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fission theory negare-ye šekâft Fr.: théorie de fission A theory that suggests the Moon was formed at the same time as Earth. A spinning Earth ejected a large piece of its material into space which then developed into the shape and orbit of the Moon. This event was also thought to be at the origin of the Pacific Ocean. This first modern idea about the formation of the Moon is due to George Darwin, the son of the great naturalist Charles Darwin. The fission theory explained the lack of volatile substances on the Earth. The volatile materials on the Earth would have been thrown out into space The fission theory is almost completely abandoned today. The analysis of lunar rocks brought to Earth by NASA astronauts showed that the Moon rocks are older than the rocks at the bottom of the Pacific Ocean. Moreover, modern → plate tectonics gives a better explanation of the origin of the Pacific Ocean. See also → giant impact hypothesis, → capture theory, → co-formation theory. |
fissionable šekâftpazir (#) Fr.: fissile The material that can be fissioned by fast neutrons, such as uranium-238. Commonly used as a synonym for → fissile material. |
fixation barjâyeš Fr.: fixation The act of fixing or the state of being fixed. |
Flamsteed designation nâmgozini-ye Flamsteed Fr.: designation de Flamsteed A stellar designation system in which each star is assigned a number followed by the Latin genitive of its corresponding → constellation, such as → 61 Cygni and 82 Eridani. Compare with the → Bayer designation. Named after John Flamsteed (1646-1719), founder of the Greenwich Observatory, and the first astronomer royal of England, who introduced this system in his catalog Historia Coelestis Britannica (1725); → designation. |
flat rotation curve xam-e carxeš-e taxt Fr.: courbe de rotation plate A galactic → rotation curve in which the → rotation velocity is constant in the outer parts. The flat component is preceded by a rising curve that shows solid body rotation in the very center of the → galaxy. A flat rotation curve implies that the mass is still increasing linearly with radius. See also → dark matter. |
flexion cafteš Fr.: 1) The act of bending, the state of being bent. |
flotation šenâvari (#) Fr.: flottation 1) The act or state of remaining on the surface of a liquid.
→ buoyancy. From float, from M.E. floten, O.E. flotian (cf. O.N. flota, M.Du. vloten), akin to fleet + -ation. Šenâvari "flotation," from šenâvar "that swims, floats," from šenâ "swimming;" Mid.Pers. šnâz "swim," šnâzidan "to swim;" Av. snā- "to wash, swim;" cf. Skt. snā- "to bathe, to wash;" L. nare, natare "to swim" (Fr. nage, nager, natation; Sp.nadar, natacion). |
fluctuation oftâxiz (#) Fr.: fluctuation Continual rise and fall. Verbal noun of → fluctuate. Oftâxiz "fall and rise," from oft "fall" stem of oftâdan "to fall" (Mid.Pers. opastan "to fall," patet "falls;" Av. pat- " to fly, fall, rush," patarəta- "winged;" cf. Skt. patati "he flies, falls," pátra- "wing, feather, leaf;" Gk. piptein "to fall," pterux "wing;" L. penna "feather, wing;" O.E. feðer "feather;" PIE base *pet- "to fly, rush") + -â- interfix + xiz present stem of xâstan, xizidan "to rise, get up" (Mid.Pers. xyz- "to stand up, rise;" Proto-Iranian *xiz- "to rise, ascend; increase"). |
flux calibration kabizeš-e šârr Fr.: calibration de flux The → calibration of the flux received by a detector in terms of absolute units. → flux; → calibration. |
fluxion fluksion Fr.: fluxion In Newton's work on → calculus, the rate of change of a fluent (i.e. a flowing quantity), today commonly known as → variable. For a fluent x, the fluxion is denoted dx/dt. An obsolete mathematical term. |
Fokker-Planck equation hamugeš-e Fokker-Planck Fr.: équation de Fokker-Planck A modified form of → Boltzmann's equation allowing for collision terms in an approximate way. It describes the rate of change of a particle's velocity as a result of small-angle collisional deflections. After Dutch physicist Adriaan Fokker (1887-1972) and the German physicist Max Planck (1858-1947); → equation. |
follow-up observation nepâheš-e peygir Fr.: An observation which expands previous observations and aims at obtaining complementary data in particular with other telescopes/instruments. Follow-up, from follow, from O.E. folgian, fylgan "to follow, pursue," from W.Gmc. *fulg- (cf. O.Fris. folgia, M.Du. volghen, Ger. folgen "to follow") + up, O.E. up, uppe (cf. Du. op, Ger. auf "up, upward"), from PIE base *upo "up from below;" cf. O.Pers./Av. upā; Skt. úpa; Gk. hypo; L. sub, → hypo-; → observation. Nepâheš, → observation; peygir, from pey "after; step," related to pâ "foot, step, track," → foot, + gir present stem of gereftan "to take, seize" (Mid.Pers. griftan, Av./O.Pers. grab- "to take, seize," cf. Skt. grah-, grabh- "to seize, take," graha "seizing, holding, perceiving," M.L.G. grabben "to grab," from P.Gmc. *grab, E. grab "to take or grasp suddenly;" PIE base *ghrebh- "to seize"). |
forbidden emission line xat-e gosili-ye bažkam Fr.: raie d'émission interdite A → forbidden line in → emission. |
forbidden transition gozareš-e bažkam Fr.: transition interdite A transition between two quantum mechanical → states that → violates the quantum mechanical → selection rules. → forbidden; → transition. |
forced oscillation naveš-e zuri Fr.: oscillation forcée The oscillation of a system or object induced by an external periodic force. See also → free oscillation. → forced; → oscillation. |
foreground absorption daršam-e pišzaminé Fr.: absorption d'avant-plan Loss of radiant energy received from an astronomical object due to the presence of absorbing matter situated between the object and observer. → foreground; → absorption. |
formalization disevareš Fr.: formalisation 1) The act of giving something a form or structure by introducing rules
and procedures. |
formation diseš Fr.: formation 1) The act or process of forming or the state of being formed, such as
→ star formation. Verbal noun of → form, + -ate + -ion. Diseš, verbal noun of disidan, → from dis-, → form, + -eš. |
formulation disuleš Fr.: formulation 1) The act or process of formulating. |
four-dimensional operator âpârgar-e cahâr-vâmuni Fr.: opérateur à quatre dimensions An operator defined as: ▫ = (∂/∂x, ∂/∂y, ∂/∂z, 1/(jc∂/∂t). → four; → dimensional; → operator. |
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