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Cartwheel Galaxy kahkašân-e carx-e arrâbé Fr.: galaxie de la roue de charette A galaxy with a striking ring-like feature lying about 400 million → light-years away in the → constellation → Sculptor. The ring-like structure, over 100,000 light-years in diameter, is composed of regions of → star formation filled with very bright, → massive stars. The shape results from collision with another smaller galaxy. Cartwheel, from cart from O.N. kartr; → wheel; → galaxy. Kahkašân, → galaxy. Carx-e arrâbé "cartwheel," from carx, → wheel + arrâbé "cart, chariot," maybe related to Mid.Pers. ras, ray "wheel," O.Pers./Av. raθa- "wheel," Khotanese rrha- "car," Skt. ratha- "wheel," L. rota "wheel," PIE base *rotos "wheel." |
charged particle zarre-ye bârdâr (#) Fr.: particule chargée Any particle containing either a → positive or → negative → electric charge. |
counterpart hamtâ (#) Fr.: contrpartie A person or thing that corresponds to or has the same function as another
person or thing in a different place or situation (OxfordDictionaries.com). M.E., from O.Fr. contrepartie, from contre "facing, opposite," → counter-, + partie "copy of a person or thing," originally feminine p.p. of partir "to divide." Hamtâ "counterpart, resembling, equal," from ham- "together, with; same, equally, even," → com-, + tâ "fold, plait, ply; piece, part," also a multiplicative suffix; Mid.Pers. tâg "piece, part." |
Descartes Descartes Fr.: Descartes René Descartes (1596-1650), French mathematician, physicist, and philosopher, who made valuable contributions to mathematics, physics, and philosophy. Descartes was a pioneer and major figure in 17th century rationalism. He represents a major break with the Aristotelianism and Scholasticism of the Medieval period. René Descartes is regarded as the father of modern philosophy. → Descartes ray, → Cartesian coordinates, → Cartesian vortex theory. |
Descartes ray partow-e Descartes Fr.: rayon de Descartes Same as → rainbow ray. |
Descartes' formula disul-e Descartes Fr.: formule de Descartes A formula that gives the position of an image formed by highly → paraxial rays from a → spherical mirror. It is quite accurately given by: 1/xo + 1/xi = 2/xC, where xo is the distance along the → principal axis from the mirror to the object, xi is the distance from mirror to image, and xC is the distance from the mirror to its center of curvature. Any distance measured on the same side of the mirror as the reflecting surface is positive; on the other side, negative. Thus for a → concave mirror xC is positive; for a → convex mirror, negative. |
disk partition parkeš-e disk, ~ gerde Fr.: partition de disque A logical division of a hard disk that is treated as a separate unit by operating systems and file systems. |
Earth zamin (#) Fr.: terre The third planet from the Sun. At → perihelion, it is 147,099,590 km
from the Sun, and at → aphelion it is 152,096.150 km, whereas its
mean distance from the Sun (→ astronomical unit) is
149,598 × 106 km.
Its orbital period is 365.2563 days (→ sidereal year)
and its → eccentricity 0.017. Other characteristics:
→ axial inclination 23.44°; rotation period 23.934 h
(→ sidereal day); mean density 5.52 g/cm3;
mass 5.974 × 1024 kg; → escape velocity 11.18 km/s; average
→ albedo 0.37. M.E. erthe, from O.E. eorðe "ground, soil, dry land;" cf. O.N. jörð, M.Du. eerde, O.H.G. erda, Goth. airþa; from PIE base *er-. Zamin, variant zami "earth, floor, land," Mid.Pers. zamig, Av. zam- "the earth;" cf. Skt. ksam- "the ground, earth;" Gk. khthôn, khamai "on the ground;" L. homo "earthly being" (as in homo sapiens, homicide, humble, humus, exhume), humus "the earth;" O.Russ. zemi "land, earth;" PIE root *dh(e)ghom "earth". |
Earth mass jerm-e zamin (#) Fr.: masse de la Terre The mass of our planet Earth, which is 5.9736 × 1024 kg (3 × 10-6 → solar masses), 317.83 times smaller than the → Jupiter mass. The Earth mass is in particular used to describe the mass of → super-Earth → extrasolar planets. |
Earth radius šo'â'-e zamin (#) Fr.: rayon terrestre The distance from the Earth's center to its surface, about 6,371 km. |
Earth's core maqze-ye Zamin Fr.: noyau terrestre The innermost part of the Earth consisting of a solid → inner core, mainly composed of → iron, and a → liquid → outer core. The → pressure and → temperature are so extreme that the molten iron solidifies. The temperature at the inner core boundary is expected to be close to the → melting point of iron at 330 gigapascal (GPa). From static laser-heated diamond anvil cell experiments up to 200 GPa, using synchrotron-based fast → X-ray diffraction as a primary melting diagnostic, S. Anzellini et al. (2013, Science 340, 484) conclude that the melting temperature of iron at the inner core boundary is 6230 ± 500 K. This estimation favors a high heat flux at the core-mantle boundary with a possible partial melting of the → mantle. The inner core, 2,400 km in diameter, is suspended in the molten metal of the → outer core, which is about 2,240 km thick. The temperature difference between the mantle and the core is the main engine for large-scale thermal movements, which coupled with the → Earth's rotation, function as a generator for the planet's → magnetic field. |
Earth's crust puste-ye Zamin (#) Fr.: croûte terrestre The rocky outermost layer of the Earth, ranging from about 10 to 65 km in thickness. It is distinguished from the underlying the → Earth's mantle layer by its more → silicon- and → aluminium-rich composition, lower density, and the lower velocity at which it conducts seismic energy. It includes → continental crust (about 40 km thick) and → oceanic crust (about 7 km thick). The crust and the topmost layer of the mantle form the → lithosphere. The five most abundant → chemical elements in the Earth's crust are, in percentage by weight of the Earth's crust: → oxygen (O) 46%, silicon (Si) 28%, aluminium (Al) 8%, → iron (Fe) 5%, and → calcium (Ca) 4%. |
Earth's mantle gušte-ye Zamin Fr.: manteau terrestre A major subdivision of Earth's internal structure, located beneath the → Earth's crust and above the central → core. On average, the mantle begins 35 km below the surface and ends at a depth of about 2,900 km. See also → upper mantle and → lower mantle, → asthenosphere, → lithosphere. |
Earth's rotation carxeš-e zamin (#) Fr.: rotation de la Terre The natural motion of the Earth around its own axis, which takes place once in a → sidereal day. The Earth rotates toward the → east, in the same direction as it revolves around the Sun. If viewed from the north celestial pole, the Earth turns → counterclockwise. The opposite is true when the Earth is viewed from the south celestial pole. The Earth's rotation is responsible for the diurnal cycles of day and night, and also causes the apparent movement of the Sun across the sky. The Earth's rotation velocity at the → equator is 1,673 km h-1 or about 465 m s-1. More generally, at the → latitude φ it is given by: vφ = veq cos φ, where veq is the rotation velocity at the equator. The Earth's rotation is gradually slowing down under the action of the → tides, which are generated by the → gravitational attraction of the → Moon. As the result of this → tidal friction, the day is becoming longer at a rate of about 2 milliseconds, or 0.002 seconds, per century (or one second every 50,000 years). Moreover, the loss of the Earth's → rotational angular momentum increases the Moon's → orbital angular momentum, because the angular momentum of the → Earth-Moon system is conserved. In consequence, the Moon slowly recedes from the Earth by about 4 cm per year, which leads to increasing its orbital period and the length of a month as well. |
earth-grazer zamin-barmaž Fr.: astéroide croiseur, comète ~ An → asteroid or → comet whose → orbit occasionally brings it relatively close to the Earth. → near-Earth object. |
Earth-Moon system râžmân-e Zamin-Mâh Fr.: système Terre-Lune A physical system composed on the → Earth and the
→ Moon in which both objects directly influence each other.
The total energy in the Earth-Moon system is conserved.
The most notable influence that the two objects have on each other is
→ tides. |
earthlight zamin-tâb (#) Fr.: lumière cendrée The illumination of the dark part of the Moon's disk by the light reflected from the Earth's surface and atmosphere. Also called → earthshine. |
earthquake zaminlarzé (#) Fr.: tremblement de terre Sudden shaking of the → Earth's surface caused by the passage of a → seismic wave whose mechanical effects can be destructive. See also → starquake. |
earthshine zamin-tâb (#) Fr.: lumière cendrée The visibility of that part of the Moon not illuminated by the Sun. The phenomenon is caused by the solar light reflected by the Earth. It was explained correctly for the first time by Leonardo da Vinci (M.S.: SDE). Same as → earthlight. |
electromagnetic counterpart hamtâ-ye barqâmeqnâti Fr.: contrpartie électromagnétique An → electromagnetic signal associated with the location on the sky and the time of a → gravitational wave event. The electromagnetic signal is predicted by models to be associated with the → merger of a → compact binary star system composed of two → neutron stars (NS) or a neutron star and a → black hole (BH). Accordingly, the gravitational waves are accompanied by a short-duration → gamma-ray burst (GRB) powered by the → accretion of material that remains in a → centrifugally supported → torus around the BH following the merger. NS-NS/BH-NS mergers are also predicted to be accompanied by a more isotropic counterpart, commonly known as a → kilonova. Kilonovae are day to week-long thermal, → supernova-like → transients, and are powered by the → radioactive decay of heavy, neutron-rich elements synthesized by the → r-process in the expanding merger ejecta (Li and Paczynski 1998). The first detection of an electromagnetic counterpart to gravitational waves belongs to → GW170817. → electromagnetic; → counterpart. |
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