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precession of the equator 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 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 pišâyân-e gereh-hâ Fr.: précession des nœuds The gradual change in he orbital planes of a binary system. → precession; → node. |
precession period 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 zamân-e pišÃ¢yân Fr.: temps de précession A time interval over which an orbit precesses by 2π radians in its plane. → precession; → time. |
precessional pišâyâni Fr.: précessionnel Of or pertaing to → precession. → precession; → -al. |
precessional circle 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 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. 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." |
precision parsuneš Fr.: précision 1) The state or quality of being → precise. Verbal noun from → precise. |
predation caveš Fr.: prédation 1) Act of plundering or robbing; predatory behavior. Verbal noun, → prey. |
prehension nuteš Fr.: préhension 1) Zoology Psychology: The action of grasping or seizing. Verbal noun of → prehend. |
preposition pišhel Fr.: préposition A word used with a noun or pronoun to mark its relation with another word. From L. praepositionem "a putting before," from praepositus, p.p. of praeponere "put before," from prae "before," → pre-, + ponere "put, set, place," → position. Pišhel, from piš-, "before," → pre-, + hel-, helidan, heštan "to place, put," → leap. |
prescription pišvešt Fr.: prescription, ordonnance 1) An act of prescribing. |
present-day mass function (PDMF) karyâ-ye jerm-e konuni, ~ ~ emruzi Fr.: fonction de masse actuelle The present number of stars on the → main sequence per unit logarithmic mass interval per square parsec. The PDMF is the basis for deriving the → initial mass function (IMF). This mass function is not corrected for stellar evolution nor losses through stellar deaths. |
pressure ionization yoneš-e fešâri Fr.: ionisation par pression A physical state of dense matter in which the electrostatic field of one atom should influence a neighboring atom and hence disturb atomic levels. In extreme case, such as white dwarfs, electron clouds practically rub and electrons are ionized off the parent atoms. → pressure; → ionization. |
primordial curvature perturbation partureš-e xamidegi-ye bonâqâzin Fr.: perturbation de courbure primordiale In cosmological models, the phenomenon that is supposed to seed the → cosmic microwave background anisotropies and the structure formation of the Universe. → primordial; → curvature; → perturbation. |
principle of action and reaction parvaz-e žireš va vâžireš, ~ koneš va vâkoneš Fr.: principe d'action et de réaction Newton's third law of motion, which states that for every action there must be an equal and opposite reaction. |
principle of least action parvaz-e kamtarin žireš, ~ ~ koneš Fr.: principe de moindre action The principle that, for a system whose total mechanical energy is conserved, the path to be taken for the system from one configuration to another is the one whose action has the least value relative to all other possible paths and from the same configurations. Also called Maupertuis' principle, least-action principle. |
principle of non-contradiction parvaz-e nâpâdguyi Fr.: principe de non-contradiction The third principle of → formal logic introduced in Aristotle's theory of the → syllogism: No statement can be both → true and → false at the same time. Also called → law of non-contradiction. → principle; → non-; → contradiction. |
privatization vâvaneš Fr.: privatisation The transfer from public to private ownership. |
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