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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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terraforming
  زمین‌دیسش   
zamin-diseš

Fr.: terraformation   

The hypothetical process of altering the environment (atmosphere, temperature, surface topography, or ecology) of another planet or moon to improve the chances of survival of an indigenous biology or to allow habitation by terrestrial life forms. See also → ecopoiesis.

Verbal noun of → terraform. The term first appeared in a science fiction novel, Seetee Shock (1949) by Jack Williamson, an American science fiction writer; but the actual concept pre-dates this work.

terrestrial
  زمینی   
zamini (#)

Fr.: terrestre   

Pertaining to, consisting of, or representing the Earth as distinct from other planets.

From L. terrestris "earthly," from terra "earth," literally "dry land" (as opposed to "sea"); from PIE base *ters- "to dry" (cf. Pers. tešné "thirsty;" Mid.Pers. tašnak "thirsty;" Av. taršu- "dry," taršna- "thirst;" Skt. trsta- "dry," tars- "to be thirsty;" Gk. teresesthai "to become or be dry," L. torrere "to dry up, roast," Goth. þaursus "dry, barren," O.H.G. derren "to make dry," durst "thirst;" Ger. dürr "arid;" O.E. þurstig "thirsty").

Zamini adj. of zamin, variant zami "earth, floor, land;" Mid.Pers. zamig; Av. zam- "the earth;" cf. Skt. ksam- "the ground, earth;" Gk. khthôn, khamai "on the ground;" L. homo "earthly being" (as in homo sapiens, homicide, humble, humus, exhume), humus "the earth;" O.Russ. zemi "land, earth;" PIE root *dh(e)ghom "earth".

Terrestrial Dynamical Time
  زمان ِ توانیک ِ زمینی   
zamân-e tavânik-e zamini

Fr.: temps dynamique terrestre   

A uniform atomic time scale for apparent geocentric ephemerides defined by a 1979 IAU resolution, which replaced Ephemeris Time. TDT is independent of the variable rotation of the Earth, and the length of the tropical year is defined in days of 86,400 seconds of international atomic time. In 1991 it was replaced by Terrestrial Time.

terrestrial; → dynamical; → time.

terrestrial gravitational constant
  پایای ِ گرانشی زمینی   
pâyâ-ye gerâneši-ye zamini

Fr.: constante gravitationnelle terrestre   

A parameter representing the product of the → gravitational constant by the Earth's mass. It is 3.987 x 1014 m3s-2 or 3.987 x 105 km3s-2.

terrestrial; → gravitational; → constant.

terrestrial planets
  سیاره‌های ِ زمینی   
sayyârehâ-ye zamini

Fr.: planètes terrestres   

The four innermost planets in the solar system, Mercury, Venus, Earth and Mars. They are called terrestrial because they have a compact, rocky surface like the Earth's. The planets, Venus, Earth, and Mars have significant atmospheres while Mercury has almost none. These planets are approximately the same size, with the Earth the largest. They are considerably denser than the Jovian planets, ranging from a specific gravity of 4 for Mars to 5.5 for the Earth.

terrestrial; → planet.

Terrestrial Time
  زمان ِ زمینی   
zamân-e zimini

Fr.: temps terrestre   

The modern astronomical standard for the passage of time on the surface of the Earth. It is the → coordinate time scale consistent with the theory of general relativity for an observer on the surface of the Earth. TT was renamed from Terrestrial Dynamical Time (TDT) in 1991. The fundamental unit of TT is the day of 86,400 SI seconds. It is related to the International Atomic Time by the relation: TDT = TAI + 32.184 sec.

terrestrial; → time.

tertiary
  ۱، ۲، ۳) سوُمان؛ ۳) دوران ِ سوم   
1, 2, 3) sevoman; 3) dowrân-e sevom (#)

Fr.: tertiarie   

1) Third in order, rank, level, stage, formation, etc.
2) Chem.: Being or containing a carbon atom having bonds to three other carbon atoms.
3) Geology: (usually with capital initial) A term formerly used to distinguish a major period of → geologic time, from the end of the → Cretaceous period about 65 million years ago to the start of the Quaternary period about 1.6 millions years ago. The International Commission on Stratigraphy no longer sustains this term as part of the formal stratigraphic nomenclature. Instead, the → Paleogene and → Neogene periods are recommended as the primary subdivisions of the Cenozoic era.

From L. tertius, → third; → period.

tesla (T)
  تسلا   
teslâ (#)

Fr.: tesla   

The unit of → magnetic induction flux density in the SI system. It is the induction of a field in which each meter of conductor with a current of one → ampere and arranged perpendicular to the direction of the vector of induction is acted upon by a force of one → newton. 1 tesla = 1 → weber/m2 = 104gauss.

Named after Nikola Tesla (1856-1943), American physicist, electrical engineer, and inventor, born in Smiljan, Lika, which was then part of the Austo-Hungarian Empire, region of Croatia.

test
  آزمون   
âzmun (#)

Fr.: test   

A procedure by which the presence, quality, or genuineness of anything is determined.

M.E. test, originally "a small vessel for refining or assaying metals," from O.Fr. test, from L. testum "earthen pot," related to testa "piece of burned clay, earthen pot, shell," related to texere "to weave;" → technique.

Âzmun, from âzmudan, âzmây- "to try, experiment, test;" Mid.Pers. uzmudan, ôzmutan "to test, try, prove;" from O.Pers./Av. *uz-mây-, from uz-, → ex-, + mť(y)- "to measure;" from PIE *me- "measure;" cf. Skt. mati "measures," matra "measure;" Gk. metra "lot, portion;" L. metri "to measure."

test mass
  جرم ِ آزمون   
jerm-e âzmun

Fr.: test masse   

Any of a pair of identical 1.96 kg gold-platinum cubes measuring 4.6 cm on a side that are planned to be used in the → eLISA experiment to detect → gravitational waves. The test masses will be released in → free fall in the the → LISA Pathfinder spacecraft. The aim is to test methods and techniques that will be used in the eLISA experiment to detect gravitational waves. Even in space there are forces capable of disturbing the cubes, including the radiation and wind from the Sun. Hence the test masses need be isolated from all of these non-gravitational influences. To do so, LISA Pathfinder continually measures their positions and manoeuvres around them with microthrusters to avoid ever touching them.

test; → mass

test of significance
  آزمون ِ نشاناری   
âzmun-e nešânâri

Fr.: test de significativité   

Same as → significance testing and → rule of decision.

test; → significance.

test particle
  ذره‌ی ِ آزمون   
zarre-ye âzmun

Fr.: particule-test   

In → plasma physics, → fluid dynamics, and → self-gravitating systems, a particle or ensemble of particles which are affected by the evolution of the rest of the system, but do not affect the rest of the system. The test particle concept is used, e.g., for revealing a flow, describing the path of fluid elements, and so on.

test; → particle.

test time
  زمان ِ آزمون   
zamân-e âzmun

Fr.: temps de test   

That part of the working time of a telescope devoted to tests of coupled instruments or the telescope itself.

test; → time.

testability
  آزمون‌پذیری   
âzmunpaziri (#)

Fr.: testabilité   

The state or fact of being → testable. See also → falsifiability.

testable; → -ity.

testable
  آزمون‌پذیر   
âzmunpazir (#)

Fr.: testable   

The quality of a claim, hypothesis, or theory that can be verified by tests or experiments. See also → falsifiable.

test; → -able.

Tethys
  تتوس   
Tetus (#)

Fr.: Téthys   

The ninth of Saturn's known satellites. It it 1060 km across and orbits at a mean distance of 294,660 km from Saturn. It has a rotational period of 1.89 days that equals its orbital period. Tethys is thought to be composed almost entirely of water-ice because of its low density (1.21 gm/cm3). The western hemisphere of Tethys is dominated by a huge impact crater called Odysseus, whose 400 km diameter is nearly 2/5 of that of Tethys itself. Tethys has two moons named Telesto and Calypso. It was discovered by J.-D. Cassini in 1684.

In Gk. mythology Tethys was a Titaness and sea goddess who was both sister and wife of Oceanus.

tetra-
  چهار-   
cahâr- (#)

Fr.: tétra-   

Combining form meaning four.

From Gk. tetra-, combining form of tettares, tessares "four," cognate with Pers. cahâr, → four.

tetrad
  چهارگان   
cahârgân

Fr.: tétrade   

1) A group of four.
2) A sequence of four → total lunar eclipses occurring at approximately six month intervals. Tetrads are relatively rare events. The first → total eclipse of a tetrad occurred on 15 April 2014, the next eclipse of the series will happen on 8 October 2014 and the next two eclipses on 4 April and 28 September 2015, respectively. The previous tetrad happened in 2003-2004 and the next one will be in 2032-2033.

From Gk. tetrad-, stem of tetras "group of four."

Cahârgân, from cahâr, → four, + -gân suffix of plurality.

tetragon
  چهارگوش   
cahârguš (#)

Fr.: tétragone   

Same as → quadrangle.

From Gk. tetragonon, from → tetra- + -gon "angled, angular," from gonia "angle," related to gony "knee;" L. genu "knee;" Mod.Pers. zânu "knee;" Av. žnav-, žnu- "knee;" Skt. janu-; PIE base *g(e)neu-.

Cahârguš "four-cornered," from cahâr, câr "four," cognate with L. quattuor, → four, + gušé, guš "corner, angle;" Mid.Pers. gôšak "corner."

tetrahedron
  چهاردیمه   
cahârdimé

Fr.: tétraèdre   

A solid figure having four plane faces.

tetra-; → -hedron.

<< < -es -it -sc 201 951 abe abs abs aca acc acc aco act ada adh ado aer aft air Alf alg alk alp Alt alt amb ana And ang ani ann ant ant ant apo app app Apu arc arg Arn art ass ast ast ast atm ato att aur aut avo azi bac bal bar bar bat Bea Bel bet bia big bin bio Bir bla bla blo Blu bol Boo bou box bre Bri bro bur cal cal Can cap car Car cat cau cel cen cen cha Cha cha che Chi chr cir cir civ cla clo clo CMB coa coe coh col col col com com com com com com com com Com con con con con con con con con con con con con coo cor cor cor Cos cos cos cou cou cra cri cro cry cul cur cyc D l dar dat day dea dec dec dec def def deg Del Den dep der det deu dew dic dif dif dil dip dir dis dis dis dis dis diu dog Dop dou Dra Dsc dus dwa dyn Dys Ear ecc eco edg egg Ein Ela ele ele ele ele ell eme emp enc eng ent epi equ equ equ eru eth Eur eve exa exc exe exi exo exp ext ext ext fab fai Fan fea fem fer fie fil fir fir fla fli flu foc for for for fra fre fre fri fun fuz gal gal gal Gam gau Gau gen geo geo geo geo Gib glo gov gra gra gra gra gre gro Gui H-a hal Ham har Hay hea hei hel Hel her het hie hig hoa hom hor hot Hub Hug hur hyd hyd hyl hyp ice ide ima ima imp imp inc inc ind ine inf inf inf ing inn ins ins int int int int int int int int inv inv ion iro Isl iso iso Jab jet Jov Jup Kar Kep kil Kip Kra Lag Lam Lan Lar las law lea Leg Leo lev lig lim lin lin lin lit loc loc log Lor low lum lun lun Lym Mac mag mag mag mag mag mai Mal map mas mas mat Mau mea mea med Men mer Mes Met met mic mic Mie mil min Mir mix mod mol mom Moo mor mov mul mur n-b nan nat nea neg Ner neu new New NGC noc nom non non nor nor nuc nuc nul nut obj obl obs occ oct off old one ope opp opt opt orb ord org Ori osc oth ove Owl P-s Pal par par par par Pas pat pec pen per per per per per Pha pha pho pho pho phy pie pix Pla pla pla pla Pli Poi pol pol pol pol por pos pos pow pre pre pre pre pri pri pri pro pro pro pro pro pro pro pub pul pyc qua qua qua qua qui rad rad rad rad rad rad rai ran rar Ray rea Rea rec rec red red ref ref reg rel rel rel ren res res res res ret rev Ric rig rin roc roo rot rot rur S5- Sal sat sca sca Sch sci Scu sec sec sed sel sel sem seq set sha she sho sid sie sil sim sin sit sky slo sno sod sol sol sol sol son sou spa spa spe spe spe spe sph spi spo squ sta sta sta sta ste ste ste Sti sto str str sub sub sub sul sup sup sup sup sur sur syl syn sys tal Tay tel ten ter tex the the the the Tho thr tid tim Tit too Tor tra tra Tra tra Tra tri Tri tru tub tur two Typ ult ult unc uni uni uni upl ura uti val var vec vel ver Ver vie vir vis vis vol W-R war wav wav wea Wei wha wid win WN3 Wol wri xen yok zen zij > >>