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Keyword: NGC 6888
![Лебедь: Пузырь и Полумесяц](https://images.astronet.ru/pubd/2020/10/18/0001702543/NGC6888WissamAyoub1024.preview.jpg)
17.10.2020
These clouds of gas and dust drift through rich star fields along the plane of our Milky Way Galaxy toward the high flying constellation Cygnus. Caught within the telescopic field of view are the Soap Bubble (lower left) and the Crescent Nebula (upper right).
![Лебедь: Пузырь и Полумесяц](https://images.astronet.ru/pubd/2023/09/04/0001907445/CrescentBubble_AlHarbi_1080.preview.jpg)
4.09.2023
As stars die, they create clouds. Two stellar death clouds of gas and dust can be found toward the high-flying constellation of the Swan (Cygnus) as they drift through rich star fields in the plane of our Milky Way Galaxy.
![NGC 6888: туманность Полумесяц](https://images.astronet.ru/pubd/2021/06/17/0001744387/CrescentHOOcombinedFinalimage1024.preview.jpg)
17.06.2021
NGC 6888, also known as the Crescent Nebula, is a about 25 light-years across blown by winds from its central, bright, massive star. A triumvirate of astroimagers ( Joe, Glenn, Russell) created this sharp portrait of the cosmic bubble.
![NGC 6888: туманность Полумесяц](https://images.astronet.ru/pubd/2016/06/10/0001364053/NGC-6888-6-3-16MillerWalker1024.preview.jpg)
10.06.2016
NGC 6888, also known as the Crescent Nebula, is a cosmic bubble about 25 light-years across, blown by winds from its central, bright, massive star. This sharp telescopic portrait uses narrow band image data that isolates light from hydrogen and oxygen atoms in the wind-blown nebula.
![Лебедь: Пузырь и Полумесяц](https://images.astronet.ru/pubd/2015/12/04/0001349923/ngc6888_soap_eder_m1024.preview.jpg)
4.12.2015
These clouds of gas and dust drift through rich star fields along the plane of our Milky Way Galaxy toward the high flying constellation Cygnus. Caught within the telescopic field of view are the Soap Bubble (lower left) and the Crescent Nebula (upper right).
![Край туманности Полумесяц](https://images.astronet.ru/pubd/2001/03/15/0001166688/crescent_hst_big.preview.jpg)
2.08.2000
The Crescent Nebula is a rapidly expanding shell of gas surrounding a dying star. In this recently released image by the Hubble Space Telescope, a bright dynamic part of the nebula three light-years across is shown in representative color.
![NGC 6888: туманность Полумесяц](https://images.astronet.ru/pubd/2008/08/13/0001229115/NGC6888_hallas_c800.preview.jpg)
13.08.2008
NGC 6888, also known as the Crescent Nebula, is a cosmic bubble about 25 light-years across, blown by winds from its central, bright, massive star. This beautiful telescopic view combines a composite color image with narrow band data that isolates light from hydrogen and oxygen atoms in the wind-blown nebula.
![Туманность Полумесяц и ее звезда](https://images.astronet.ru/pubd/2003/04/15/0001189024/crescent_kpno.preview.jpg)
15.04.2003
What caused the Crescent Nebula? Looking like an emerging space cocoon, the Crescent Nebula, visible on the right, was created by the brightest star in its center. A leading progenitor hypothesis has the Crescent Nebula beginning to form about 250,000 years ago.
![Пейзаж в центре Лебедя](https://images.astronet.ru/pubd/2009/10/27/0001236689/cygn_ha_dani900.preview.jpg)
27.10.2009
In cosmic brush strokes of glowing hydrogen gas, this beautiful skyscape unfolds across the plane of our Milky Way Galaxy and the center of the northern constellation Cygnus the Swan. Recorded from a premier remote observatory site (ROSA) in southern France, the image spans about 6 degrees.
![NGC 6888: туманность Полумесяц](https://images.astronet.ru/pubd/2007/11/11/0001224446/crescent_bugnet.preview.jpg)
11.11.2007
What caused the Crescent Nebula? Looking like an emerging space cocoon, the Crescent Nebula, visible in the center of the above image, was created by the brightest star in its center. A leading progenitor hypothesis has the Crescent Nebula beginning to form about 250,000 years ago.
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