<< < -ci cal Cal can Cap car cas cat cau cel cen cen cha cha cha che Chi chr cir cir civ Cla clo clu CNO coa coe coh col col col com com com com com com com com Com con con con con con con con con con con con con Coo cor cor cor cos cos cos cou cov cra cri cro cry cum cur cyc > >>
coast rahâraftan Fr.: accoster To move without further use of propelling power. → coasting flight, → coasting Universe. M.E. coste, from O.Fr., from L. costa "rib, side," cf. Mid.Pers. kust, kustag "side, direction; district," Mod.Pers. xost, xwast "a beaten road; island;" PIE *kost- "leg, bone." Rahâraftan, from rahâ "free, set free" (O.Pers. rad- "to leave," Skt. rah-, rahati "separates, leaves," Av. razah- "isolation;" PIE *redh-) + raftan "to go, walk" (Mid.Pers. raftan, raw-, Proto-Iranian *rab/f- "to go; to attack"). |
coasting flight parvâz-e rahârow Fr.: vol d'accostage The unpowered flight of a spacecraft or missile after propulsion cutoff or between the burnout of one stage and the ignition of the next. |
coasting Universe giti-ye rahârow Fr.: Univers à densité critique A Universe whose density is just less than or equal to the critical value and expands forever with no change in the expansion rate. |
coat andudan (#) Fr.: revêtir, couvrir To → cover with a → thin → layer of a → substance, as → aluminum over the → surface of a → mirror, → aluminize. Verb from noun coat, from M.E. cote, from O.Fr. cote "coat, robe," from some Germanic source; cf. O.S. kot "woolen mantle," O.H.G. chozza "cloak of coarse wool," Ger. Kotze "a coarse coat," of unknown origin. Andudan, variant andâyidan, from Mid.Pers. handudan, from O.Iranian *ham-dâvaya-, from ham- "together" + *dâvaya-, from dav- "to rub, clear," cf. Av. dav- "to clean, polish," Skt. dhâv-, PIE *dheu- "to shine". |
Coathanger raxtâviz (#) Fr.: amas du Cintre An open cluster of about 40 stars at the border of → Vulpecula and → Sagitta. It has an apparent size of about 1° and lies 420 → light-years away. Also called Collinder 399 and → Brocchi's Cluster. Six of its brighter stars, of sixth and seventh magnitude, are lined up in a nearly perfect row, from the center of which four stars form a hook to resemble the coathanger shape. To the naked eye, it appears as an unresolved patch first recorded by the Persian astronomer Sufi in A.D. 964. It was later rediscovered by Giovanni Battista Hodierna (1597-1660). The Coathanger shares roughly the same motion with several other clusters, including the → Pleiades. → coat; hanger, from hang, M.E. han(i)gen, fusion of O.E. hon "suspend" and hangian "be suspended;" also probably influenced by O.N. hengja "suspend" and hanga "be suspended" (cf. O.Frisian hangia, Du. hangen, Germ. hängen). Raxtâviz, from raxt "clothes, garment, wearing apparel" + âviz "hang," → pendulum. |
coating andud (#) Fr.: revêtement |
cobalt kobâlt (#) Fr.: cobalt A silver gray, brittle, hard metallic → chemical element which is highly magnetic; symbol Co. → Atomic number 27; → atomic weight 58.9332; → melting point 1,495°C; → boiling point about 2,870°C; → specific gravity 8.9 at 20°C. It is used in many → alloys, and in particular its compounds have been used since ancient times (Egyptians, Persians, Greeks) to produce a blue color in glass and ceramics. Cobalt was discovered in 1735 by the Swedish chemist Georg Brandt (1694-1768). It has several radioactive isotopes, including Co-56, half-life about 77 days, Co-57, 272 days, Co-58, 71 days, Co-60, 5.27 years. The → light curve of → type I supernovae is explained by the radioactive decay of nickel-56 through cobalt-56 to iron-56. From Ger. kobold "evil spirits or goblins," who were superstitiously thought to cause trouble for miners, since the mineral contained arsenic which injured their health and the metallic ores did not yield metals when treated with the normal methods. |
cobble qolve (#) Fr.: Geology: A → sedimentary particle that is between 64 and 256 mm in size. Cobbles are larger than → pebbles but smaller than → boulders. Cobbles have typically been rounded by abrasion during sedimentary transport (geology.com/dictionary). From M.E. cobill, kobill, probably a diminutive of M.E. *cob, *cobb, ultimately from Proto-Germanic *kubb- ("lump; round object") + -le. Qolve, variant of gorde "kidney." |
cobweb karu (#), kâtené (#) Fr.: toile d'arraignée A web spun by a spider to entrap its prey; a single thread spun by a spider; something resembling a cobweb; anything finespun, flimsy, or insubstantial (Dictionary.com). M.E. coppeweb, derivative of O.E. -coppe "spider" in atorcoppe "poison spider;" + → web. Karu "cobweb, web," variants kari, kartané, kartiné, kârtanak, kârtané, kare tan (all in Dehxodâ), (Malâyeri, Hamadâni) kâtena, (Gilaki) kârtang, (Kermâni) kerâš, (Qêyeni) kalaš, (Qomi) kârye, (Tabari) kel, kuli, (Yazdi) kare, from *kar-, *kâr-, *kel- "to weave;" cf. (Ormuri, in Pakistan, Afghanistan) gal-/galôk- "to weave;" PIE base *ker- "to weave; rope." |
Cocoon Nebula (IC 5146) miq-e pilé Fr.: nébuleuse du cocon An emission nebula located about 3,000 light-years away toward the → constellation → Cygnus. It is thought to be a region of active → star formation. Cocoon, from Provençal Fr. coucoun, from O.Fr. coque "egg shell, nut shell," L. coccum "berry," from Gk. kokkos "berry, seed;" → star; → nebula. Miq, → nebula; pilé "the silkworm's cocoon; a purse", cf. Skt. patta- "woven silk." |
cocoon star setâre-ye pileyi Fr.: étoile dans son cocon A star hidden in a dense envelope of gas and dust which is a strong source of infrared emission. → Cocoon nebula; → star. |
code ramz (#) Fr.: code 1) A system used for brevity or secrecy of communication, in which arbitrarily chosen words,
letters, or symbols are assigned definite meanings. M.E., from O.Fr. code, from L. codex "book, book of laws," later form of caudex "tree trunk," hence "document made up of wooden tablets." Ramz "secret writing, enigma," loan from Ar. |
codeclination hamvâkileš Fr.: codéclinaison The complement of → declination; the angular distance along a great circle from the celestial pole, i.e., 90° - declination. Codeclination, from → co- + → declination. Hamvâkil, from ham-, → co-, + vâkil, → declination. |
codex nebigân Fr.: codex A manuscript text in book form which was common before the invention of printing. The codex is the earliest known form of a bound book which replaced the scroll. It was a Roman invention. → Dresden codex. From L. codex "book," → code. Nebigân, from nebi / nepi / nevi "book, scripture," from Mid.Pers. nibêg "writing, scripture, book," related to neveštan, → write, + -gân suffix denoting collective nature. |
codomain ham-daman Fr.: ensemble d'arrivée The set of values that a → function is allowed to take (i.e. may possibly come out of a function), as opposed to the → range. |
coefficient hamgar (#) Fr.: coefficient 1) Math.: A number or letter placed before an
algebraic expression to indicate that the expression is to
be multiplied by that factor, e.g. in the expression 2 x3,
2 is the coefficient of x3. In general, any factor of
a product is called the coefficient of the product of the remaining
factors. Hamgar, from ham- "together," → com- + -gar agent suffix, from kar-, kardan "to do, to make," Mid.Pers. kardan, O.Pers./Av. kar- "to do, make, build," Av. kərənaoiti "makes," cf. Skt. kr- "to do, to make," krnoti "makes," karma "act, deed;" PIE base kwer- "to do, to make." |
coefficient of viscosity hamgar-e vošksâni Fr.: coefficient de viscosité A quantity that indicates a property of fluids and is defined by the ratio of shearing → stress to the rate of change of shearing → strain. It is also simply called viscosity. The coefficient of viscosity is expressed by: μ = (F/A) / (dv/dy), where F is the force required to maintain a steady velocity difference dv between any two parallel layers of the fluid, A is the area of the layers, and dv/dy is the → velocity gradient between two points separated by a small distance measured at right angles to the direction of flow. The unit of viscosity is that of force times distance divided by area times velocity. Thus, in the cgs system, the unit is 1 dyne.cm/cm2.(cm/s), which reduces to 1 dyne.s/cm2. This unit is called 1 → poise. → viscosity; → coefficient. |
coelostat âsmândâštâr Fr.: coelestat A flat mirror with a clock-drive mounted in such a way that it moves from east to west to compensate for the apparent rotation of the Earth in order that the image of a particular area of sky remains fixed in the focal plane. See also → siderostat and → heliostat. Coelostat, from L. coelo-, for caeli-, combination form of coelum "sky" + -stat prefix denoting something that stabilizes, keeps, fixes, from -stata, from Gk. -states "one that causes to stand," or statos "standing," from *sta- "to stand." Âsmândâštâr, from âsmân, → sky, + dâštâr "holder, maintainer," from dâštan "to hold, maintain; to have; to possess," Mid.Pers. dâštan, O.Pers./Av. root dar- "to hold, keep back, maitain, keep in mind," Skt. dhr-, dharma- "law," Gk. thronos "elevated seat, throne," L. firmus "firm, stable," Lith. daryti "to make," PIE *dher- "to hold, support." |
coerce pazuridan Fr.: contraindre, forcer 1) To compel by force, especially by law or authority. M.E., from O.Fr. cohercier, from L. coercere "to restrain, surround," form → com- "together" + arcere "to enclose, confine, keep off," from PIE *ark- "to hold, contain, guard." Pazuridan, literally "to force against," from pa- "contrary to; against; opposing," → counter- + zur "power, force," → strength, + infinitive suffix -idan. |
coercion pazureš Fr.: coercition The act, practice, or power of using physical or moral force to compel a person to do something. Verbal noun of → coerce. |
<< < -ci cal Cal can Cap car cas cat cau cel cen cen cha cha cha che Chi chr cir cir civ Cla clo clu CNO coa coe coh col col col com com com com com com com com Com con con con con con con con con con con con con Coo cor cor cor cos cos cos cou cov cra cri cro cry cum cur cyc > >>