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: 1223
-cide
   -کشی   
-koši (#)

Fr.: -cide   

A suffix meaning "killer; act of killing." → genocide.

M.E., from L. -cida "cutter, killer," -cidium "act of killing," from combining form -cidere, from caedere "to strike down, kill."

-koši, from koštan "to kill," Mid.Pers. kuštan "to kill, to stuggle;" related to košti "fighting, wrestling;" Av. kuš- "to fight, to struggle" (Cheung 2007).

-cline
     
-šib

Fr.: -cline   

A suffix indicating a slope, as in → barocline, → thermocline, → tachocline.

Back formation from incline, → inclination.

Šib, → slope.

-cracy
   -سالاری   
-sâlâri

Fr.: -cracie   

A combining form occurring in loanwords from Greek with the meaning "rule, government, governing body." → theocracy.

From Fr. -cratie, from M.L. -cratia, from Gk. -kratia "power, might; rule; authority," from kratos "strength," from PIE *kre-tes- "power, strength," suffixed form of root *kar-/*ker- "→ hard." "hard."

From sâlâr "leader, chieftain, commander;" Mid.Pers. sâlâr "leader, master;" variant of sardâr "commander, chief, general," from sar "chief, → head," + dâr "having, possessor," from dâštan "to have, to possess," Mid.Pers. dâštan; O.Pers./Av. root dar- "to hold, keep back, maintain, keep in mind;" Skt. dhr-, dharma- "law;" Gk. thronos "elevated seat, throne;" L. firmus "firm, stable;" Lith. daryti "to make;" PIE *dher- "to hold, support."

C ring
  حلقه‌ی ِ C   
halqe-ye C

Fr.: anneau C   

One of → Saturn's rings, lying beyond the → D ring and before the → B ring, at 74,658 km from the center of Saturn, with a width of 17,500 km. Same as the → Crepe ring.

ring.

C-symmetry
  همامونی ِ بار   
hamâmuni-ye bâr

Fr.: symétrie de charge   

Same as → charge conjugation and → charge symmetry.

charge; → symmetry.

C-type asteroid
  سیارک ِ گونه‌ی ِ C   
sayârak-e gune-ye C

Fr.: astéroïde de type C   

An → asteroid that belongs to the family of → carbonaceous asteroids. They are → depleted in → hydrogen and → helium, have chemical ratios akin to solar composition, and show low → albedo (0.03-0.09). C-type asteroids are the most common variety, forming around 75% of known asteroids. They inhabit → main belt's outer regions.

C stands for → carbonaceous; → type; → asteroid.

Caelum
  قلم   
qalam (#)

Fr.: Burin   

The Sculptor's Chisel. A small inconspicuous → constellation in the southern sky, representing a sculptor's chisel. Its brightest star, Alpha Caeli, is magnitude 4.5. Approximate position: R.A. 4.5 h, Dec.: -40°; abbreviation: Cae, genitive form Caeli.

L. caelum sculptor's "chisel."

Qalam "chisel," from Ar., related to L. caelum?

cage
  قفس   
qafas (#)

Fr.: cage   

1) An enclosure, usually made with bars or wire, for keeping birds or wild animals.
2) An enclosed structure resembling a cage. → observer's cage, → Faraday cage.

M.E. from O.Fr. cage, from L. cavea "hollow place, enclosure for animals," cognate with Pers. kâv "hollow," → concave.

Qafas "cage," of unknown origin.

CAI meteorite
  شخانه‌ی ِ CAI، شهاب‌سنگ ِ ~   
šaxâne-ye CAI, šahânsang-e ~

Fr.: météorite de type CAI   

A member of a group of tiny (millimeter to centimeter) light-colored meteorites found often with → chondrules. They consist of high vaporization minerals, including → silicates and → oxides of Ca, Al, and Ti, but are quite poor in Fe. Compared to common → chondrules, which are uniformly spherical, their shapes are less regular. They appear to be 2-3 million years older than chondrules. CAI meteorites are probably the oldest solid materials to have formed in the → solar nebula.

CAI, short for → Calcium, → Aluminium, and → Inclusion; → meteorite.

CAK model
  مدل ِ CAK   
model-e CAK

Fr.: modèle CAK   

The standard model of → radiation-driven winds in which the acceleration of → stellar wind is provided by the → absorption and → scattering of ultraviolet photons in ions of abundant elements (→ CNO, → iron peak) in the → Lyman continuum. The model was developed by Castor et al. (1975), who assumed that the forces due to the radiative lines and the pressure gradients are functions of local velocity gradient, and used a large number (~ 105) of lines which have a statistical distribution in line strengths. The model led to predictions of → mass loss rates (M_dot) and terminal velocities as a function of stellar properties and the line statistics parameters. With the modifications by Friend and Abbott (1986), Pauldrach et al. (1986), and Kudritzki et al. (1989), CAK multi-line theory gives good agreement with observationally derived values of mass loss rate and → terminal velocity (v). CAK wind solutions predict the terminal velocity to be proportional to the → escape velocity and the mass loss rate to depend strongly on the stellar → luminosity. Observations over the past decades have shown that these main wind parameters, M_dot and v, indeed behave as predicted by CAK. This basic agreement between observations and theory provides strong evidence that the winds from → massive stars are driven by → radiation pressure and this has favored the CAK formalism. See also → multiple scattering. See the review by J. Puls et al. 2008, Astron. Astrophys. Rev. 16, 209.

CAK, the initials of the researchers who developed the model: J.I. Castor, D.C. Abbott, and R.I. Klein(1975, Radiation-driven winds in Of stars, ApJ 195, 157); → model.

Calabash Nebula
  میغ ِ کالاباش   
Miq-e Kââbâš

Fr.: nébuleuse de l'œuf pourri   

A → bipolar nebula and → OH/IR source with technical designation OH 231.8+4.2. It is a → proto-planetary nebula (PPN) 1.4 → light-years long and located some 5,000 light-years from Earth in the constellation → Puppis. The obscured → central star, named QX Pup, is classified as M9-10 III and has a → Mira-like variability consistent with an evolved → asymptotic giant branch (AGB) star. The late evolution of this object may have been complex since it has a binary → companion star (of type A0 V) that has been indirectly identified from analysis of the spectrum of the hidden central source reflected by the nebular dust. The system has a total luminosity of ~ 104 Lsun and its systemic velocity relative to the → Local Standard of Rest is VLSR ~ 34 km s-1. OH 231.8+4.2 is very likely a member of the → open cluster M46 with a progenitor mass of ~ 3 Msun. The nebula is also known as the Rotten Egg Nebula because it contains a lot of sulphur, an element that, when combined with other elements, smells like a rotten egg (see, e.g., Prieto et al., 2015, A&A, 575, A84).

The name "Calabash Nebula" was first proposed by Icke & Preston, 1989, A&A, 211, 409. It refers to the apparent form of the object which resembles a calabash "a tree that has large, rounded gourdlike fruit; the fruit of any of these plants," from Sp. calabaza, possibly from Ar. qar'ah yâbisah "dry gourd," from Pers. kharabuz, used of various large melons; → nebula.

calcium
  کلسیوم   
kalsiom (#)

Fr.: calcium   

A metallic chemical element; symbol Ca. → Atomic number 20; → atomic weight 40.08; → melting point about 839°C; → boiling point 1,484°C; → specific gravity 1.55 at 20°C; → valence +2. It is fifth in abundance in the Earth's crust, of which it forms more than 3%. It is an essential constituent of leaves, bones, teeth, and shells. Never found in nature uncombined, it occurs abundantly as limestone, gypsum, and fluorite. Calcium has several radioactive isotopes. It was first isolated by the British chemist Humphry Davy in 1808.

Coined by Sir Humphry Davy from L. calx (genitive calcis) "lime (CaO) or limestone (CaCO3)" in which it was found, from Gk. khalix "small pebble," see also → calculate, + → -ium.

calcium break
  گسست ِ کلسیوم   
gosast-e kalsiom

Fr.: coupure de calcium   

A discontinuity in the spectrum of galaxies near the Ca II → H and K lines at about 4000 Å. The Ca break is the most prominent feature in the spectra of elliptical galaxies. Its strength is given by the → calcium break index.

calcium; → break.

calcium break index
  دیشن ِ گسست ِ کلسیوم   
dišan-e gosast-e kalsiom

Fr.: indice de la coupure de calcium   

The strength of the → calcium break, as measured from the fluxes in the intervals 3750-3950 Å and 4050-4250 Å. It is given by the expression Ca-break[%] = 100 · (fupper - flower)/fupper, where fupper and flower are the mean fluxes measured in the 3750-3950 Å and 4050-4250 Å bands, respectively, in the rest frame (Dressler & Shectman 1987, AJ 94, 899).

calcium; → break; → index.

calculate
  افماردن   
afmârdan

Fr.: calculer   

To perform a mathematical process; to reckon; to make an estimate of; evaluate. → compute; → count; → mathematics; → statistics.

Calculate, from L.L. calculare, calculat-, from L. calculus "small stone, pebble" (used in reckoning), dim. of calx, calc- "limestone," from Gk. khalix "small pebble," kakhlex "round pebble,"cf. O.E. hægl, hagol "hale," from W.Gmc. *haglaz, O.H.G. hagal, O.N. hagl, Ger. Hagel "hail", PIE *kaghlo- "pebble, hail." The Pers. cognate is probably the Lori hogela "big stone."

Afmârdan, from prefix af- + stem mar- + infinitive suffix -idan. The Mod.Pers. prefix af- "to, up, upon," occurring in several words (e.g. afzudan, afruxtan, afsar, afsâr, afqân), derives from O.Pers./Av. abiy-/aiwi- "to, upon, against;" cf. Skt. abhi-, Gk. amphi-. The stem mar-, mâr- "count, reckon, measure," which occurs in several Mid./Mod.Pers. terms (e.g. ošmârdan, šomârdan, šomordan "to count, to calculate," âmâr "computation, arithmetic; statistics," âmârdan "to reckon, to calculate," bimar "countless," nahmâr "great, large, big"), is related to the Av. base mar- "to have in mind, remember, recall," hišmar-; cf. Skt. smr-, smarati "to remember, he remembers," L. memor, memoria, Gk. mermera "care," martyr "witness."

calculation
  افمارش   
afmâreš

Fr.: calcul   

The act, process, or result of calculating.

Calculation, noun from → calculate.

Afmâreš, verbal noun from afmârdancalculate.

calculator
  افمارگر   
afmârgar

Fr.: calculateur   

A small electronic device that performs calculations.

Calculator, from → calculate + → -tor.

Afmârgar, from afmârcalculate + -gar agent suffix, from kar-, kardan "to do, to make" (Mid.Pers. kardan, O.Pers./Av. kar- "to do, make, build," Av. kərənaoiti "makes," cf. Skt. kr- "to do, to make," krnoti "makes," karma "act, deed;" PIE base kwer- "to do, to make").

calculus
  افماریک   
afmârik

Fr.: calcul différentiel et intégral   

The branch of mathematics that deals with limits and the differentiation and integration of functions of one or more variables; differential calculus, infinitesimal calculus.

L. calculus "small stone," from calx, calcis "limestone," → calculate, + -ulus diminutive suffix, → -ule.

Afmârik, from afmârcalculate + Pers. suffix -ik denoting a subject, a branch of sciences, a discipline, → ics.

calculus of finite differences
  افماریک ِ دگرسانی‌ها‌ی ِ کرانمند   
afmârik-e degarsânihâ-ye karânmand

Fr.: calcul des différences finies   

A calculus based on the properties of the successive values of variable quantities and their differences or increments.

calculus, → finite, → difference.

Afmârik, → calculus, degarsânihâ, plural of degarsân, → difference, karânmandfinite.

calculus of probabilities
  افماریک ِ شوانایی‌ها   
afmârik-e šavânâihâ

Fr.: calcul des probabilités   

A branch of mathematics that deals with the calculation of the probabilities of events.

calculus; → probability.

Afmârik, → calculus; šavânâihâ, plural of šavânâiprobability.

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