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 217 A s abe abs abs acc acc Ach act act ADa adi adv aff age Alc Alf ali all alp alt ama amp ana ang ang ann ano ant ant ape apo app aps arc Arg arm art ass ast ast ast atm ato att aur aut axi B-t Bai Bal bar bar Be bed Bes BHB bif bim bin Bio bis bla ble blu bod Bol bor bou bra Bre bro Bul cag cal can Can car Car Cas cat CCD cel cen Cet 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 coo cor cor cor Cos cos cos cou cou cra cri cro cry cum cur cyc d'A dar dat DB dea dec dec dec def def deh del den dep des det deu dia dif dif dif dim dip Dir dis dis dis dis dis div dom dou dou dri duo dus dyn dyn ear eas ecl Edd eff Ein eje ele ele ele ele ell emb emi enc ene ent eph equ equ equ eru eth Eul eve ewe exc exc exi exo exp ext ext ext fab fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre Fre fro fus G t gal gal Gam gas Gau Gem gen geo geo geo gia gla God gra gra gra gra Gre Gre gue GZK Haf hal har har He hea hel hel Her Her hid hig hip hom hor hot Hub Hug hur hyd hyd hyg hyp ice ide ima imp imp imp inc ind ind ine inf inf inf ini ins ins int int int int int int int int inv inv ion iro Isl iso iso Jac jet jud jur Kel Kep kil Klo kur Lag lam Lap Lar lat law lea len lep lib lig Lin lin lin liq lit loc log lon Lor low lum lun Lut Lyo mac mag mag mag Mag mag maj man Mar mas mas mat May mea mec mel mer mes met met met mic mid mil min mir mix mod mol mom Moo mos Mu mul mus nad nas nat neb neg net neu New New nig Noe non non non nor nuc nuc nul nut Obe obl obs occ Oct off old one ope opp opt opt orb ord org Ori osc oth ova oxi P-w pal par par par par Pas pat pej per per per per per per pha phi pho pho pho phy pin 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 rad rad rad rad rad rad raf ran rar ray rea rea rec rec red red ref ref reg rel rel rel rep res res res res ret rev ric rig rin roc ROS rot Rox rus Sad sam sat sca sca Sch sci sea sec sec see sel sem sen ser Sgr sha shi sho sid sig sim sin Sir ske sli Smo soc sol sol sol Sol Som sou spa spa spe spe spe sph spi spi Spo squ sta sta sta sta Ste ste ste Sto str str str sub sub suc sun sup sup sup sup sur Swa syn syn tac tas tel tem ter tes the the the the Tho thr tid tim tit top tot tra tra tra tra tre tri Tro tru tun tut Tyn typ ult unb und uni uni uns ups Urv vag van vec vei Ven ver Vic Vir vir vis vol W b war wav wav wea wee Wey Wid win WN2 Wol wro XMM YOR zen zir > >>

Number of Results: 12934 Search : far
Octans
  هشتکان   
Haštakân (#)

Fr.: Octant   

The Octant. A faint and obscure constellation, at 21h right ascension, 80° south declination, containing the south celestial pole. Its star Sigma Octantis is the closest naked-eye star to the pole, but it is so faint (magnitude 5.47) that it is practically useless as a polar star for navigation purposes. Abbreviation: Oct; Genitive: Octantis. It was introduced by the French astronomer Nicolas Louis de Lacaille (1713-1762).

From L.L. octans "eighth part of a circle," from → octa-, oct- + -ans, as in quadrans; → quadrant.

Haštakân, → octant.

octant
  هشتکان   
haštakân (#)

Fr.: octant   

1) A portion of a circle cut off by an arc and two radii at 45°, one-eighth of the area of a circle.
2) A instrument incorporating a telescope, the predecessor of the → sextant, used to measure angular distances, mainly in nautical astronomy. It spanned an angular range of 45°.

From L.L. octans "eighth part of a circle," from → octa-, oct- + -ans, as in quadrans; → quadrant.

Haštakân, from haštak "one-eigth," from hašt "eight" (Mid.Pers. hašt, O.Pers.*aštahva- "eighth;" Av. ašta; cf. Skt. astā; Ossetic ast; (Buddhist) Sogdian 'št; Gk. okto, L. octo (Fr. huit; Sp. ocho); P.Gmc. *akhto(u) (O.E. eahta, æhta, E. eight, O.N. atta, Ger. acht, Goth. ahtau); PIE base *oktô(u) + -ak, contraction of yak "one," (Mid.Pers. êwak (Proto-Iranian *aiua-ka-); O.Pers. aiva- "one, alone;" Av. aēuua- "one, alone" (cf. Skt. éka- "one, alone, single;" Gk. oios "alone, lonely;" L. unus "one;" E. one) + -ân nuance suffix.

octave
  اکتاو   
octâv (#)

Fr.: octave   

The interval between two musical notes, the fundamental components of which have frequencies in the ratio two to one.

M.E., from O.Fr. otaves, from L. octava feminine of octavus, from → octa-, oct- + -avus adj. suffix.

Octâv, loan from Fr. as above.

octet
  هشتایه   
haštâyé

Fr.: octet   

General: A group or series of eight.
Chemistry: A stable group of eight electrons which constitutes the outer electron shell of an atom of an inert gas (except helium whose only electron shell contains two electrons).

From → oct-, octa- + -et, as in duet.

Haštâyé, from haštâ "eightfold" + (y)é nuance suffix, as in dotâyé, → doublet.

octuple
  هشتایی   
haštâyi (#)

Fr.: octuple   

Eightfold; eight times as great.

L. octuplus, from octu- variant (before labials) of → oct- octa- + -plus "fold," from base of plicare "to fold, twist."

Haštâyi, from hašt "eight," → oct- octa- + -tâyi, from "fold, plait, ply; piece, part," also a multiplicative suffix; Mid.Pers. tâg "piece, part."

octupole
  هشت‌قطبه   
haštqotbé

Fr.: octupôle   

A → multipole consisting of eight point charges. Octupole moments are much smaller than → quadrupole moments and very much smaller than → dipole moment.

oct-; → pole.

ocular
  چشمی، دیدگانی   
cašmi, didgâni

Fr.: oculaire   

1) Of, pertaining to, or for the eyes.
2) Optics: An alternative term for → eyepiece.

From L. ocularis "of the eyes," from oculus "eye," from PIE base *okw- "to see;" cf; Av. aši- "(both) eyes;" E. → eye.

Cašmi, related to cašm "eye" (Mid.Pers. cašm, Av. cašman- "eye," ākas- "to look," from prefix ā- + Proto-Iranian *kas- "to look, appear," cf. Skt. cáksus- "seeing"); didgâni, related to didgân "eyes," plural of didé "eye," from didan "to see" (Mid.Pers. ditan "to see, regard, catch sight of, contemplate, experience;" O.Pers. dī- "to see;" Av. dā(y)- "to see," didāti "sees;" cf. Skt. dhī- "to perceive, think, ponder; thought, reflection, meditation," dādhye; Gk. dedorka "have seen").

odd
  تاق   
tâq

Fr.: impair   

Of a number, not divisible by two.
A function such as f(x) with the property that f(-x) = - f(x) for any value of x; e.g. sin(x).

From M.E. odde, from O.N. oddi "odd (number)."

Tâq, related to tak "single, alone", from Mid.Pers. tak, tâg "single, alone," maybe related to tâi, tâ "unit, piece."

odd-even nucleus
  هسته‌ی ِ تاق-جفت   
haste-ye tâq-joft

Fr.: noyau impair-pair   

Nucleus which contains an odd number of protons and an even number of neutrons.

odd; → even; → nucleus.

odd-odd nucleus
  هسته‌ی ِ تاق-تاق   
haste-ye tâq-tâq

Fr.: noyau impair-impair   

Nucleus which contains an odd number of both protons and neutrons.

odd; → nucleus.

oenology
  باده‌شناسی   
bâdešenâsi

Fr.: oenologie   

The science of → wines. Same as enology.

From Gk. oeno-, from oinos cognate with → wine.

Bâdešenâsi, from bâdé, bâda "wine," from Mid.Pers. bâtak "wine," + -šenâsi, → -logy.

oersted
  ا ُرستد   
oersted (#)

Fr.: oersted   

The unit of magnitude of magnetic field strength or magnetic intensity in c.g.s. units, i.e. the force in dynes which a unit magnetic pole would experience at any point in a magnetic field.

In honor of Hans Christian Ørsted (1777-1851), the Danish physicist and philosopher, who was the first to notice the interaction of electric current and the magnetic needle (1819) thereby initiating the study of electromagnetism.

Of star
  ستاره‌ی ِ Of   
setâre-ye Of

Fr.: étoile Of   

An → O star whose spectrum displays strong N III 4634-4640-4642 emission and strong He II 4686 emission. The N III lines are always much stronger than C III 4647-4650-4651 when the latter are present. Historically, Of stars were considered to belong to the peculiar category, hence the f notation (see below). In his thesis work, Walborn (1971, ApJS 23, 257) removed them from that category and established them as the normal O-type → supergiants. He also used the notation ((f)), (f), and f to describe the progression from strong He II 4686 absorption, through weakened/absent, to emission, respectively, correlated with increasing N III emission strength, subsequently showing that it is a luminosity sequence -- the first such for stars earlier than O9.

The reason for the Of designation is that the letters Oa-Oe were used in the original Harvard classification to denote various types of → Wolf-Rayet and OB spectra. Therefore Of was the next available when Plaskett and Pearce (1931, Pub. Dominion Ap. Obs 5, 99) wished to distinguish O-type spectra with selective emission in N III 4634-4640-4642 and He II 4686 ("selective" because other lines from the same ions appear in absorption); → star.

Of?p star
  ستاره‌ی ِ Of?p   
setâre-ye Of?p

Fr.: étoile Of?p   

A → massive star spectrum whose principal defining characteristics is the presence of C III 4647, 4650, 4651 emission lines with strength comparable to that of N III 4634, 4640, 4642. This category was introduced by Walborn (1972) to describe two well-known peculiar stars, HD 108 and HD 148937. → Of star

Of star; the question mark was intended to denote doubt that these stars are normal Of supergiants; p for "peculiar."

off
  دور از، بر، جدا، ...   
dur az, bar, jodâ, ...

Fr.:   

(adverb & preposition) From a place or position; at a distance in space or time. So as to be separated from support.

M.E., from O.E. of "away, away from;" cf. Du. af "off, down," Ger. ab "off, from, down;" PIE *apo- "off, away," → apo-.

off-
  اپ-   
ap-

Fr.: hors   

Away from a place.

off; cognate with Av. and O.Pers. apā "away from, from," as below.

Ap-, from apâ-, from Av. and O.Pers. apā "away from, from;" cf. Skt. apa "away, off;" L. ab- "from, away;" Hittite appa; Gothic af-; Ger. ab-; E. of, as above; PIE base *apo- "off, away"

off-axis optical system
  راژمان ِ نوریک ِ اپ-آسه   
râžmân-e nurik-e ap-âsé

Fr.: système optique hors axe   

An → optical system in which the → optical axis of the → aperture is not coincident with the mechanical center of the aperture.

off; → axis; → optical; → system.

off-line
  اپ-تان، اپ-خط   
ap-tân, ap-xatt

Fr.:   

Of computers, operating independently of, or disconnected from, an associated computer.

off; → line.

off-source observation
  نپاهش ِ اپ-خن   
nepâheš-e ap-xan

Fr.: observation hors source   

An observation when the telescope is pointed away from the source in order to measure the sky background contribution.

off-; → source; → observation.

offend
  آفندیدن   
âfandidan (#)

Fr.: offencer   

1) Cause to feel upset, annoyed, or resentful.
2) Commit an illegal act; break a commonly accepted rule or principle (OxfordDictionaries.com).

M.E. offenden, from O.Fr. ofendre "transgress, antagonize," and directly from L. offendere "to hit, strike against," figuratively "to stumble, commit a fault, displease," from assimilated form of ob "in front of against" + -fendere "to strike, push," from PIE root *gwhen- "to strike, kill;" cf. Av. -γna- "slaying," → murder.

Âfandidan, from âfand "strife, war," probably from Proto-Iranian *â-fanda-, from prefix *â- + *fanda-, from *fan- "to move;" cf. Yazghulami fin-/fud "to descend, come down," fəndan- "to bring down;" Roshani sifan-, Bartangi sifân- "to rise;" Skt. phan- "to jump" (Cheung 2007).

<< < -es -iv -ti 217 A s abe abs abs acc acc Ach act act ADa adi adv aff age Alc Alf ali all alp alt ama amp ana ang ang ann ano ant ant ape apo app aps arc Arg arm art ass ast ast ast atm ato att aur aut axi B-t Bai Bal bar bar Be bed Bes BHB bif bim bin Bio bis bla ble blu bod Bol bor bou bra Bre bro Bul cag cal can Can car Car Cas cat CCD cel cen Cet 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 coo cor cor cor Cos cos cos cou cou cra cri cro cry cum cur cyc d'A dar dat DB dea dec dec dec def def deh del den dep des det deu dia dif dif dif dim dip Dir dis dis dis dis dis div dom dou dou dri duo dus dyn dyn ear eas ecl Edd eff Ein eje ele ele ele ele ell emb emi enc ene ent eph equ equ equ eru eth Eul eve ewe exc exc exi exo exp ext ext ext fab fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre Fre fro fus G t gal gal Gam gas Gau Gem gen geo geo geo gia gla God gra gra gra gra Gre Gre gue GZK Haf hal har har He hea hel hel Her Her hid hig hip hom hor hot Hub Hug hur hyd hyd hyg hyp ice ide ima imp imp imp inc ind ind ine inf inf inf ini ins ins int int int int int int int int inv inv ion iro Isl iso iso Jac jet jud jur Kel Kep kil Klo kur Lag lam Lap Lar lat law lea len lep lib lig Lin lin lin liq lit loc log lon Lor low lum lun Lut Lyo mac mag mag mag Mag mag maj man Mar mas mas mat May mea mec mel mer mes met met met mic mid mil min mir mix mod mol mom Moo mos Mu mul mus nad nas nat neb neg net neu New New nig Noe non non non nor nuc nuc nul nut Obe obl obs occ Oct off old one ope opp opt opt orb ord org Ori osc oth ova oxi P-w pal par par par par Pas pat pej per per per per per per pha phi pho pho pho phy pin 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 rad rad rad rad rad rad raf ran rar ray rea rea rec rec red red ref ref reg rel rel rel rep res res res res ret rev ric rig rin roc ROS rot Rox rus Sad sam sat sca sca Sch sci sea sec sec see sel sem sen ser Sgr sha shi sho sid sig sim sin Sir ske sli Smo soc sol sol sol Sol Som sou spa spa spe spe spe sph spi spi Spo squ sta sta sta sta Ste ste ste Sto str str str sub sub suc sun sup sup sup sup sur Swa syn syn tac tas tel tem ter tes the the the the Tho thr tid tim tit top tot tra tra tra tra tre tri Tro tru tun tut Tyn typ ult unb und uni uni uns ups Urv vag van vec vei Ven ver Vic Vir vir vis vol W b war wav wav wea wee Wey Wid win WN2 Wol wro XMM YOR zen zir > >>