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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

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<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer AGB air Alf Alg all alp alt AM amo ana And ang ani ano Ant Ant apa apo app app Ara Arc ari Arr ash ass ast ast asy atm ato att aut ave axi Bab bal Bal bar bar bea Bek Bes bia Big bin bin bip biv bla bli blu Boh Bol Bos bou bra bri bro buo cal cal can cap car Car cat cat CCD Cen cen CH cha cha che Che chr cir cir cit cla clo clo clu 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 Cop Cor cor cor cos cos cou cou Cow cre cri cro cry cur cya Cyg dan dar dat de- deb dec dec ded def deg del dem den dep des det dev dia dif dif dih dio Dir dis dis dis dis dis dis DO don dou dow dro dur dwa dyn Dys ear ebb ecl edg egg Ein Ela ele ele ele ele ell eme emp enc eng ent epi equ equ equ esc eth Eur Eve exa exc exe exi exp exp ext ext ext fac fal far fed Fer fer fie fin fir fis fla flo flu fol for for fou fra fre Fre fro fut G-t gal gal gam gas Gau Gem gen geo geo geo gia Gli Gol gra gra gra gra gre gri gui H I Hag hal har hat He- hea hel Hel her Hes hie hig his hom hor hot Hub Hug hur hyd hyd hyg 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 Io ion iro isl iso iso Jac jet jud jur Kel Kep kil Klo Kui Lag lam Lap Lar lat law lea len lep Lib lig lim lin lin Lio lit loc LOF lon Lor low lum lun Lup Lyo mac mag mag mag mag mag mai man Mar mas mas mat Max mea mec Meg Mer Mer met met Met mic Mid Mil min Mir mit mod mod mol mon Mor mou mul mul mys nan Nat nau nec neo neu nev New NGC no nom non non nor not nuc nuc num nut obj obs obs occ ocu oft ome Oor ope opp opt opt orb ord ori ort osc out ove oxi pai pan par par par par pas pea pen per per per per Per per pha phi pho pho pho phy pio Pla pla pla pla Pla plu Poi pol pol pol poo pos pos pot pra pre pre pre pre pri pri pro pro pro pro pro Pro pro pse pul pur qua qua qua qua que rac rad rad rad rad rad rad 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 Rus Sac sal sat sca sca Sch sci Scu sec sec Sed sel Sel sen ser Sex Sha she sho sid sig sil sim sin siz sla Sma sno sof sol sol sol sol sou sou spa spa spe spe spe sph spi spi spr squ sta sta sta sta ste ste ste Sto Str str str sub sub suc sun sup sup sup sup sur swa syn syn tab tar tek tem ter tes the the the the Tho thr tid tim Tis Too Tor tra tra Tra tra tra tri tri tru Tul tur two Typ ult un- und uni uni unk upp Urc utt val var vec vel ver vib vio vir vis voi vor wan wat wav wax wea Wei whi Wil win WN9 wor X-r yel you zer zod > >>

Number of Results: 13048 Search : far
judgment
  داوری   
dâvari (#)

Fr.: jugement   

11 An act or instance of judging.
2) The ability to judge, make a decision, or form an opinion objectively, authoritatively, and wisely, especially in matters affecting action; good sense (Dictionary.com).

judge; → -ment.

judicial
  داورانه، داوریک   
dâvarâné, dâvarik

Fr.: judiciaire   

1) Pertaining to judgment in courts of justice or to the administration of justice: judicial proceedings; the judicial system.
2) Pertaining to courts of law or to judges; judiciary: judicial functions.
3) Of or relating to a judge; proper to the character of a judge; judgelike: judicial gravity.
4) Inclined to make or give judgments; critical; discriminating: a judicial mind.
5) Decreed, sanctioned, or enforced by a court (Dictionary.com).

From L. iudicalis "of or belonging to a court of justice," from iudicium "judgment, decision," from iudicem, → judge.

Dâvarâné, dâvarik, of or relating to dâvari, → judgment.

Julian calendar
  گاهشمار ِ یولیانی   
gâhšomâr-e Yuliyâni (#)

Fr.: calendrier julien   

A → solar calendar established by Julius Caesar in 46 B.C. to replace the → Roman calendar. It was inspired by the Egyptian calendar year of 365 days. The astronomer Sosigenes set up the months (January to December) and added an extra day in February every fourth year (→ leap year). This gave an average year of 365.25 days. The Julian calendar remained unchanged for 1,600 years, and was replaced by the → Gregorian calendar to correct its errors. The Roman calendar before the reform was running 80 days out of alignment with the seasons of a true year. Sosigenes fixed the calendar by having 445 days in the year 46 B.C., which brought the seasons in line with the calendar. The year 45 B.C. is known as the first leap year of the Julian calendar. However, Sosigenes' work was misinterpreted and they were placing leap years every 3 years instead of every 4 years.

Julian, adj. of L. Julius.

Julian date (JD)
  گاهداد ِ ژولی‌ین   
gâhdâd-e žulian

Fr.: date julienne   

A timekeeping system which does not have months and years. It is used primarily by astronomers to avoid confusion due to the use of different calendars at different times and places. Julian date is the interval of time in days and fractions of a day since noon 1 January 4713 B.C. (12h Universal Time). For example, January 1, 1970 is JD 2440588. Decimal fractions correspond to fractions of a day so that, for example, an observation made at 15h on June 24, 1962 is given as JD 2437840.13. → modified Julian date (MJD). Note that the "Julius" involved is not Julius Caesar, and this system is unrelated to the Julian calendar, as explained below.

The system was proposed by the French scholar Joseph Justus Scaliger (1540-1609) in 1583 and named after his father, Julius Caesar Scaliger. His choice of starting year was based on the convergence in 4713 B.C. of three calendrical cycles (indication cycle, Metonic cycle, and solar cycle). → date.

Julian day
  روز ِ ژولی‌ین   
ruz-e žulian (#)

Fr.: jour julien   

Same as → Julian date.

Julian date; → day.

Julian epoch
  زیمه‌ی ِ یولیانی   
zime-ye Yuliyâni

Fr.: époch julienne   

A way of specifying the date as a year with a decimal based on the Julian year of 365.25 days and the Barycentric Dynamical Time (TDB). The standard epoch currently in use is J2000.0, which corresponds to January 1, 2000 12:00 Terrestrial Time.

Julian calendar; → epoch.

Julian year
  سال ِ یولیانی   
sâl-e yuliyâni (#)

Fr.: année julienne   

A period of 365.25 days adopted in the Julian calendar for the length of the year.

Julian calendar; &rarr ;year.

jump
  جهش   
jaheš (#)

Fr.: saut   

A point of discontinuity in a function or a derivative of a function.

Etymology unclear, probably akin to L.G. gumpen "to jump."

Jaheš, verbal noun of jahidan, jastan "to jump, to leap," from Mid.Pers. jastan, jahidan "to jump," figuratively "to happen, occur;" Av. yaēš-, yas- "to boil;" cf. Skt. yas-, yásyati "to boil, to heat; to make effort."

jump conditions
  بوتارهای ِ جهش   
butârhâ-ye jaheš

Fr.: conditions de saut   

Very different values of pressure and density (or temperature or energy) across a shock wave.

jump; → condition.

junction
  جوهش   
juheš

Fr.: jonction   

In a → semiconductor device, a region of transition between semiconducting regions of different electrical properties.

Junction "act of joining," from L. junctionem, noun of action from jungere "to join," cognate with Pers. yuq, juhé, as below; PIE base *yeug- "to join,"

Juheš, from juh, variant of yuq "yoke," Mid.Pers. jug, ayoxtan "to join, yoke;" Av. yaog- "to yoke, put to; to join, unite;" cf. Skt. yugam "yoke;" Hittite yugan "yoke;" Gk. zygon "yoke," zeugnyanai "to join, unite;" L. jungere "to join," as above; O.C.S. igo, O.Welsh iou, Lith. jungas O.E. geoc.

junior
  کهتر   
kehtar (#)

Fr.: jeune, cadet   

1) Of more recent appointment or admission, as to an office or status; of lower rank or standing.
2) (in American universities, colleges, and schools) noting or pertaining to the class or year next below that of the senior
3) Younger, designating the younger of two men bearing the same full name, as a son named after his father; often written as Jr. or jr. following the name (Dictionary.com).

From L. iunior, comparative of iuvenis "young, young man," cognate with Pers. javân, → young.

Kehtar, comparative of keh "small, little," → decrease.

Juno
  جونو   
Juno

Fr.: Juno   

A → NASA → space mission devoted to the study of the planet → Jupiter. Juno was launched on August 5, 2011 and traveled over a total distance of roughly 2.8 billion km (1.8 → astronomical units) to reach Jupiter on July 4, 2016, after a journey of about five years. Two years after its launch Juno used a → gravity assist through an Earth → flyby in October 2013. The spacecraft will make 37 turns around Jupiter in a → polar orbit over the course of 20 months, until February 2018. Juno has nine different instruments to achieve its scientific goals. Its main goal is to understand the origin and evolution of Jupiter. Among Juno's scientific objectives, it will:
1) Determine how much water is in Jupiter's atmosphere, which helps find out which planet formation theory is correct (or if new theories are needed);
2) Look deep into Jupiter's atmosphere to measure composition, temperature, cloud motions and other properties;
3) Map Jupiter's magnetic and gravity fields, revealing the planet's deep structure;
4) Explore and study Jupiter's → magnetosphere near the planet's poles, especially the auroras, providing new insights about how the planet's enormous → magnetic field affects its atmosphere.

The spacecraft's name comes from Greco-Roman mythology. The god Jupiter drew a veil of clouds around himself to hide his mischief, but his wife, the goddess Juno, was able to peer through the clouds and see Jupiter's true nature.

Jupiter
  هرمز   
Hormoz (#)

Fr.: Jupiter   

The largest → planet in the → Solar System and the fifth from the Sun, lying at a mean distance of about 5.2 → astronomical units from the Sun. Jupiter is a → gas giant, mostly → hydrogen and → helium, with a mass of 1.898 × 1027 kg, or about 0.001 → solar masses, or 318 times → Earth masses. It is more than twice as massive as all the other solar system planets combined. Jupiter's diameter measures 11 times that of Earth. Its → rotation period, 9.93 hours (Jupiter/Earth ratio = 0.41), is the shortest of all the solar system planets. Its → orbital period is 11.857 Earth years. Jupiter has an extensive family of → satellites (79 known) and a faint → ring system; → Jupiter's ring. Jupiter probably has a core of rocky material amounting to something like 10 to 15 Earth masses. Above the core lies the main bulk of the planet in the form of liquid → metallic hydrogen. This exotic form of the most common of elements is possible only at pressures about 3 million bars, as is the case in the interior of Jupiter (and Saturn). Under the extreme pressure found deep inside Jupiter, the electrons are released from the hydrogen molecules and are free to move about the interior. This causes hydrogen to behave as a metal; it becomes conducting for both heat and electricity. See also → Jupiter's atmosphere.

Jupiter "the king of ancient Roman gods, the ruler of Olympus," from L. Iupeter, from PIE *dyeu-peter- "god-father," from *deiw-os "god" (cf. Pers. div "devil, demon;" Mid.Pers. dêw; O.Pers. daiva- "evil god, demon;" Av. daēva- "evil spirit, false god;" Skt. deva-; Gk. Zeus "supreme god;" from *dei- "to gleam, to shine") + *peter "father" (cf. Pers. pedar "father;" O.Pers. pitā- "father;" Av. patar-, ptā-; Skt. pitár-; Gk. pater; L. pater, O.H.G. fater).

Hormoz, from Mid.Pers. Ohrmazd "name of the highest god in Zoroastrianism," from O.Pers. aura-mazdā-, Av. ahura-mazdā- "Wise Lord," from ahura- "lord, god;" cf. Skt. ásura- "god, lord;" Hittite hassu- "king;" M.H.G. Asen "name of a group of gods;" O.N. āss "god;" PIE *ansu- "spirit, demon" + mazdā- "wisdom," mazdāθa- "what must be borne in mind," mazdāh- "memory;" cf. Skt. medhā- "mental power, wisdom, intelligence;" Gk. mathein "to learn, to know" (root of → mathematics).

JUpiter ICy moons Explorer (JUICE)
  پویشگر ِ مانگهای ِ یخی ِ هرمز   
Puyešgar-e Mânghâ-ye Yaxi-ye Hormoz

Fr.: Jupiter ICy moons Explorer   

An interplanetary mission currently in development by the → European Space Agency planned for launch in 2020. It is aimed mainly at in-depth studies of three potentially ocean-bearing satellites, → Ganymede, → Europa, and → Callisto. JUICE will complete a unique tour of the Jupiter system including several flybys of each planet-sized world, culminating with orbit insertion around Ganymede, the largest moon in the Solar System, followed by nine months of operations in its orbit. JUICE will carry the most powerful scientific payload ever flown to the outer Solar System. It consists of 10 state-of-the-art instruments plus one experiment that uses the spacecraft telecommunication system with ground-based instruments.

Jupiter; → icy; → explorer; → moon.

Jupiter mass
  جرم ِ هرمز   
jerm-e Hormoz

Fr.: masse de Jupiter   

A quantity of mass equal to 1.898 × 1027 kg, about 0.000954 → solar masses, or 317.83 → Earth masses. Jupiter mass, MJ, is used as a → unit to describe masses of the → gas giant, such as the outer planets and → extrasolar planets. Similarly, → brown dwarf masses are expressed in terms of Jupiter mass.

Jupiter; → mass.

Jupiter's atmosphere
  جو ِ هرمز، هواسپهر ِ ~   
javv-e Hormoz, havâsepehr-e ~

Fr.: atmosphère de Jupiter   

The gaseous envelope surrounding Jupiter. It is about 90% → hydrogen and 10% → helium (by numbers of atoms, 75/25% by mass) with traces of → methane, → water, and → ammonia. This is very close to the composition of the primordial → solar nebula from which the entire solar system was formed. Saturn has a similar composition, but Uranus and Neptune have much less hydrogen and helium. The outermost layer is composed primarily of ordinary → molecular hydrogen and helium. Visually, Jupiter is dominated by two atmospheric features; a series of ever-changing atmospheric cloud bands arranged parallel to the equator and an oval atmospheric blob called the → Great Red Spot.

Jupiter; → atmosphere.

Jupiter's ring
  حلقه‌های ِ هرمز   
halqehâ-ye Hormoz

Fr.: anneaux de Jupiter   

Any of several faint, dark, narrow rings around Jupiter. Jupiter's rings are so faint and tenuous that are only visible when viewed from behind Jupiter and are lit by the Sun, or directly viewed in the infrared where they faintly glow. Unlike → Saturn's rings full of large icy and rock chunks, they are composed of tiny rock fragments and dust. Jupiter's rings are continuously losing material and being resupplied with new dust from → meteorite impacts with Jupiter's four inner moons (→ Metis, → Adrastea, → Amalthea, and → Thebe). Jupiter's rings were discovered by NASA's Voyager 1 in 1979. They are composed of three parts: the → Main ring, a → Halo ring that orbits closer to Jupiter, and a very wide → Gossamer ring that extends far from Jupiter.

Jupiter; → ring.

Jurassic
  ژوراسیک   
Žurâsik (#)

Fr.: jurassique   

Jurassic era.

Named for the Jura Mountains on the border between France and Switzerland, where rocks of this age were first studied, + -assic, suffix extracted from Triassic.

Jurassic era
  دوره‌ی ِ ژوراسیک   
dowre-ye Žurasik (#)

Fr.: ère jurassique   

A period of the Mesozoic era, spanning the time between the Triassic and the → Cretaceous periods, about 200 to 145 million years ago. The start of the period is marked by the major Triassic-Jurassic → mass extinction event.

Jurassic; → era.

juridical
  دادشناختی   
dâdšenâxti

Fr.: juridique   

1) Of or relating to the administration of justice.
2) Of or relating to law or jurisprudence; legal (Dictionary.com).

From L. iuridicalis "relating to right; pertaining to justice," from iuridicus, from ius "right, law," → jurist, + dicere "to say, to speak."

Dâdšenâxti, of or relating to dâdšenâxt, → jurisprudence

<< < -es -iv -ti 21 a p abe abs abs aca acc acc acr act ada adh Adr aer AGB air Alf Alg all alp alt AM amo ana And ang ani ano Ant Ant apa apo app app Ara Arc ari Arr ash ass ast ast asy atm ato att aut ave axi Bab bal Bal bar bar bea Bek Bes bia Big bin bin bip biv bla bli blu Boh Bol Bos bou bra bri bro buo cal cal can cap car Car cat cat CCD Cen cen CH cha cha che Che chr cir cir cit cla clo clo clu 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 Cop Cor cor cor cos cos cou cou Cow cre cri cro cry cur cya Cyg dan dar dat de- deb dec dec ded def deg del dem den dep des det dev dia dif dif dih dio Dir dis dis dis dis dis dis DO don dou dow dro dur dwa dyn Dys ear ebb ecl edg egg Ein Ela ele ele ele ele ell eme emp enc eng ent epi equ equ equ esc eth Eur Eve exa exc exe exi exp exp ext ext ext fac fal far fed Fer fer fie fin fir fis fla flo flu fol for for fou fra fre Fre fro fut G-t gal gal gam gas Gau Gem gen geo geo geo gia Gli Gol gra gra gra gra gre gri gui H I Hag hal har hat He- hea hel Hel her Hes hie hig his hom hor hot Hub Hug hur hyd hyd hyg 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 Io ion iro isl iso iso Jac jet jud jur Kel Kep kil Klo Kui Lag lam Lap Lar lat law lea len lep Lib lig lim lin lin Lio lit loc LOF lon Lor low lum lun Lup Lyo mac mag mag mag mag mag mai man Mar mas mas mat Max mea mec Meg Mer Mer met met Met mic Mid Mil min Mir mit mod mod mol mon Mor mou mul mul mys nan Nat nau nec neo neu nev New NGC no nom non non nor not nuc nuc num nut obj obs obs occ ocu oft ome Oor ope opp opt opt orb ord ori ort osc out ove oxi pai pan par par par par pas pea pen per per per per Per per pha phi pho pho pho phy pio Pla pla pla pla Pla plu Poi pol pol pol poo pos pos pot pra pre pre pre pre pri pri pro pro pro pro pro Pro pro pse pul pur qua qua qua qua que rac rad rad rad rad rad rad 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 Rus Sac sal sat sca sca Sch sci Scu sec sec Sed sel Sel sen ser Sex Sha she sho sid sig sil sim sin siz sla Sma sno sof sol sol sol sol sou sou spa spa spe spe spe sph spi spi spr squ sta sta sta sta ste ste ste Sto Str str str sub sub suc sun sup sup sup sup sur swa syn syn tab tar tek tem ter tes the the the the Tho thr tid tim Tis Too Tor tra tra Tra tra tra tri tri tru Tul tur two Typ ult un- und uni uni unk upp Urc utt val var vec vel ver vib vio vir vis voi vor wan wat wav wax wea Wei whi Wil win WN9 wor X-r yel you zer zod > >>