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Description
English: Spiral galaxies together with irregular galaxies make up approximately 60% of the galaxies in the local Universe. However, despite their prevalence, each spiral galaxy is unique — like snowflakes, no two are alike. This is demonstrated by the striking face-on spiral galaxy NGC 6814, whose luminous nucleus and spectacular sweeping arms, rippled with an intricate pattern of dark dust, are captured in this NASA/ESA Hubble Space Telescope image.

NGC 6814 has an extremely bright nucleus, a telltale sign that the galaxy is a Seyfert galaxy. These galaxies have very active centres that can emit strong bursts of radiation. The luminous heart of NGC 6814 is a highly variable source of X-ray radiation, causing scientists to suspect that it hosts a supermassive black hole with a mass about 18 million times that of the Sun.

As NGC 6814 is a very active galaxy, many regions of ionised gas are studded along its spiral arms. In these large clouds of gas, a burst of star formation has recently taken place, forging the brilliant blue stars that are visible scattered throughout the galaxy.
Date
Source http://spacetelescope.org/images/potw1619a/
Author

ESA/Hubble & NASA

Acknowledgement: Judy Schmidt (Geckzilla)

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This file is licensed under the Creative Commons Attribution 4.0 International license.
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Date/TimeThumbnailDimensionsUserComment
current11:38, 16 May 2016Thumbnail for version as of 11:38, 16 May 20163,970 × 3,970 (7.32 MB)Szczureqfull resolution
08:51, 9 May 2016Thumbnail for version as of 08:51, 9 May 20161,280 × 1,280 (473 KB)JmencisomUser created page with UploadWizard

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