What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. What is a News Nugget? News Nuggets are bulletins from the world of astronomy. NASA's Hubble Space Telescope photographed three magnificent sections of the Veil Nebula -- the shattered remains of a supernova that exploded thousands of years ago. This series of images provides beautifully detailed views of the delicate, wispy structure resulting from this cosmic explosion. The Veil Nebula is one of the most spectacular supernova remnants in the sky. The entire shell spans about 3 degrees on the sky, corresponding to about 6 full moons.
*Acknowledgment:* J. Hester (Arizona State University)
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Technical facts about this news release: About the Object Object Name: Veil Nebula Object Description: Supernova Remnant Position (J2000): R.A. 20h 50m Dec. +30° 30' Constellation: Cygnus Distance: Approximately 1,500 light-years (460 pc) away. About the Data Data Description: The Hubble image was created from HST data from proposals 5774 and 5779: J. Hester (Arizona State Universitry) and J. Westphal (Caltech). Instrument: WFPC2 Exposure Date(s): November 1994, August 1997 Filters: F502N ([O III]), F656N (Halpha), and F673N ([S II]) About the Image Image Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hub ble Collaboration Release Date: August 2, 2007 Color: This image is a composite of many separate exposures made by the WFPC2 instrument on the Hubble Space Telescope. Three filters were used to sample narrow wavelength ranges. The color results from assigning different hues (colors) to each monochromatic image. In this case, the assigned colors are: F502N ([O III]) blue F656N (Halpha) green F673N ([S II]) red Orientation: Veil Nebula - Segment #2 [ http://imgsrc.hubbl…]
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*Image Type:*: Astronomical
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*Release Date*:August 2, 2007 04:00 PM (EDT)
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*News Release Number:*: STScI-2007-30a
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*Title*:Uncovering the Veil Nebula
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*Description*: NASA's Hubble Space Telescope photographed three magnificent sections of the Veil Nebula ? the shattered remains of a supernova that exploded thousands of years ago. This series of images provides beautifully detailed views of the delicate, wispy structure resulting from this cosmic explosion. The Veil Nebula is one of the most spectacular supernova remnants in the sky. The entire shell spans about 3 degrees on the sky, corresponding to about 6 full moons. The Veil Nebula is a prototypical middle-aged supernova remnant, and is an ideal laboratory for studying the physics of supernova remnants because of its unobscured location in our Galaxy, its relative closeness, and its large size. Also known as the Cygnus Loop, the Veil Nebula is located in the constellation of Cygnus, the Swan. It is about 1,500 light-years away from Earth. Stars in our Galaxy, and in other galaxies, are born and then die. How long a star lives depends on how massive it is. The more massive the star, the shorter its life. When a star significantly more massive than our Sun runs out of fuel, it collapses and blows itself apart in a catastrophic supernova explosion. A supernova releases so much light that it can outshine a whole galaxy of stars put together. The exploding star sweeps out a huge bubble in its surroundings, fringed with actual stellar debris along with material swept up by the blast wave. This glowing, brightly colored shell of gas forms a nebula that astronomers call a "supernova remnant." Such a remnant can remain visible long after the initial explosion fades away. Scientists estimate that the Veil supernova explosion occurred some 5,000 to 10,000 years ago. The small regions captured in these Hubble images provide stunning close-ups of the Veil. Fascinating smoke-like wisps of gas are all that remain visible of what was once a star in our Milky Way Galaxy. The intertwined rope-like filaments of gas in the Veil Nebula result from the enormous amounts of energy released as the fast-moving debris from the explosion plows into its surroundings and creates shock fronts. These shocks, driven by debris moving at 600,000 kilometers per hour, heat the gas to millions of degrees. It is the subsequent cooling of this material that produces the brilliant glowing colors. The Hubble images of the Veil Nebula are striking examples of how processes that take place hundreds of light-years away can sometimes resemble effects we see around us in our daily life. Although caused by different forces, the structures show similarities to the patterns formed by the interplay of light and shadow on the bottom of a swimming pool, rising smoke, or a ragged cirrus cloud. Although only about one star per century in our Galaxy will end its life in this spectacular way, these explosions are responsible for making all chemical elements heavier than iron, as well as being the main producers of oxygen in the universe. Elements such as copper, mercury, gold, and lead are
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forged in these violent events. The expanding shells of supernova remnants mix with other clouds in the Milky Way and become the raw material for new generations of stars and planets. The chemical elements that constitute Earth, and indeed those of which we ourselves are made, were formed deep inside ancient stars and distributed by supernova explosions in nebulae like the one we see here. The images were taken with Hubble's Wide Field Planetary Camera 2 (WFPC2) in November 1994 and August 1997. The color is produced by creating a composite of three different images. The colors indicate emission from different kinds of atoms excited by the shock: blue shows oxygen, green shows sulfur, and red shows hydrogen. For additional information, contact: Ray Villard Space Telescope Science Institute, Baltimore, Md. 410-338-4514 villard@stsci.edu Keith Noll Space Telescope Science Institute, Baltimore, Md. 410-338-1828 noll@stsci.edu Lars Lindberg Christensen Hubble/ESA, Garching, Germany 011-49-89-3200-6306 lars@eso.org
