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strontium estonsiom (#) Fr.: strontium A metallic chemical element; symbol Sr. Atomic number 38; atomic weight 87.62; melting point 769°C; boiling point 1,384°C; specific gravity 2.6 at 20°C. Strontium is a soft, silver-yellow metal with three allotropic crystalline forms. It is found in nature only in the combined state, as in strontianite. It is used in fireworks, flares, and tracer bullets. The radioactive isotope Strontium-87, the daughter of Rubidium-87, has a half-life of 48.8 x 109 years. The name derives from Strontian "a town in Scotland." The mineral strontianite is found in mines in Strontian. The element was discovered by the Scottish chemist and physician Thomas Charles Hope in 1792 observing the brilliant red flame color of strontium. It was first isolated by the English chemist Humphry Davy in 1808. |
structure sâxtâr (#) Fr.: structure The arrangement of parts in an object or organism. M.E., from L. structura "a fitting together, adjustment, building," from structus, p.p. of struere "to pile, build, assemble," related to strues "heap," from PIE *stere- "to spread, extend, stretch out;" cf. Pers. gostar-, gostardan "to spread;" Av. star- "to spread," starati "spreads;" Skt. star- "to spread out, extend, strew," strnati "spreads;" Gk. stornumi "I spread out," strotos "spread, laid out;" Ger. Strahlung "radiation," from strahlen "to radiate," from Strahl "ray;" from M.H.G. strāle; from O.H.G. strāla "arrow, stripe." Sâxtâr, from sâxt "made; make, construction, structure; style," past stem of sâxtan, sâzidan "to build, make, fashion; to adapt, adjust, be fit" (Mid.Pers. sâxtan, sâz-, Manichean Parthian s'c'dn "to prepare, to form;" Av. sak- "to understand, to mark," sâcaya- (causative) "to teach") + -âr verbal noun suffix. |
structure formation diseš-e sâxtâr Fr.: formation des structures The study of the processes that gave rise to the apparition of matter concentrations,
such as → superclusters of galaxies,
→ galaxy clusters, and galaxies, in a homogeneous
→ expanding Universe.
Cosmic structures are believed to result from → density fluctuations
that existed in the → early Universe
before radiation and matter decoupled (→ decoupling era
or → recombination era). Initial
→ quantum fluctuations in the → inflaton field
were expanded by → inflation. Inflation amplified
them up to scales that correspond to those of galaxy clusters and beyond.
Generally, a model of structure formation includes three main ingredients: 1) background
cosmology, 2) model for fluctuation generation, and 3) types of
→ dark matter. |
study 1) parhâné; 2) parhândan Fr.: 1) étude; 2) étudier 1a) Application of the mind to the acquisition of knowledge, as by
reading, investigation, or reflection. M.E. studie, from O.Fr. estudie "care, skill, thought; study, school," from L. studium "study, application;" originally "eagerness," from studere "to press forward, be eager for, pursue," from PIE *(s)teu- "to push, stick, beat;" cf. Gk. typtein "to strike," typos "a blow, mold;" Skt. tup- "harm," tundate "pushes, stabs;" Gothic stautan "push." Parhâné, from Proto-Ir. *pari-huan- "to read thoroughly, to read through," from *pari- "through, throughout; thoroughly" (O.Pers. pariy "around, about;" Av. pairi "around, over") + *huanH- "to call;" cf. Pers. xândan, xvandan "to read, to sing" (Av. xvan- "to sound;" Skt. svana- "sound," svan- "to sound," svanati "it sounds;" O.E. swinn "music, song"); cf. Kurd. xwendin "to study, read;" Lori hané "to read;" Karingâni hoyniyan, Baluci vonag, Awromâni wânây "to read;" Khotanese hâvn- "to speak." |
Styx Styx, Stux Fr.: Styx The fifth confirmed → satellite of → Pluto discovered in 2012 using a set of the → Hubble Space Telescope. Also called Pluto V (P5). It orbits Pluto between → Charon and → Nix at a distance of about 42,000 km. Styx is estimated to have a diameter of between 10 and 30 km, and an → orbital period of 20.2 days. Named for the Greek mythological river that separates the world of the living from the realm of the dead. |
sub- zir- (#), ir- Fr.: sub- A prefix occurring originally in loanwords from L. but freely attached to elements of any origin and used with the meaning "under, below, beneath." From L. preposition sub "under" (also "next to, up to, toward"), from PIE base *upo- "from below," hence "turning upward, upward, up, over, beyond;" cf. O.Pers. upā (prep.) "under, with;" Av. upā, upa (prep.; prevb) "toward, with, on, in" (upā.gam- "to arrive at," upāpa- "living in the water," upa.naxturušu "bordering on the night"); Mod.Pers. bâ "with," from abâ; Skt. úpa (adv., prevb., prep.) "toward, with, under, on;" Gk. hypo "under;" Goth. iup, O.N., O.E. upp "up, upward." Zir- "below, down;" Mid.Pers. azêr "below, under," êr "below, down; low, under," adar "low;" Av. aδara- (adj.), aδairi- (prep.) "below;" cf. Skt. ádhara- "lower;" L. infra (adv., prep.) "below, underneath, beneath," inferus "lower;" O.E. under "under, among"); PIE base *ndher. |
sub-arcsecond zir-sâniye-yi Fr.: A measure of angle smaller than 1 arcsecond, usually until 0.1 arcsecond. → sub-; → arc second. |
sub-arcsecond imaging tasvir-gari-ye zir-sâniye-yi Fr.: Imaging in excellent seeing conditions using an adequate detector to obtain stellar images whose profile lies in the sub-arcsecond range. → sub-arcsecond; → imaging. |
sub-image zir-vine, zir-tasvir Fr.: sous-image A part of a larger image. |
subatomic zir-atomi (#) Fr.: subatomique Of, relating to, or being smaller than the atom; of or relating to the inside of the atom. |
subatomic particle zarre-ye zir-atomi (#) Fr.: particule subatomique Any particle that is small compared to the size of the atom, e.g. an electron, proton, neutron, neutrino, quark, meson, all of which are either bosons or fermions. |
subclass zir-radé (#) Fr.: sous-classe A smaller group among several into which a main class is divided, e.g. subclasses a and b among supergiants. → subtype. |
subcritical zir-paržani Fr.: sous-critique Of or pertaining to a state, value, or quantity that is less than critical, especially the condition of a → subcritical reactor. |
subcritical mass jerm-e zir-paržani Fr.: masse sous-critique An amount of → fissile material that by its mass or geometry is incapable of sustaining a → fission → chain reaction. → subcritical; → mass. |
subcritical reactor vâžirgar-e zir-paržani Fr.: réacteur sous-critique A → nuclear reactor in which the rate of production of → fission neutrons is lower than the rate of production in the previous generation, and therefore the number of fissions decreases over time. → subcritical; → reactor. |
subduction zir-hâzeš Fr.: subduction Geology: The process by which one tectonic plate slides down and below another tectonic plate as the two converge. The subduction zone is the zone of convergence of two tectonic plates, one of which usually overrides the other. From L. subductionem (nominative subductio), from subductus, p.p. of subducere "to draw away, withdraw, remove," from → sub- + ducere "to lead." Zir-hâzeš, verbal noun of zir-hâzidan, from zir-→ sub- + hâzidan, hâxtan, from Mid.Pers. "to lead, guide, persuade;" Av. hak-, hacaiti "to attach oneself to, to join;" cf. Skt. sacate "accompanies, follows;" Gk. hepesthai "to follow,"; L. sequi "to follow;" PIE *sekw-. |
subdwarf zir-kutulé Fr.: sous-naine A metal-poor main-sequence star with spectral type later than M7 and luminosity class VI. They are population II dwarfs which appear less luminous than their solar metallicity counterparts due to the dearth of metals in their atmospheres. Subdwarfs are halo members with high proper motions and large heliocentric velocities. They are important tracers of the chemical enrichment history of the Galaxy and belong to the first generation of stars formed in the Galaxy (at least 10 billion years old). |
subgiant zir-qul Fr.: sous-géante A star with a lower absolute magnitude than a normal giant star of its → spectral type. It is a star that has exhausted the hydrogen at its center and is evolving into a → red giant. Subgiants are luminosity class IV. |
subject 1, 2, 3) darâxt; 4) karin Fr.: sujet 1) Something that is being discussed, examined, or otherwise dealt with. M.E. suget, from O.Fr. suget, subget "a subject person or thing," from L. subjectus "placed beneath, inferior, open to inspection," noun use of p.p. of subicere "to place under," from → sub-"under" + combining form of jacere "to throw,"from PIE base *ye- "to do" (cf. Gk. iemi, ienai "to send, throw," Hitt. ijami "I make"). Darâxt "thing drawn in, under" from dar- + âxt.
The prefix dar-, from preposition dar "in, into, within; on, upon, above;
of, about, concerning;"
from Mid.Pers. andar "in, into, within,"
→ inter-. |
subjective 1) darâxti; 2) karini Fr.: subjectif 1) That which depends upon the personal or individual, especially where it
is supposed to be an arbitrary expression of private taste, in contrast
with the objective. Adjective of → subject. |
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