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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

   Homepage   
   


A B C D E F G H I J K L M N O P Q R S T U V W X Y Z

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer AGB air Alf Alg all alp alt AM amo ana And ang ani ano Ant Ant apa apo app app Ara Arc ari Arr ash ass ast ast asy atm ato att aut ave axi Bab bal Bal bar bar bea Bek Bes bia Big bin bin bip biv bla bli blu Boh Bol Bos bou bra bri bro buo cal cal can cap car Car cat cat CCD Cen cen CH cha cha che Che chr cir cir cit cla clo clo clu Coa coe 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 Cop Cor cor cor cos cos cou cou Cow cre cri cro cry cur cya Cyg dan dar dat de- deb dec dec ded def deg del dem den dep des det dev dia dif dif dih dio Dir dis dis dis dis dis dis DO don dou dow dro dur dwa dyn Dys ear ebb ecl edg egg Ein Ela ele ele ele ele ell eme emp enc eng ent epi equ equ equ esc eth Eur Eve exa exc exe exi exp exp ext ext ext fac fal far fed Fer fer fie fin fir fis fla flo flu fol for for fou fra fre Fre fro fut G-t gal gal gam gas Gau Gem gen geo geo geo gia Gli Gol gra gra gra gra gre gri gui H I Hag hal har hat He- hea hel Hel her Hes hie hig his hom hor hot Hub Hug hur hyd hyd hyg hyp ice ide ima Ima imp imp inc inc 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 Klo Kui Lag lam Lap Lar lat law lea len lep Lib lig lim lin lin Lio lit loc LOF lon Lor low lum lun Lup Lyo mac mag mag mag mag mag mai man Mar mas mas mat Max mea mec Meg Mer Mer met met Met mic Mid Mil min Mir mit mod mod mol mon Mor mou mul mul mys nan Nat nau nec neo neu nev New NGC no nom non non nor not nuc nuc num nut obj obs obs occ ocu oft ome Oor ope opp opt opt orb ord ori ort osc out ove oxi pai pan par par par par pas pea pen per per per per Per per pha phi pho pho pho phy pio Pla pla pla pla Pla plu Poi pol pol pol poo pos pos pot pra pre pre pre pre pri pri pro pro pro pro pro Pro pro pse pul pur qua qua qua qua que rac rad rad rad rad rad rad ran rar ray rea rea rec rec red red ref ref reg rel rel rel ren res res res res ret rev Ric rig rin roc roo rot rot Rus Sac sal sat sca sca Sch sci Scu sec sec Sed sel Sel sen ser Sex Sha she sho sid sig sil sim sin siz sla Sma sno sof sol sol sol sol sou sou spa spa spe spe spe sph spi spi spr squ sta sta sta sta ste ste ste Sto Str str str sub sub suc sun sup sup sup sup sur swa syn syn tab tar tek tem ter tes the the the the Tho thr tid tim Tis Too Tor tra tra Tra tra tra tri tri tru Tul tur two Typ ult un- und uni uni unk upp Urc utt val var vec vel ver vib vio vir vis voi vor wan wat wav wax wea Wei whi Wil win WN9 wor X-r yel you zer zod > >>

Number of Results: 13048 Search : far
Small Magellanic Cloud (SMC)
  ابر ِ کوچک ِ ماژلان   
Abr-e Kucak-e Magellan (#)

Fr.: Petit Nuage de Magellan   

An irregular galaxy, the smaller of the two → Magellanic Clouds that are satellites of our own Galaxy, lying in the southern constellation → Tucana about 20 degrees from the → south celestial pole. The SMC covers an area roughly 3 by 5 degrees in dimension and has an overall → visual magnitude about +2.7. The SMC is about 10,000 → light-years in diameter and some 210,000 light-years (61 → kpc) away. It has a visible mass of about 1/50-th that of our Galaxy and 1/10-th of that of the → Large Magellanic Cloud (LMC). Its → heavy element content is about a factor 5 smaller than that of the Galaxy. The SMC is the third-nearest external galaxy after the → Sagittarius Dwarf Elliptical Galaxy and the LMC.

small; → Magellanic; → cloud.

small solar system body
  جسم ِ کوچک ِ راژمان ِ خورشیدی   
jesm-e kucak-e râžmân-e xoršidi

Fr.: petit corps du système solaire   

A term introduced by the → International Astronomical Union (August 2006) to name the → solar system bodies other than → planets and → dwarf planets. Small solar system bodies include → asteroids, → comets, and → meteoroids.

small; → solar; → system; → body.

SMASS classification
  رده‌بندی ِ SMASS   
radebandi-ye SMASS

Fr.: classification SMASS   

An asteroid taxonomy built on the → Tholen classification but based on the presence or absence of → absorption features in the visible part of the spectrum. In many cases the two classifications are the same, but the Tholen C and S classes are subdivided in the SMASS classification.

SMASS stands for the Small Main-belt Asteroid Spectroscopic Survey, → small; → main belt; → asteroid; → spectroscopic; → survey; → classification.

Smith's cloud
  ابر ِ اسمیت   
abr-e Smith

Fr.: nuage de Smith   

A huge, → high-velocity cloud of hydrogen gas that measures some 9,800 × 3,300 → light-years. It is located between 36,000 and 45,000 light-years away from Earth in the northern constellation of → Aquila. It has a mass of at least 106 → solar masses. It is now moving toward the disk of the → Milky Way at 73 ± 26 km/s and is expected to hit the disk of our Galaxy in about 27 million years, at an angle of approximately 45° at a point in the → Perseus Arm, one of two major → spiral arms of the Galaxy.

Named after Gail Bieger, née Smith, who discovered the cloud in 1963, when she was an astronomy student at Leiden University in the Netherlands; → cloud.

smog
  دودمه   
dudmeh (#)

Fr.: smog   

A fog combined with smoke or other forms of atmospheric pollutants in an unhealthy or irritating mixture.

From sm(oke) + (f)og; → smoke; → fog.

Dudmeh, from dud, → smoke, + meh, → fog.

smoke
  دود   
dud (#)

Fr.: fumée   

A mass of tiny particles in the air that rises up from something burning.

M.E., O.E. smoca, related to smeocan "give off smoke;" cf. M.Du. smooc, Du. smook, M.H.G. smouch, Ger. Schmauch; PIE base *smeug(h)- "smoke" (cf. Arm. mux "smoke," Gk. smukho "to burn in a smoldering fire," O.Ir. much, Welsh mwg "smoke").

Dud, from Mid.Pers. dût, dûd "smoke;" Av. dunman- "cloud," duuan- "to fly;" cf. Skt. dhvan- "to smoke;" Hittite tuhhae- "to prouce smoke;" PIE base *dheu- "to blow, reel; smoke, dark."

smooth
  ۱) هموار؛ ۲) هموار کردن   
1) hamvâr (#); 2) hamvâr kardan (#)

Fr.: 1) lisse; 2) lisser   

1) Of a curve, free from bumps or abrupt irregularities.
2) To modify a sequential set of numerical data by reducing the differences in magnitude between adjacent values.

O.E. smoð "free from roughness, not harsh," of unknown origin.

Hamvâr "level, equal, an even place or thing," from ham- "same, equally, even; together, with" (Mid.Pers. ham-, like L. com- and Gk. syn- with neither of which it is cognate. O.Pers./Av. ham-, Skt. sam-; also O.Pers./Av. hama- "one and the same," Skt. sama-, Gk. homos-; originally identical with PIE numeral *sam- "one," from *som-. The Av. ham- appears in various forms: han- (before gutturals, palatals, dentals) and also hem-, hen-) + -vâr similarity suffix.

smooth curve
  خم ِ هموار   
xam-e hamvâr

Fr.: courbe lisse   

1) A curve which is free from abrupt fluctuations.
2) A curve if it has tangents at all points and the angle of inclination of the tangent is a continuous function of the arc length.

smooth; → curve.

Smoothed Particle Hydrodynamics (SPH)
  هیدروتوانیک ِ ذره‌های ِ همواریده   
hidrotavânik-e zarrehâ-ye hamvâridé

Fr.: hydrodynamique des particules lissées   

A numerical method for modeling → compressible hydrodynamic flows, which uses particles to simulate a continuous fluid flow. Because the system of hydrodynamical basic equations can be analytically solved only for few exceptional cases, the SPH method provides a numerical algorithm to solve systems of coupled → partial differential equations for continuous field quantities. The main advantage of the method is that it does not require a computational grid to calculate spatial → derivatives and that it is a Lagrangian method, which automatically focuses attention on fluid elements. The equations of motion and continuity are expressed in terms of ordinary differential equations where the body forces become classical forces between particles. This method was first independently developed by Lucy (1977, AJ 82, 1013) and Gingold & Monaghan (1977, MNRAS 181, 375).

Smoothed Particle Hydrodynamics, first used by Gingold & Monaghan (1977); → smooth; → particle; → hydrodynamics.

smoothing
  هموارش   
hamvâreš

Fr.: lissage   

The mathematical process that makes a curve smooth.

Verbal noun of → smooth.

smoothing circuit
  برقراه ِ هموارگر   
narqrâh-e hamvârgar

Fr.: circuit atténuateur   

A low-pass filter designed to reduce the amplitude of a ripple while freely passing the direct current obtained from a rectifier or direct-current generator. Also known as smoothing filter.

smoothing; → circuit.

snail
  راب، حلزون   
râb (#), halazun (#)

Fr.: escargot   

A general name for a member of the large group of terrestrial and fresh-water gastropod molluscs which have a coiled shell. → slug.

M.E. snail, snayl(e), O.E. snegel; cognate with M.H.G. snagel, dialectal Ger. Schnegel.

Râb, dialectal Gilaki and Tabari (also see Dehxodâ). Halazun, from Ar.

Snell's law
  قانون ِ اسنل   
qânun-e Snell (#)

Fr.: loi de Snell, loi de Descartes   

The relationship between angles of incidence and refraction for a wave incident on an interface between two media with different indices of refraction. The law states that the ratio of the sine of the → angle of incidence to the sine of the → angle of refraction is a constant: n1/n2 = sinθ2/sinθ1. See also → refractive index. Also known as Descartes' law or the law of refraction.

Named after Dutch mathematician Willebrord Snellius (1580-1626), one of the discoverers of the law; → law.

snow
  برف   
barf (#)

Fr.: neige   

A precipitation in the form of → ice crystals that falls from clouds when the air temperature is below 0 °C. Snow occurs when → water vapor in the → atmosphere forms directly into ice and completely bypasses the liquid stage of → precipitation. Once an ice crystal has formed, it absorbs up even more water vapor and freezes due to the surrounding atmosphere. The ice crystal then falls down to earth's surface in the form of a → snow crystal, snow → pellet, or more commonly known as the → snowflake. In short, snow formation requires the following conditions: 1) → relative humidity ≥ 100%, 2) → temperature < 0 °C, 3) presence of → condensation nuclei, and 4) → supercooled droplets.

O.E. snaw "snow;" cf. O.S., O.H.G. sneo, O.Fris., M.L.G. sne, M.Du. snee, Du. sneeuw, Ger. Schnee, O.N. snjor, Goth. snaiws "snow;" PIE base *sneigwh- "to snow, snow;" cf. Mid.Pers. snêx, snêxr "snow;" Av. snaēg- "to snow," snaēžaiti "snows;" Skt. snih- "wet;" Gk. nipha "snowflake," neiphei "snows;" L. nix (genitive nivis); O.Ir. snigid "snows;" Lith. sniegas; Rus. snieg'.

Barf "snow," dialectal vafr "snow," var, from Mid.Pers. vafr "snow;" Av. vafra- in jaiwi.vafra- "with deep snow."

snow crystal
  بلور برف   
bolur-e barf

Fr.: cristal de neige   

An → ice crystal forming snow in a → cloud.

snow; → crystal.

snow line
  مرز ِ یخ، یخ-مرز   
marz-e yax, yax-marz

Fr.: limite de glace   

In a → protoplanetary disk, the limit between the regions where water is gaseous and the region where it is cold enough for water to become ice. The core accretion theory predicts that → giant planets form just outside the snow line where they can accrete enough rock and ice to generate a core. Subsequently the core grows into a gas giant like → Jupiter or → Saturn via the → accretion of hydrogen and helium. The snow line location depends on the → luminosity of the central star. For solar system it is about 5 AU, the position of Jupiter. Also known as ice line.

snow; → line.

Marz, → frontier; yax, → ice.

snowball
  برف-گوله   
barf-gule

Fr.: boule de neige   

A mass of snow packed into a ball or rolled together, as for throwing.

snow; → ball.

snowball Earth
  زمین ِ برف-گوله   
Zamin-e barf-gule

Fr.: Terre boule de neige   

Any of several episodes in the history of the Earth where our planet was entirely covered by glacial ice from pole to pole. There are at least three such episodes. The first one, called the Huronian glaciation, extended from 2.4 billion years ago to 2.1 billion years (lasting about 300 million years). In the last billion years, the Earth has experienced two more global glaciations: the Sturtian glaciation, which began 720 million years ago and, following a brief interglacial episode, the Marinoan glaciation, which ended 635 million years ago. During such episodes the global mean temperature would be about -50°C because most of the Sun's radiation would be reflected back to space by the icy surface. The average equatorial temperature would be about -20°C, roughly similar to present Antarctica. Without the moderating effect of the oceans, temperature fluctuations associated with the day-night and seasonal cycles would be greatly enhanced. Because of its solid surface, the climate on a snowball earth would have much in common with present Mars (http://www.snowballearth.org).

The term snowball Earth was coined in 1989 by Joe Kirschvink, a biomagnetist and paleomagnetist at the Caifornia Institute of Technology in Pasadena, USA; → earth.

snowdrift
  برف-راند   
barf-rând

Fr.: congère   

A mound or bank of snow deposited as sloping surfaces and peaks, often behind obstacles and irregularities, due to eddies in the wind field.

snow; → drift.

Barf-rând "snowdrift, drfited snow" from barf, → snow, + rând "driving, drfit; drifted," from rândan "to push, drive, cause to go," causative of raftan "to go, walk, proceed" (present tense stem row-, Mid.Pers. raftan, raw-, Proto-Iranian *rab/f- "to go; to attack"); barf-e bâd âvard "snow brought by wind," from barf + bâdwind + âvard, short for âvardé "brought," p.p. of âvardan "to bring; to cause, produce" (Mid.Pers. âwurtan, âvaritan; Av. ābar- "to bring; to possess," from prefix ā- + Av./O.Pers. bar- "to bear, carry," bareθre "to bear (infinitive)," bareθri "a female that bears (children), a mother;" Mod.Pers. bordan "to carry;" Skt. bharati "he carries;" Gk. pherein; L. fero "to carry").

snowflake
  گلیچ ِ برف، دانه‌ی ِ ~   
golic-e barf, dâne-ye ~

Fr.: flocon de neige   

An agglomeration of many → ice crystals that falls as a unit from a cloud. Snowflakes possess a six-fold symmetry that ultimately derives from the six-fold symmetry of the ice crystal lattice. Typical snowflakes fall at a rate of 1-2 m s-1. The shape of snowflakes is influenced by the → temperature and → humidity of the atmosphere. Snowflakes form in the atmosphere when cold water droplets freeze onto dust particles. Depending on the temperature and humidity of the air where the snowflakes form, the resulting ice crystals will grow into a myriad of different shapes. Snowflakes formed in temperatures below -22 °C consist primarily of simple crystal plates and columns whereas snowflakes with extensive branching patterns are formed in warmer temperatures. Snowflakes are not frozen raindrops. Sometimes raindrops do freeze as they fall, but this is called → sleet. Sleet particles do not have any of the elaborate and symmetrical patterning found in snow crystals.

From → snow + flake, from M.E. akin to O.E. flac- in flacox "flying" (said of arrows), O.N. flakka "to wander," M.Du. vlac "flat, level," M.H.G. vlach, Ger. Flocke "flake."

Golic "snowflake" in dialectal Lori and Laki (originally *geli-ka), variants Laki gal "seed (of millet)," gella "grape berry," Torbat-Heydariyei gella "grape berry," golla "ball, reel," Kurd. kuli, kilole "snowflake," Malâyeri gulu "bead," Qâyeni golle "bead," Qasrâni gella, golla "bead," Tabari gəlilə "bead," Gilaki gudé "ball, bowl, tumour," literary Pers. golulé, goruk "ball;" cf. Skt. guda- "ball, mouthful, lump, tumour;" Pali gula- "ball;" Gk. gloutos "rump;" L. glomus "ball," globus "globe;" Ger. Kugel; E. clot; PIE base *gel- "to make into a ball;" barf, → snow; dâné, → grain.

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer AGB air Alf Alg all alp alt AM amo ana And ang ani ano Ant Ant apa apo app app Ara Arc ari Arr ash ass ast ast asy atm ato att aut ave axi Bab bal Bal bar bar bea Bek Bes bia Big bin bin bip biv bla bli blu Boh Bol Bos bou bra bri bro buo cal cal can cap car Car cat cat CCD Cen cen CH cha cha che Che chr cir cir cit cla clo clo clu Coa coe 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 Cop Cor cor cor cos cos cou cou Cow cre cri cro cry cur cya Cyg dan dar dat de- deb dec dec ded def deg del dem den dep des det dev dia dif dif dih dio Dir dis dis dis dis dis dis DO don dou dow dro dur dwa dyn Dys ear ebb ecl edg egg Ein Ela ele ele ele ele ell eme emp enc eng ent epi equ equ equ esc eth Eur Eve exa exc exe exi exp exp ext ext ext fac fal far fed Fer fer fie fin fir fis fla flo flu fol for for fou fra fre Fre fro fut G-t gal gal gam gas Gau Gem gen geo geo geo gia Gli Gol gra gra gra gra gre gri gui H I Hag hal har hat He- hea hel Hel her Hes hie hig his hom hor hot Hub Hug hur hyd hyd hyg hyp ice ide ima Ima imp imp inc inc 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 Klo Kui Lag lam Lap Lar lat law lea len lep Lib lig lim lin lin Lio lit loc LOF lon Lor low lum lun Lup Lyo mac mag mag mag mag mag mai man Mar mas mas mat Max mea mec Meg Mer Mer met met Met mic Mid Mil min Mir mit mod mod mol mon Mor mou mul mul mys nan Nat nau nec neo neu nev New NGC no nom non non nor not nuc nuc num nut obj obs obs occ ocu oft ome Oor ope opp opt opt orb ord ori ort osc out ove oxi pai pan par par par par pas pea pen per per per per Per per pha phi pho pho pho phy pio Pla pla pla pla Pla plu Poi pol pol pol poo pos pos pot pra pre pre pre pre pri pri pro pro pro pro pro Pro pro pse pul pur qua qua qua qua que rac rad rad rad rad rad rad ran rar ray rea rea rec rec red red ref ref reg rel rel rel ren res res res res ret rev Ric rig rin roc roo rot rot Rus Sac sal sat sca sca Sch sci Scu sec sec Sed sel Sel sen ser Sex Sha she sho sid sig sil sim sin siz sla Sma sno sof sol sol sol sol sou sou spa spa spe spe spe sph spi spi spr squ sta sta sta sta ste ste ste Sto Str str str sub sub suc sun sup sup sup sup sur swa syn syn tab tar tek tem ter tes the the the the Tho thr tid tim Tis Too Tor tra tra Tra tra tra tri tri tru Tul tur two Typ ult un- und uni uni unk upp Urc utt val var vec vel ver vib vio vir vis voi vor wan wat wav wax wea Wei whi Wil win WN9 wor X-r yel you zer zod > >>