An Etymological Dictionary of Astronomy and Astrophysics
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فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 12982 Search : far
circumcircle
  پیراپرهون   
pirâparhun

Fr.: cercle circonscrit   

A circle which passes through all three vertices of a triangle Also "Circumscribed circle".

circum-; → circle.

circumference
  پیرامون   
pirâmun (#)

Fr.: circonférence   

1) The boundary line of a circle.
2) The boundary line of a figure, area, or object.

From M.E., from O.Fr. circonference, from L. circumferentia, from circumferens, circumferent-, pr.p. of circumferre "to carry around," from → circum- + ferre "to carry," from PIE root *bher-; "to carry;" cf. Av./O.Pers. bar- "to bear, carry," barəθre "to bear (infinitive)," barəθri- "a female that bears (children), a mother," Mod.Pers. bordan "to carry," Skt. bharati "he carries," Gk. pherein, P.Gmc. *beranan (O.H.G. beran, Goth. bairan "to carry").

Pirâmun, from Mid.Pers. pêrâmôn, from O.Pers./Av. mâ-, mây- "to measure," from PIE *me- "measure," cf. Skt. mati "measures," matra "measure," Gk. metra "lot, portion," L. metri "to measure." In Mod.Pers. this stem is extant in peymaân, peymaâné, âzmun, âzmâyeš.

circumfix
  پیراوند   
pirâvand

Fr.: circumfixe   

An → affix made up of two separate parts which surround and attach to a base.

circum-; → affix.

circumgalactic medium (CGM)
  مدیم ِ پیراکهکشانی   
madim-e pirâkahkešâni

Fr.: milieu circumgalactique   

The interface between a galaxy and the → intergalactic medium. The circumgalactic medium comprises gas located in the → halo of a galaxy extending out to the → virial radius.

circum-; → galactic.

circumlunar
  پیرامانگی، پیراماهی   
pirâmângi, pirâmâhi (#)

Fr.: circumlunaire   

Surrounding or revolving around the Moon.

Circumlunar, from → circum- + → lunar.

circumnuclear
  پیراهسته‌ای   
pirâhasteyi

Fr.: circumnucléaire   

Situated around a → nucleus, as of a → circumnuclear disk.

circum- + → nuclear.

circumnuclear disk
  گرده‌ی ِ پیراهسته‌ای   
gerde-ye pirâhasteyi

Fr.: disque circumnucléaire   

A thick disk of gas and dust clouds surrounding the → Galactic Center up to about 20 → light-years. The disk is very clumpy; the → clumps have densities of several 105 particles/cm3, radii of about 0.3 light-years, and gas temperatures above 100 K. The hydrogen mass of the disk is a few 104 → solar masses. Such circumnuclear disks are present also in other galaxies.

circumnuclear; → disk.

circumpolar
  پیراقطبی   
pirâqotbi (#)

Fr.: circumpolaire   

Situated around or near a pole, as of the Earth or the sky. → circumpolar star.

circum-; → polar.

circumpolar star
  ستاره‌ی ِ پیراقطبی   
setâre-ye pirâqotbi (#)

Fr.: étoile circumpolaire   

Star that, from a given observer's → latitude, does not rise or set, but circles around the → celestial pole. To be circumpolar, a star must have a polar distance that is less than the observer's latitude. Whether a given star is circumpolar at the observer's latitude (φ) may be calculated in terms of the star's → declination (δ). The star is circumpolar if φ + δ ≥ +90° (observer in northern hemisphere), or φ + δ ≤ -90° (observer in southern hemisphere).

circumpolar; → star.

circumscribe
  پیراکشیدن   
pirâkašidan

Fr.: circonscrire   

To draw a line around; encircle.

L. circumscribere "to draw a line around, confine," from → circum- + scribere "write," from PIE *skreibh-, from *sker- "to cut, incise."

Pirâkašidan, from pirâ-, → circum- + kašidan "to draw," Mid.Pers. kašitan, Av. karš- "to draw," Skt. kars-, kársati "to pull, drag, plough."

circumscribed sphere
  سپهر ِ پیراکشیده، کره‌ی ِ ~، گوی ِ ~   
sepehr-e pirâkašidé, kore-ye ~, guy-e ~

Fr.: sphère circonscrite   

A sphere containing a polyhedron (such as a pyramid) all of whose vertices lie on the surface of the sphere. The polyhedron so contained is said to be inscribed in the sphere.

Circumscribed p.p. of → circumscribe; → sphere.

circumsolar
  پیراخورشیدی   
pirâxoršidi

Fr.: circumsolaire   

Surrounding or revolving around the Sun, such as circumsolar space, circumsolar dust.

Circumsolar, from → circum- + → solar.

circumspect
  پیراگاس   
pirâgâs

Fr.: circonspect   

Watchful and discreet; cautious; prudent:

circum-; → suspect.

circumspection
  پیراگاسش   
pirâgâseš

Fr.: circonspection   

Circumspect observation or action; caution; prudence.

circumspect.

circumstance
  پیراستاد   
pirâstâd

Fr.: circonstance   

A condition or fact attending an event and having some bearing on it.

L. circumstantia "surrounding condition," neut. pl. of circumstans, pr.p. of circumstare "to stand around," from → circum- + stare "to stand" from PIE *sta- "to stand."

Pirâstâd, from pirâ-, → circum-, + âstâd, istâd "standing," from istâdan "to stand," Mid.Pers. êstâtan, O.Pers./Av. sta- "to stand, stand still; set," Av. hištaiti, cf. Skt. sthâ- "to stand," âsthâ- "condition, circumstance," Gk. histemi "put, place, weigh," stasis "a standing still," L. stare "to stand."

circumstellar
  پیراستاره‌ای   
pirâsetâreyi

Fr.: circumstellaire   

Surrounding or occurring around a star.

Circumstellar, from → circum- + → stellar.

circumstellar disk
  گرده‌ی ِ پیراستاره‌ای   
gerde-ye pirâsetâreyi

Fr.: disque circumstellaire   

Any concentration of material in the form of a disk orbiting around a star. → accretion disk; → protoplanetary disk.

circumstellar; → disk.

circumstellar dust
  غبار ِ پیراستاره‌ای   
qobâr-e pirâsetâreyi

Fr.: poussière circumstellaire   

Interstellar → dust grains localized around various types of stars, such as → asymptotic giant branch stars. Circumstellar dust occurs in the form of a spherical shell or a disk and is at the origin of an → infrared excess for the central star. See also → circumstellar matter.

circumstellar; → dust.

circumstellar envelope
  پوشه‌ی ِ پیراستاره‌ای   
puše-ye pirâsetâre-yi

Fr.: enveloppe circumstellaire   

A very extensive envelope of cold gaseous materials surrounding evolved cool stars, notably → red giants, → red supergiants (→ Mira variables), or → asymptotic giant branch stars. The typical size of such envelopes is several thousands times that of the stellar radius and their temperature ranges from 1000 to10 K. Circumstellar envelopes result from mass loss from the central star (10-7 to 10-4solar masses per year) and expand with moderate velocities (10 to 15 km sec-1). The low temperature of the envelope is at the origin of the formation of molecules, which in certain conditions provide → maser emission (H2O, OH, SiO). Similarly, dust grains form in the envelope produce an → infrared excess emission.

circumstellar; → envelope.

circumstellar environment
  پرگیر ِ پیراستاره‌ای   
pargir-e pirâsetâre-yi

Fr.: environnement circumstellaire   

The circumstances or physical conditions related to the immediate surroundings of a star.

circumstellar; → environment.

<< < -es -iv -ti 21- a p abe abs abs acc acc acc act act ada adi ads aes Age Alb Alf ali all alp alt ama amp ana ang ang ann ano ant ant ape apo app app arc Arg ari art ass ast ast ast atm ato att Aur aut axi azi bac Bal Bar Bar Bay Bec Ber bet bic bij bin bio Bir bla Bla blu blu bol Boo bou bra Bre bro bug C r cal Cal can car Car Cas cat cau cel cen cer Cha cha Cha che chl cir cir cir Cla cli clo clu co- coc 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 cut Cyg dam dar dat de deb dec dec ded def deg del dem den dep des det dev dia dif dif dig dio Dir dis dis dis dis dis dis div 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 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 hum Huy hyd hyd hyl hyp ice ide ima imp imp imp inc ind ind ine inf inf inf ini ins ins ins int int int int Int int int int inv ion iro irr iso iso ite jel Jou Jup kao Kep kil Kip Kra Lag Lam lan lar las law lea leg Leo lex lig lim lin lin lin lit Loc loc log Lor low lum lun lun Lym mac mag mag mag mag mag mai Mal mar mas mas mat max mea mec meg men mer met met met mic mic Mik min min mis mob mod mol mon moo 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 odd OH 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 phl pho pho pho pi pip Pla pla pla pla ple poa pol Pol pol pol pop pos pos pot pra pre pre pre pri pri pri pro pro pro pro pro pro pro Pto pul puz qua qua qua qua qui rad rad rad rad rad rad rai ran rar Ray rea Rea rec rec red red ref ref reg rel rel rel rep res res res res ret Rhe rid rig ris Roe Ros rot rub rut Sag sam sat sca sca Sch sci sea sec sec see sel sem sen ser Sh2 sha shi sho sid sig sim sin Sir ske sli Smo soc sol sol sol sol sol sou spa spa spe spe spe spe sph spi spo Squ sta sta sta sta ste ste ste sto str str str sub sub sub sum sup sup sup sup sur sus sym syn T d tap tec tem ten tes the the the the thi thr tid tim tip ton tor tow tra tra tra tra tri tri tru tub tur two Typ ult un- und uni uni unp upp urg V20 Van var veg vel ver vib vio vir vis Vol Vul wan wat wav WC4 wea wel whi Wil wis WNL wor X-r Yer Z s zer [C > >>