An Etymological Dictionary of Astronomy and Astrophysics

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory



<< < -ti Tam Tay tel ten ter The the the the thi thr tid tig tin tol tor tot tra tra tra tra tri tri Tro tsu tur two Typ > >>

Number of Results: 569
  ارزیز، قلعی   
arziz (#), qal'y (#)

Fr.: étain   

A metallic chemical element; symbol Sn (L. stannum for → alloys containing → lead). → Atomic number 50; → atomic weight 118.69; → melting point 231.9681°C; → boiling point 2,270°C; → specific gravity 5.75 (gray), 7.3 (white). The element was known in prehistoric times.

M.E., O.E. tin; cf. M.Du., Du. tin, O.H.G. zin, Ger. Zinn, O.N. tin; related to Fr. étain?

Arziz "tin," from Mid.Pers. arziz "tin, lead," arus "white, bright;" Av. ərəzata- "silver," auruša- "white;" cf. Skt. arjuna- "white, shining," rajata- "silver;" Gk. argos "white," arguron "silver," L. argentum "silver," arguere "to make clear," argmentum "argument;" PIE *arg- "to shine, be white, bright, clear."
Qal'y of unknown origin.

TiO band
  باند ِ TiO   
bând-e TiO

Fr.: bandes TiO   

Any of the several → absorption bands due to the molecule → titanium oxide that are prominent in the spectra of cool → K and → M stars.

titanium oxide; → band.

tip of the red giant branch method
  روش ِ نوک ِ شاخه‌ی غول‌های ِ سرخ   
raveš-e nok-e šâxe-ye qulhâ-ye sorx

Fr.: méthode du haut de la branche des géantes   

A technique for deriving extragalactic distances which uses the → luminosity of the brightest → red giant branch stars in old → stellar populations as a "standard candle." For old (> 2-3 Gyr), metal-poor ([Fe/H] < -0.7) stellar populations, this luminosity is relatively well determined, and the → absolute magnitude of these stars in the I band is roughly constant (MI = -4.1 ± 0.1).

M.E. tip; from M.L.G. or M.Du. tip "utmost point, extremity" (cf. Ger. zipfel, a diminutive formation); → red giant; → branch; → method.

Raveš, → method; nok "tip;" šâxé, → branch; qulhâ-ye sorx plural of qul-e sorx, → red giant.

tip-tilt mirror
  آینه‌یِ کج-و-راست-گر   
âyene-ye kaj-o-râst-gar

Fr.: miroir inclinable   

A rapidly moving → mirror used in → adaptive optics to correct overall movements of the incoming → wavefront of light caused by → atmospheric turbulence. The simplest form of adaptive optics is tip-tilt correction, which corresponds to correction of the tilts of the wavefront in two dimensions. This is done by tipping and tilting the mirror rapidly in response to overall changes in position of a reference star. See also → deformable mirror.

From, tip noun from tip (v.) "to overturn, upset," from M.E. typen "to upset, overturn" + tilt noun from tilt (v.) "to cause to lean, incline, slope, or slant," → tilt; → mirror.

Âyené, → mirror; kaj "turned aside; crooked, bent" (cf. Skt. kubja- "hump-backed, crooked," Pali kujja- "bent," L. gibbus "hump, hunch," Lith. kupra "hump") + -o- "and" + râstright + -gar agent noun suffix → -or.

xasté (#)

Fr.: fatigué   

Exhausted of strength and energy.

Past participle of tire "to weary; become weary," M.E. tyren, O.E. teorian, of unknown origin.

Xasté "tired; hurt, wounded;" Mid.Pers. xastan, xad- "to injure, wound;" Av. vīxaδ- "to crush;" Proto-Iranian *xad- "to wound, hurt."

tired light
  نور ِ خسته   
nur-e xasté

Fr.: fatigue de la lumière   

The hypothesis that photons from distant objects lose energy during their intergalactic journey to us, thereby increasing in wavelength and becoming redshifted. This would provide an alternative to the → Big Bang model in accounting for the → redshifts of distant galaxies. However, there is no evidence for any such tired-light effect. First discussed by F. Zwicky (1929, Proceedings of the National Academy of Sciences, 15, 773).

tired; → light.

Tisserand's parameter
  پارامون ِ تیسران   
pârâmun-e Tisserand

Fr.: paramètre de Tisserand   

In celestial mechanics, a combination of orbital elements commonly used to distinguish between comets and asteroids. Objects whose Tisserand's parameter value is smaller than 3 are considered to be dynamically cometary, and those with a value larger than 3 asteroidal. Also called Tisserand's invariant.

Named after François Félix Tisserand (1845-1896), French astronomer, Director of the Paris Observatory (1892).

Titân (#)

Fr.: Titan   

The largest and the sixth moon of → Saturn discovered by Christiaan Huygens in 1655. Called also Saturn VI. Titan has a diameter of 5,150 km, about half the size of Earth and almost as large as Mars. It orbits Saturn at a mean distance of 1,221,830 km every 15.945 days. It is the only moon known to have an → atmosphere. Its surface temperature is -179 °C, which makes water as hard as rocks and allows → methane to be found in its liquid form. Its surface pressure is slightly higher than Earth's pressure (1.6 bars against 1 bar at sea level). The Huygens probe released from → Cassini-Huygens landed on Titan on December 25, 2004. From the data obtained by Cassini-Huygens, we know that Titan is a world with lakes and seas composed of liquid methane and → ethane near its poles, with vast, arid regions not made of silicates as on Earth, but of solid water ice coated with → hydrocarbons that fall from the atmosphere. Titan's icy dunes are gigantic, reaching, on average, 1 to 2 km wide, hundreds kilometers long and around 100 m high. Titan is the only other place in the solar system known to have an Earth-like cycle of liquids flowing across its surface as the planet cycles through its seasons. Each Titan season lasts about 7.5 Earth years. The Huygens probe made the first direct measurements of Titan's lower atmosphere. Huygens also directly sampled → aerosols in the atmosphere and confirmed that → carbon and → nitrogen are their major constituents. Cassini followed up Huygens' measurements from orbit, detecting other chemicals that include → propylene and poisonous → hydrogen cyanide, in Titan's atmosphere. Cassini's gravity measurements of Titan revealed that this moon is hiding an internal, liquid water and → ammonia ocean beneath its surface. Huygens also measured radio signals during its descent that strongly suggested the presence of an ocean 55 to 80 km below the moon's surface.

In Gk. mythology the Titans were a family of giants, the children of Uranus and Gaia, who sought to rule the heavens but were overthrown and supplanted by the family of Zeus.

Titâniyâ (#)

Fr.: Titania   

The fourteenth and largest of → Uranus's known satellites. It has a diameter of 1578 km and orbits its planet at a mean distance of 436,270 km. Titania was discovered by Herschel in 1787. Also called Uranus IV.

Titania is the Queen of the Fairies and wife of Oberon in Shakespeare's Midsummer-Night's Dream.

titan (#)

Fr.: titane   

A dark-gray or silvery, very hard, light metallic element, occurring combined in various minerals; symbol Ti. Atomic number 22; atomic weight 47.88; melting point 1,675°C; boiling point 3,260°C; specific gravity 4.54 at 20°C. It is used in metallurgy to remove oxygen and nitrogen from steel and to toughen it.

It was originally discovered by the English clergyman William Gregor in the mineral ilmenite (FeTiO3) in 1791. It was rediscovered in 1795 by the German chemist Martin Heinrich Klaproth, who called it titanium because it had no characteristic properties to use as a name; from Titan + -ium.

Titan, loan from Fr., as above.

titanium oxide, TiO
  اکسید ِ تیتان   
oksid-e titân

Fr.: oxide de titane   

A → diatomic molecule made up of → titanium and → oxygen atoms. See → TiO band.

titanium; → band.

Titius-Bode law
  قانون ِ تیتیوس-بوده   
qânun-e Titius-Bode (#)

Fr.: loi de Titius-Bode   

The empirical rule relating the approximate distances of the → solar system  → planets from the → Sun. The original formulation was: a = (n + 4) / 10, where a is the mean distance of a planet from the Sun in → astronomical units and n = 0, 3, 6, 12, 24, 48, 96, 192 (doubling for each successive planet). The planets were seen to fit this sequence quite well, provided the → asteroids between → Mars and → Jupiter are counted as one planet, as did → Uranus discovered in 1781. However, → Neptune and the ex-planet → Pluto do not conform to the rule. The question of whether there is any physical significance to the "law," i.e. some dynamical reason that will explain planetary orbit spacing has led to much discussion during the past two centuries. Today, many astronomers are very skeptical and consider this "laws" to be numerical coincidence.

Named after the German mathematician Johann Titius (1729-1796), who first found the law in 1766, and the German astronomer Johann Elert Bode (1747-1826), who published it in 1772; → law.


Fr.: titre   

The distinguishing name of a book, poem, picture, piece of music, or the like (

M.E., from O.Fr. title and in part from O.E. titul, both from L. titulus "inscription, label, heading; honorable appellation," of unknown origin.

Sarâl, from sar, → head, + noun suffix -âl, → -al.

TNT equivalent
  هموگ‌ارز ِ TNT   
hamug-arz-e TNT

Fr.: équivalent TNT   

A measure of the explosive strength of a nuclear bomb, expressed in terms of the weight of → trinitrotoluene which could release the same amount of energy when exploded. The Hiroshima atomic (fission) bomb created a blast equivalent to 16 kilotons of TNT. The first hydrogen (thermonuclear) bomb test released an energy of about 10 megatons of TNT. See also → megaton of TNT.

trinitrotoluene (TNT); → equivalent.

vazaq (#)

Fr.: crapaud   

A tailless amphibian with a short stout body and related to → frogs. In contrast to frogs, it has short legs and dry warty skin that can secrete a toxic, milky substance.

M.E. tode, toode, tade, tadde, from O.E. tadige, tadie, of unknown origin, cognate with Scots tade, taid, taed, ted "toad;" Dan. tudse, Swed. tassa, tossa, O.E. taxe, tosca "toad."

Vazaq "toad," variants Tabari, Aftari vak, Tabari vag, (prefixed) qurbâqé, Lori, Laki qorvâ, korvâx, Kurd. baq, Zâzâ baqa; Mid.Pers. vazak, vak; Av. vazaγa- "frog."

emruz (#)

Fr.: aujourd'hui   

1) The present day, time, or age.
2) The present epoch in the cosmic evolution since the → Big Bang characterizd by the → redshift  z = 0.

M.E. today, from O.E. todæge, to dæge "on (this) day," from to "at, on" + dæge, dative of dæg "→ day."

Emruz "today," from Mid.Pers. imrôc, imrôz, from im "this; here" + rôz, ruz, → day.


Fr.: orteil   

Each of the five digits on the end of the foot.

M.E. to, from O.E. akin to Ger. Zehe "toe," Du. teen.

Pângol, literally "foot finger," from , → foot, + ângol (Dehxodâ) "finger," variant of angošt, → finger.

tokâmak (#)

Fr.: tokamak   

A machine producing a → toroidal magnetic field for confining a → plasma in → nuclear fusion research.

From Rus. Tokamak, acronym from toroidal'naya kamera s magnitnymi katushkami "toroidal chamber with magnetic coils." It was invented in the 1950s by Soviet physicists Igor Yevgenyevich Tamm and Andrei Sakharov (who had been inspired by an original idea of Oleg Lavrentyev).

Toledan Tables
  زیج ِ تولد   
zij-e Toled

Fr.: Tables de Tolède   

A set of astronomical tables drawn up by a group of astronomers in Toledo, Spain, mainly Zarqâli, and compiled after 1068. This work, which represents the first original development of Andalusian astronomy, was extremely influential in Europe for three centuries until the advent of the → Alfonsine Tables. The main sources for the bulk of the table collections were those of the Persian astronomer Khwârizmi (mainly planetary latitudes), Battâni (planetary equations), and Ptolemy. In fact the oldest version of the Toledan Tables was mainly modeled on Khwârizmi's Sindhind, but had admixture from Battâni. In addition, the oldest versions of the Toledan Tables preserve some tables of Khwârizmi that are rare or absent elsewhere. The Toledan Tables also incorporated the theory of → trepidation. The original Arabic version of the Toledan Tables has been lost, but two Latin versions have survived, one by Gerard of Cremona (12th century) and one by an unknown author.

Toledo, a city in central Spain, 70 km south of Madrid; → table.

ravâdâri (#)

Fr.: tolérance   

The maximum permissible error or variation in a dimension of an object.

M.E., from O.Fr. tolerance, from L. tolerantia "endurance," from tolerans, pr.p. of tolerare "to bear, endure, tolerate."

Ravâdâri, noun from ravâdâr "consenter; judging right; lawful," from ravâ "admissible; allowable; tolerated" (from raftan "to go, walk; to flow;" Mid.Pers. raftan, raw-, Proto-Iranian *rab/f- "to go; to attack" + -dâr "having, possessor" (from dâštan "to have, to possess," Mid.Pers. dâštan, O.Pers./Av. root dar- "to hold, keep back, maitain, keep in mind," Skt. dhr-, dharma- "law," Gk. thronos "elevated seat, throne," L. firmus "firm, stable," Lith. daryti "to make," PIE *dher- "to hold, support").

<< < -ti Tam Tay tel ten ter The the the the thi thr tid tig tin tol tor tot tra tra tra tra tri tri Tro tsu tur two Typ > >>