An Etymological Dictionary of Astronomy and Astrophysics
English-French-Persian

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 466 Search : pH
echelle spectrograph
  بیناب‌نگار ِ نرده‌ای   
binâbnegâr-e narde-yi (#)

Fr.: spectrographe à échelle   

A spectrograph that uses an echelle grating to disperse the light.

echelle grating; → spectrograph.

ecosphere
  بوم‌سپهر   
bumsepehr (#)

Fr.: écosphère   

The space around a star in which a planet would experience external conditions that are not incompatible with the existence of life.

Ecosphere, from eco-, → ecology, + → sphere.

Bumsepehr, from bum "eco-," → ecology, + sepehr, → sphere.

elephant trunk
  خرطوم ِ فیل   
xortum-e fil

Fr.: trompe d'éléphant   

An elongated structure of → interstellar dust and gas which absorbs the radiation from background stars in an → H II region. These structures are the denser remnants of → molecular clouds from which → massive stars are formed. Elephant trunks are eventually dissipated by the action of the → ionizing radiation and → stellar wind of the associated massive stars. A remarkable example of these structures is displayed by the → HST image of the → Eagle Nebula as → pillars of obscuring matter protruding from the interior wall of a dark molecular cloud. Some → Bok globules may represent the remaining densest fragments of elephant trunks.

M.E. elephant, from O.Fr. olifant, from L. elephantus, from Gk. elephas "elephant, ivory," probably from a non-I.E. language, likely via Phoenician; trunk, from M.E. trunke, O.Fr. tronc, from L. truncus "stem, trunk, stump."

Xortum "the proboscis of an elephant," loanword from Ar. xartum; fil, pil "elephant," from Mid.Pers. pil "elephant;" O.Pers. piru- "ivory."

Elephant's Trunk Nebula
  میغ ِ خرطوم ِ فیل   
miq-e xortum-e fil

Fr.: Nébuleuse de la trompe d'éléphant   

An elongated dark structure of gas and dust in the → H II region IC 1396. It spans about 5 degrees on the sky in the constellation → Cepheus, about 2400 → light-years from the Earth. The Elephant Trunk Nebula is believed to be site of star formation, containing several very young stars. It is an example of → elephant trunks associated with star forming regions.

elephant trunk; → nebula.

emphasis
  براوژ   
barâvaž

Fr.: accentuation, accent   

Special stress laid upon, or importance attached to (Dictionary.com).

From L. emphasis, from Gk. emphasis "significance, implied meaning," from emphainein "to show, indicate," from en "in" + phainein "to show." It developed a sense of "extra stress" laid on a word or words to make the significance clear, or to show their importance.

Barâvaž, present stem of barâvažidan, literally "to speak loudly," from bar- "on, upon, up," → over-, + âvaž variant of âvâz "voice, sound, noise, clamour," cf. Sariqoli awuj "voice, sound," Wakhi awôγ "voice, sound," related to vâž, → word.

emphasize
  براوژیدن   
barâvažidan

Fr.: appuyer sur, insister sur, souligner   

To give → emphasis to; lay stress upon; stress (Dictionary.com).

emphasis + → -ize.

emphatic
  براوژی   
barâvaži

Fr.: énergique, catégorique   

1) Uttered, or to be uttered, with emphasis; strongly expressive.
2) Using emphasis in speech or action (Dictionary.com).

From Gk. emphatikos, variant of emphantikos, from emphainein, → emphasis.

Barâvaži, from barâvaž + -i adj. suffix.

empty graph
  نگاره‌ی ِ تهی   
negâre-ye tohi

Fr.: graphe vide   

In → graph theory, a graph with any number of → vertices which do not have → edges.

empty; → graph.

endomorphism
  درون-ریخت‌مندی   
darun-rixtmandi

Fr.: endomorphisme   

A → morphism from an → object to itself.

endo-; → morphism.

ephemeris
  روزیج   
ruzij

Fr.: éphéméride   

A table of computed positions occupied by a celestial body over successive intervals of time such as daily; plural ephemerides.

From L. ephemeris "day book, diary," from Gk. ephemeris "diary, account book," from ephemeros "short-lived, lasting but a day," from → epi "on, upon" + hemerai, dative of hemera "day."

Ruzij, from ruz, → day + zij "astronomical table," from Mid.Pers. zig "astronomical table," originally "string," since the lines of a table were compared to strings used on a weaver's instrument, variant zih, meaning "cord, string" (Modern Persian zeh "cord, string"); Av. jiiā- "bow-string;" cf. Skt. jiyā- "bow-string;" PIE base *gwhi- "thread, tendon" (from which derive also Gk. bios "bow;" L. filum "thread;" Russ. žca "thread").

ephemeris day
  روز ِ روزیجی   
ruz-e ruziji

Fr.: jour des éphémérides   

86,400 → ephemeris seconds.

ephemeris; → day.

ephemeris meridian
  نیمروزان ِ روزیجی   
nimruzân-e ruziji

Fr.: méridien des éphémérides   

A fictitious meridian that rotates independently of the Earth at the uniform rate implicitly defined by → Terrestrial Dynamical Time (TDT).

ephemeris; → meridian.

ephemeris second
  ثانیه‌ی ِ روزیجی   
sâniye-ye ruziji

Fr.: seconde des éphémérides   

The length of a tropical second (1/31,556,925.97474 of the tropical year) on 1900 January 0.5 → ephemeris time.

ephemeris; → second.

ephemeris time (ET)
  زمان ِ روزیجی   
zamân-e ruziji

Fr.: Temps des éphémérides   

The uniform time-scale used as the independent variable to calculate the orbits in the solar system prior to 1984. Ephemeris Time was adopted in 1960 to deal with irregularities in the → Earth's rotation that had been found to affect the course of mean solar time. The definition of Ephemeris Time is based on Newcomb's analytical theory of the Earth's motion around the Sun (Newcomb 1898), according to which the geometric mean longitude of the Sun with respect to the Earth-Moon barycenter is expressed by:
L = 279° 41' 48".04 + 129 602 768".13 T + 1''.089 T2,
where L refers to the → mean equinox of date while T measures time from noon 1900 January 0 GMT in Julian centuries of 36525 days. Ephemeris Time is therefore defined as the instant near the beginning of the calendar year A.D. 1900 when the mean longitude of the Sun was 279° 41' 48''.04, at which instant the measure of ET was 1900 January 0, 12h precisely. In this system the fundamental unit was the → ephemeris second, which was defined so that the → tropical year at the epoch 1900.0 should be exactly 31 556 925,9747 seconds of ephemerides. Ephemeris Time was inconvenient in many ways and was supeseded with the → Terrestrial Dynamical Time (TDT), whose fundamental unit is the SI second.

ephemeris; → time.

ephemeris transit
  گذر ِ روزیجی   
gozar-e ruziji

Fr.: transit au méridien des éphémérides   

The passage of a celestial body or point across the → ephemeris meridian.

ephemeris; → transit.

epimorphism
  اپی-ریخت‌مندی   
api-rixtmandi

Fr.: épimorphisme   

A → morphism f : Y → X if, for any two morphisms u,v : X → Z, u f = v f  implies u = v.

epi-; → morphism.

ergosphere
  ارگ‌سپهر   
ergsepehr

Fr.: ergosphère   

The region between the → event horizon and the → stationary limit of a rotating → Kerr black hole. It is possible for a particle falling inside the ergosphere to break into two parts, one of which will fall into the black hole and the other will come out.

erg + → sphere.

Eudoxan spheres
  سپهرهای ِ اءودوکسوس   
sepehrhâ-ye Eudoxus

Fr.: sphères d'Eudoxe   

spheres of Eudoxus.

spheres of Eudoxus.

euphemism
  خوشگویی، خوشزبانی   
xošguyi, xošzabâni

Fr.: euphémisme   

An inoffensive word or phrase substituted for one considered offensive or hurtful, especially one concerned with religion, sex, death, or excreta (TheFreeDictionary.com).

From Gk. euphemismos, from euphemizein "speak with fair words, use words of good omen," from → eu- "well," + pheme "speech, voice, talk," from phanai "to speak," ultimately from PIE *bha- "to speak, tell, say;" cf. Skt. bhanati "speaks;" L. fari "to say," fabula "tale, story," fama "talk, rumor, report; reputation;" Armenian ban, bay "word, term."

Xošguyi, xošzabâni, literally "pleasant talking, ~ speach," from xoš "well, pleasant," → eu- + guyi verbal noun of goftan "to say, talk, speak," → logic; zabâni, from zabân, → language.

exosphere
  برون‌سپهر   
borun-sepehr

Fr.: exosphère   

1) The outermost portion of the Earth's → atmosphere. Extremely tenuous, it lies above the → ionosphere from a height of about 500 km, to the edge of → interplanetary space.
2) An extremely tenuous kind of atmosphere surrounding a → solar system body. Since the → mean free path is much greater than the atmospheric scale height. The → atoms or → molecules never collide with each other. → lunar exosphere.

exo- + → sphere.

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