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- PHOTO RELEASE NO.: STScI-PRC95-11
- FOR RELEASE: February 20, 1995
-
-
- HUBBLE'S CLOSE-UP VIEW OF
- A SHOCKWAVE FROM A STELLAR EXPLOSION
-
- This image shows a small portion of a nebula called the "Cygnus Loop."
- Covering a region on the sky six times the diameter of the full Moon,
- the Cygnus Loop is actually the expanding blastwave from a stellar
- cataclysm - a supernova explosion - which occurred about 15,000 years
- ago.
-
- In this image the supernova blast wave, which is moving from left to
- right across the field of view, has recently hit a cloud of denser
- than average interstellar gas. This collision drives shock waves into
- the cloud that heats interstellar gas, causing it to glow.
-
- Just as the microscope revolutionized the study of the human body by
- revealing the workings of cells, the Hubble Space Telescope is offering
- astronomers an unprecedented look at fine structure within these shock
- fronts. Astronomers have been performing calculations of what should
- go on behind shock fronts for about the last 20 years, but detailed
- observations have not been possible until Hubble.
-
- This image was taken with Hubble's Wide Field and Planetary Camera 2
- (WFPC2). The color is produced by composite of three different
- images. Blue shows emission from "doubly ionized" oxygen atoms (atoms
- that have had two electrons stripped away) produced by the heat behind
- the shock front. Red shows light given off by "singly ionized" sulfur
- atoms (sulfur atoms that are missing a single electron). This sulfur
- emission arises well behind the shock front, in gas that has had a
- chance to cool since the passage of the shock. Green shows light
- emitted by hydrogen atoms. Much of the hydrogen emission comes from an
- extremely thin zone (only several times the distance between the Sun
- and Earth) immediately behind the shock front itself. These thin
- regions appear as sharp, green, filaments in the image.
-
- This supernova remnant lies 2,500 light-years away in the constellation
- Cygnus the Swan.
-
- Credit: Jeff Hester (Arizona State University) and NASA
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