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We Finally Know What Elements Are Contained in an Exploded Supernova

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NASA’s Chandra X-Ray Observatory has been taking a long, hard look at one of the Milky Way’s most famous and studied objects – the remnant of an exploded star, Cassiopeia A. And it’s revealed the location of the elements left behind in the star’s remains.

This is because it only exploded very recently – probably in around the year 1680 CE. Because it’s so close and so new, it can help us figure out how stars help produce and spread common elements throughout the Universe, as well as provide clues as to what really happens when a star explodes.

According to Chandra’s data, the exploding star blasted off 10,000 Earth masses of sulphur; 20,000 Earth masses of silicon; 70,000 Earth masses of iron; and 1 million Earth masses of oxygen, which is not shown in the new image because it occurs across too broad a range of the X-ray spectrum, and could not be isolated like the other elements.

Combined with oxygen and the elements Chandra has isolated, all the elements needed to make DNA are being blasted into space in Cassiopeia A. All the oxygen in our Solar System would have come from explosions such as the one that produced Cassiopeia A, as would about half the calcium and 40 percent of the iron.

The remainder would have come from smaller stellar explosions – because stars are the only forge that can create these elements. Inside the remnant is a neutron star, the remains of the star that exploded in the 17th century.

As nucleosynthesis fused lighter elements into heavier ones, radiation pressure was no longer sufficient to keep the star’s outer layer intact.


Article originally posted at

Post Author: John Koetsier

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