An Etymological Dictionary of Astronomy and Astrophysics

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory



<< < -ph pal pap par par par par pat pec pen per per per per per PG pha pho pho pho phy pie Pit Pla pla pla pla ple Poi pol pol pol pol pop pos pos pow pre pre pre pre pri pri pri pro pro pro pro pro pro pro pub pul pyr > >>

Number of Results: 1068
  فرکشنیدن، فرکشن کردن   
farkašanidan, farkašan kardan

Fr.: promouvoir   

1) To further or encourage the progress or existence of.
2) To raise to a higher rank, status, degree, etc.
3) (Education) To advance (a pupil or student) to a higher course, class, etc.
4) To urge the adoption of; work for.
5) (Marketing) To encourage the sale of (a product) by advertising or securing financial support (

M.E. promoten, from O.Fr. promoter and directly from L. promotus, p.p. of promoverepro- "forward" + movere "to → move."

Farkašanidan, farkašan kardan, verb from farkašan, → promotion.


Fr.: promotion   

1) The act of promoting someone to a higher job, grade, or rank, or the fact of being so promoted.
2) Support or encouragement of the progress, growth, or acceptance of something.
3) An act, event, or offer that helps to increase interest in or demand for something (

Verbal noun of → promote.

Farkašan, literally "draw forward, pull up," from far-, variant of farâ-, → pro-, + kašan "drawing, pull," from kaš present stem of kašidan, → galaxy, + noun suffix -an.

  تند، بی‌درنگ   
tond (#), biderang (#)

Fr.: rapide, instantané, prompt   

Quick, at once or without delay.

M.E., from O.Fr. prompt, from L. promptus "brought forth, ready, quick," p.p. of promere "to bring forth," from → pro- "forward" + emere "to take."

Tond, "swift, rapid, brisk; fierce, severe," Mid.Pers. tund "sharp, violent;" Sogdian tund "violent;" cf. Skt. tod- "to thrust, give a push," tudáti "he thrusts;" L. tundere "to thrust, to hit" (Fr. percer, E. pierce, ultimately from L. pertusus, from p.p. of pertundere "to thrust or bore through," from per- + tundere, as explained); PIE base *(s)teud- "to thrust, to beat."
Biderang "without delay," from bi- negation prefix, → in-, + derang, → delay.

prompt neutrons
  نوترون‌های ِ تند   
notronhâ-ye tond (#)

Fr.: neutrons instantanés   

Neutrons emitted immediately by a nucleus undergoing fission, as opposed to → delayed neutrons, which are emitted by one of the fission products an appreciable time interval after the fission event (from a few milliseconds to a few minutes).

prompt; → neutron.

prompt supernova explosion
  اسکفت ِ تند ِ نو‌اختر، ~ بی‌درنگ ِ ~   
oskaft-e tond-e abar-now-axtar, ~ biderang-e ~

Fr.: explosion rapide de supernova   

A mechanism predicted by theoretical models of → supernova explosion in the case when the → supernova shock breaks through the outer edge of the collapsing → iron core before losing all of its energy (through → photodisintegration of the iron nuclei) and manages to expel the stellar envelope. Compare with → delayed supernova explosion.

prompt; → supernova; → explosion. See also → delay.


Fr.: pronom   

A grammatical element which replaces a noun previously mentioned.

From M.Fr. pronom, from L. pronomen, from → pro- "in place of" + nomen, → name.

Farânâm, literally "noun (put) forth (to replace)," from farâ- "forward, along, opposing, facing," → pro- + nâm, → name.


Fr.: prononcer   

1) To enunciate or articulate (sounds, words, sentences, etc.).
2) To utter or sound in a particular manner in speaking:

pro-; → announce.


Fr.: prononciation   

1) The act or result of producing the sounds of speech, including articulation, stress, and intonation, often with reference to some standard of correctness or acceptability.
2) An accepted standard of the sound and stress patterns of a syllable, word, phrase, etc.(

Verbal noun of → pronounce.


Fr.: preuve   

1) A particular piece of evidence that is sufficient to show or helps to establish a fact.
2) The establishment of the truth of anything; demonstration.
3) Math. Logic: A sequence of statements that establishes the truth of a proposition.

M.E. prove, prooff, prof, proufe, O.Fr. prueve, from L.L. proba "a proof," a back-formation from L. probare "to prove," from probus "worthy, good, upright," from PIE *pro-bhwo- "being in front," from → pro- + *bhu- "to be;" cf. Pers. budan "to be," → condition.

Âvin, on the model of Ger. Beweis "proof," from weisen "to show, point out;" O.E. witan "to see." âvin "to show, see," from intensive prefix â- + vin "to see" (as in a large number of dialects), variant bin, present stem of didan "to see;" Mid.Pers. wyn-; O.Pers. vain- "to see;" Av. vaēn- "to see;" cf. Skt. veda "I know;" Gk. oida "I know," idein "to see;" L. videre "to see;" Ger. weisen "to show," as above; PIE base *weid- "to know, to see."


Fr.: propagande   

Information, ideas, or rumors deliberately spread widely to help or harm a person, group, movement, institution, nation, etc. (

From N.L. propaganda, short for Congregatio de Propaganda Fide, "congregation for propagating the faith," a committee of cardinals established in 1622 by Gregory XV to supervise foreign missions, from L. propagare, → propagate.

Farâtucân, from prefix farâ-, → pro-, + tucân from tucidan, → propagate.

  ۱) توچیدن؛ ۲) توچاندن   
1) tucidan; 2) tucândan

Fr.: 1) se propager; 2) propager   

1) v.intr.: (of → electromagnetic waves, → compression waves, etc.) To travel through space or a physical → medium.
2) To create (an effect) at a distance, as by electromagnetic waves, compression waves, etc., traveling through space or a physical medium.

From L. propagatus, p.p. of propagare "multiply plants by layers, spread for sprouting, propagate, enlarge," from propag(es) "something set out, scion, slip," from → pro- "forth" + pag base of pangere "to fasten" + es noun suffix + -atus "-ate."

Tucidan, from several dialects: Malayeri "to scatter, disperse; to diffuse;" Lori tic "scattered, dispersed," ticene "to scatter, disperse; to diffuse;" Laki tvic "dispersed, scattered;" Aligudarzi tij "scattered, dispersed;" Borujerdi tuc "scatter," tucessan "to scatter, diffuse," tucesa "dispersed, scattered, diffused;" probably related to Proto-Ir. θrāš- "to scatter, spread, strew" cf. Yaghnobi côš- "to spread, scatter, sow," tiráš-, têráš-, tirayš-/tirášta "to fall (down, off); to become ill; to drop;" (+*ui- ?) Ossetic .I. irtasyn/irtæst, D. ærtasun/ærtast "to separate, distinguish; to take away; to choose;" Sogd. š'š "to scatter, disperse;" šyš- "to be scattered" (Cheung, 2007)


Fr.: propagation   

Physics: The act or process of propagating, especially the process by which a disturbance, such as the motion of electromagnetic or sound waves, is transmitted through a medium such as air or water. Linguistically related notions: → diffusion (پخش); → dispersion(پاشش); → scattering (پراکنش); → diffraction (پراش).

Verbal noun of → propagate.

propagation number
  عدد ِ توچش   
'adad-e tuceš

Fr.: nombre d'onde   

A parameter, denoted k = 2π/λ, that along with the → angular frequency, ω = 2πν, is used to express the equation of → simple harmonic motion, y = cos (ωt - kx + π/2). Same as → wave number.

propagation; → number.

pišrândan (#)

Fr.: propulser   

To drive, or cause to move, forward or onward.

From L. propellere "to push forward," from → pro- "forward" + pellere "to push, drive."

Pišrândan, from piš "before; in front," from Mid.Pers. pêš "before, earlier," O.Pers. paišiya "before; in the presence of" + rândan "to push, drive, cause to go," causative of raftan "to go, walk, proceed" (present tense stem row-, Mid.Pers. raftan, raw-, Proto-Iranian *rab/f- "to go; to attack").

pišrâné (#)

Fr.: propulseur   

A propelling agent. A substance, usually a mixture of fuel and oxidizer, for propelling a rocket.

From → propel + suffix -ant.

Pišrâné, from pišrândan, → propel.

saré (#)

Fr.: propre   

Belonging or pertaining exclusively or distinctly to a person, thing, or group. → proper mass; → proper motion; → proper time.

M.E., from O.Fr. propre, from L. proprius "one's own."

Saré "pure; principal."

proper distance
  اپست ِ سره   
apest-e saré

Fr.: distance propre   

A distance between two nearby events in the frame in which they occur at the same time. It is the distance measured by a ruler at the time of observation. Hence, for a cosmological time t, Dproper = DC . a(t), where DC is the → comoving distance, and a(t) is the → scale factor. In the present epoch a = a(tobs) = 1, and Dproper = DC.

proper; → distance.

proper mass
  جرم ِ سره   
jerm-e saré

Fr.: masse propre   

Same as → rest mass.

proper; → mass.

proper motion
  جنبش ِ سره   
jonbeš-e saré

Fr.: mouvement propre   

The apparent motion of a star across the sky (not including a star's parallax), arising from the star's velocity through space with respect to the Sun. Proper motion is usually tabulated in star catalogs as changes in right ascension and declination per year or century. See also: → proper motion distance.

proper; → motion.

proper motion distance
  دورای ِ جنبش ِ سره   
durâ-ye jonbeš-e saré

Fr.: distance mouvement propre   

The distance derived from the → proper motion of an object. If an object has a known → transverse velocity  u, and has an observed angular motion of dθ/dt, then the proper motion distance is defined as: d = u/(dθ/dt).

proper; → motion; → distance

<< < -ph pal pap par par par par pat pec pen per per per per per PG pha pho pho pho phy pie Pit Pla pla pla pla ple Poi pol pol pol pol pop pos pos pow pre pre pre pre pri pri pri pro pro pro pro pro pro pro pub pul pyr > >>