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transmutation tarâmuteš Fr.: transmutation The act or process of transmuting. Verbal noun of → transmute. |
transonic tarâsedâyi Fr.: transsonique Of or pertaining to the speed of a body in a surrounding fluid when the relative speed of the fluid is → subsonic in some places and → supersonic in others. |
transonic flow tacân-e tarâsedâyi Fr.: écoulement transsonique Flow of a fluid over a body with a speed in the range just above and below the → Mach number 1. |
transponder tarâgu Fr.: transpondeur An emitter-receiver device that automatically responds upon reception of a designated incoming radar, radio or sonar signal |
transposition tarâneheš Fr.: transposition Math.: A permutation of a set of elements that interchanges two elements and
leaves the remaining elements in their original positions.
For example, the swapping of 2 and 5 to take the list 123456 to 153426 is a transposition. |
trepidation larzeš Fr.: trépidation In medieval astronomy, a spurious oscillatory motion of the equinoxes thought to have a period of 7,000 years. This concept, attributed to Thâbit ibn Qurra (c. 830-901), had a profound influence on medieval astronomy. In order to explain trepidation, Thâbit was said to have added a new sphere to the eight Ptolemaic spheres beyond the sphere of fixed stars. From L. trepidationem "agitation, trembling," from trepidare "to tremble, hurry," from trepidus "anxious, scared;" cf. Skt. trprá- "hasty;" PIE base *trep- "to shake, tremble." Larzeš, verbal noun of larzidan "to tremble, shiver;" Mid.Pers. larzidan "to shake, tremble;" Manichean Mid.Pers. rarz- "to shiver with fever;" Proto-Iranian *rarz- "to shake, tremble." |
triangulation segušbandi (#) Fr.: triangulation In surveying and navigation, the process of deriving the linear distance between any two remote points by the division of a large area into adjacent triangles and using trigonometric relationships. See also → trilateration. From M.L. triangulation-, from triangulare "to make triangles," → triangle. Seguš-bandi, from sé, → three, + guš/gušé, → angle, + bandi verbal noun from bastan "to form, bind, tie" (Mid.Pers. bastan/vastan "to bind, shut;" Av./O.Pers. band- "to bind, fetter," banda- "band, tie;" cf. Skt. bandh- "to bind, tie, fasten;" Ger. binden; E. bind; PIE base *bhendh- "to bind"). |
triatomic hydrogen molecular ion yon-e molekuli-ye se-atomi-ye hidrožen Fr.: ion moléculaire d'hydrogène triatomique, H3+ The hydrogen molecule composed of three atoms in which one of the atoms is ionized. The molecular ion H3+ plays a key role in the chemistry of gaseous → interstellar medium. It reacts efficiently with almost any neutral atom or molecule to initiate a network of ion-neutral reactions. It is responsible for producing molecules such as OH, CO, and H2O. The first detection of H3+ in the interstellar medium, via two closely spaced absorption lines (doublet) near 3.668 μm, were reported in two dense → molecular cloud cores along the lines of sight to the embedded → young stellar objects W33A and GL2136 (Geballe & Oka 1996). Since then H3+ has been detected in several molecular clouds. It is believed that H3+ forms via → cosmic ray → ionization of H2 producing H2+, which quickly reacts to another H2 molecule to form H3+ ( H2 + CR → H2+ and H2+ + H2→ H3+ + H + 1.7 eV). |
triggered star formation diseš-e mâše-yi-ye setâré Fr.: formation d'étoiles déclanchée The formation of second-generation stars in a → molecular cloud, as set off by the action of → massive stars. → sequential star formation; → radiation-driven implosion. → trigger; → star formation. |
trigonometric sebarsanjik Fr.: trigonométrique, circulaire Relating to or used in → trigonometry. → trigonometric function. → trigonometry; → -ic. |
trigonometric function karyâ-ye sebarsanjik Fr.: fonction circulaire, ~ trigonomtérique A function of an angle, one of six functions (sine, cosine, tangent, cotangent, secant, and cosecant) that represent ratios of sides of right triangles. Also called circular function. → trigonometric; → function. |
trigonometric parallax didgašt-e sebarsanji, ~ sebarsanjik Fr.: parallaxe trigonométrique The → parallax of a nearby star (less than 300 → light-years) against the background of more distant stars resulting from the motion of the Earth in its orbit around the Sun. → trigonometric; → parallax. |
trigonometry sebarsanji Fr.: trigonométrie The branch of mathematics dealing with the relations of the sides and angles of triangles; also the various algebraic functions of these relations. From N.L. trigonometria, from Gk. trigonon "triangle" (from tri-, → three, + gonia "angle," cognate with Pers. zânu "knee") + metron, → -metry. |
trilateration sebarbandi Fr.: trilatération A geometrical method in land surveying for the determination of the relative position of points. In contrast to → triangulation, trilateration involves measuring the lengths of the three sides of touching or overlapping triangles and not their angles. |
triphthong sévâké Fr.: triphthongue A compound → vowel sound resulting from the succession of three simple vowels pronounced in a single syllable (as in power, hour, fire). |
triple conjunction hamistân-e setâyi Fr.: conjonction triple A rare event involving a particularly intricate set of movements of two planets or a planet and a star where they meet each other three times in a short period either in opposition or at the time of inferior conjunction, if an inferior planet is involved. The visible movement of the planet or the planets in the sky is therefore normally prograde at the first conjunction, retrograde at the second conjunction and again prograde at the third conjunction. → triple; → conjunction. |
Triton Triton (#) Fr.: Triton The seventh and the largest of → Neptune's satellites. It has a diameter of 2,700 km and orbits its planet at a mean distance of 354,760 km every 5.877 days. Triton was discovered by William Lassell in 1846 scarcely a month after Neptune was discovered. Triton is colder than any other measured object in the solar system with a surface temperature of -235° C. It has an extremely thin atmosphere. Nitrogen ice particles might form thin clouds a few kilometers above the surface. The atmospheric pressure at Triton's surface is about 15 microbars, 0.000015 times the sea-level surface pressure on Earth. Triton is the only large satellite in the solar system to circle a planet in a → retrograde motion, that is in a direction opposite to the rotation of the planet. In Gk. mythology, Triton is a god of the sea, the son of Poseidon (Neptune); usually portrayed as having the head and trunk of a man and the tail of a fish. |
tropical month mâh-e hamugâni Fr.: mois tropique The average period of the revolution of the Moon about the Earth with respect to the → vernal equinox, a period of 27.321 582 days (27d 7h 43m 4.7s). Mâh, → month; hamugâni, of or pertaining to hamugân, → equinox. |
Trouton's rule razan-e Trouton Fr.: règle de Trouton The ratio of the → molar heat of vaporization of any liquid to its → boiling point is a constant, about 88 joules per mole per Kelvin. The rule is equivalent to the statement that the → entropy of vaporization is constant. It is not always followed, especially by liquids such as water in which hydrogen bonding occurs between the molecules. Named after Frederick Thomas Trouton (1863-1922), an Irish physicist; → rule. |
Trouton-Noble experiment âzmâyeš-e Trouton-Noble Fr.: expérience de Trouton-Noble An experiment first carried out in 1903 to reveal the absolute motion of the Earth with respect to the → ether. The experiment consists of detecting a torque on a charged parallel-plate → capacitor that was suspended so that its plates were vertical. Since the Earth moves around the Sun, the moving charges were expected to produce magnetic fields, and the resulting torque should tend to turn the capacitor bringing its plates parallel to its velocity. No such effect was observed, and the absence of the torque supports the theory of → special relativity. Named after Frederick T. Trouton (1863-1922) and Henry R. Noble; → experiment. |
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