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: 13048 Search : far
isotopic
  ایزوتوپی   
izotopi (#)

Fr.: isotopique   

Of or relating to an → isotope.

isotope; → -ic.

isotopic fractionation
  برخانش ِ ایزوتوپی   
barxâneš-e izotopi

Fr.: fractionnement isotopique   

Same as → isotope fractionation.

isotopic; → fractionation

isotopic number
  عدد ِ ایزوتوپی   
adad-e izotopi

Fr.: nombre isotopique   

The difference between the number of neutrons in an isotope and the number of protons. Neutron excess.

isotopic; → number.

isotopic ratio
  وابر ِ ایزوتوپی   
vâbar-e izotopi

Fr.: rapport isotopique   

The relative abundances of two isotopes of a given chemical element, such as D/H (deuterium/hydrogen), (carbon) 12C/13C, and (uranium) 235U/238U.

isotopic; → ratio.

isotopic spin
  اسپین ِ ایزوتوپی، ایزو-اسپین   
spin-e izotopi (#), izospin (#)

Fr.: spin isotopique   

Same as → isospin.

isotopic; → spin.

isotopologue
  ایزوتوپولوگ   
izotopolog

Fr.: isotopologue   

Any of molecular entities which differ in their isotopic composition but retain the same → chemical elements, e.g. H2O and HDO.

Abbreviation of → isotopic → analogue.

isotopomer
  ایزوتوپومر   
izotopomer

Fr.: isotopomère   

Any of → isomers having the same number of each isotopic atom but differing in their positions. For example, CH3CHDCH3 and CH3CH2CH2D are a pair of isotopomers.

Short for isotopic isomers.

isotropic
  ایزوگرد، همسان‌گرد   
izogard, hamsângard (#)

Fr.: isotrope   

Having physical properties that do not vary with direction.

iso- + → -tropic.

isotropic Universe
  گیتی ِ ایزوگرد، ~ ِ همسان‌گرد   
giti-ye izogard, ~ hamsângard (#)

Fr.: Univers isotrope   

A Universe having observed properties that appear identical in every direction.

isotropic; → universe.

isotropy
  ایزوگردی، هم‌سان‌گردی   
izogardi, hamsângardi (#)

Fr.: isotropie   

The property by which physical properties are equal along all directions. → anisotropy.

Isotropy, noun of → isotropic.

issue
  ۱) برونای؛ ۲) بروناییدن   
1) borunây; 2) borunâyidan

Fr.: issue, question, problème   

1a) A result or outcome of something.
1b) The action of flowing or coming out.
1c) Each of a regular series of publications.
1d) An important topic or problem for debate or discussion.
2) Formally send out or make known (OxfordDictionaries.com).

M.E., from O.Fr. issue "a way out, a going out, exit; final event," from L. exire "to go out, go forth; become public; flow, pour forth," from → ex- "out," + ire "to go,"

Borunây, literally "what comes out, exits," from borun, → out, + ây- present stem of âmadan "to come, arrive, become," → precession.

item
  یوتر   
yutar

Fr.: article, objet, point, ordre de jour   

1) A distinct part in an enumeration, account, collection, or set.
2) An object of attention, concern, or interest.
3) A separate piece of news or information.

From M.E. item, from L. item ("also; in the same manner"), from a L. usage in lists, where the first entry would begin in primis ("firstly") and the other entries with item ("also, moreover").

Yutar, from Sogd. yûtar "one of several," from ēw-tar, from ēw "→ one" + -tar distinction suffix.

itemize
  یوتریدن   
yutaridan

Fr.: détailler, spécifier   

1) To present as a list of items.
2) To list the items of.

item; → -ize.

iterate
  ایتریدن   
itaridan

Fr.: itérer   

1) To utter or to do something over again or repeatedly. → repeat.
2) Math.: → iteration.

Iterate "to do again, repeat," back-formation from iteration, from L. iterationem (nom. iteratio) "repetition," noun of action from iterare "to do again, repeat," from iterum "again, for the second time;" cf. Skt. itara- "the other (of the two), another."

Itaridan, from L. iter(um), Skt. itar(a-), as above, and Pers. dialects Kâšâni (Voništun) târ "the other;" Kurd. tir "the other" + -idan Pers. infinitive suffix.

iteration
  ایترش   
itareš

Fr.: itération   

A computational process involving a succession of approximations, which consists of repeating the operation by inputting the outcome of each preceding operation to improve the final result until a desired accuracy is achieved. Compare → repetition.

Verbal noun of → iterate.

iterative method
  روش ِ ایترشی   
raveš-e itareši

Fr.: méthode itérative   

A method of computation in mathematics using → iteration.

Iterative, characterized by or involving → iteration; → method.

Izar (ε Boötis)
  ایزار   
Izâr

Fr.: Izar   

A bright giant star in the constellation → Boötes lying 210 light-years away. It is a close double consisting of K0 and A0 dwarfs of magnitudes 2.5 and 4.6.

From Ar. Al-Izâr (الازار) "a cloth worn round the loins and passed between the legs," Ar. rendering of the Herdsman's skirt; → Boötes.

Jablonski diagram
  نمودار ِ یابلونسکی   
nemudâr-e Jablonski

Fr.: diagram de Jablonski   

An energy schematic representing the → electronic states of a → molecule and the → transitions between them. The vertical axis shows energies whereas → energy states are grouped horizontally according to their spin → multiplicity. Radiation-less transitions are symbolized by usual arrows, while → radiative transitions are represented by wavy arrows. The vibrational ground states of each electronic state are indicated with thick lines and the higher → vibrational states with thinner lines.

Named after Aleksander Jablonski (1898-1980), a Polish physicist who was an expert in the field of luminescence and atomic optics; → diagram.

Jacobi integral
  درستال ِ یاکوبی   
dorostâl-e Jacobi

Fr.: intégrale de Jacobi   

The integral admitted by the equations of a body of infinitesimal mass moving under the → gravitational attractions of two massive bodies, which move in circles about their → center of gravity. The Jacobi integral is the only known conserved quantity for the circular → restricted three-body problem. In the co-rotating system it is expressed by the equation: (1/2) (x·2 + y·2 + z·2) = U - CJ, where the dotted coordinates represent velocities, U is potential energy, and CJ the constant of integration (→ zero-velocity surface). The Jacobi integral has been used for two different purposes: 1) to construct surfaces of zero velocity which limit the regions of space in which the small body, under given initial conditions, can move, and 2) to derive a criterion (→ Tisserand's parameter) for re-identification of a → comet whose orbit has suffered severe perturbations by a planet. Also known as Jacobi constant.

Named after Karl Gustav Jacobi (1804-1851), a German mathematician who did important work on elliptic functions, partial differential equations, and mechanics; → integral.

Jacobian
  یاکوبی   
Jacobi

Fr.: jacobien   

Jacobian determinant, → Jacobian matrix.

Named after Karl Gustav Jacobi (1804-1851), a German mathematician who did important work on elliptic functions, partial differential equations, and mechanics. The "Jacobian" first appeared in an 1815 paper of the French mathematician Augustin Louis Cauchy (1789-1857), but Jacobi did write a detailed memoir about it in 1841.

<< < -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 > >>