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

فرهنگ ریشه شناختی اخترشناسی-اخترفیزیک

M. Heydari-Malayeri    -    Paris Observatory

   Homepage   
   


A B C D E F G H I J K L M N O P Q R S T U V W X Y Z

<< < -ph pal par par par par Pas pat Pel per per per per Per per pha phi pho pho pho phy pip Pla pla pla pla ple poa pol pol pol pol pop pos pos pow pra pre pre pre pri pri pri pro pro pro pro pro pro pse pul pup > >>

Number of Results: 1037
polar alignment
  آخطش ِ قطبی   
âxateš-e qotbi

Fr.: alignement polaire   

The process or the state of making a → telescope's → polar axis → parallel to the → Earth's → rotation axis, that is with the → true North or → South  → celestial pole. When this is accomplished, the sky's motion can be cancelled out simply by turning the axis (either by hand or with a motor → drive) at the same rate as the rotation of the Earth, but in the opposite direction.

polar; → alignment.

polar axis
  آسه‌ی ِ قطبی   
âse-ye qotbi (#)

Fr.: axe polaire   

The axis of an → equatorial mounting that is parallel to the Earth's axis, and consequently points to the celestial pole.

polar; → axis.

polar bond
  بند ِ قطبی   
band-e qotbi

Fr.: lien polaire   

A chemical bond where the electrons are shared unequally between atoms. The atom that is more electronegative will pull the electrons closer to itself.

polar; → bond.

polar cap
  کلاهک ِ قطبی   
kolâhak-e qotbi

Fr.: calotte polaire   

1) Either of the regions around the poles of the Earth that are permanently covered with ice.
2) Either of the two regions around the poles of the planet Mars, consisting of frozen carbon dioxide and water ice.
3) An area of a → pulsar's surface from where open magnetic field lines emanate.

polar; → cap.

polar circle
  پرهون ِ قطبی، دایره‌ی ِ ~   
parhun-e qotbi, dâyere-ye ~ (#)

Fr.: cercle polaire   

An imaginary parallel circle on the celestial sphere or on the Earth at a distance of 23°.5 from either poles.

polar; → circle.

polar coordinates
  هم‌آراهای ِ قطبی   
hamârâhâ-ye qotbi (#)

Fr.: coordonnées polaires   

A coordinate system in which the position of any point (M) in a plane is specified by two coordinates: 1) ρ, which expresses the distance from a fixed point (the pole, denoted O), and 2) the number φ, which is the angle formed by the line segment OM and a fixed reference line passing through the pole.

polar; → coordinate.

polar cusp
  تیزه‌ی ِ قطبی   
tize-ye qotbi

Fr.: cuspide polaire   

An area in the Earth's → magnetosphere, where the → magnetosheath plasma has direct access to the → ionosphere.

polar; → cusp.

polar day
  روز ِ قطبی   
ruz-e qotbi (#)

Fr.: jour polaire   

In polar regions, the portion of the year when the Sun is continuously in the sky. Its length changes from twenty hours at the Arctic/Antarctic Circle (latitude 66°33' N or S) to 186 days at the North/South Pole.

polar; → day.

polar distance
  دورای ِ قطبی   
durâ-ye qotbi

Fr.: distance polaire   

The angular distance of an object from a celestial pole. It is equal to 90° minus the object's declination.

polar; → distance.

polar equation
  هموگش ِ قطبی   
hamugeš-e qotbi

Fr.: équation polaire   

An equation for a curve written in terms of the → polar coordinates.

polar; → equation.

polar faculae
  پریسک‌های ِ قطبی   
periskhâ-ye qotbi

Fr.: facules polaires   

Solar faculae occurring in regions of high heliographic latitudes. They are smaller than the main-zone faculae; their shape is point-like or oval. Their lifetimes range from a few minutes to some hours, but the decisive difference from the main-zone faculae lies in their activity cycle. When spots and faculae of the main zone are at minimum, the polar faculae have their maximum activity, and vice versa.

polar; → facula.

polar molecule
  مولکول ِ قطبی   
molekul-e qotbi

Fr.: molécule polaire   

A molecule in which the centers of positive and negative charge distribution do not converge and therefore has a mostly positive charge on one side and a mostly negative charge on the other. Different atoms around a central atom will always be polar molecules. Some polar molecules are H2O, HF, COS, and CH3Cl. Polar molecules are characterized by a → dipole moment.

polar; → molecule.

polar motion
  جنبش ِ قطبی   
jonbeš-e qotbi

Fr.: mouvement du pôle   

The irregularly varying motion of the Earth's pole of rotation with respect to the Earth's crust.

polar; → motion.

polar night
  شب ِ قطبی   
šab-e qotbi

Fr.: nuit polaire   

In polar regions, the portion of the year when the Sun does not rise above the horizon. Its length changes from twenty hours at the Arctic/Antarctic Circle (latitude 66°33' N or S) to 179 days at the North/South Pole.

polar; → day.

polar orbit
  مدار ِ قطبی   
madâr-e qotbi (#)

Fr.: orbite polaire   

A spacecraft orbit that passes over, or close to, the geographic poles of the Earth or some other solar system object.

polar; → orbit.

polar orbiting satellite
  ماهواره با مدار ِ قطبی   
mâhvâré bâ madâr-e qotbi

Fr.: satellite en orbite polaire   

A satellite that revolves around the Earth in an almost north-south orbit, passing close to both poles. The orbits are sun synchronous, allowing the satellite to cross the equator at the same local time each day. These satellites orbit at a height of 830-880 km and take about 100 minutes to complete a turn around the Earth.

polar; → orbit; → satellite.

polar plume
  پرک ِ قطبی   
parrak-e qotbi

Fr.: plume polaire   

A coronal feature of the Sun, which appears as long, thin streamers that project outward from the Sun's north and south poles

polar; → plume.

polar wind
  باد ِ قطبی   
bâd-e qotbi

Fr.: vent polaire   

1) The → solar wind occurring at high latitudes during low → solar activity as a fast (around 750 km s-1) and relatively steady flow. A remarkable feature of the polar wind is the ubiquitous presence of an intense flow of → Alfvénic fluctuations.
2) One of the two main wind components in → B[e] stars. The pole is hotter than the equator due to the → gravity darkening effect leading to a relatively fast, low-density wind driven by Fe IV lines. The other component is the → equatorial wind. The mechanism put forward to explain this wind morphology is the rotationally induced → bistability mechanism.
3) An extremely cold wind blowing from the north or south polar regions of the Earth.

polar; → wind.

polarimetry
  قطبش‌سنجی   
qotbešsanji

Fr.: polarimétrie   

The measurement of the → polarization state of light, usually through the use of a polarimeter.

From polari, from → polarization + → -metry.

Polaris
  ستاره‌ی ِ قطبی، جدی، میخ ِ گاه   
setâre-ye qotbi, jodey, mix-e gâh

Fr.: étoile polaire   

The brightest star associated with the → north celestial pole. Polaris, also called the Pole Star, is a → triple system lying at about 433 → light-years (133 → parsecs) from the Earth. It is not exactly located on the Earth → rotation axis, because an → angular distance of 42 degrees (about 1.4 lunar diameter) separates it from the true north pole. The main star, Polaris Aa (→ visual magnitude about 2), is a variable → pulsating star of type → Cepheid. It is a hot, blue F7 Ib → supergiant star having a → luminosity about 1,260 times that of the Sun. It has a mass of 5.4 Msun, a radius of 37.5 Rsun, and a → surface temperature of 6,015 K. The close companion Ab apparent magnitude 9.2) is only 0''.17 (about 18.5 → astronomical units) from Polaris A. It was discovered in 1929 through examining the spectrum of Polaris A. It orbits Aa every 29.59 years. Ab is a → main sequence star of → spectral type F6 V. It has a mass of 1.26 Msun, a radius of 1.04 Rsun, and a luminosity of 3 Lsun. The third component, Polaris B (visual magnitude 8.7), is separated from A by 18.2 arc sec, corresponding to approximately 2,400 AU. It was first noticed by William Herschel in 1780. Polaris B is a main sequence star of type F3 V with a mass 1.39 Msun, a radius 1.8 Rsun, a luminosity of 3.9 Lsun, and a surface temperature of 6,900 K. Due to the → precession of equinoxes, the direction that Earth's axis points at changes slowly with time. Hence, Polaris has not always been, nor will it always be, the Pole Star. Polaris is actually drawing closer to the pole and in 2100 it will be as close to it as it ever will come, just 27.15 arc-minutes or slightly less than the Moon's apparent diameter. It will continue its reign as the North Star for many centuries to come. Historically, around 400 B.C., during Plato's time the nearest star to the Pole star was → Kochab (β Ursae Minoris). Some 4,600 years ago, when the Egyptians constructed the Pyramids, the Pole star was → Thuban (α Draconis). In 2,000 years the star → Errai (γ Cephei) will become the Pole Star. And around the year 14,000, Earth's axis will point reasonably close to the star → Vega, the fifth brightest star in the sky.

Mod.L. short for stella polaris "the pole star," → polar.

Setâre-ye qotbi "polar star," from setâré, → star, + qotbi, → polar.
Jodey, from Ar. Judaiy.
Mix-e gâh, Mid.Pers. name of the star, literally "the nail (peg) of time/place," from mix, → nail, + gâh "time; place," → origin.

<< < -ph pal par par par par Pas pat Pel per per per per Per per pha phi pho pho pho phy pip Pla pla pla pla ple poa pol pol pol pol pop pos pos pow pra pre pre pre pri pri pri pro pro pro pro pro pro pse pul pup > >>