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Capella

 
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When? This feed was archived on January 01, 2017 12:48 (7+ y ago). Last successful fetch was on January 01, 2017 07:38 (7+ y ago)

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Manage episode 168761438 series 1329684
Content provided by McDonald Observatory. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by McDonald Observatory or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://player.fm/legal.

For a star like the Sun, which travels through the galaxy alone, the future is pretty certain. But for stars with close companions, the future is tougher to see. Interactions between the two stars change their evolution, fuzzing the view through the astronomer’s crystal ball.

Consider Capella, one of the brightest stars in the night sky. The yellow star is in the northeast at nightfall, and soars high overhead later on.

What we see as Capella is really two stars. Each star is bigger, brighter, and heavier than the Sun.

The stars are only about 10 percent the age of the Sun. But because of their greater heft, they’ve aged much more quickly. Both stars have completed their “normal” lifetimes. Now, thanks to changes in their cores, their outer layers are puffing outward — especially the heavier star.

The stars are close together — only about two-thirds the distance from Earth to the Sun. So as the stars puff up, their surfaces will get closer and closer to each other. Eventually, the heavier star will begin to dump some of its gas on the companion. It’ll also generate strong “winds” that’ll surround both stars in a cloud of gas.

And that’s likely to alter the evolution of the smaller star. As it adds mass, its own nuclear reactions will crank up. The two stars also may spiral closer together — and could even merge. That could create a bigger star, or it could trigger an explosion. For now, though, just how it all plays out remains hard to foresee.

Script by Damond Benningfield

  continue reading

27 episodes

Artwork

Capella

StarDate Premium Audio

published

iconShare
 

Archived series ("HTTP Redirect" status)

Replaced by: StarDate Premium Audio

When? This feed was archived on January 01, 2017 12:48 (7+ y ago). Last successful fetch was on January 01, 2017 07:38 (7+ y ago)

Why? HTTP Redirect status. The feed permanently redirected to another series.

What now? If you were subscribed to this series when it was replaced, you will now be subscribed to the replacement series. This series will no longer be checked for updates. If you believe this to be in error, please check if the publisher's feed link below is valid and contact support to request the feed be restored or if you have any other concerns about this.

Manage episode 168761438 series 1329684
Content provided by McDonald Observatory. All podcast content including episodes, graphics, and podcast descriptions are uploaded and provided directly by McDonald Observatory or their podcast platform partner. If you believe someone is using your copyrighted work without your permission, you can follow the process outlined here https://player.fm/legal.

For a star like the Sun, which travels through the galaxy alone, the future is pretty certain. But for stars with close companions, the future is tougher to see. Interactions between the two stars change their evolution, fuzzing the view through the astronomer’s crystal ball.

Consider Capella, one of the brightest stars in the night sky. The yellow star is in the northeast at nightfall, and soars high overhead later on.

What we see as Capella is really two stars. Each star is bigger, brighter, and heavier than the Sun.

The stars are only about 10 percent the age of the Sun. But because of their greater heft, they’ve aged much more quickly. Both stars have completed their “normal” lifetimes. Now, thanks to changes in their cores, their outer layers are puffing outward — especially the heavier star.

The stars are close together — only about two-thirds the distance from Earth to the Sun. So as the stars puff up, their surfaces will get closer and closer to each other. Eventually, the heavier star will begin to dump some of its gas on the companion. It’ll also generate strong “winds” that’ll surround both stars in a cloud of gas.

And that’s likely to alter the evolution of the smaller star. As it adds mass, its own nuclear reactions will crank up. The two stars also may spiral closer together — and could even merge. That could create a bigger star, or it could trigger an explosion. For now, though, just how it all plays out remains hard to foresee.

Script by Damond Benningfield

  continue reading

27 episodes

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