Перевод и анализ слов искусственным интеллектом ChatGPT
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interlineation$40013$ - перевод на немецкий
![ESA]] photo.](https://commons.wikimedia.org/wiki/Special:FilePath/Andromeda active core.jpg?width=200 "ESA]] photo.")
![The Andromeda Galaxy pictured in [[ultraviolet]] by [[GALEX]] (2003).](https://commons.wikimedia.org/wiki/Special:FilePath/Andromeda galaxy.jpg?width=200 "The Andromeda Galaxy pictured in [[ultraviolet]] by [[GALEX]] (2003).")
![Image of the Andromeda Galaxy taken by Spitzer in infrared, 24 [[micrometre]]s (Credit:[[NASA]]/[[JPL]]–[[Caltech]]/Karl D. Gordon, [[University of Arizona]]).](https://commons.wikimedia.org/wiki/Special:FilePath/Andromeda galaxy Ssc2005-20a1.jpg?width=200 "Image of the Andromeda Galaxy taken by Spitzer in infrared, 24 [[micrometre]]s (Credit:[[NASA]]/[[JPL]]–[[Caltech]]/Karl D. Gordon, [[University of Arizona]]).")
![Great Space Observatories]].](https://commons.wikimedia.org/wiki/Special:FilePath/Infraredandromeda.jpg?width=200 "Great Space Observatories]].")
![Chandra X-ray telescope]] image of the center of the Andromeda Galaxy. Several X-ray sources, likely X-ray binary stars, within the galaxy's central region appear as yellowish dots. The blue source at the center is at the position of the [[supermassive black hole]].](https://commons.wikimedia.org/wiki/Special:FilePath/M31 Core in X-rays.jpg?width=200 "Chandra X-ray telescope]] image of the center of the Andromeda Galaxy. Several X-ray sources, likely X-ray binary stars, within the galaxy's central region appear as yellowish dots. The blue source at the center is at the position of the [[supermassive black hole]].")
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![M110]] to upper left), by [[Isaac Roberts]], 1899.](https://commons.wikimedia.org/wiki/Special:FilePath/Pic iroberts1.jpg?width=200 "M110]] to upper left), by [[Isaac Roberts]], 1899.")
![Galaxy Evolution Explorer]] image of the Andromeda Galaxy. The bands of blue-white making up the galaxy's striking rings are neighborhoods that harbor hot, young, massive stars. Dark blue-grey lanes of cooler dust show up starkly against these bright rings, tracing the regions where star formation is currently taking place in dense cloudy cocoons. When observed in visible light, the Andromeda Galaxy's rings look more like spiral arms. The ultraviolet view shows that these arms more closely resemble the ring-like structure previously observed in infrared wavelengths with NASA's [[Spitzer Space Telescope]]. Astronomers using the latter interpreted these rings as evidence that the galaxy was involved in a direct collision with its neighbor, M32, more than 200 million years ago.](https://commons.wikimedia.org/wiki/Special:FilePath/The Galaxy Next Door.jpg?width=200 "Galaxy Evolution Explorer]] image of the Andromeda Galaxy. The bands of blue-white making up the galaxy's striking rings are neighborhoods that harbor hot, young, massive stars. Dark blue-grey lanes of cooler dust show up starkly against these bright rings, tracing the regions where star formation is currently taking place in dense cloudy cocoons. When observed in visible light, the Andromeda Galaxy's rings look more like spiral arms. The ultraviolet view shows that these arms more closely resemble the ring-like structure previously observed in infrared wavelengths with NASA's [[Spitzer Space Telescope]]. Astronomers using the latter interpreted these rings as evidence that the galaxy was involved in a direct collision with its neighbor, M32, more than 200 million years ago.")
![The Andromeda Galaxy as seen by [[NASA]]'s [[Wide-field Infrared Survey Explorer]].](https://commons.wikimedia.org/wiki/Special:FilePath/WISE- Andromeda.jpg?width=200 "The Andromeda Galaxy as seen by [[NASA]]'s [[Wide-field Infrared Survey Explorer]].")
![Andromeda Galaxy near upper-left of the [[Very Large Telescope]].<ref name="nake"/> The [[Triangulum Galaxy]] is visible on the top.](https://commons.wikimedia.org/wiki/Special:FilePath/Над VLT – две галактики, видимые простым глазом.jpg?width=200 "Andromeda Galaxy near upper-left of the [[Very Large Telescope]].<ref name=\"nake\"/> The [[Triangulum Galaxy]] is visible on the top.")
Определение
Википедия
The Andromeda Galaxy (IPA: ), also known as Messier 31, M31, or NGC 224 and originally the Andromeda Nebula, is a barred spiral galaxy with the diameter of about 46.56 kiloparsecs (152,000 light-years) approximately 765 kpc (2.5 million light-years) from Earth and the nearest large galaxy to the Milky Way. The galaxy's name stems from the area of Earth's sky in which it appears, the constellation of Andromeda, which itself is named after the princess who was the wife of Perseus in Greek mythology.
The virial mass of the Andromeda Galaxy is of the same order of magnitude as that of the Milky Way, at 1 trillion solar masses (2.0×1042 kilograms). The mass of either galaxy is difficult to estimate with any accuracy, but it was long thought that the Andromeda Galaxy is more massive than the Milky Way by a margin of some 25% to 50%. This has been called into question by early 21st-century studies indicating a possibly lower mass for the Andromeda Galaxy and a higher mass for the Milky Way. The Andromeda Galaxy has a diameter of about 46.56 kpc (152,000 ly), making it the largest member of the Local Group in terms of extension.
The Milky Way and Andromeda galaxies are expected to collide in around 4–5 billion years, merging to potentially form a giant elliptical galaxy or a large lenticular galaxy. With an apparent magnitude of 3.4, the Andromeda Galaxy is among the brightest of the Messier objects, and is visible to the naked eye from Earth on moonless nights, even when viewed from areas with moderate light pollution.
