An overview of the Chandra mission and goals, Chandra's namesake, top 10 facts.
Classroom activities, printable materials, interactive games & more.
Overview of X-ray Astronomy and X-ray sources: black holes to galaxy clusters.
All Chandra images released to the public listed by date & by category
Current Chandra press releases, status reports, interviews & biographies.
A collection of multimedia, illustrations & animations, a glossary, FAQ & more.
A collection of illustrations, animations and video.
Chandra discoveries in an audio/video format.
Q&A: Normal Stars, White Dwarf Stars, and Star Clusters

Q:
Is Antares showing signs of pre-Supernova activity like Eta Carinae or Betelgeuse?

A:
We believe it will be many years before Antares shows any signs of pre-supernova activity. More information on this star may be found at:
http://imagine.gsfc.nasa.gov/docs/ask_astro/answers/970221b.html


Eta Carinae
The Chandra site has a field guide to supernovas:
http://chandra.harvard.edu/xray_sources/supernovas.html
which explains the process by which the star evolves and explodes. Another site you may appreciate is at the University of Michigan, again on the evolution of stars:
http://www.umich.edu/~gs265/star.htm
If you consider that even the most massive stars, with the shortest lifetimes before exploding, still live for about 2 million years, then you can see that it would be an amazingly lucky coincidence if we happened to look with a telescope at a star at the exact moment it began to show signs of pre-explosion activity. Although, as you'll read in the Chandra site mentioned above, if we had had a telescope in the year 1054, we would have observed an event just like this. We may get lucky again in our lifetime!

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