An Etymological Dictionary of Astronomy and Astrophysics
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فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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Number of Results: 13176 Search : far
liter
  لیتر   
litr

Fr.: litre   

A metric unit of volume, formerly defined as the volume of one kilogram of pure water under standard conditions; now equal to 1 cubic decimeter (dm3); hence 1 liter = 0.001 m3 and 1000 liter = 1 m3.

From Fr. litre, from litron, obsolete Fr. measure of capacity for grain, from M.L. litra, from Gk. litra "pound."

literature
  نوشتارگان   
neveštârgân (#)

Fr.: littérature   

1) Writings in which expression and form, in connection with ideas of permanent and universal interest, are characteristic or essential features, as poetry, novels, history, biography, and essays.
2) The entire body of writings of a specific language, period, people, etc.
3) The writings dealing with a particular subject (Dictionary.com).

From L. literatura/litteratura "writing, grammar, learning," from litera/littera "letter."

Neveštârgân, from neveštâr, literally "written; writing," verbal noun from neveštan, nevis- "to write;" Mid.Pers. nibištan, nibes- "to write;" Av./O.Pers. nī- "down; in, into," → ni- (PIE), + paēs- "to paint; to adorn," paēsa- "adornment" (Mid.Pers. pēsīdan "to adorn"); O.Pers. pais- "to adorn, cut, engrave" (Mod.Pers. pisé "variegated"); cf. Skt. piśáti "adorns; cuts;" Gk. poikilos "multicolored;" L. pingit "embroiders, paints;" O.C.S. pisati "to write;" O.H.G. fēh "multicolored;" Lith. piēšti "to draw, adorn;" PIE base *peik- "colored, speckled," + -gân suffix of suffix forming plural entities, from Mid.Pers. -gânag.

lithium
  لیتیوم   
litiom (#)

Fr.: lithium   

A metallic → chemical element; symbol Li. → Atomic number 3; → atomic weight 6.941; → melting point about 180.54°C; → boiling point about 1,342°C. Lithium is a soft, silver-white metal. It is the lightest metal and one of the alkali metals in Group 1 of the → periodic table. Lithium does not occur on Earth in its free form. It is a minor part of almost all igneous rocks and is found in many natural brines, in total 0.0007% of the Earth's crust. It has two stable → isotopes, 7Li (92.5%) and 6Li (7.5%). The element was discovered in the mineral petalite, LiAl(Si2O5)2, by the Swedish mineralogist Johan August Arfwedson in 1817. It was isolated by W.T. Brande and Sir Humphrey Davy. Many uses have been found for lithium and its compounds. Lithium has the highest → specific heat (3.6 J/gK) of any solid element and is used in heat transfer applications. It is used in rechargeable lithium ion batteries. It is also used as an alloy with → aluminum, → copper, and → manganese to make high performance aircraft parts. It is used to make special glasses and ceramics, including the Mount Palomar telescope's 5 m mirror. Lithium also has various nuclear applications, for example as a coolant in nuclear breeder reactors and a source of → tritium, which is formed by bombarding lithium with neutrons. In medicine it is used to treat bipolar disorder (manic depression), a serious mental illness that causes extreme shifts in mood, energy, and functioning.
In astrophysics, → Spite plateau.

Lithium, from L. lithos "stone" because lithium was thought to exist only in minerals.

lithium I line
  خط ِ لیتیوم I   
xatt-e litiom I

Fr.: raie de lithium I   

A → resonance line of → lithium at 6707.81 Å doublet 6707.76 and 6707.91 Å.

lithium; I for → neutral atom; → line.

lithium star
  ستاره‌ی ِ لیتیومی   
setâre-ye litiomi (#)

Fr.: étoile à lithium   

A peculiar evolved star of spectral type G or M whose spectrum displays a high abundance of lithium.

lithium; → star.

lithium test
  آزمون ِ لیتیوم   
âzmun-e litiom

Fr.: test du lithium   

The presence or not of the lithium absorption line at 6708 Å, which is considered to be a sufficient condition for → substellarity in → L dwarfs. It has been shown that any object with lithium absorption and → effective temperature less than 2670 K is a → brown dwarf. For a discussion of potential problems with the lithium test see Kirkpatrick et al. (1993, ApJ 406, 701).

lithium; → test.

litho-
  لیتو-، سنگ-   
lito-, sang-

Fr.: litho-   

A prefix meaning "stone," used in the formation of compound words.

From Gk. lithos "stone."

Lito-, loan from Gk., as above.
Sang-, from sang, → stone.

lithophile
  سنگدوست، لیتودوست   
sangdust, litodust

Fr.: lithophile   

lithophile element.

litho-; → -phile.

lithophile element
  بن‌پار ِ سنگدوست، ~ لیتودوست   
bonpâr-e sangdust, ~ litodust

Fr.: élément lithophile   

In the → Goldschmidt classification, a → chemical element that shows an → affinity for → silicate phases and is concentrated in the silicate portion of the Earth (→ crust and → mantle). This group includes → lithium (Li), → beryllium (Be), → sodium (Na), → magnesium (Mg), → potassium (K), → calcium (Ca), → barium (Ba), → titanium (Ti), → chromium (Cr), → aluminium (Al), → silicon (Si), → phosphorus (P), → chlorine (Cl), etc.

lithophile; → element.

lithosphere
  سنگ‌سپهر، لیتوسپهر   
sangsepehr (#), litosepehr

Fr.: lithosphère   

The solid portion of the → Earth, as compared to the → atmosphere and the → hydrosphere. The lithosphere consists of semi-rigid plates that move relative to each other on the underlying → asthenosphere. The process is known as → plate tectonics and helps explain → continental drift.

litho-; → sphere.

Little Dipper
  هفت خواهران، چمچه‌ی ِ کوچک   
haft xâharân (#), camce-ye kucak (#)

Fr.:   

An asterism in the constellation → Ursa Minor. This group of stars ends at → Polaris, the pole star of the Northern Hemisphere.

Little, from M.E., O.E. lytel, from W.Gmc. *lutila- (cf. Du. luttel, O.H.G. luzzil, Ger. lützel, Goth. leitils), from PIE *leud- "small;" dipper, from dip, O.E. dyppan "immerse," from P.Gmc. *dupjanan.

Haft xâharân "the seven sisters," from haft "seven" (Mid.Pers. haft; Av. hapta; cf. Skt. sapta; Gk. hepta; L. septem; P.Gmc. *sebun; Du. zeven; O.H.G. sibun; Ger. sieben; E. seven; PIE *septm) + xâharân plural of xâhar "sister;" Mid.Pers. xwâhar "sister;" Av. xvanhar- "sister;" cf. Skt. svásar- "sister;" Sogdian xwār; Gk. eor; L. soror (Fr. soeur); Arm. k'oyr; O.C.S., Rus. sestra; Lith. sesuo; O.Ir. siur; Welsh chwaer; M.Du. suster; Du. zuster; O.H.G. swester; Goth. swistar; Ger. Schwester; Swed. sister; Dan. søster; O.E. sweostor, swuster; E. sister.
Camcé "a spoon, ladle; a wooden bowl or cup;" kucak "small" (Mid.Pers. kucak "small"), related to kutâh "short, small, little," kudak "child, infant," kutulé, → dwarf, Mid.Pers. kôtâh "low," kôtak "small, young; baby;" Av. kutaka- "little, small").

Little Ice Age
  عصر ِ یخ ِ کوچک   
asr-e yax-e kucek

Fr.: petit âge glaciaire   

A roughly 400-year period from the mid-16th through the mid-19th centuries when temperatures over much of Europe were unusually cold. Glaciers in the Alps advanced and European rivers froze much more often than during the past century. Harvests failed, livestock perished, and poor people suffered from famine and disease. The Little Ice Age coincided with two successive low → solar activity periods, the → Sporer minimum and the → Maunder minimum.

little; → ice; → age.

Littrow prism
  منشور ِ لیترو   
manšur-e Littrow

Fr.: prisme de Littrow   

A prism having angles of 30, 60, and 90°, which uses the same face for input and dispersed radiation. The beam is reflected at the face opposite to the 60° angle because it is coated to be highly reflecting. A beam entering at the → Brewster angle undergoes minimum deviation and hence maximum dispersion. Littrow prisms are used in laser cavities to fine tune lasers by selection of wavelength.

Joseph Johann Littrow (1781-1840), Austrian astronomer; → prism.

Lloyd's mirror
  آینه‌ی ِ لوید   
âyene-ye Lloyd (#)

Fr.: miroir de Lloyd   

An optical arrangement in which light from a source is allowed to fall on a plane mirror at → grazing incidence. The light directly coming from the source interferes with the light reflected from the mirror forming an → interference pattern. See also → Fresnel's biprism, → Fresnel's mirrors.

After the Irish physicist Humphry Lloyd (1800-1881); → mirror.

load
  ۱) بار؛ ۲) بار کردن   
1) bâr; 2) bâr kardan (#)

Fr.: 1) charge; 2) charger   

1) Something that is borne or carried.
2) Computers: To bring (a program or data) into main storage from external or auxiliary storage.
To place (an input/output medium) into an appropriate device, as by inserting a disk into a disk drive. See also: → download, → upload, → overload.

From M.E. lode, originally the same word as lode, from O.E. lāad "way, course, carrying;" cf. O.N. leith "way, route," O.H.G. leita "procession."

Bâr kardan "to load," composite verb from bâr "load, charhe, burden," (Mid.Pers. bâr, from O.Pers./Av. base bar- "to bear, carry;" Mod.Pers. bordan "to carry;" L. brutus "heavy, dull, stupid, brutish;" Skt. bhara- "burden, load," bharati "he carries;" Gk. baros "weight;" Mod.Pers. gerân "heavy;" Skt. guru; L. gravis; PIE *gwere- "heavy," *bher- "carry, give birth") + kardan "to do, to make" (Mid.Pers. kardan; O.Pers./Av. kar- "to do, make, build;" Av. kərənaoiti "he makes;" cf. Skt. kr- "to do, to make," krnoti "he makes, he does," karoti "he makes, he does," karma "act, deed;" PIE base kwer- "to do, to make").

loading
  بارکرد   
bârkard

Fr.: chargement   

The act of a person or thing that loads. See also: → download, → upload.

Verbal noun of → load.

lobate scarp
  تنده‌ی ِ لاپه‌ای   
tonde-ye lâpe-yi

Fr.: escarpe lobée   

A surface feature on a planet or satellite in the form of a line of cliffs. Lobate scarps are formed when planetary or lunar mantle cools down and contracts inside. The loss of volume squeezes portions of the outer crust together. Eventually, the crust breaks and some of it is pushed up, creating long cliffs that look like wrinkles. Lunar scarps are generally tens of kilometers long and less than 100 m high. They have formed during the last billion years.

Lobate "having the form of a → lobe;" → scarp.

lobe
  لپ   
lap (#)

Fr.: lobe   

General: A roundish projection that is part of a larger structure.
Radioastronomy: In an antenna pattern, a region of local maximum in the emitted intensity. The strongest lobe is in the pointing direction of a directional antenna and is called the main lobe.
Quasar: One of the two lobe-like structures well apart from the central source, observed in radio images of some quasars. Same as radio lobe.

From M.L. lobus, from L.L. lobus "hull, husk, pod," from Gk. lobos "lobe of the ear, vegetable pod," probably related to leberis "husk of fruits;" from PIE base *lep- "to peel, flay."

Lap "lobe," variants lâp, lâb "piece, big piece, big cut," lappé "split pea; any of the two parts of a timber split through the length," maybe cognate with Gk. lobos, as above. Alternatively, related to Pers. las "loose," PIE *leu- "to loosen, divide, cut apart" (cf. Gk. lyein "to loosen, untie, slacken," lysus "a loosening;" L. luere "to loose, release;" → analysis).

lobe pattern
  ا ُلگوی ِ لپ‌ها   
olgu-ye laphâ

Fr.: fonction de lobe   

The configuration of the response lobes of a radiotelescope.

lobe; → pattern.

lobe-dominated quasar
  کو‌آسار ِ لپ چیره   
kuasâr-e lap ciré

Fr.: quasar à lobes dominants   

A → radio-loud quasar in which the lobes dominate the whole emission. It has been conjectured that this phenomenon is an → orientation effect. If the → jet is close to the plane of the sky, the lobes will dominate. See also → core-dominated quasar.

lobe; → dominate; → quasar.

<< < -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 > >>