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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, blurring 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.
Capella consists of two stars. Each 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’s.
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 gas on the companion. It’ll also generate strong “winds” that’ll surround both stars in a cloud of gas.
That’s likely to alter the evolution of the smaller star. As it adds mass, its own 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 plays out remains hard to predict.
Script by Damond Benningfield
Support McDonald Observatory
By Billy Henry4.6
251251 ratings
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, blurring 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.
Capella consists of two stars. Each 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’s.
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 gas on the companion. It’ll also generate strong “winds” that’ll surround both stars in a cloud of gas.
That’s likely to alter the evolution of the smaller star. As it adds mass, its own 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 plays out remains hard to predict.
Script by Damond Benningfield
Support McDonald Observatory

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