GALAXIES - traducción al árabe
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GALAXIES - traducción al árabe

LARGE GRAVITATIONALLY BOUND SYSTEM OF STARS AND INTERSTELLAR MATTER
Galaxies; Island universe; Galaxial center; Galaxy nucleus; List of hypothetical galaxies; Galixies; Gallaxy; Galactic magnetic fields; Galactic magnetic field; Wikipedia:WikiProject Outlines/Drafts/Outline of galaxies; Draft:Outline of galaxies; Shell galaxy; Isophotal diameter; Early galaxies; Early galaxy; Earliest galaxies; Earliest galaxy; Galactocentric orbit
  • [[Hercules A]] supergiant elliptical radio galaxy
  • The [[Antennae Galaxies]] are undergoing a collision that will result in their eventual merger.
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  • The shape of the Milky Way as estimated from star counts by [[William Herschel]] in 1785; the Solar System was assumed to be near the center.
  • [[Hoag's Object]], an example of a [[ring galaxy]]
  • NGC 3447]]}}
  • [[NGC 1300]], an example of a [[barred spiral galaxy]]
  • spiral]]; and ''SB'' is a [[barred spiral galaxy]].<ref group=note>Galaxies to the left side of the Hubble classification scheme are sometimes referred to as "early-type", while those to the right are "late-type".</ref>
  • The [[Pinwheel Galaxy]], NGC 5457
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  • M87]].
  • [[NGC 3923]] Elliptical Shell Galaxy (Hubble photograph)
  • Photograph of the "Great Andromeda Nebula" by [[Isaac Roberts]], 1899, later identified as the [[Andromeda Galaxy]]
  • [[Galaxy cluster]] [[SDSS J1152+3313]]. SDSS stands for [[Sloan Digital Sky Survey]], J for [[Julian epoch]], and 1152+3313 for [[right ascension]] and [[declination]] respectively.
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  • Artist's impression of a young galaxy accreting material

GALAXIES         

ألاسم

دَرْبُ التَّبَّانَة ; مَجَرَّة

galaxy         
N
cap: المجرة الكوكبة
GALAXY         

ألاسم

دَرْبُ التَّبَّانَة ; مَجَرَّة

Definición

Galaxies
·pl of Galaxy.

Wikipedia

Galaxy

A galaxy is a system of stars, stellar remnants, interstellar gas, dust, dark matter, bound together by gravity. The word is derived from the Greek galaxias (γαλαξίας), literally 'milky', a reference to the Milky Way galaxy that contains the Solar System. Galaxies, averaging an estimated 100 million stars, range in size from dwarfs with less than a hundred million stars, to the largest galaxies known – supergiants with one hundred trillion stars, each orbiting its galaxy's center of mass. Most of the mass in a typical galaxy is in the form of dark matter, with only a few percent of that mass visible in the form of stars and nebulae. Supermassive black holes are a common feature at the centres of galaxies.

Galaxies are categorized according to their visual morphology as elliptical, spiral, or irregular. Many are thought to have supermassive black holes at their centers. The Milky Way's central black hole, known as Sagittarius A*, has a mass four million times greater than the Sun. As of March 2016, GN-z11 is the oldest and most distant galaxy observed. It has a comoving distance of 32 billion light-years from Earth, and is seen as it existed just 400 million years after the Big Bang.

In 2016, using 20 years of images from the Hubble space telescope, it was estimated that there were in total two trillion (2×1012) or more galaxies in the observable universe, and as many as an estimated 1×1024 stars (more stars than all the grains of sand on all beaches of the planet Earth).

In 2021, data from NASA's New Horizons space probe was used to revise the earlier estimate to roughly 200 billion galaxies (2×1011),

Most galaxies are 1,000 to 100,000 parsecs in diameter (approximately 3,000 to 300,000 light years) and are separated by distances on the order of millions of parsecs (or megaparsecs). For comparison, the Milky Way has a diameter of at least 26,800 parsecs (87,400 ly) and is separated from the Andromeda Galaxy (with diameter of about 152,000 ly), its nearest large neighbor, by 780,000 parsecs (2.5 million ly.)

The space between galaxies is filled with a tenuous gas (the intergalactic medium) with an average density of less than one atom per cubic meter. Most galaxies are gravitationally organized into groups, clusters and superclusters. The Milky Way is part of the Local Group, which it dominates along with Andromeda Galaxy. The group is part of the Virgo Supercluster. At the largest scale, these associations are generally arranged into sheets and filaments surrounded by immense voids. Both the Local Group and the Virgo Supercluster are contained in a much larger cosmic structure named Laniakea.

Ejemplos de pronunciación para GALAXIES
1. galaxies.
Dr. Becky Smethurst _ Supermassive Black Holes - The Ultimate Galaxy Killers _ Talks at Google
2. and further, galaxies, and further, more galaxies.
ted-talks_1963_AllanAdams_2014-320k
3. little galaxies merge with big galaxies
Building a Galaxy-Scale Gravitational Wave Detector _ Dr. Shami Chatterjee _ Talks at Google
4. of galaxies, and even galaxies together.
Dark Energy and the Runaway Universe _ Alex Filippenko _ Talks at Google
5. Lower-mass galaxies and higher-mass galaxies
New Galaxy Formation Insights _ Joel Primack _ Talks at Google
Ejemplos de uso de GALAXIES
1. The discovery was surprising, since astronomers have long theorised that galaxies form when stars gradually cluster together, with small galaxies preceding bigger galaxies.
2. The telescope will also look for the farthest galaxies and provide clues on how galaxies form.
3. "All galaxies are composed of stars and we understand stars very well so we can use them to understand galaxies.
4. This model could also explain the warps in other galaxies.
5. Musgrave said astronauts should also look upward to see galaxies.