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hydrocarbon hidrokarbon (#) Fr.: hydrocarbure Any of a class of compounds containing only → hydrogen and → carbon. Hydrocarbons are organic compounds found in coal, petroleum, natural gas, and plant life. They are used as fuels, solvents, and as raw materials for numerous products such as dyes, pesticides, and plastics. Petroleum is a mixture of several hydrocarbons. |
hydrodynamic equation hamugeš-e hirdrotavânik Fr.: équation hydrodynamique Fluid mechanics: A → partial differential equation which describes the motion of an element of fluid subjected to different forces such as pressure, gravity, and frictions. → hydrodynamic; → equation. |
hydrogen bond band-e hidroženi Fr.: liaison hydrogène The attractive force between the hydrogen attached to an electronegative atom of one molecule and an electronegative atom of a different molecule. Usually the electronegative atom is oxygen, nitrogen, or fluorine, which has a partial negative charge. The hydrogen then has the partial positive charge. |
hydrogen fusion iveš-e hidrožen Fr.: fusion de l'hydrogène A → nuclear reaction where hydrogen (H) nuclei combine to form helium (4He) nuclei. Same as the → proton-proton chain. |
hydrogen ion hidron, yon-e hidrož Fr.: hydron, ion hydrogène Chemistry: The → positively charged hydrogen atom, H+, formed by removal of the orbital electron. Same as → proton. |
hydrogenation hidroženeš Fr.: hydrogénisation The process of combining or exposing to → hydrogen. |
hydron hidron (#) Fr.: hydron The general name for the atomic hydrogen → cation H+. |
hydronium hidroniom Fr.: hydronium A → water, → molecule with an additional hydrogen ion (H3O+). Also called hydronium ion. Hydronium is an abundant molecular ion in the interstellar diffuse and dense molecular clouds (→ Sagittarius B2, → Orion molecular cloud OMC-1) as well as the plasma tails of → comets (→ Halley, → Hale-Bopp). From hydr-, → hydro- + -onium a suffix used in the names of complex cations, extrcated from ammonium "ionized ammonia" (NH4+). |
hydrostatic equation hamugeš-e hidristâik Fr.: équation hydrostatique The equation describing the → hydrostatic equilibrium in a star, expressed as: dP/dr = -GMρ/r2, where P and M are the mass and pressure of a spherical shell with thickness dr at some distance r around the center of the star, ρ is the density of the gas, and G the → gravitational constant. → hydrostatic; → equation. |
hyperbolic function karyâ-ye hozluli Fr.: fonction hyperbolique Any of the six functions sinh, cosh, tanh, coth, csch, and sech that are related to the → hyperbola in the same way the → trigonometric functions relate to the → circle. Many of the formulae satisfied by the hyperbolic functions are similar to corresponding formulae for the trigonometric functions, except for + and - signs. For example: cosh2x - sinh2x = 1. See also: → hyperbolic cosine, → hyperbolic sine. Hyperbolic functions were first introduced by the Swiss mathematician Johann Heinrich Lambert (1728-1777). → hyperbolic; → function. |
hyperfine transition gozareš-e abar-nâzok Fr.: transition hyperfine An → atomic transition involving a → hyperfine structure. → hyperfine; → transition. |
Hyperion (Saturn VII) Huperion (#) Fr.: Hypérion The sixteenth of → Saturn's known → natural satellites. It is shaped like a potato with dimensions of 410 x 260 x 220 km and has a bizarre porous, sponge-like appearance. Many of the sponge holes or craters have bright walls, which suggests an abundance of → water → ice. The crater floors are mostly the areas of the lowest → albedo and greatest red coloration. This may be because the average temperature of roughly -180 °C might be close enough to a temperature that would cause → volatiles to → sublimate, leaving the darker materials accumulated on the crater floors. Hyperion is one of the largest bodies in the → Solar System known to be so irregular. Its density is so low that it might house a vast system of caverns inside. Hyperion rotates chaotically and revolves around Saturn at a mean distance of 1,481,100 km. It was discovered by two astronomers independently in 1848, the American William C. Bond (1789-1859) and the British William Lassell (1799-1880). Hyperion, in Gk. mythology was the Titan god of light, one of the sons of Ouranos (Heaven) and Gaia (Earth), and the father of the lights of heaven, Eos the Dawn, Helios the Sun, and Selene the Moon. |
hyperon hiperon (#) Fr.: hypéron An unstable elementary particles, belonging to the class called → baryons, which have greater mass than the neutron but very short lives (10-8 to 10-10 seconds). From → hyper- + → -on a suffix used in the names of elementary particles (gluon; meson; neutron; graviton, and so on). |
hypersonic hipersedâyi Fr.: hypersonique In aerodynamics, adjective used to describe a → sound speed in excess of Mach 5. See also → supersonic. |
ice accretion farbâl-e yax Fr.: accrétion de glace Meteo.: The process by which a layer of ice builds up on solid objects that are exposed to freezing precipitation or to supercooled fog or cloud droplets. |
icon zodiš Fr.: icone 1) An image; a representation. From Gk. eikon "likeness, image, portrait; a semblance;" in philosophy, "an image in the mind," related to eikenai "be like, look like," from PIE *weik- "to be like." Zodiš, variant of Mid.Pers. uzdês "icon; image; idol," from uz-, → ex-, + dês, Av. daēs- "to show;" cognate with Gk. deiknumai "to show;" L. dicere "to utter, say, proclaim;" N.H.G. zeigen "to say;" O.E. têon "to annoince;" PIE *deik- "to show, point out; announce." |
identification idâneš Fr.: identification 1) An act or instance of identifying; the state of being identified. Verbal noun of → identify. Idâneš, verbal noun of idânidan→ identify. |
identification of lines idâneš-e xatthâ Fr.: identification de raies Recognizing the lines in the spectrum of a star, nebula, galaxy, etc. using a calibration template. → identification; → line. |
identity function karyâ-ye idâni Fr.: fonction d'identité Math.: Any function f for which f(x) = x for all x in the domain of definition. |
if and only if (iff) agar va ivâz agar, ~ ~ tanhâ ~ Fr.: si et seulement si Logic, Math.: An → expression indicating that two → statements so connected are → necessary and sufficient conditions for one another. The corresponding logical symbols usually used are: ↔, ⇔, ≡, and iff. |
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