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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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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

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Number of Results: 1022
pre-WD star
  ستاره‌ی ِ پیش-کوتوله‌ی ِ سفید   
setâre-ye piš-kutule-ye sefid

Fr.: étoile pré-naine blanche   

A → post-planetary nebula star that is approaching the top of the → white dwarf sequence. These stars have exhausted the capacity of → nuclear burning in their cores.

pre-; → white; → dwarf.

prebiotic
  پیشزیستی   
pišzisti

Fr.: prébiotique   

Existing before or making possible the appearance of living organisms. Prebiotic molecules are biologically essential components such as amino acids, sugars, and nucleic-acid bases which are precursors of the origin of life.

pre- + → bio- + -tic equivalent of → -ic.

precess
  پیشایانیدن   
pišâyânidan

Fr.: précesser   

1) To correct celestial coordinates for → precession.
2) To undergo → precession.

Back formation from → precession.

Back formation from pišâyân, → precession.

precessed coordinates
  هم‌آراهای ِ پیشایانیده   
hamârâhâ-ye pišâyânidé

Fr.: coordonnées précessées, ~ corrigées de la précession   

The apparent position of a celestial object corrected for the epoch → precession.

Precessed, p.p. of → precess; → coordinates.

precession
  پیشایان   
pišâyân

Fr.: précession   

The periodic motion of the → rotation axis of a body such as a → spinning top in which the axis of rotation gradually sweeps out a conical shape. In the case of the spinning Earth, it is due to the combined → gravitational attractions of the → Sun, the → Moon, and → planets on Earth's → equatorial bulge. Since the Earth's axis is tilted to its → orbital plane or → ecliptic, the gravitational force of the Sun and the Moon on the Earth's equatorial bulge tend to pull it back toward the plane of ecliptic. As a result, the axis → precesses. Earth's axis of rotation precesses with a period of about 25,770 years, describing one complete circle on the → celestial sphere (→ precession constant). This circle has a radius of approximately 23°.5, equal to the → inclination of the Earth's orbit. Since the → vernal equinox is the reference direction for the → equatorial coordinate system, the coordinates of "fixed" objects change with time and must therefore be referred to an → epoch at which they are correct. → sign of zodiac.
See also → general precession; → precession of the ecliptic; → precession of the equator; → precession of the equinoxes; → precessional circle; → precession time; → geodetic precession; → general precession in longitude; → general precession in right ascension; → orbital precession; → perihelion precession; → planetary precession; → precession period.

L.L. præcissionem "a coming before," from L. præcessus, p.p. of præcedere "to happen before," from the fact that the equinoxes occur earlier each year with respect to the preceding year, from præ- "before," → pre-, + cedere "to walk, to go, to happen."

Pišâyân, literally "coming before," from piš- "before" → pre- + ây- (present stem of âmadan "to come, arrive, become"), from Av. ay- "to go, to come," aēiti "goes;" O.Pers. aitiy "goes;" Skt. e- "to come near," eti "arrival;" L. ire "to go;" Goth. iddja "went," Lith. eiti "to go;" Rus. idti "to go;" + -ân suffix of space and time.

precession constant
  پایای ِ پیشایان   
pâyâ-ye pišâyân

Fr.: constante de précession   

The amount by which the equinoctial points drift westward annually due to precession. Its value for epoch J2000.0 is 50''.26, resulting from the westward → precession of the equator (50".38), and the eastward → precession of the ecliptic (0".12).

precession; → constant.

precession of the ecliptic
  پیشایان ِ هورپه   
pišâyân-e hurpeh

Fr.: précession de l'écliptique   

The component of general precession caused by the gravitational attraction of the planets on the Earth's center of mass. It causes the equinox to move eastward by about 0''.12 per year in the opposite direction to the → precession of the equator. This terminology replaces → planetary precession, according to an IAU resolution adopted in August 2006.

precession; → ecliptic.

precession of the equator
  پیشایان ِ هموگار   
pišâyân-e hamugâr

Fr.: précession de l'équateur   

That component of general precession caused by the combined effect of the Moon, the Sun and the planets on the equatorial protuberance of the Earth, producing a westward motion of the equinoxes along the ecliptic about 50'' per year. According to an IAU resolution adopted in August 2006, the present terminology replaces lunisolar precession.

precession; → equator.

precession of the equinoxes
  پیشایان ِ هموگان‌ها   
pišâyân-e hamugânhâ

Fr.: précession des équinoxes   

The slow motion of the equinoxes along the ecliptic, resulting from the combined motion of the equator (→ precession of the equator) and the ecliptic (→ precession of the ecliptic), or in other words the precession of the Earth's axis of rotation. Also know as → general precession. The First Point of Aries moves westward along the ecliptic at 50.38 arcseconds per year (1 degree every 71.6 years), causing the equinoxes to occur about twenty minutes earlier each sidereal year. See also → nutation.

precession; → equinox.

precession of the nodes
  پیشایان ِ گره‌ها   
pišâyân-e gereh-hâ

Fr.: précession des nœuds   

The gradual change in he orbital planes of a binary system.

precession; → node.

precession period
  دوره‌ی ِ پیشایان   
dowre-ye pišâyân

Fr.: période de précession   

The interval with which a rotating body precesses. The precession period of the Earth is 25,770 years. For a → spinning top it is given by: Tp = (4π2I)/(mgrTs), where I is the → moment of inertia, m the mass of the top, g gravity, r the distance between the center of mass and the contact point, and Ts is the spinning period of the top.

precession; → period.

precession time
  زمان ِ پیشایان   
zamân-e pišâyân

Fr.: temps de précession   

A time interval over which an orbit precesses by 2π radians in its plane.

precession; → time.

precessional
  پیشایانی   
pišâyâni

Fr.: précessionnel   

Of or pertaing to → precession.

precession; → -al.

precessional circle
  پرهون ِ پیشایانی   
parhun-e pišâyâni

Fr.: circle précessionnel   

The path of either → celestial poles around the → ecliptic pole due to the → precession of equinox. It takes about 26,000 years for the celestial pole to complete path.

precessional; → circle.

precipitation
  ۱) بارش، ریزش؛ ۲) ته‌نشست   
1) bâreš (#), rizeš (#); 2) tahnešast (#)

Fr.: précipitation   

1) Meteo.: Any form of water, such as rain, snow, sleet, or hail, that falls to the Earth's surface. The quantity of such water falling in a specific area within a specific period.
2) Chemistry: The process of separating a solid substance from a solution.

From M.Fr. précipitation, from L. præcipitationem "act or fact of falling headlong, haste," from præcipitare "fall, be hasty," from præceps "steep, headlong, headfirst," from præ- "forth" + caput, → head.

1) Bâreš, verbal noun of bâridan "to rain," bârân "rain;" Mid.Pers. vâritan, vârân; Av. vār- "rain; to rain;" cf. Skt. vār- "rain, water; to rain;" PIE base *uer- "water, rain, river."
Rizeš, verbal noun of rixtan "to flow, to pour," → overflow.
2) Tahnešast "to settle down, precipitate," from tah "→ bottom, end;" + nešast past stem of nešastan "to sit down; to settle down; to sink," → sit.

precise
  پرسون   
parsun

Fr.: précis   

1) Definitely or sharply stated, or defined.
2) Designating → precision.
See also: → accurate, → exact.

M.E., from M.Fr. précis "cut short" from M.L. precisus, from L. præcisus "abridged, cut off," p.p. of præcidere "to cut off, shorten," from præ- "in front," → pre-, + cædere "to cut down, chop, beat, hew, slay."

Parsun literally "cut around" (compare with Skt. pariccheda "precise, accurate definition, exact discrimination," from pari- + cheda "cut, cutting off," from chid- "to cut, split"), from par-, variant of pirâ- "around, about," → peri-, + sun "to cut;" cf. Kurd. Sorani su, sun "to sharpen, whet;" Kurd. Kurmanji (prefixed ha-, contraction of *ham-) hasun "to sharpen, whet;" Mod.Pers. sân "whetstone," variants fasân, afsân, awsân; Av. si-, sā- "to cut;" cf. Skt. śā- "to sharpen, whet" (see also → concrete).

precisely
  پرسونانه   
parsunâné

Fr.: précisement   

In a precise manner.

precise; → -ly.

preciseness
  پرسونی   
parsuni

Fr.: précision   

The quality or state of being very accurate.

precise; → -ness.

precision
  پرسونش   
parsuneš

Fr.: précision   

1) The state or quality of being → precise.
2) The degree to which repeated measurements of a quantity give the same results under unchanged conditions. Not the same as → accuracy, but often confused as such. See → accuracy for the difference between precision and accuracy.

Verbal noun from → precise.

precursor
  پیشگام   
pišgâm (#)

Fr.: précurseur   

1) A person or thing that comes before another of the same kind; a forerunner.
2) A substance from which another is formed, especially by metabolic reaction (OxforddDctionaries.com)

M.E., from L. præcursor "forerunner," from præcursus, p.p. of præcurrere, from præ- "before," → pre-, + currere "to run," → current.

Pišgâm, from piš- "before," → pre-, + gâm "step, pace," → stage.

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