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agglomeration bargolemeš Fr.: agglomération 1) A jumbled cluster or mass of varied parts. Verbal noun of → agglomerate. |
Agilkia Agilkia Fr.: Agilkia The site where → Rosetta's Philae lander is scheduled to touch down on Comet 67P/→ Churyumov-Gerasimenko on 12 November 2014. Named for Agilkia Island ( |
agitate žilidan Fr.: 1) agiter, remuer; 2) émouvoir, troubler; 3) faire de
l'agitation, exciter l'opinion publique 1) To move or force into violent, irregular action. To shake or move briskly. From L. agitatus, p.p. of agitare "move to and fro," frequentative of agere "to drive," → act. Žilidan, from Lori, Laki žil "shaking, moving," related to žir, → act. |
agitation žileš Fr.: agitation The act or process of agitating; state of being agitated. → thermal agitation. Verbal noun of → agitate. |
agitator žilešgar Fr.: agitateur 1) A person who stirs up others in order to upset the status quo and further a
political, social, or other cause. → agitate; → -or; → turbulence. |
agree sâcandan Fr.: consentir, convenir, être d'accord 1) To have the same views, emotions, etc.; harmonize in opinion or feeling
(often followed by with). M.E. agre, agreen, from O.Fr. agreer "to receive with favor, take pleasure in," from phrase a gré "favorably, of good will," from L. → ad- "to" + gratum "pleasing," neuter of gratus "pleasing, agreeable," from PIE root *gwer- "to praise;" cf. Pers. gerâmi "dear, revered," from Av. gar- "to praise;" Skt. grnati "sings, praises," Lith. giriu "to praise, celebrate." Infinitive from sâcan, → agreement. |
agreement sâcan Fr.: accord 1) The act of agreeing or of coming to a mutual arrangement. Verbal noun from → agree + → -ment. Sâcan, from sâz-, saz, sac-, sâj-, Pers. sâz-, sâxtan "to build, prepare; to agree, be compatible; to adapt, adjust;" sazidan "to suit, fit, be worthy," sazâ "suitable, agreeing with, congruous, deserving of;" Baluchi sâc-/sâcit "to adjust, be suitable, agree;" Mid.Pers. sacitan/sazidan "to fit," sazešn "fitness," sazâg "fitting, worth;" Av. sak- "to understand, to mark," sâcaya- (causative) "to teach;" Proto-Ir. *sac- "to fit, be suitable; to prepare;" + suffix -an, → minus. |
agriculture kešâvarzi (#) Fr.: agriculture The occupation or science of cultivating the land, producing crops, and feeding, breeding, and raising livestock; farming. M.E., from M.Fr., from L. agricultura, compound of agri cultura "cultivation of land," from agri, genitive of ager "a field" + cultura "cultivation," → culture. Kešâvarzi "agriculture," from kešâvarz "farmer, cultivator," from kešt-varz. The first component kešt, variant kâšt, from kâštan, keštan, variants of kâridan "to cultivate, to plant;" Mid.Pers. kištan, kâridan "to sow, plant; to make furrows;" Av. kar- "to strew seed, cultivate," kāraiieiti "cultivates;" cf. Skt. kar- "to scatter, strew, pour out." The second component varz agent noun of varzidan "to labor, exercise, practise;" cf. Gk. ergon "work;" Arm. gorc "work;" Lith. verziu "tie, fasten, squeeze," vargas "need, distress;" Goth. waurkjan; O.E. wyrcan "work," wrecan "to drive, hunt, pursue;" PIE base *werg- "to do, to work." |
air havâ (#) Fr.: air The mixture of gases of which the earth's atmosphere is composed. It is chiefly made up of Nitrogen (about 78%) and Oxygen (about 20%). Air, from O.Fr. air, L. aer, Gk. aer, related to Gk. aura "breath, vapor;" PIE *wer- "to raise, lift." Havâ, from Ar., probably a loanword from Mid.Pers. vây "weather," Av. vayah-, vaya- "weather, atmosphere," from va- "to blow." Cf. Skt. va-, Gk. aemi- "to blow;" Av. vâta- "wind," Skt. vata-, L. ventus, Mod. Pers. bâd "wind." PIE *we- "to blow". |
air shower tondbâr-e partowhâ-ye keyhâni, ragbâ;r-e ~ ~ Fr.: gerbe (de rayons cosmiques) Same as → cosmic-ray shower. |
aircraft havânâv Fr.: avion A machine capable of flying by means of → buoyancy or → aerodynamic forces, such as an airplane, helicopter, glider, or balloon. |
airglow havâforuz, šabforuq Fr.: luminescence nocturne The faint ever-present glow in the → night time → sky caused by the → collision of → atoms and → molecules in Earth's → upper atmosphere with high energy → particles and → radiation, mainly from the → Sun. The airglow, also called nightglow, varies with time of night, → latitude, and → season. |
airmass havâtud, tude-ye havâ (#) Fr.: masse d'air A measure of the path length traversed by starlight through Earth's atmosphere before it reaches the detector; it is taken relative to the length at the zenith. |
Airy disk gerde-ye Eyri Fr.: tache de diffraction, ~ d'Airy The bright disk-like image of a point source of light, such as a star, as seen in an optical system with a circular → aperture. Named after Sir George Biddell Airy (1801-1892), Astronomer Royal, great administrator, who much improved the equipment at Greenwich Observatory. → disk. Gerdé, → disk; Airy, see above. |
Airy transit circle parhun-e nimruzâni-ye Airy Fr.: circle méridien d'Airy A → transit circle that defines the position of the → Greenwich Meridian since the first observation was taken with it in 1851. Airy's transit circle lies at longitude 0°, by definition, and latitude 51° 28' 38'' N. Named after Sir George Biddell Airy (1801-1892), Astronomer Royal, at the Royal Observatory in Greenwich from 1835 to 1881. Airy transformed the observatory, installing some of the most advanced astronomical apparatus of his day and expanded both staff numbers and their workload; → transit; → circle. |
albedo sepidâ (#) Fr.: albedo The fraction of the total light or other radiation which falls on a non-luminous body, such as a → planet, → satellite, or → asteroid, and which is reflected by it. Generally, the albedo is equal to the ratio between the light quantity reflected and the light quantity received. The albedo values range between 0.0 (0%), for a perfectly black area, which absorbs all incident light, and 1.0 (100%) for a perfect reflector. The planets or planetary satellites with dense atmospheres have greater albedos than those of transparent atmospheres or of no atmospheres. The albedo can vary from one surface point to another, so that a mean albedo is given for practical purposes. The natural surfaces reflect different light quantities in different directions and the albedo can be expressed in several ways, depending on the way in which the measurement was made: in one direction or, on the average, in all directions (M.S.: SDE). See also → Bond albedo, → geometric albedo. Albedo, L. "whiteness," from albus "white," from PIE base *albho- "white". Compare with Gk. alphos "white leprosy," O.H.G. albig, O.E. elfet "swan, the white bird". The idea of whiteness derives from the fact that whiter bodies have a higher reflective power, while opaque objects are more absorptive. Sepidâ, from sepid, →, white, + -â noun-forming prefix from certain adjectives. |
Albireo (β Cygni) Menqâr-e Dajâjé (#), Nok-e Mâkiyân Fr.: Albiero The second brightest star of the constellation → Cygnus, with a visual magnitude of 3.0. It is a double star of strikingly different colors, with components separated by 35''. The brighter component is a K3 giant while its partner is a main-sequence B9 star. About 380 → light-years away, the two rotate around each other with a period of about 75,000 years. The main component is itself a binary system. Albireo may be a corruption of the L. phrase ab ireo "from the rainbow," as suggested by some writers on star names. It does not mean "the hen's beak". Menqâr-e Dajâjé "hen's beak," from Ar. Minqâr
al-Dajâjah, from minqâr "beak" + dajâjah "hen". |
alcohol alkol (#) Fr.: alcool An organic compound having a → hydroxyl (-OH) group attached to a carbon atom. Specifically the term is applied to ethyl alcohol or → ethanol (C2H5OH). Alcohol exists abundantly in the → interstellar medium in gaseous state also in the form of → methanol. The discovery of alcohol is attributed to the Iranian physician and scientist
Mohammad son of Zakariyâ Râzi (864-930 AD, known in Europe as Razes or Rhazes).
He wrote in Ar., which was the scientific language of
that period. However, he himself did not use a specific term for this substance
as far as we know.
Alcohol was first used in medicine about 1250 by two Italian physicians Valis de Furo and
Thaddaeus of Florence. It was not yet called alcohol, but aqua ardens or
aqua vini. The name alcohol, of Arabic origin, was introduced by
the Swiss alchemist and physician Paracelsus (1493-1541) in the
sixteenth century. It is composed of two parts,
al-, a definite article (like "the"), plus a second component the origin of
which is not clear.
A broadly spread explanation for the second component is (kuHl)
|
Alcor Sohâ (#) Fr.: Alcor A 4th magnitude star lying in the constellation → Ursa Major (also called 80 Ursae Majoris) which forms a visual pair with the brighter star → Mizar (Zeta Ursae Majoris). Alcor is separated by about 11.5 minutes of arc from Mizar. It is a → main sequence star of type A5 with a mass of 1.8 Msun. Recent observations show that Alcor is a → spectroscopic binary, whose → companion has M-band (λ = 4.8 μm) magnitude 8.8 and projected separation 1''.11 (28 AU) from Alcor. The companion is most likely a low-mass (~ 0.3 Msun) active star which is responsible for Alcor's → X-ray emission detected by → ROSAT (LX ~ 1028.3 erg/s). Alcor is a nuclear member of the → Ursa Major star cluster (distance ~ 25 pc, age ~ 0.5 Gyr). The Alcor binary is probably → gravitationally bound to the Mizar star system, making them a → sextuplet with physical separation 0.36 pc, or 74,000 → astronomical units (Mamajek et al., 2010, AJ 139, 919). Alcor, perhaps from Ar. al-khawr "the low ground." Sohâ, from Ar. Suhâ. |
Alcyone (η Tauri) Alkuone, Nayyer-e Sorayyâ, Raxšân-e Parvin Fr.: Alcyone The brightest star in the → Pleiades, located in the constellation → Taurus. → Apparent visual magnitude 2.87, → spectral type B7 III. In Gk. mythology, a daughter of Aelous who, with her husband, Ceyx, was transformed into a kingfisher. Nayyer-e Sorayyâ "the bight of the Pleiades," from Ar. nayyir
"luminous" + Thorayyâ "the Pleiades". |
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