An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 644
ethnoastronomy
  قوم‌اخترشناسی   
qowm-axtarshenâsi

Fr.: ethnologie   

The study of the beliefs, interpretations, and practices of specific cultures regarding celestial objects or phenomena. Ethnoastronomy uses the tools and methodologies of → ethnology in the study of astronomical conceptions.

ethno-; → astronomy.

ethnology
  قوم‌شناسی   
qowmšenâsi

Fr.: ethnologie   

The study of specific cultures (ethnic groups) in their different aspects (anthropological, social, cultural, etc.) to establish similarities and disparities between them.

ethno-; → logy.

ethyl
  اتیل   
etil (#)

Fr.: éthyl   

A chemical group, C2H5, produced by removing a hydrogen atom from → ethane. For example, ethyl chloride is C2H5Cl

From Ger. Ethyl, from eth-, from → ether, + -yl a suffixed used in the names of radicals.

ethyl alcohol
  اتیل الکل   
etil alkol (#)

Fr.: éthyl alcool   

Same as → ethanol.

ethyl; → alcohol.

etymology
  ریشه‌شناسی   
riše-šenâsi (#)

Fr.: étymologie   

The study of the origins and history of the form and meaning of → words.

M.E., from L. etymologia, from Gk. etymologia, from etymon "true sense" (neuter of etymos) + logos, → -logy.

Riše-šenâsi, from rišé "root" (dialectal Tabari rexa; Kurd. regez, riše), from Mid.Pers. rêšak "root," maybe ultimately related to PIE *u(e)rad-, although the Skt. offshoot is absent (Gk. rhiza "root;" L. radix, radius "staff;" O.H.G. wurz "plant, herb;" Ger. Wurz; O.E. rot; E. root) + -šenâsi, → -logy.

eu-
  هو-   
hu- (#)

Fr.: eu-   

A prefix meaning "good, well; true, genuine" (eupepsia; eukaryote); opposed to → dys-.

L. from Gk. eu "well," combining form of eus "good" (hu-gies "healthy"); cf. Mid.Pers. hu-; Av. hu- "good;" PIE base *su- "good," see below.

Mid.Pers. hu- "good, well" (hu-boy "sweet-smelling," hu-cihr "beautiful," hu-mânih "good-mindedness"); O.Pers. hu- "good, well" (ukāra- "having good people"); Av. hu-, hū- "well, good, beautiful" (hu-kərp- "well-shapen," hūxta- "well spoken," hu-manah- "good-minded"); Skt. su- "good" (svasti "well-being, good luck," sumánas- "good-minded," sūktá- "well spoken"); Gallic su-; O.S. su-; Welsh hy-; PIE base *su-, as above.

Euclidean
  اقلیدوسی   
Oqlidosi (#)

Fr.: euclidien   

Of or pertaining to Euclid, or his postulates. → Euclidean division, → Euclidean geometry, → Euclidean space, → non-Euclidean geometry.

After the Gk. geometrician and educator at Alexandria, around 300 B.C., who applied the deductive principles of logic to geometry, thereby deriving statements from clearly defined axioms.

Euclidean division
  بخش ِ اقلیدوسی   
baxš-e Oqlidosi

Fr.: division euclidienne   

In arithmetic, the conventional process of division of two → integers. For a → real number a divided by b > 0, there exists a unique integer q and a real number r, 0 ≤ r <b, such that a = qb + r.

Euclidean; → division.

Euclidean geometry
  هندسه‌ی ِ اقلیدوسی   
hendese-ye Oqlidosi (#)

Fr.: géométrie euclidienne   

The geometry based on the postulates or descriptions of Euclid. One of the critical assumptions of the Euclidean geometry is given in his fifth postulate: through a point not on a line, one and only one line be drawn parallel to the given line. See also → non-Euclidean geometry.

Euclidean; → geometry.

Euclidean space
  فضای ِ اقلیدوسی   
fazâ-ye Oqlidosi

Fr.: espace euclidean   

A space in which the → distance between any two points is given by the → Pythagorean theorem: d2 = (Δx)2 + (Δy)2 + (Δz)2, where d is distance and Δx, Δy, and Δz are differential → Cartesian coordinates. Euclidean n-space Rn is the set of all column vectors with n real entries.

Euclidean; → space.

Eudoxan spheres
  سپهرهای ِ اءودوکسوس   
sepehrhâ-ye Eudoxus

Fr.: sphères d'Eudoxe   

spheres of Eudoxus.

spheres of Eudoxus.

Euler
  اویلر   
Euler

Fr.: Euler   

Leonhard Euler (1707-1783), the eminent Swiss mathematician, physicist, and astronomer.

Euler equation
  هموگش ِ اویلر   
hamugeš-e Euler

Fr.: équation d'Euler   

In → fluid mechanics, one of a set of → differential equations that govern the motion of a → compressible, → inviscid fluid. Euler equations correspond to the → Navier-Stokes equations with zero → viscosity.

Euler; → equation.

Euler line
  خط ِ اویلر   
xatt-e Euler

Fr.: droite d'Euler   

In any → triangle, the straight line on which always lie the → centroid, → circumcenter, and → orthocenter.

Euler; → line.

Euler's broken line
  خط ِ شکسته‌ی ِ اویلر   
xatt-e šekaste-ye Euler

Fr.: ligne brisée   

The line drawn in a coordinate plane connecting the approximate values of the solution of a → first-order differential equation.

Euler; → broken line.

Euler's formula
  دیسول ِ اویلر   
disul-e Euler

Fr.: formule d'Euler   

A formula which expresses an → exponential function with an → imaginary number  → exponent in terms of → trigonometric functions:
e = cos θ + i sinθ,
e-iθ = cos θ - i sinθ,
cosθ = (e + e-iθ)/2,
sinθ = (e - e-iθ)/2i.
In the particular case of θ = π, Euler's formula becomes: eiπ + 1 = 0, which is considered by many mathematicians to be the most elegant mathematical equation. → mathematical elegance.

Euler; → formula.

Eulerian method
  روش ِ اویلری   
raveš-e Euleri

Fr.: méthode eulérienne   

Fluid mechanics: A method in which the changes in the physical properties of the fluid, such as velocity, acceleration, and density are described at a fixed point in space occupied by the fluid. Compare with → Lagrangian method.

Euler; → method.

Europa (Jupiter II)
  اءوروپا، اروپا   
Europâ, orupâ (#)

Fr.: Europe   

The sixth of → Jupiter's known moons and the fourth largest; it is the second of the → Galilean satellites. With a diameter of 3140 km, Europa is slightly smaller than Earth's Moon. Its mass is 4.80 × 1022 kg, i.e. 1.5 times less massive than Earth Moon. Its distance to Jupiter is 670,900 km, or about 9 Jovian radii. Its → orbital period is 3.55 Earth days which equals its → rotation period. Europa's density is 3.0 g cm-3, typical of a mixture of rocks including → ice. Its high → albedo (0.67) suggests that its surface is mostly → water ice. The → surface temperature of Europa ranges between about 125 K (-150 °C) at the equator and about 50 K (-220 °C) at the poles. There are few → impact craters on Europa, because its surface is too active and therefore young. The most striking features of Europa's surface are structures called → lineae and → lenticulae. The thickness of the ice crust could range between a few kilometers to a few tens of kilometers. It is now believed that there is an ocean of salty water, up to 100 km deep, flowing under Europa's ice. Europa's ocean is kept liquid due to → tidal heating by Jupiter.

In Gk. mythology, Europa was a Phoenician princess (Agenor's daughter) abducted to Crete by Zeus, who had assumed the form of a white bull, and by him the mother of Minos, Sarpedon, and Rhadamanthys.

European Southern Observatory (ESO)
  نپاهشگاه ِ اروپایی ِ دشتری   
nepâhešgâh-e orupâyi-ye daštari

Fr.: Organisation européenne pour la recherche astronomique dans l'hémisphère austral   

An major intergovernmental research organisation in astronomy supported by 14 European countries. ESO was founded in 1962 as a consortium among Belgium, Denmark, France, Germany, the Netherlands, and Sweden. The ESO Headquarters are located in Garching near Munich, Germany. The organization operates three outstanding observing sites in the Atacama Desert region of Chile: → La Silla, → Paranal, and Chajnantor. The → Very Large Telescope (VLT), the world's most advanced visible-light astronomical facility, is located on the 2600 m high mountain of Paranal, which also hosts the → VLT Interferometer (VLTI). The Chajnantor site, 5000 m above sea level, near San Pedro de Atacama, operates a submillimeter telescope (APEX). Moreover, a giant array of 12 m submillimeter antennas, called → ALMA, is being constructed in collaboration with North America, East Asia and Chile. ESO is currently planning a 42 m European Extremely Large optical/near-infrared Telescope, the → E-ELT.

European, from Europe, → Europa; → southern; → observatory.

European Space Agency (ESA)
  سازمان ِ فضایی ِ اروپا   
Sâzmân-e Fazâyi-ye Orupâ

Fr.: Agence spatiale européenne   

An intergovernmental organisation dedicated to space research and technology as well as peaceful exploration of space, founded in 1975. It is headquartered in Paris and currently comprises 18 member states and one associated state (Canada). ESA has developed the Ariane series of space launch vehicles, and supports a launch facility in French Guiana. Moreover, ESA has four major research centers: The European Space Research and Technology Center (ESTEC), located in Noordwijk, the Netherlands, is the primary research center and manages the satellite projects. The European Space Operations Center (ESOC), situated in Darmstadt, Germany, is responsible for satellite control, monitoring, and data retrieval. The European Space Research Institute (ESRIN), located in Frascati, Italy, supports the ESA documentation service and manages the data obtained from remote sensing satellites. The European Astronaut Center (EAC), located in Cologne, Germany, is responsible for the selection and training of astronauts for space station missions. The European Space Astronomy Centre (ESAC), located in Villafranca del Castillo, Madrid, Spain, which holds scientific operations centres as well as archives. Some of the past ESA missions are the following ones. The Giotto space probe, which enabled examination of the core of → Halley's Comet in 1986. ESA also developed the Ulysses spacecraft (launched 1990) to explore the Sun's polar regions. Similarly, ESA established a system of meteorological satellites known as Meteosat. In 2003 ESA launched the Mars Express orbiter and its lander, Beagle 2. In 2009 ESA launched → Planck Satellite, that is designed to study the → cosmic microwave background, and the → Herschel Satellite, an infrared observatory that is the largest telescope in space.

European, from Europe, → Europa; → space; agency, from M.L. agentia, from L. ag-, root of agere, → act + -entia noun suffix.

Sâzmân, → organization; fazâyi adj. of fazâ, → space; Orupâ, → Europa.

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