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ore kâné (#) Fr.: minerai A natural deposit containing a mineral of an element to be extracted. Ore, merger of M.E. ore, O.E. ora "ore, unworked metal" and M.E. or(e) "ore, metal," O.E. ar "brass, copper, bronze" (cf. O.N. eir "brass, copper;" Ger. ehern "brazen;" Erz "oar;" Goth. aiz "bronze;" O.H.G. ēr "ore"), from PIE *aus- "gold;" cf. Mod/Mid..Pers. âhan "iron;" Av. aiianhaēna- "made of metal," from aiiah- "metal;" Skt. áyas- "iron, metal;" L. aes "brass" Kâné, from kân "mine," from kandan "to dig" (Mid.Pers. kandan "to dig;" O.Pers. kan- "to dig," akaniya- "it was dug;" Av. kan- "to dig," uskən- "to dig out" (→ ex- for prefix us-); cf. Skt. khan- "to dig," khanati "he digs"). |
Orion correlation theory negare-ye hambâzâneš-e Oryon Fr.: théorie de la corrélation d'Orion A controversial proposition according to which a coincidence would exist between the mutual positions of the three stars of → Orion's Belt and those of the main Giza pyramids. More specifically, Khufu, Khafre, and Menkaure would be the monumental representation of → Alnitak, → Alnilam, and → Mintaka, respectively. → Orion; → correlation; → theory. |
orrery oreri Fr.: planétaire A mechanical device that illustrates the relative positions and motions of the planets and moons in the solar system in heliocentric model. Named after Charles Boyle, 4th Earl of Orrery (1676-1731), for whom the device was first made. |
oscillator strength zur-e navešgar Fr.: force d'oscillateur A quantum-mechanical measure of the probability that a specific atomic transition will occur. It is used in the equation for the absorption coefficient of a spectral line. Also known as f value. → oscillator; → strength. |
osculating sphere sepehr-e âbusandé, kore-ye ~ Fr.: sphère osculatrice For a curve C at a point p, the limiting sphere obtained by taking the sphere that passes through p and three other points on C and then letting these three points approach p independently along C. → osculating; → sphere. |
OSIRIS-REx OSIRIS-REx Fr.: OSIRIS-REx A → spacecraft whose goal is to collect a sample from the asteroid → 101955 Bennu and bring it back to Earth. It was launched by → NASA on September 8, 2016. OSIRIS-REx will spend two years chasing Bennu down, finally rendezvousing with the → near-Earth asteroid in August 2018. The spacecraft will then study the → asteroid Bennu from orbit for another two years before grabbing at least 60 grams of surface material in July 2020. The sample should reach Earth in 2023. The analysis of the sample would allow to study the role that → B-type asteroids like Bennu, which are primitive and apparently carbon-rich, may have played in helping life appear on Earth. The name is short for Origins, Spectral Interpretation, Resource Identification, Security, Regolith Explorer . |
osmotic pressure fešâr-e tarârâni Fr.: pression osmotique The hydrostatic pressure produced on the surface of a partially permeable membrane by osmosis. |
outer core maqze-ye biruni Fr.: noyau externe The upper zone of the → Earth's core, just below the → mantle, extending from a depth of about 2900 km to 5100 km. It is presumed to be → liquid because it sharply reduces → compressional wave velocities and does not transmit → shear waves. Its density is from 9 to 11 g/cm3. The → temperature ranges from 4400 °C in the outer areas to 6100 °C near the → inner core. Since shear waves do not propagate through a fluid, the Earth's outer core is considered to be liquid because the shear wave velocity is zero. Convection motion within the outer core, along with the rotation of the Earth creates an effect that maintains the Earth's → magnetic field. |
outer Lindblad resonance (OLP) bâzâvâyi-ye Lindblad-e boruni Fr.: résonance de Lindblad externe A → Lindblad resonance expressed by: Ωp = Ω + κ/m. → outer; → Lindblad resonance. |
outreach borun-rasâni, hame-âmuzi Fr.: éducation grand public The act of extending research activities beyond its current or conventional limits to a wide section of the population for educational purposes. → out; reach, M.E. rechen, O.E. ræcan "to extend, hold forth;" cf. O.Fris. reka, M.Du. reiken; cognate with Pers. râst, → right. Borun-rasâni, from borun, → out, +
rasâni verbal noun of rasândan "to carry, guide, send," transitive
of rasidan "to reach, arrive," → access. |
over-exposure bišnurdâd Fr.: surexposition Excessive exposure of a detector, → over-expose. |
overestimate biš-barâvardan; 2) biš-barâvard Fr.: 1) surestimer; 2) surestimation 1) To estimate at too high a value, amount, rate, or the like. |
parallel axis theorem farbin-e âsehâ-ye parâsu Fr.: théorème des axes parallèles The → moment of inertia of a body about any given axis is the moment of inertia about a parallel axis through the center of mass, plus the moment of inertia about the given axis if the mass were located at the center of mass. same as → Steiner's theorem. |
Parenago catalog kâlâlog-e Parenago Fr.: catalogue de Parenago A catalog of stars in the → Orion Nebula created by P. P. Parenago in 1954 (Publ. Astr. Inst. Sternberg, Band 25, p. 393-437, Moskau). Pavel Petrovich Parenago (1906-1960), a Soviet astronomer. |
parent permâr Fr.: parent 1) General: A father or a mother. A precursor, or
→ progenitor. From O.Fr. parent, from L. parentem (nominative parens) "father or mother, ancestor," from parere "to bring forth, give birth to, produce," from PIE base *per- "to bring forth" Permâr, literally "father-mother" (as in Sogd. māt-pitri "parent"), from Gilaki per, → father, + Gilaki mâr, → mother. |
parent cloud abr-e permâr Fr.: nuage parent Usually of a newborn star, the molecular cloud in which the star has formed. |
parent element bonpâr-e permâr Fr.: élément parent A radioactive element that spontaneously decays into a new substance. The product of this decay is known as a "daughter" element. |
parent galaxy kahkešân-e permâr Fr.: galaxie parente Of a high redshift supernova, the galaxy in which the event has occurred. |
parent molecule molekul-e permâr Fr.: molécule parente The molecule initially produced when a comet nucleus sublimates, soon changed to different daughter molecules because of solar radiation. |
Parkes Selected Region (PSR) nâhiye-ye gozide-ye Parkes Fr.: Région sélectionnée de Parkes A catalog of 397 radio sources between declinations +20° and +27° which were compiled from a finding survey made at 635 MHz with the 64m radio telescope at the Australian National Radio Astronomy Observatory, Parkes, N.S.W. and published in 1968. Originally abbreviated PSR, this catalog, which is also called PKS, replaces and improves on four earlier lists (1964 to 1966). |
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