By Definition
High Definition
Standard Definition
By Length
Full (4-12 min)
Short (1-4 min)
By Date
2014 | 2013 | 2012 | 2011 | 2010
2009 | 2008 | 2007 | 2006
By Category
Solar System
Stars
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Groups of Galaxies
Cosmology/Deep Field
Miscellaneous
HTE
STOP
Space Scoop for Kids!
Subscribe
How To
Apple iTunes
RSS Reader
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
Recent Podcast
A Tour of M82X-2
A Tour of M82X-2
Ultraluminous X-ray Sources, or ULXs, are unusual objects. They are rare and, as their name implies, give off enormous amounts of X-rays. (2014-10-08)


Supernovas: When Stars Die

View/Listen
NASA: We have booster ignition and liftoff of Columbia, reaching new heights for women and X-ray Astronomy.

Martin Elvis: The main thing Chandra does is take these superb, sharp images.

Cady Coleman: Nothing as beautiful as Chandra trailing off on its way to work

Narrator: A supernova is the explosive death of a star. As one of the most energetic events in the universe, a supernova may temporarily outshine the rest of the galaxy in which it resides. But what are supernovas? Every 50 years or so, a massive star in our galaxy blows itself apart in what astronomers call a "supernova". Supernovas are some of the most violent events in the universe. The force of the explosion generates an intense flash of radiation, as well as shock waves analogous to sonic booms. These supernovas are often best seen through X-ray telescopes like Chandra.

Dr. Patrick Slane of the Chandra X-ray Center talks about supernovas in our own Galaxy.

Pat Slane: In our own Galaxy, these types of supernova explosions occur every fifty years or so. The explosions pound the nuclei of atoms together so violently that they build up all of the heavier elements of the periodic table. These are flung out into space where, eventually, they mix with other interstellar gas and form new stars and planetary systems enriched with these heavy elements. Although our Galaxy seems to be in somewhat of a drought for supernova explosions, with the last one being observed in 1604, we see the remnants of these explosions all over the place. The outgoing blast wave from the explosion sweeps up the interstellar gas and heats it to temperatures so high that they glow in X-rays. They can be 40 or 50 light years across, and for the youngest ones we can actually still see them expanding.

Narrator: Pat Slane explains how one kind of supernova, called Type 1a, works.

Pat Slane: Many stars are formed in binary systems. After one star in the system evolves into a white dwarf, it's possible for the companion star to approach the end of its life, in which the hot interior causes the outer layers to expand. If they expand enough, some of the gas can fall over onto the white dwarf. This transfer of matter onto the dense white dwarf can eventually increase its central temperature enough to detonate the entire compact star in what's called a Type Ia supernova explosion. Here the entire white dwarf star is obliterated. This type of supernova always produces about the same brightness, unlike supernova explosions of massive stars, which can vary a lot depending upon the mass of the star. These Type Ia explosions can be seen in other galaxies out to incredible distances. In fact, they provided the first evidence that the most distant objects are moving away from us more rapidly than expected, the result of dark energy accelerating the expansion of the universe.

Narrator: X-ray telescopes, particularly Chandra, are very important tools for astronomers to study supernovas. A supernova explosion is incredibly energetic, and can heat any gas that surrounds it to millions of degrees. The debris field and the high-energy particles within it are what astronomers refer to as a supernova remnant. Such remnants are known to produce intense X-ray radiation that can last for thousands of years. Pat Slane explains how Chandra's images are used to analyze the debris field and reconstruct the star's explosion.

Pat Slane: Because the gas in supernova remnants is so hot, it radiates in X-rays. By measuring the spectrum of the X-rays - that is, the energies of the different X-rays that come from the remnant - we can tell how hot the gas is and what it's composed of. This lets us identify the heavy elements that were produced in the star and its explosion, and compare these with our theoretical models of how these explosions occur.

Narrator: Scientists think that supernovas can trigger star formation and probably led to the formation of our very own solar system some 5 billion years ago. This supernova also likely seeded the cloud with elements like carbon, nitrogen and oxygen that eventually went into the Sun, planets, and ultimately us. These elements are manufactured deep in the interior of massive stars and would, for the most part, remain there if not for the cataclysmic supernova explosions. For these reasons that are very close to home and to others ranging to the quest to understand the history of the universe, Chandra will continue to study these fascinating objects we call supernovas.

Narrator: For more information about the Chandra X-ray Observatory, visit our website at chandra.harvard.edu.

Return to Podcasts