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: 13116 Search : far
hydrogen coma
  گیس ِ هیدروژنی   
gis-e hidroženi

Fr.: chevelure d'hydrogène   

The cometary cloud of hydrogen, detectable in ultraviolet light, that is immensely bigger than even the huge visible coma it surrounds. It is produced by the dissociation of water into hydrogen and oxygen and by other processes set into motion by solar radiation and and the solar wind.

hydrogen, → coma.

hydrogen cyanide (HCN)
  سیانور ِ هیدروژن   
siyânur-e hidrožen (#)

Fr.: cyanure d'hydrogène   

A colorless or light blue liquid or gas, a triatomic cyanide, which is extremely flammable. HCN is an important industrial chemical and over a million tonnes are produced yearly in the world. It is produced industrially by reacting methane and ammonia in air at high temperature. A wide range of combustion processes produce HCN gas in the smoke or fumes. HCN is found naturally throughout the environment at low levels as it is released from volcanoes and certain plants and bacteria. Hydrogen cyanide is abundant in all kinds of astronomical environments, from dark clouds to star-forming regions and circumstellar envelopes. The first detection of interstellar HCN (at 88.6 GHz) and H13N (at 86.3 GHz) was reported by Buhl & Snyder (1971, ApJ 163, L47). Also called → hydrocyanic acid and → prussic acid.

hydrogen; → cyanide.

hydrogen fusion
  ایوش ِ هیدروژن   
iveš-e hidrožen

Fr.: fusion de l'hydrogène   

A → nuclear reaction where hydrogen (H) nuclei combine to form helium (4He) nuclei. Same as the → proton-proton chain.

hydrogen; → fusion.

hydrogen ion
  هیدرون، یون ِ هیدروژن   
hidron, yon-e hidrož

Fr.: hydron, ion hydrogène   

Chemistry: The → positively charged hydrogen atom, H+, formed by removal of the orbital electron. Same as → proton.

hydrogen; → ion.

hydrogen line
  خط ِ هیدروژن   
xatt-e hidrožen (#)

Fr.: raie de l'hydrogène   

An → emission or → absorption line in the spectra of various astronomical objects produced by the presence of hydrogen atoms in particular physical conditions.

hydrogen, → line.

hydrogen shell burning
  سوزش ِ پوسته‌ی ِ هیدروژن   
suzeš-e puste-ye hidrožen

Fr.: combustion de la coquille d'hydrogène   

A phase in the life of a star that has left the → main sequence. When no more hydrogen is available in the core, the core will start to contract as it is no longer releasing the necessary energy whose pressure supports the surrounding layers. As a result of this contraction, gravitational energy is converted into thermal energy and the temperature will rise. Therefore a shell of unprocessed material surrounding the original core will be heated sufficiently for hydrogen burning to start. During the evolution of → asymptotic giant branch stars hydrogen shell burning occurs alternatively with helium shell burning. → double shell burning.

hydrogen; → shell; → burning.

hydrogenate
  هیدروژنیدن   
hidroženidan

Fr.: hydrogéner   

To undergo or cause to undergo a reaction with hydrogen. Same as → hydrogenize.

hydrogen; → -ate.

hydrogenation
  هیدروژنش   
hidroženeš

Fr.: hydrogénisation   

The process of combining or exposing to → hydrogen.

hydrogenize
  هیدروژنیدن   
hidroženidan

Fr.: hydrogéner   

hydrogenate.

hydrogen; → -ize.

hydrography
  آب‌نگاری   
âbnegâri (#)

Fr.: hydrographie   

The study, measurement, and description of depths and currents in open seas, lakes, estuaries, and rivers.

hydro- + → -graphy.

hydrologic cycle
  چرخه‌ی ِ آب‌شناسیک، ~ آب‌شناختی   
carxe-ye âbšenâsik (#), ~ âbšenâxti (#)

Fr.: cycle hydrologique   

The vertical and horizontal transport of water in all its states between the earth, the atmosphere, and the seas; often called the water cycle.

Hydrologic, pertaining to → hydrology; → cycle.

hydrology
  آب‌شناسی   
âbšenâsi (#)

Fr.: hydrologie   

The study of the waters of the earth, especially with relation to the effects of precipitation and evaporation upon the occurrence and character of water in streams, lakes, and on or below the land surface.

Hydrology, from → hydro-; + → -logy.

hydromagnetics
  هیدرومغناتیک   
hidromeqnâtik

Fr.: hydromagnétisme   

Same as → magnetohydrodynamics.

hydro-; → magnetics.

hydron
  هیدرون   
hidron (#)

Fr.: hydron   

The general name for the atomic hydrogen → cation H+.

hydro-; → -on.

hydronium
  هیدرونیوم   
hidroniom

Fr.: hydronium   

A → water, → molecule with an additional hydrogen ion (H3O+). Also called hydronium ion. Hydronium is an abundant molecular ion in the interstellar diffuse and dense molecular clouds (→ Sagittarius B2, → Orion molecular cloud OMC-1) as well as the plasma tails of → comets (→ Halley, → Hale-Bopp).

From hydr-, → hydro- + -onium a suffix used in the names of complex cations, extrcated from ammonium "ionized ammonia" (NH4+).

hydrosphere
  آب‌سپهر   
âbsepehr (#)

Fr.: hydrosphère   

A term denoting the water portion of the Earth's surface.

hydro-; → sphere.

hydrostatic
  هیدر-ایستاییک، هیدر-ایستا   
hidristâik

Fr.: hydrostatique   

Of or pertaining to → hydrostatics.

hydro- + → static.

hydrostatic equation
  هموگش ِ هیدر-ایستاییک   
hamugeš-e hidristâik

Fr.: équation hydrostatique   

The equation describing the → hydrostatic equilibrium in a star, expressed as: dP/dr = -GMρ/r2, where P and M are the mass and pressure of a spherical shell with thickness dr at some distance r around the center of the star, ρ is the density of the gas, and G the → gravitational constant.

hydrostatic; → equation.

hydrostatic equilibrium
  ترازمندی ِ هیدر-ایستاییک، ~ هیدر-ایستا   
tarâzmandi-ye hidristâik

Fr.: équilibre hydrostatique   

1) The physical situation reached in a fluid when complete balance exists between the internal pressure at any point and the weight of the material above the point.
2) For a star, the balance between the inward → gravitational force and the outward gas pressure everywhere in the star. → hydrostatic equation. See also → hydrodynamic equilibrium.

hydrostatic; → equilibrium.

hydrostatic halo
  هاله‌ی ِ هیدر-ایستا   
hâle-ye hidristâ

Fr.: halo hydrostatique   

A model of the → Milky Way galaxy in which the → Galactic halo (composed of → gas, → magnetic fields, and → cosmic rays) is assumed to be in → hydrostatic equilibrium. Parker (1966) presented the first study of stability considerations between gas, magnetic fields and cosmic rays in an equilibrium configuration. He found that it is difficult to maintain a stable configuration due to magnetohydrodynamic self-attraction (→ Parker instability). Subsequent works taking into account turbulent motions showed that turbulent pressure can mitigate the influence of Parker instabilities. This enabled new attempts to find conditions under which a stable equilibrium configuration of the Galaxy could exist.

hydrostatic; → halo.

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer aga air Alf Alg alk Alp alt alu amm ana And ang ani ano ant ant Ap apo app app Aqu Arc arg arr asc ass ast ast asy atm ato att aur aut axi B-m bad Bal bar bar Bay Bed ber Bet bif bim bin bio bis bla ble blu Bod Bol bor bou Bra Bre bro bul C-t Cal Cam can car Car Cas cat cav cel cen cer Cha cha Cha che chl Cir cir cir Cla cli clo clu co- coc 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 Cre cri cro cub cur cyc cyl Dan dat Dav de- Deb dec dec dee def deg del Den den der det deu dew dic dif dif dil Dip dir dis dis dis dis dis diu dod Dop dou Dra dua dus dwa dyn DZ Ear ecc eco edi EHB Ein ela ele ele ele ele ell eme emp end Eng ent epi equ equ era ESP eth Eur evi exa exc exe exi exp exp ext ext ext fac fal far fec Fer fer fie fin fir fis fla Flo flu fog for for Fou fra fre fre Fro fun G s Gal gal gal Gar gau geg gen geo geo geo ger gla gly gra gra gra gra gra Gre gro GYR Had Hal hap Har HD hea hel hel Hen Her hex hig Hil hol Hoo hor hou Hub hum hyb hyd hyd hyp hys ide ign ima imp imp in- inc Ind ind ine inf inf inf ini ins ins ins int int int int Int int int int inv ion iri irr iso iso iso Jea Jor jum K c Kep Ker kin kno lab Lam Lan Lap las lat Le lef len lev lig lig lin lin lin liq Lit loc log lon lou LS lun lun Lym M s Mag mag mag mag mag mag maj man Mar mas mas mat May mea mec mel mer mes met met met mic mid mil Min Mir mix mod mod mol mon mor mov mul mur mys nan nat nav nec Nep neu New New NGC nob nom non non nor nos nuc nuc num nut obj obl obs occ oct off oli oni ope opp opt opt orb ord org orp osc out ove oxi P-w pal par par par par Pas pat pej per per per per per per pha Phe pho pho pho phy pin pla Pla pla pla pla plu poi pol pol Pol pol por pos pot Poy pre pre pre pre pri pri pri pro pro pro pro pro pro Psa pul pum Q i qua qua qua qua R A rad rad rad rad rad rad Ram Ran rat rea rea rec rec red red ref ref reg rei rel rel rem rep res res res ret rev Rho Rie ril riv rog Ros rot rul S A Sag sam sat sca sca Sch Sco Sec sec sec seg sel sem sen set Sha sha shi sho sid sig sim sin Sir ske sli Smo soc sof sol sol sol sol sou sou spa spe spe Spe spe sph spi Spi spr sta sta sta sta sta ste ste ste Sto str str sub sub sub suc sun sup sup sup sup sur swa syn syn tac tas tel tem ter tes the the the the thi thr tid til tip ton tor tou tra tra tra tra Tri tri tru tsu tur two Typ UHE ult unc uni uni uni upg 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 > >>