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 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- 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 coo Cor Cor cor cos cos cos Cou cou Cra Cre cri cro cub cur cyc cyl Dan dat Dav de- Deb dec dec dee def deg del Den den der det deu dew dic dif dif dil Dip dir dis dis dis dis dis diu dod Dop dou Dra dua dus dwa dyn DZ Ear ecc eco edi EHB Ein ela ele ele ele ele ell eme emp end Eng ent epi equ equ era ESP eth Eur evi exa exc exe exi exp exp ext ext ext fac fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre fre Fro fun G s Gal gal gal Gar gau geg gen geo geo geo ger gla gly gra gra gra gra gra Gre gro GYR Had Hal hap Har HD hea hel hel Hen Her hex hig Hil hol Hoo hor hou Hub hum hyb hyd hyd hyp hys ide ign ima imp imp in- inc Ind ind ine inf inf inf ini ins ins ins int int int int Int int int int inv ion iri irr iso iso iso Jea Jor jum K c Kep Ker kin kno lab Lam Lan Lap las lat Le lef len lev lig lig lin lin lin liq Lit loc log lon lou LS lun lun Lym M s Mag 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 mod mol mon mor mov mul mur mys nan nat nav nec Nep neu New New NGC nob nom non non nor nos nuc nuc num nut obj obl obs occ oct off oli oni ope opp opt opt orb ord org orp osc out ove oxi P-w pal par par par par Pas pat pej per per per per per per pha Phe pho pho pho phy pin 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 Psa pul pum Q i qua qua qua qua R A rad rad rad rad rad rad Ram Ran rat rea rea rec rec red red ref ref reg rei rel rel rem rep res res res ret rev Rho Rie ril riv rog Ros rot rul S A Sag sam sat sca sca Sch Sco Sec sec sec seg sel sem sen set Sha sha shi sho sid sig sim sin Sir 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 sub 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 wha wid win WN3 Wol wri xen yok zen zij > >>

Number of Results: 13116 Search : far
Very Large Baseline Array (VLBA)
  آرست با پایه-خط ِ بسیار بزرگ   
ârast bâ pâye-xatt-e besyâr bozorg

Fr.: Very Large Baseline Array (VLBA)   

A network of ten 25-m radio telescopes for → very-long-baseline interferometry (VLBI), operated by the U.S. National Radio Astronomy Observatory. Eight of the VLBA telescopes are distributed across the continental United States, while the other two are in Hawaii and the Virgin Islands, giving a maximum baseline of about 8,000 km and a resolution better than a milliarcsecond at its shortest wavelength.

very; → large; → baseline; → array.

Very Large Telescope (VLT)
  تلسکوپ ِ بسیار بزرگ   
tleskop-e besyâr bozorg

Fr.: Très Grand Télescope, VLT   

An observing facility consisting of four 8.2 m telescopes, with the combined collecting area of a 16 m mirror, owned and operated by the European Southern Observatory at an altitude of 2635 m at the Paranal Observatory in Chile. The four reflecting unit telescopes are called Antu "Sun" in the language of Chile's indigenous Mapuche people, Kueyen "Moon," Melipal "Southern Cross," and Yepun "Venus." Each unit is equipped with several sophisticated instruments. The light of the individual telescopes can be combined using interferometric techniques to achieve superior resolution. → VLT Interferometer (VLTI). The wavelength range covered by the VLT is extremely wide, ranging from deep ultraviolet to mid-infrared.

very; → large; → telescope.

very late thermal pulse (VLTP)
  تپه‌ی ِ گرمای ِ بسیار دیر   
tape-ye garmâyi-ye besyâr dir

Fr.: flash de l'hélium très tardif   

In evolutionary models of → post-asymptotic giant branch stars, the occurrence of the helium shell burning when the star has reached the → white dwarf cooling track. This leads to the possibility of a violent → helium shell flash and expansion on a time-scale of ≤ 10 years. The rapid expansion and prompt change in surface composition observed in → Sakurai's Object are thought to be due to such a very late thermal pulse.

very; → late; → thermal; → pulse.

very low-mass star
  ستاره‌ی ِ بسیار کم‌جرم   
setâre-ye besyâr kamjerm

Fr.: étoile de très faible masse   

A star with a typical mass of one-hundredth of the mass of the Sun (→ solar mass) and a luminosity of about one-millionth that of the Sun (→ solar luminosity). Same as → brown dwarf.

very; → low; → mass; → star.

very massive star
  ستاره‌ی ِ بسیار پرجرم   
setâre-ye besyâr porjerm

Fr.: étoile très massive   

A star of mass around 100 → solar masses. See also: → supermassive star, → massive star, → canonical upper limit.

very; → massive; → star.

very small grain (VSG)
  دانه‌ی ِ بسیار کوچک   
dâne-ye besyâr kucak

Fr.: très petit grain   

A special type of carbonaceous → interstellar dust grains with a size ranging from 10 to 150 Å and consisting of tens to hundreds of atoms. In contrast to → big grains, VSGs are not in → thermal equilibrium. They can be heated to very high temperatures (~ 1000 K) by the absorption of a single photon. It is thought that VSGs are clusters of → PAH.

very; → small; → grain.

very-long-baseline interferometry (VLBI)
  اندرزنش‌سنجی با پایه-خط ِ بسیار بزرگ   
andarzanešsanji bâ pâye-xatt-e besyâr bozorg

Fr.: interférométrie à très longue base   

A technique in radio interferometry in which the individual telescopes are not directly connected together, but instead make their observations separately with very accurate timings. The data are later sent to a central correlator to be combined. With this technique the individual telescopes can be arbitrarily far apart, and so the technique provides the highest resolution images in astronomy, typically down to a few milliarcseconds.

very; → large; → baseline; → interferometry.

vessel
  ۱) رگ؛ ۲) آوند   
1) rag (#); 2) âvand

Fr.: vaisseau   

1) A tube or duct, as an artery or vein, containing or conveying blood or some other body fluid.
2) Botany: A duct formed in the xylem, composed of connected cells that have lost their intervening partitions, that conducts water and mineral nutrients (Dictionary.com).

M.E., from O.Fr. vessel "container, receptacle; ship," from L.L. vascellum "small vase or urn," also "a ship," alteration of L. vasculum, diminutive of vas "vessel."

1) Rag "blood vessel, vein; lineage, race, stock," from Mid.Pers. rag, from Proto-Iranian *raha-ka-, from *raha- "liquid, essence," + suffix -ka-; cf. Av. ranhā- "name of a mythical stream;" Skt. rása- "juice (of plants), liquid, essence," rásavant-, rasin- "juicy;" L. ros "dew;" Lith. ràsa "dew;" O.C.S. rosa "dew."
2) Âvand "vessel," contraction of âbvand, literally "water utensil," from âb, → water, + vand "vessel, vase, cup," from bastan "to bind, shut," → shutter.

vibrate
  شیویدن   
šividan (#)

Fr.: vibrer   

To oscillate with a continuing periodic change relative to a fixed reference point or state of equilibrium. → oscillate.

From L. vibratus, p.p. of vibrare "to move quickly to and fro, shake" (cf. Lith. wyburiu "to wag the tail," Dan. vippe, Du. wippen "to swing," O.E. wipan "to wipe").

Šividan "to vibrate, move to and fro, to tremble," related to šodan, šow- "to go; to become;" Av. šiyav-, š(ii)auu- "to move, go," šiyavati "goes," šyaoθna- "activity; action; doing, working;" O.Pers. šiyav- "to go forth, set," ašiyavam "I set forth;" Skt. cyu- "to move to and fro, shake about; to stir," cyávate "stirs himself, goes;" Gk. kinein "to move;" Goth. haitan "call, be called;" O.E. hatan "command, call;" PIE base *kei- "to move to and fro."

vibration
  شیوش   
šiveš (#)

Fr.: vibration   

1) The act of vibrating. The state of being vibrated.
2) A continuing → periodic  → oscillation relative to a fixed reference point or → equilibrium state.

Verbal noun from → vibrate.

vibrational
  شیوشی   
šiveši (#)

Fr.: vibrationnel   

Of or pertaining to → vibration. → vibrational mode.

vibration; → -al.

vibrational energy
  کاروژ ِ شیوشی   
kâruž-e šiveši

Fr.: énergie de vibration, ~ vibratoire   

The energy due to the vibration of the molecules making up atoms (→ molecular vibration). A molecule in space can have energies in various forms: → rotational energy, vibrational energy, or electronic energy. These energies of molecules are → quantized and a particular molecule can exist in different rotational and vibrational → energy levels. The molecules can move from one level to another level only by a jump involving a finite amount of energy. → Quantum mechanics predicts that any molecule can never have zero vibrational energy, that is atoms can never be completely at rest relative to each other. The harmonically oscillating molecules can undergo vibrational changes determined by simple selection rules obtained from → Schrödinger equation.

vibrational; → energy.

vibrational frequency
  بسامد ِ شیوشی   
basâmad-e šiveši (#)

Fr.: fréquence de vibration, ~ vibrationnelle   

The frequency at which the atoms in a molecule vibrate. The frequencies of → molecular vibrations in diatomic molecules are in the order of 10-12 to 10-14 Hz. In such molecules, the only → vibrational mode available is along the bond. More complicated molecules have many types of vibration and stretching modes.

vibrational; → frequency.

vibrational mode
  ترز ِ شیوشی   
tarz-e šiveši

Fr.: mode de vibration, ~ vibratoire   

Any of the ways in which a → molecule vibrates. Each vibrational mode has a different → frequency frequency. The number of vibrational modes of a molecule is determined by the number of atoms in it. The number of vibrational modes for a non-linear molecule is 3N - 6, where N is the number of atoms making up the molecule. For a linear molecule it is 3N - 5.

vibrational; → mode.

vibrational transition
  گذرش ِ شیوشی   
gozareš-e šiveši

Fr.: transition vibrationnelle   

A transition between two → quantized  → levels of a → molecule that have different vibrational energies.

vibrational; → transition.

vibrational-rotational transition
  گذرش ِ چرخشی-شیوشی   
gozareš-e carxeši-šiveši

Fr.: transition vibrationnelle-rotationnelle   

A slight change in the → energy level of a → molecule due to → vibrational transition and/or → rotational transition.

vibrational; → rotational; → transition.

victim
  لیشه   
lišé

Fr.: victime   

A person or thing that suffers harm or death, from another or from some adverse act or circumstance.

M.Fr. victime, from L. victima "sacrificial animal."

Lišé, from Mid.Pers. lyš- / rêš- "to wound, hurt;" Pers. riš, rêš "wound;" Av. raēš- "to get hurt, suffer damage;" cf. Skt. reṣ "to get harmed."

Victorian period
  دوره‌ی ِ ویکتوریایی   
dowre-ye Viktoriyâ-yi

Fr.: période victorienne   

A series of 532 years, arising from the cycles of the Sun and Moon multiplied into one another. It was used by the Western churches for many years, in computing the time of Easter, till the → Gregorian calendar was established.

Named after Victorius (a French clergyman), who invented the period about the middle of the 5th century.

video
  ۱) دیداره؛ ۲) دیداری   
1) didâré; 2) didâri

Fr.: vidéo   

1) (n.) The visual part of a television broadcast.
Something that has been recorded on videotape, especially a movie or music performance.
2) (adj.) Of or pertaining to the electronic apparatus for producing the television picture.

From L. video "I see," from viderevision.

Didâré, didâri, from didâr "vision, sight," verbal noun 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").

Vietnamese calendar
  گاهشمار ِ ویتنامی   
gâhšomâr-e Vietnâmi

Fr.: calendrier vietnamien   

A → lunisolar calendar used now in Vietnam mainly for determining seasonal holidays and cultural events. It is in fact the → Chinese calendar computed for Hanoi. It has 12 months of 29 or 30 days each (→ synodic month) and the year totals 355 days. The → lunar year is therefore 11 days shorter than its solar counterpart. To keep up with the solar pace, every 19 years seven extra months are added to the calendar. In practice, approximately every third year an → embolismic month is included. The New Year, called Tet, begins at the second → new moon after the → winter solstice. The Vietnamese calendar has some minor differences with the Chinese calendar. For example, it uses the cat and buffalo instead of the Chinese rabbit and cow respectively in the → zodiac.

From Vietnam "Viets of the South," from Viet the people's name + nam "south;" → lunar; → calendar.

<< < -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- 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 coo Cor Cor cor cos cos cos Cou cou Cra Cre cri cro cub cur cyc cyl Dan dat Dav de- Deb dec dec dee def deg del Den den der det deu dew dic dif dif dil Dip dir dis dis dis dis dis diu dod Dop dou Dra dua dus dwa dyn DZ Ear ecc eco edi EHB Ein ela ele ele ele ele ell eme emp end Eng ent epi equ equ era ESP eth Eur evi exa exc exe exi exp exp ext ext ext fac fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre fre Fro fun G s Gal gal gal Gar gau geg gen geo geo geo ger gla gly gra gra gra gra gra Gre gro GYR Had Hal hap Har HD hea hel hel Hen Her hex hig Hil hol Hoo hor hou Hub hum hyb hyd hyd hyp hys ide ign ima imp imp in- inc Ind ind ine inf inf inf ini ins ins ins int int int int Int int int int inv ion iri irr iso iso iso Jea Jor jum K c Kep Ker kin kno lab Lam Lan Lap las lat Le lef len lev lig lig lin lin lin liq Lit loc log lon lou LS lun lun Lym M s Mag 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 mod mol mon mor mov mul mur mys nan nat nav nec Nep neu New New NGC nob nom non non nor nos nuc nuc num nut obj obl obs occ oct off oli oni ope opp opt opt orb ord org orp osc out ove oxi P-w pal par par par par Pas pat pej per per per per per per pha Phe pho pho pho phy pin 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 Psa pul pum Q i qua qua qua qua R A rad rad rad rad rad rad Ram Ran rat rea rea rec rec red red ref ref reg rei rel rel rem rep res res res ret rev Rho Rie ril riv rog Ros rot rul S A Sag sam sat sca sca Sch Sco Sec sec sec seg sel sem sen set Sha sha shi sho sid sig sim sin Sir 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 sub 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 wha wid win WN3 Wol wri xen yok zen zij > >>