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

<< < -en ear eav ecl Edd eff Ein eje ele ele ele ele ell emb emi Enc ene ens eph EPR equ equ eru eth Eul eve evo exc exc exi exo exp exp ext ext > >>

Number of Results: 696
evection
  اسبز   
osbaz

Fr.: évection   

A periodic perturbation in the motion of the → Moon caused by the variation in the gravitational pull of the Sun, which causes a change in the → eccentricity of the Moon's orbit during its monthly revolution. As a result, the Moon's → ecliptic longitude oscillates with a amplitude of ± 1°16' during a period of about 31.8 days.

From L. evection- "carrying away, going upwards, flight," from evect(us) p.p. of evehere "to carry forth, move forth," from e-, → ex- + vehere "to carry," cognate with Av. vaz- "to carry, move," as below.

Osbaz "carrying away," from os-, → ex-, + *baz "to carry," ultimately from Proto-Ir. *uaz- "to carry, drive;" from which Av. vaz- "to move, carry, drive (a chariot)," vazaiti "to lead;" Kurd. (Kurmanji) bazin/baz- "to run;" Mod./Mid.Pers. bazidan, vazidan "to blow (as the wind)," parvâz, → flight; cf. Skt. vah- "to ride, drive, transport;" Gk. oxos "carriage;" L. vehere "to carry;" Lith. veži "I ride;" O.H.G. wegan "to move, carry;" PIE base *wegh- "to go, carry, drive." See also: → advection; → convection.

even parity
  همالی ِ زوج   
hamâli-ye zowj

Fr.: parité paire   

A classical variable which does not change upon spatial inversion, such as time, energy, angular momentum and so on. → odd parity.

Even, from O.E. efen "level; equal," from P.Gmc. *ebnaz (cf. Ger. eben; Goth. ibns); → parity.

Hamâli, → parity; zowj "pair, couple; an even number," from Ar.

evening
  ایوار   
ivâr (#)

Fr.: soir, soirée   

The latter part of the → day and early part of the → night. Not an astronomical term proper. → evening star.

From O.E. verb æfnung "to grow toward evening," from æfnian "to become evening," from æfen "evening," from P.Gmc. *æbando- (cf. O.H.G. aband, Ger. abend).

Ivâr "evening" (Lori, Laki êvâra; Borujerdi ivâra; Kurd. ewâra); Mid.Pers. êwârak "evening," ultimately from Proto-Ir. *upa-ayara- "end of the day," from *upa- "up, on," + *ayara- "day;" cf. Av. ayar- (aiiar-) "day;" Shughni, Roshani, Bartangi prefixed (*api-) biyôr, Sariqoli biyur "yesterday;" PIE *ayer- "day, morning;" cf. Gk. eerios "at breakfast," ariston "breakfast;" Du. eer, Ger. eher "earlier;" E. ere "soon, before (in time)."

evening star
  ستاره‌ی ِ شامگاه   
setâre-ye šâmgâh (#)

Fr.: étoile du soir   

Any bright → planet, often → Venus, seen low in the western sky after → sunset. → Hesperus.

evening; → dusk; → star.

event
  رویداد   
ruydâd (#)

Fr.: événement   

1) General: Something that happens or is regarded as happening; an occurrence, especially one of some importance.
2) Einstein's relativity: An occurrence in the → space-time continuum referenced by three spatial coordinates and a complementary temporal ordinate. → world line; → space-time diagram.
3) Statistics: A subset of the → sample space.

From M.Fr. event, from L. eventus "occurrence, issue," from evenire "to come out, happen, result," from → ex- "out" + venire "to come," from PIE base *gwem- "to go, come;" cf. Mod/Mid.Pers. gâm "step, pace;" O.Pers. gam- "to come; to go;" Av. gam- "to come; to go," jamaiti "goes;" Mod.Pers. âmadan "to come;" Skt. gamati "goes;" Gk. bainein "to go, walk, step;" L. venire "to come;" Tocharian A käm- "to come;" O.H.G. queman "to come;" E. come.

Ruydâd, noun from ruy dâdan "to occur, happen," originally "to appear," from ruy "face; aspect; appearance" (Mid.Pers. rôy, rôdh "face;" Av. raoδa- "growth," in plural "appearance," from raod- "to grow, sprout, shoot;" cf. Skt. róha- "rising, height") + dâdan "to give; to command" (Mid.Pers. dâdan "to give;" O.Pers./Av. dā- "to give, grant, yield," dadāiti "he gives;" cf. Skt. dadáti "he gives;" Gk. didomi "I give;" L. dare "to give, offer," facere to make;" PIE base *do- to give").

event horizon
  افق ِ رویداد   
ofoq-e ruydâd (#)

Fr.: horizon d'événement   

1) The surface surrounding a → black hole with the property that any light ray emitted inside it cannot escape to the outer space because of the strength of the → gravitational field. The radius of the event horizon is called the → Schwarzschild radius. See also → photon sphere.
2) For an observer A at the instant t0, the surface in the → space-time that divides the collection of all events into two non-empty classes: those events that have been, are being, or will be observed by A, and those that A has never observed and will never be able to observe (J. Plebanski, A. Krasinski, 2006, An Introduction to General Relativity and Cosmology, Cambridge Univ. Press).

event; → horizon.

Event Horizon Telescope (EHT)
  تلسکوپ ِ افق ِ رویداد   
Teleskop-e Ofoq-e Ruydâd

Fr.: Télescope de l'horizon des évènements   

An international collaboration using a → very-long-baseline interferometry (VLBI) array comprising millimeter- and → submillimeter- wavelength telescopes separated by distances comparable to the diameter of the Earth. At a nominal operating wavelength of ~1.3 mm, the EHT → angular resolution (λ/D) is ~25 μas (→ micro- → arcseconds), which is sufficient to resolve nearby → supermassive black hole candidates on spatial and temporal scales that correspond to their → event horizons. EHT observations toward the elliptical → galaxy M87 succeeded in obtaining the first ever image of its supermassive black hole (EHT Collaboration, 2019, ApJL 875, L1-L6). The telescopes contributing to this result were ALMA, APEX, the IRAM 30-m telescope, the James Clerk Maxwell Telescope, the Large Millimeter Telescope Alfonso Serrano, the Submillimeter Array, the Submillimeter Telescope, and the South Pole Telescope. Petabytes of raw data from the telescopes were combined by highly specialized supercomputers hosted by the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory. The construction of the EHT and the M87 black hole observation result from decades of observational, technical, and theoretical work in close collaboration by researchers from around the world. Thirteen partner institutions worked together to create the EHT, using both pre-existing infrastructure and support from a variety of agencies. Key funding was provided by the US National Science Foundation (NSF), the EU's European Research Council (ERC), and funding agencies in East Asia.

event; → horizon; → telescope.

ever-expanding Universe
  گیتی ِ هماره‌سپانا   
giti-ye hamâré sopânâ

Fr.: Univers en expansion continue   

Same as → accelerating Universe.

expand; → Universe.

evidence
  آویشه   
âvišé

Fr.: évidence, preuve   

That which tends to prove or disprove something; something that makes plain or clear.

Noun form of → evident.

Âvišé, from âviš, → evident + noun suffix , Mid.Pers. -ak/-ag.

evident
  آویش   
âviš

Fr.: évident   

Plain or clear to the sight or understanding.

From L. evidentem (nom. evidens) "perceptible, obvious," from → ex- "fully, out of" + videntem (nom. videns), pr.p. of videre "to see," from PIE base *weid- "to know, to see;" cf. Mod.Pers. bin- "to see" (present stem of didan); Mid.Pers. wyn-; O.Pers. vain- "to see;" Av. vaēn- "to see;" Skt. veda "I know;" Gk. oida "I know," idein "to see;" O.E. witan "to know;" Goth. weitan "to see;" E. wise; Ger. wissen "to know;" Lith. vysti "to see;" Rus. videt' "to see," vest' "news."

Âviš, from Av. āviš, āuuiš "evidently, before the eyes," āuuišiia- "manifest;" Mid.Pers. âškârâg "manifest;" Mod.Pers. âškâr (Proto-Iranian *āuiš-kâr); Arm. loanword from Iranian aškaray "open, not hidden;" cf. Skt. āvis "evidently, before the eyes;" O.C.S. (j)avé "manifest, known" (loanword from Iranian); L. audire "to hear;" Gk. aisthanesthai "to feel."

evocation
  زاوچ   
zâvac

Fr.: évocation   

The act or fact of evoking.

Verbal noun of → evoke.

evoke
  زاوچیدن   
zâvacidan

Fr.: évoquer   

1) To call up or produce (memories, feelings, etc.).
2) To elicit or draw forth (Dictionary.com).

From Fr. évoquer or directly from L. evocare "call out, rouse, summon," from → ex- "out" + vocare "to call," → voice .

Zâvacidan, from zâ-, → ex-, + vacidan "to call," → convoke.

evolution
  فرگشت   
fargašt (#)

Fr.: évolution   

Any process of formation or growth; development; a process of gradual, progressive change; a product of such development; something evolved.
Astro.: A continuous and progressive change according to certain laws and by means of acting physical forces.
Biology: A process of development in which a living organism, through major environmental changes, becomes more and more complex by the differentiation of its parts.

Verbal noun of → evolve.

evolutionary
  فرگشتی   
fargašti (#)

Fr.: évolutif   

Of, pertaining to, or in accordance with a theory of evolution.

Adjective of → evolution.

evolutionary mass
  جرم ِ فرگشتی   
jerm-e fargašti (#)

Fr.: masse évolutive   

The stellar mass based on → effective temperature and → luminosity, as derived from → evolutionary tracks.

evolutionary; → mass.

evolutionary model
  مدل ِ فرگشت   
model-e fargašt (#)

Fr.: modèle d'évolution   

A model, based on theoretical calculations, which predicts the behavior of an astronomical entity (stars, galaxies, Universe) over time.

evolutionary; → model.

evolutionary stage
  گامه‌ی ِ فرگشت   
gâmeye fargašt

Fr.: étape d'évolution   

A particular step or phase in the evolution of an astronomical object.

evolutionary; → stage.

evolutionary time scale
  زمان-مرپل ِ فرگشت   
zamân-marpel-e fargašt

Fr.: échelle de temps d'évolution   

The characteristic time it takes an evolving astronomical object to pass from a step to another.

evolutionary; → time scale.

evolutionary track
  تر ِ فرگشت   
tor-e fargašt

Fr.: trajet évolutif   

In a theoretical → Hertzsprung-Russell diagram, the path taken by an evolving star.

evolutionary; → track.

evolve
  فرگشتن، فرگشت کردن   
fargaštan (#), fargašt kardan (#)

Fr.: évoluer   

To come forth gradually into being; undergo evolution.
Astro.: To change with time by the action of varying physical conditions.
Biology: To develop by a process of evolution to a different adaptive state or condition.

L. evolvere "to unroll, open, unfold," from → ex- "out" + volvere "to roll, turn, twist;" PIE base *wel- "to turn, revolve;" cf. Skt. valate "turns round;" Gk. eilein "to turn, squeeze," helix "spiral object;" O.H.G. walzan "to roll, waltz;" Lith. valtis "twine, net," apvalus "round;" O.E. wealwian "to roll (in mud);" Welsh olwyn "wheel."

Fargaštan, fargašt kardan, from fargašt, from far- "forward" (Mid.Pers. fra- "forward, before; much; around;" O.Pers. fra- "forward, forth;" Av. frā, fərā-, fra- "forward, forth; excessive;" cf. Skt. prá- "before; forward, in fron;" Gk. pro "before, in front of;" L. pro "on behalf of, in place of, before, for;" PIE *pro-) + gašt, present stem of gaštan, gardidan "to change; to turn" (Mid.Pers. vartitan; Av. varət- "to turn, revolve;" cf. Skt. vartati; L. vertere; O.H.G. werden "to become;" PIE *werto, *wer-).

<< < -en ear eav ecl Edd eff Ein eje ele ele ele ele ell emb emi Enc ene ens eph EPR equ equ eru eth Eul eve evo exc exc exi exo exp exp ext ext > >>