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chalcophile xâlkdust, mesdust Fr.: élémznt chalcophilz |
chalcophile element bonpâr-e xâlkdust, ~ mesdust Fr.: élément chalcophile In the → Goldschmidt classification, a → chemical element that has an → affinity for sulphur, and therefore tending to be more abundant in sulphide minerals and ores than in other types of rock. This group is depleted in the silicate Earth and may be concentrated in the core. The group includes → silver (Ag), → arsenic (As), → bismuth (Bi), → cadmium (Cd), → copper (Cu), → mercury (Hg), → indium (In), → lead (Pb), → sulfur (S), → antimony (Sb), → selenium (Se), → tellurium (Te), and → thallium (Tl). As a consequence of their relatively low condensation temperatures (500-1100 K), most of these elements are depleted in terrestrial planets with respect to chondrites. → chalcophile; → element. |
Chamaeleon Âftâbparast (#) Fr.: Caméléon The Chameleon. A small inconspicuous → constellation in the southern hemisphere near → Crux, lying at approximate position: R.A. 11 h, Dec. -80°. Abbreviation: Cha; genitive form: Chamaeleonis; From O.Fr. chaméléon, from L. chamaeleon, from Gk. khamaileon, from khamai "on the ground" (akin to chthon "earth;" cf. Av. zam- "the earth," Mid.Pers. zamig, Mod.Pers. zami, zamin "the earth," Skt. ksam, L. homo "earthly being" and humus "the earth," PIE *dh(e)ghom "earth") + leon "lion." Âftâbparast "chameleon," literally "sun adorer," from âftâb "Sun, sunlight" + parast "worshipper," |
chamber otâqak (#) Fr.: chambre An enclosed space making part of a laboratory apparatus, such as → bubble chamber, → cloud chamber, → multiwire proportional chamber. M.E., from O.Fr. chambre, from L.L. camera "a chamber, room." Otâqak "small room, small chamber," cf. Sogdian ôtâk "place, region," ôtâkcik "local, regional, native" + -ak diminutive suffix. |
champagne effect oskar-e šâmpâyn Fr.: effet champagne Blowing out of → ionized gas from a → molecular cloud when the → ionization front of an → H II region created by an → embedded → massive star arrives at the molecular cloud edge. The large → pressure gradient set up between the H II region and the → interstellar medium ejects the ionized material with velocities larger than 30 km/s, in a way comparable to champagne flowing out of a bottle. From a hydrodynamical model first proposed by Guillermo Tenorio-Tagle (1979). Champagne, Fr., short for vin de Champagne "wine from Champagne," a historical region at northeast France, from L.L. campania "flat open country," from L. campus "field;" → effect. |
champagne flow tacân-e šâmpâyn Fr.: flot champagne The flow of → ionized gas escaping from a → molecular cloud due to the → champagne effect. → flow. |
Chandler wobble palâpel-e Candler Fr.: mouvement de Chandler Small-scale variations in the position of the Earth's geographical poles within an irregular circle of 3 to 15 metres in diameter. It seems to result from two nearly circular components, a seasonal variation in the mass distribution on the Earth (ice, snow, atmosphere) and movements of matter within the Earth. Named after Seth Carlo Chandler (1846-1913), the American astronomer who discovered the phenomenon; → wobble. |
Chandra X-ray Observatory nepâhešgâh-e partowhâ-ye X-e Chandra Fr.: Observatoire des rayons X Chandra An astronomy satellite launched by NASA in 1999 July, specially designed to detect X-ray emission from very hot regions of the Universe such as exploded stars, clusters of galaxies, and matter around black holes. Chandra carries a high resolution mirror (aperture 1.2 m, focal length 10 m), two imaging detectors (HRC and ACIS), and two sets of transmission grating spectrometer (LETG and HETG). Important Chandra features are: an order of magnitude improvement in spatial resolution, good sensitivity from 0.1 to 10 keV, and the capability for high spectral resolution observations over most of this range. Chandra was initially given an expected lifetime of 5 years, but on 4 September 2001 NASA extended its lifetime to 10 years "based on the observatory's outstanding results." Among the results obtained using Chandra one can mention the spectacular image of the → supernova remnant Cassiopeia A. See also → X-ray astronomy. Initially called Advanced X-ray Astrophysics Facility (AXAF), the satellite was renamed the Chandra X-ray Observatory in honor of Subrahmanyan Chandrasekhar, the 1983 Nobel Prize in Physics, → Chandrasekhar limit. Moreover, Chandra, or candra- means "moon" or "shining" in Skt., from cand- "to give light, shine;" cf. Gk. kandaros "coal;" L. candela "a light, torch," from candere "to shine;" → X-ray; → Observatory. |
Chandrasekhar limit hadd-e Chandrasekhar (#) Fr.: limite de Chandrasekhar A limiting mass of about 1.44 Solar masses that the theory predicts a non-rotating → white dwarf can attain without collapsing to become a → neutron star or a → black hole. Over this → critical mass, the degeneracy pressure will be unable to bear the load of the bulk mass. Named after Subrahmayan Chandrasekhar (1910-1995), Indian-born American astrophysicist who, with William A. Fowler, won the 1983 Nobel Prize for Physics for his research on white dwarfs; → limit. |
change 1) galnidan; 2) galnândan; 3) âlešidan; 4)
galn, galne Fr.: 1, 2) changer; 3) changement 1) (v.intr.) To undergo change. M.E., from O.Fr. changier, from L.L. cambiare, from L. cambire "to exchange, barter," of Celtic origin, cf. Breton kamm "curved, bent;" Gk. kampe "a corner, a joint;" L. campus "a field;" Lith. kampus "corner;" PIE *kamb- "to bend, crook." Galnidan, variant of gardidan, gaštan "to change, to turn," → Universe, cf. Awromani gelnây, geln- "to turn over" (Cheung 2007). |
chaos 1) varšun; 2) šivâr Fr.: chaos 1a) General: A condition or place of great disorder or confusion. Chaos, in Gk. mythology and cosmology, the void existing at the beginning of
the creation, as evoked in Hesiod's (c. 850 B.C.) Theogony.
However, the meaning of chaos, used by Hesiod, is a matter of debate.
Some have interpreted it as the primeval absence of order (hence
→ confusion). Subsequently, the Roman
writer Ovid (43 BC-17? AD) described Chaos in his Metamorphoses
as an unordered and formless primordial mass, and opposed
Chaos to Cosmos "the ordered universe."
1) Varšun, from Tabari varâšun, Gilaki varâšin,
daršin, uršin all meaning "confused, unordered, untidy,"
cf. Qomi šur-o-šin "chaos, confusion". The stem
šun-/šin- is related to Mod.Pers. šân- in
afšândan, šândan "to disperse, scatter, stew"
(Mid.Pers. afšândan "to spread, scatter"), Gilaki šondan
"to disperse," Hamadani šuândan "to derange, disorder,"
Laki veršânâ "to disperse, scatter," Šuštari
šayn "to shake, agitate,"
Kermâni owšin "a winnowing fork to separate chaff from the grain,"
Laki šovâné "scattered household furniture," Tabari timšan
"sowing seeds;" all ultimately from Proto-Ir. *šan- "to shake;" see also
→ confuse.
The prefix var-, variant bar- "up, over"
(as well as dar- "in"), denotes "disorder, confusion"
as in darham barham "upside-down, helter-skelter". |
chaos theory negare-ye varšun Fr.: théorie du chaos The theory of unpredictable behavior that can arise in systems obeying deterministic scientific laws. |
chaotic varšungin, varšunnâk Fr.: chaotique Or, or relating to → chaos. Chaotic, adj. from → chaos. |
chaotic behavior raftâr-e varšungin Fr.: comportement chaotique The behavior of a → chaotic system. |
chaotic system râžmân-e varšungin Fr.: système chaotique A system that is → deterministic through → description by mathematical rules but can evolve highly → nonlinearly depending on → initial conditions. See also → chaos. |
chaoticity varšungini Fr.: chaoticité The condition of being → chaotic. |
Chaplygin gas gâz-e Chaplygin Fr.: gaz de Tchaplyguin In → dark energy models, a hypothetical fluid that can lead to cosmic acceleration at late times. In its simplest form, the Chaplygin gas has the → equation of statep = - A/ρ, where p and ρ denote the → pressure and → energy density, respectively, and A is a positive model parameter. This equation was introduced by Chaplygin (1904, Sci. Mem. Moscow Univ. Math., 21) to study the lifting force on a plane wing in aerodynamics. Named after Sergey Chaplygin (1869-1942), Russian physicist; → gas. |
Chappuis band bând-e Chappuis Fr.: bande de Chappuis A band in the → absorption spectrum of → ozone (O3) extending in the → visible from 400 nm to 700 nm. → Hartley band, → Huggins band. J. Chappuis, Acad. Sci., Paris, C. R. 91, 985 (1880). |
character 1) serešt (#), sereštâr; 2) sereštâr; 3) daxšé (#) Fr.: 1, 3) caractère; 2) personnage 1a) The aggregate of features and traits that form the individual nature of some person
or thing. M.E. carecter "distinctive mark," from O.Fr. caractère, from L. character, from Gk. kharakter "graving tool, its mark," from kharassein "to engrave," from kharax "pointed stick." 1, 2) Serešt "nature, temperament, constitution; mixed,"
sereštan "to mix, mingle; knead;" serišom "glue;"
Mid.Pers. srištan "to mix, knead;" cf. Av. ham-sriš-
"to put together;" Skt. śres- "to cling, stick, be attached;"
Proto-Ir. root *sraiš- "to put together, attach" (Cheung 2007). |
characteristic 1) serežtâr; 2) serežtâri Fr.: caractéristique 1a ) A distinguishing feature or quality. |
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