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Moon and Aldebaran

 
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Manage episode 177415192 series 1424004
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.

The Moon goes nose to nose with the bull this evening. It stands just below the V-shaped pattern of stars that outlines the head of Taurus the bull. The brightest member of that pattern is Aldebaran, the bull’s orange eye. The other members of the V, including the one at the nose, all belong to the Hyades, one of the most prominent star clusters in the sky.

Aldebaran looks so impressive because it’s a stellar giant. It’s at the end of its life, so it’s puffed up to many times its original size. It’s dozens of times wider than the Sun, and hundreds of times brighter.

Several of the stars of the Hyades are also giants. They don’t look as impressive as Aldebaran, though, in part because they’re more than twice as far away.

One of those giants is Gamma Tauri, the star that marks the bull’s nose. It’s heavier than Aldebaran, but not quite as big or bright. That may be because the two stars are in different phases of their “gianthood.”

Aldebaran has converted the original hydrogen fuel in its core to helium. Now, it’s getting ready to burn the helium to make even heavier elements. Changes in the star during this transition have caused it to expand and brighten.

When it starts burning the helium, it’ll get a little smaller and fainter — and that’s the stage that Gamma Tauri is already in. It’s still big and bright, but not as big and bright as it once was. But it’ll puff up again when the helium is gone — giving the bull a big, bright nose.

Script by Damond Benningfield

  continue reading

28 episodes

Artwork
iconShare
 

Archived series ("HTTP Redirect" status)

Replaced by: StarDate Premium Audio

When? This feed was archived on April 19, 2017 18:43 (7y ago). Last successful fetch was on April 19, 2017 18:05 (7y 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 177415192 series 1424004
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.

The Moon goes nose to nose with the bull this evening. It stands just below the V-shaped pattern of stars that outlines the head of Taurus the bull. The brightest member of that pattern is Aldebaran, the bull’s orange eye. The other members of the V, including the one at the nose, all belong to the Hyades, one of the most prominent star clusters in the sky.

Aldebaran looks so impressive because it’s a stellar giant. It’s at the end of its life, so it’s puffed up to many times its original size. It’s dozens of times wider than the Sun, and hundreds of times brighter.

Several of the stars of the Hyades are also giants. They don’t look as impressive as Aldebaran, though, in part because they’re more than twice as far away.

One of those giants is Gamma Tauri, the star that marks the bull’s nose. It’s heavier than Aldebaran, but not quite as big or bright. That may be because the two stars are in different phases of their “gianthood.”

Aldebaran has converted the original hydrogen fuel in its core to helium. Now, it’s getting ready to burn the helium to make even heavier elements. Changes in the star during this transition have caused it to expand and brighten.

When it starts burning the helium, it’ll get a little smaller and fainter — and that’s the stage that Gamma Tauri is already in. It’s still big and bright, but not as big and bright as it once was. But it’ll puff up again when the helium is gone — giving the bull a big, bright nose.

Script by Damond Benningfield

  continue reading

28 episodes

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