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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer aga air Alf Alg alk Alp alt alu amm ana And ang ani ano ant ant Ap apo app app Aqu Arc arg arr asc ass ast ast asy atm ato att aur aut axi B-m bad Bal bar bar Bay Bed ber Bet bif bim bin bio bis bla ble blu Bod Bol bor bou Bra Bre bro bul C-t Cal Cam can car Car Cas cat cav cel cen cer Cha cha Cha che chl Cir cir cir Cla cli clo clu co- cod coh col col col com com com com com com com com Com con con con con con con con con con con con con coo cor Cor cor cos cos cos Cou cou cra Cre cro Cru cub cur cyc cyl dar dat daw de- Deb dec dec dee def deg del Den dep der det deu dew dic dif dif dil dip dir dis dis dis dis dis diu dog Dop dou dra dua dus dwa dyn E r Ear ech eco edi eig Ein ela ele ele ele ele elo emi emp end enh ent epi equ equ erg est ety eur evo exa exc Exe exo exp exp ext ext eye fac fal Far fed Fer fer fie fin fir fit fla flo flu fol for for Fou fra fre Fre fro fuz gai Gal Gal gam gas Gau gen gen geo geo geo gia glo gol gra gra gra gra gre gri gui H I hai Ham har Hau hea hec hel hel her HES hie hig his hom hor hot Hub Hug hur hyd hyd hyl hyp ice ide ima ima imp imp inc ind ind ine inf inf inf ing inn ins ins int int int int int int int int inv Io ion iro isl iso iso Jac jet jud jur kel Kep kil kit kry Lag lam lan Lar lat law lea lem lep Li lig lim lin lin lin lit loc loc lon Lor low lum lun Lup Lym mac mag mag mag mag mag mai man Mar mas mas mat max mea mec meg men mer met met met mic mic Mik min min mis mne mod mol mon moo Mou mul mul myo nak Nas nat neb neg neu neu New New nit noi non non non Nor nuc nuc nul nut obe obl obs occ oct off Olb one ope opp opt opt orb orb org Ori ort oth out ove P C pal par par par par Pas pat pec peo per per per per per Pha pha pho pho pho phy pil pla Pla pla pla pla plu poi pol pol pol pol por pos pot Poy pre pre pre pre pri pri pri pro pro pro pro Pro pro Pru pul pul Pyt qua qua qua qua quo rad rad rad rad rad rad ram ran rat RCW rea rec rec red red ref ref reg reg rel rel rem rep res res res res rev rhe Rie rig Rit roe Ros rot Ruh Ryd Sag sam sat sca sca Sch Sco sea sec sec see sel sem sen set Sgr sha shi sho sid sig sim sin sip ske sli smo soc sof sol sol sol sol sou sou spa spe spe spe spe sph spi Spi spr sta sta sta sta sta ste ste ste sto str str Sty sub sub suc sun sup sup sup sup sur Swa syn syn tac tas tel tem ter tes the the the the thi thr tid til tip ton tor tou tra tra tra tra Tri tri tru tsu tur two Typ UHE ult unc uni uni uni upg ura uti val var vec Vel ver Ver vie vir vis vis vol W-R war wav wav wea wei Whe Wid win WN4 Wol wro XMM yok zen zin > >>

Number of Results: 13095 Search : far
fitting
  سزکرد، سز   
saz-kard, saz

Fr.: ajustement   

The process or instance of adapting a mathematical curve to data points.

Verbal form of → fit.

fitting error
  ایرنگ ِ سزکرد، ~ سز   
irang-e saz-kard, ~ saz

Fr.: erreur d'ajustement   

The discrepancy between the mathematical curve and data points. → fit.

fitting; → error.

five
  پنج   
panj (#)

Fr.: cinq   

A cardinal number whose symbol is 5, V, or ۵.

Five, from O.E. fif, from P.Gmc. *fimfe (cf. O.S. fif, O.H.G. funf), from PIE *penkwe "five;" cognate with Pers. panj, as below.

Panj, from Mid.Pers. panj; Av. panca; cf. Skt. páñca; Gk. pente; L. quinque; E. five, as above.

five-color system
  راژمان ِ پنج‌رنگه   
râžmân-e panj-rangé

Fr.: système à cinq couleurs   

A photometric system which uses five filters, from ultraviolet to the red part of the visual spectrum: U, B, V, R and I.

five; → color; → system.

Five-hundred-meter Aperture Spherical radio Telescope (FAST)
     
FAST

Fr.: FAST   

The 500 m diameter → radio telescope which is the largest → single-dish antenna in the world. It is an Arecibo type telescope nestled within a natural basin in China's remote and mountainous Dawodang, Kedu Town, in southeastern China's Guizhou Province. The → reflector consists of 4,450 triangular panels, each with a side length of 11 m. More than 2,000 → actuators are used, according to the feedback from the measuring system, to deform the whole reflector surface and directly correct for → spherical aberration. Several detectors are used to cover a frequency range of 70 MHz to 3 GHz.

five; → hundred; → meter; → aperture; → spherical; → radio; → telescope.

fix
  برجاییدن   
barjâyidan

Fr.: fixer   

1) To make fast, firm, or stable.
2) To place definitely and more or less permanently (Dictionary.com).

M.E. fixen, probably from O.Fr. fixe "fixed," from L. fixus "fixed, fast, established, settled," p.p. of figere "to fix, fasten."

Infinitive, from barjâ, → fixed.

fixation
  برجایش   
barjâyeš

Fr.: fixation   

The act of fixing or the state of being fixed.

Verbal noun of → fix; → -tion.

fixed
  برجا   
barjâ

Fr.: fixe   

1) Fastened, attached, or placed so as to be firm and not readily movable; firmly implanted; stationary; rigid.
2) Rendered stable or permanent, as color.
3) Set or intent upon something; steadily directed (Dictionary.com).

Past participle from → fix.

Barjâ "fixed; in place; properly placed," from bar "on, upon, up," → object, + , → place,

fixed star
  ستاره‌ی ِ برجا، ~ ایستاده، ~ بیابانی   
setâre-ye barjâ, ~ istâdé, ~ biyâbâni (#)

Fr.: étoile fixe   

A → heavenly body that, in → contrast to the → planets, does not appear to change its relative → position on the → celestial sphere.

Fixed, p.p. of → fix; → star.

Setâré, → star; barjâ, → fixed.
Istâdé (Biruni in at-Tafhim) "standing," from istâdan "to stand;" O.Pers./Av. sta- "to stand, stand still; set" (cf. Skt. sthâ- "to stand;" Gk. histemi "put, place, weigh;" stasis "a standing still;" Lith. statau "place;" Goth. standan; L. stare "to stand;" PIE base *sta- "to stand");
Biyâbâni (Biruni in at-Tafhim), from Mid.Pers. awiyâbânig "fixed," from negation prefix → a- + wiyâbânig "wandering," from wiyâbân "deluded, seduced," wiyâbânênidan "to lead astray, deceive," from Av. vi- "apart, away from, out" (O.Pers. viy- "apart, away;" cf. Skt. vi- "apart, asunder, away, out;" L. vitare "to avoid, turn aside") + dab- "to deceive;" cf. Skt. vimugdha- "confused, bewildered," vimohita- "confused, infatuated." Note that biyâbân "desert" is from an other origin.

Fizeau test
  آزمون ِ فیزو   
âzmun-e Fizeau

Fr.: test de Fizeau   

The determination of the shape of an optical surface by means of → interferometry using a → fringe pattern formed with respect to a reference surface.

Named after the French physicist Armand Hippolyte Louis Fizeau (1819-1896), see also → toothed-wheel experiment; → test.

flame
  آیژ   
âyež (#)

Fr.: flamme   

1) Burning gas or vapor, as from wood or coal, that is undergoing combustion; a portion of ignited gas or vapor.
2) Any flame-like condition; glow; inflamed condition (Dictionary.com).

M.E. flaume, variant of flaumbe from Anglo-French flaume, flaumbe "a flame;" O.Fr. flambe, from L. flammula "small flame," diminutive of flamma "flame, blazing fire," from PIE *bhleg- "to shine, flash," from root *bhel- (1) "to shine, flash, burn."

Âyež, from (Dehxodâ) âyež "flame," variants âyiž, âyežé, ižak, of unknown origin.

Flamsteed designation
  نامگزینی ِ فلمستید   
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.

flare
  آلاو   
âlâv (#)

Fr.: éruption, sursaut   

1) A sudden blaze or burst of fire or light.
2) → solar flare.

From v. flare "to spread out," said of hair, a ship's sides, etc., of unknown origin.

Âlâv, "blaze, fire," variants alow, Borujerdi elew "fire," Garkuyeyi alôv "flame," Hamadâni elow "flame," Lori alô "flame," Tabari aluk "flame, spark," Torbat-Heydariyeyi alow "flame;" cf. Gk. aithos "fire," aitho "to kindle;" Skt. edh- "to set alight, kindle," édha-, édhas- "firewood;" Av. aēsma- "firewood;" Mod.Pers. hizom, himé "firewood;" PIE base *aidh- "to burn," *aidhos- "fire."

flare star
  ستاره‌ی ِ آلاوی، آلاو-ستاره   
setâre-ye âlâvi, âlâv-setâré

Fr.: étoile à éruption   

A member of a class of dwarf stars that undergoes sudden, intense outbursts of light (mean amplitude about 0.5-0.6 mag).

flare; → star.

flared disk
  گرده‌ی ِ برون‌گشا، دیسک ِ ~   
gerde-ye borun-gošâ, disk-e ~

Fr.: disque évasé   

A model of → accretion disk around a → pre-main sequence star or a → protostar in which the ratio of the disk thickness to the distance from the star increases outward. Current models of the irradiation of flared disks by stellar radiation predict that a central hole is created around the young star due to the evaporation of dust by the stellar radiation. The inner rim of the disk, at 0.5 to 1 AU from the star, is irradiated by the star "frontally" (at 90° angle). The heat produced by the irradiation causes the inner rim to puff up. A part of the disk, from about 1 to 6 AU, lies in the shadow of the puffed-up inner rim. The surface layers in this region do not receive stellar photons directly. Therefore, there is no significant heating of the disk midplane by reprocessed stellar flux from the disk surface. The midplane temperatures in the shadowed part of the disk are governed by the → near infrared emission of the inner rim, scattering of stellar light by dust particles outside the disk plane, and radial diffusion which exchanges energy between adjacent slabs. As for the outer parts of the disk, the surface is irradiated by the central star thanks to the outward widening of the disk. These parts remain flared, because the absorbed stellar flux is partially emitted toward the midplane, keeping the internal temperatures high enough to push the surface layers up. The flattened-disk model explains the observed → spectral energy distribution of some objects such as HD 179218. It also accounts for the observed strong → far-infrared, → excess, strong → PAH emission, and strong [O I] emission. Compare with → self-shadowed disk. See also → protoplanetary disk.

Flared, from flare "to spread gradually outward, as the end of a trumpet, having a gradual increase in width," of unknown origin; → disk.

Gerdé, → disk; borun-gošâ "opening outward," from borun "out, the outside" (Mid.Pers. bêron, from "outside, out, away" + rôn "side, direction;" Av. ravan- "(course of a) river") + gošâ stem of gošâdan, gošudan "to open;" Mid.Pers. wišâdan "to open, let free;" Khotanese hiyā "bound;" O.Pers. višta "untied, loosend;" vištāspa- (personal name) "with loosened horses;" Av. višta "untied," hita- "fastened, tied on;" cf. Skt. sā- "to bind, fasten," syáti "binds."

flash
  درخش   
deraxš (#)

Fr.: flash, éclair   

A Sudden, brief burst of light. In particular, → green flash.

From M.E. flasshen "to sprinkle, splash," from flasken, probably imitative.

Deraxš, present stem of deraxšidan "to shine, radiate," from raxš "lightening, reflection of light," raxšidan "to shine, flash," O.Pers. raucah-, Av. raocah- "light" (cf. Skt. roka- "brightness, light," Gk. leukos "white, clear," L. lux "light" (also lumen, luna), E. light, Ger. Licht, Fr. lumière; PIE base *leuk- "light, brightness"); cognate with Mod.Pers. words ruz "day," rowšan "bright, clear," foruq "light," and afruxtan "to light, kindle."

flash spectrum
  بیناب ِ درخشی   
binâb-e deraxši

Fr.: spectre-éclair   

The spectrum of the solar → chromosphere obtained during a → solar eclipse in the instant before or after → totality. In the flash spectrum the usual solar → absorption lines are replaced with bright → emission lines. This is because in that very short interval only the → photosphere is eclipsed by the Moon, and not the chromosphere. The American astronomer Charles A. Young was the first to observe it during the the solar eclipse of 1870 (December 22) in Spain.

The flash designation comes from the fact that the change from dark-line to bright-line spectrum is very rapid; → flash; → spectrum.

flat
  تخت   
taxt (#)

Fr.: plat   

Level and horizontal, without any slope; even and smooth, without any bumps or hollows.
See also:
flat manifold, → flat Universe, → flat-field, → flatness problem.

Flat, from O.N. flatr, from P.Gmc. *flataz (cf. O.H.G. flaz "flat, level," O.E. flet, O.H.G. flezzi "floor"), perhaps from PIE *pla- (cf. Gk. platys "broad, flat;" Av. pərətu- "broad, wide;" Skt. prthu- "broad, wide, large").

Taxt "flat;" Mid.Pers. taxtag "tablet, plank, (chess)board."

flat manifold
  بسلای ِ تخت   
baslâ-ye taxt

Fr.: variété plate   

A manifold with a → Riemannian metric that has → zero → curvature.

flat; → manifold.

flat rotation curve
  خم ِ چرخش ِ تخت   
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.

flat; → rotation; → curve.

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer aga air Alf Alg alk Alp alt alu amm ana And ang ani ano ant ant Ap apo app app Aqu Arc arg arr asc ass ast ast asy atm ato att aur aut axi B-m bad Bal bar bar Bay Bed ber Bet bif bim bin bio bis bla ble blu Bod Bol bor bou Bra Bre bro bul C-t Cal Cam can car Car Cas cat cav cel cen cer Cha cha Cha che chl Cir cir cir Cla cli clo clu co- cod coh col col col com com com com com com com com Com con con con con con con con con con con con con coo cor Cor cor cos cos cos Cou cou cra Cre cro Cru cub cur cyc cyl dar dat daw de- Deb dec dec dee def deg del Den dep der det deu dew dic dif dif dil dip dir dis dis dis dis dis diu dog Dop dou dra dua dus dwa dyn E r Ear ech eco edi eig Ein ela ele ele ele ele elo emi emp end enh ent epi equ equ erg est ety eur evo exa exc Exe exo exp exp ext ext eye fac fal Far fed Fer fer fie fin fir fit fla flo flu fol for for Fou fra fre Fre fro fuz gai Gal Gal gam gas Gau gen gen geo geo geo gia glo gol gra gra gra gra gre gri gui H I hai Ham har Hau hea hec hel hel her HES hie hig his hom hor hot Hub Hug hur hyd hyd hyl hyp ice ide ima ima imp imp inc ind ind ine inf inf inf ing inn ins ins int int int int int int int int inv Io ion iro isl iso iso Jac jet jud jur kel Kep kil kit kry Lag lam lan Lar lat law lea lem lep Li lig lim lin lin lin lit loc loc lon Lor low lum lun Lup Lym mac mag mag mag mag mag mai man Mar mas mas mat max mea mec meg men mer met met met mic mic Mik min min mis mne mod mol mon moo Mou mul mul myo nak Nas nat neb neg neu neu New New nit noi non non non Nor nuc nuc nul nut obe obl obs occ oct off Olb one ope opp opt opt orb orb org Ori ort oth out ove P C pal par par par par Pas pat pec peo per per per per per Pha pha pho pho pho phy pil pla Pla pla pla pla plu poi pol pol pol pol por pos pot Poy pre pre pre pre pri pri pri pro pro pro pro Pro pro Pru pul pul Pyt qua qua qua qua quo rad rad rad rad rad rad ram ran rat RCW rea rec rec red red ref ref reg reg rel rel rem rep res res res res rev rhe Rie rig Rit roe Ros rot Ruh Ryd Sag sam sat sca sca Sch Sco sea sec sec see sel sem sen set Sgr sha shi sho sid sig sim sin sip ske sli smo soc sof sol sol sol sol sou sou spa spe spe spe spe sph spi Spi spr sta sta sta sta sta ste ste ste sto str str Sty sub sub suc sun sup sup sup sup sur Swa syn syn tac tas tel tem ter tes the the the the thi thr tid til tip ton tor tou tra tra tra tra Tri tri tru tsu tur two Typ UHE ult unc uni uni uni upg ura uti val var vec Vel ver Ver vie vir vis vis vol W-R war wav wav wea wei Whe Wid win WN4 Wol wro XMM yok zen zin > >>