File:Caldwell 55.jpg
Caldwell_55.jpg (512 × 512 pixels, file size: 183 KB, MIME type: image/jpeg)
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Summary
[edit]DescriptionCaldwell 55.jpg |
English: Garden-variety stars like the Sun live fairly placid lives in their galactic neighborhoods, steadily churning out heat and light for billions of years. When these stars reach retirement age, however, they transform into unique and often psychedelic works of art. This Hubble Space Telescope image of Caldwell 55, also known as the Saturn Nebula and NGC 7009, shows the result, called a planetary nebula. While it looks like a piece of wrapped cosmic candy, what we see is actually the outer gaseous layers of a dying star.
Stars are powered by nuclear fusion, but each one comes with a limited supply of fuel. When a medium-mass star exhausts its nuclear fuel, it will swell up and shrug off its outer layers until only a small, hot core remains. The leftover core, called a white dwarf, is a lot like a hot coal that glows after a barbecue — eventually it will fade out. Until then, the cast-off gaseous debris fluoresces as it expands out into the cosmos, possibly destined to be recycled into later generations of stars and planets. The Saturn Nebula is only about 1,400 light-years away in the direction of the Aquarius constellation. Its proximity has made it a popular target for study by telescopes all around the world. Hubble took this image in visible light using the Wide Field and Planetary Camera 2 in 1996. Using Hubble’s observations, scientists have characterized the nebula’s composition, structure, temperature and the way it interacts with surrounding material. Studying planetary nebulas is particularly interesting since our Sun will experience a similar fate around five billion years down the road. The Saturn Nebula has been known since 1782 when it was discovered by astronomer William Herschel. Late summer skies will provide ideal viewing of this kaleidoscopic structure for Northern Hemisphere observers (late winter for those in the Southern Hemisphere). This magnitude-8 nebula will look like a star in smaller telescopes, but larger telescopes will reveal more detail, including two extended lobes on either side of the nebula that resemble the rings of Saturn, lending the nebula its nickname. Using high magnification along with averted vision (looking away from the center of the object) will provide the best views of the fainter exterior regions of the nebula. For more information about Hubble’s observations of Caldwell 55, see: hubblesite.org/image/575 Credit: Bruce Balick (University of Washington), Jason Alexander (University of Washington), Arsen Hajian (U.S. Naval Observatory), Yervant Terzian (Cornell University), Mario Perinotto (University of Florence, Italy), Patrizio Patriarchi (Arcetri Observatory, Italy), NASA/ESA For Hubble's Caldwell catalog site and information on how to find these objects in the night sky, visit: www.nasa.gov/content/goddard/hubble-s-caldwell-catalog |
Date | |
Source | https://www.flickr.com/photos/144614754@N02/49201186201/ |
Author | NASA Hubble |
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This image was originally posted to Flickr by NASA Hubble at https://flickr.com/photos/144614754@N02/49201186201 (archive). It was reviewed on 23 February 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0. |
23 February 2020
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Metadata
This file contains additional information such as Exif metadata which may have been added by the digital camera, scanner, or software program used to create or digitize it. If the file has been modified from its original state, some details such as the timestamp may not fully reflect those of the original file. The timestamp is only as accurate as the clock in the camera, and it may be completely wrong.
Image title |
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Date and time of data generation | 06:00, 17 December 1997 |
Short title | Hubble's Planetary Nebula Gallery. A View of NGC 7009 |
Credit/Provider | Bruce Balick (University of Wash |
Source | ESA/Hubble |
Publisher | ESA/Hubble |
Usage terms |
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JPEG file comment | NGC 7009 has a bright central star at the centre of a dark cavity bounded by a football-shaped rim of dense, blue and red gas. The cavity and its rim are trapped inside smoothly-distributed greenish material in the shape of a barrel and comprised of the star's former outer layers. At larger distances, and lying along the long axis of the nebula, a pair of red 'ansae', or 'handles' appears. Each ansa is joined to the tips of the cavity by a long greenish jet of material. The handles are clouds of low-density gas. NGC 7009 is 1, 400 light-years away in the constellation Aquarius. The Hubble telescope observation was taken April 28, 1996 by the Wide Field and Planetary Camera 2. |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Software used | Adobe Photoshop CS Windows |
File change date and time | 17:49, 9 December 2003 |
Y and C positioning | Centered |
Exif version | 2.31 |
Date and time of digitizing | 17:49, 9 December 2003 |
Meaning of each component |
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Supported Flashpix version | 1 |
Color space | sRGB |
IIM version | 4 |
Keywords |
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Bits per component |
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Height | 512 px |
Width | 512 px |
Pixel composition | RGB |
Number of components | 3 |
Contact information |
http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
Type of media | Observation |
Date metadata was last modified | 18:49, 9 December 2003 |