroid
usually caused by the high-speed impact of a colliding object. From Gk. krater "a wide, two-handled bowl for mixing wine with water," from kerannynai "to mix;" PIE base *kere- "to mix, confuse." Lâvak "a large wooden bowl for kneading dough." |
crater floor kaff-e lâvak Fr.: sol de cratère The lower part of an → impact crater bounded by the rising → crater rim. |
crater rim labe-ye lâvak Fr.: bords de cratère That part an → impact crater that extends above the height of the local surface, usually in a circular or elliptical pattern. |
cratering lâvakzâyi, kandâlzâyi Fr.: cratérisation The process by which craters form on the surface of Solar System objects. From lâvak or kandâl, → crater, + zâyi from zâ- present tense stem of zâdan "to give birth," Mid.Pers. zâtan, Av. zan- "to bear, give birth to a child, be born," infinitive zazâite, zâta- "born," cf. Skt. janati "begets, bears," L. gignere "to beget," PIE base *gen- "to give birth, beget." |
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