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Moon, Jupiter, and Spica

 
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Manage episode 177458707 series 1424224
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 is just past full this evening. Sunlight illuminates all but a sliver of the lunar hemisphere that faces our way, so the Moon is bright and beautiful. And it has a couple of bright, beautiful companions. The star Spica stands to its upper right, with the brilliant planet Jupiter above Spica.

If you look at the Moon, you’ll see the same features that are always in view — dark volcanic plains and lighter-colored highland regions. They’re the same features you’ll see tomorrow night, and a month from now, and a hundred years from now.

Since the same side of the Moon always faces our way, you might think that the Moon doesn’t turn on its axis. But that’s not the case. In fact, if it didn’t turn we’d see the entire Moon — the familiar near side and the hidden far side. Instead, it’s the rate at which it turns that keeps it aiming our way.

Over the eons, Earth’s gravity created tides in the lunar surface. That slowed the Moon’s rotation. Eventually, it slowed enough that the same side always faces our way. So the Moon turns on its axis at the same rate at which it orbits Earth. By the time it’s moved a quarter of the way around us, it’s also completed a quarter turn on its axis, and so on.

The Moon, of course, creates tides in Earth’s oceans, which are slowing its rotation. So if Earth and Moon are around long enough, then just as the same hemisphere of the Moon always faces Earth, the same hemisphere of Earth will always face the Moon.

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 20, 2017 14:46 (7+ y ago). Last successful fetch was on April 20, 2017 12:56 (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 177458707 series 1424224
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 is just past full this evening. Sunlight illuminates all but a sliver of the lunar hemisphere that faces our way, so the Moon is bright and beautiful. And it has a couple of bright, beautiful companions. The star Spica stands to its upper right, with the brilliant planet Jupiter above Spica.

If you look at the Moon, you’ll see the same features that are always in view — dark volcanic plains and lighter-colored highland regions. They’re the same features you’ll see tomorrow night, and a month from now, and a hundred years from now.

Since the same side of the Moon always faces our way, you might think that the Moon doesn’t turn on its axis. But that’s not the case. In fact, if it didn’t turn we’d see the entire Moon — the familiar near side and the hidden far side. Instead, it’s the rate at which it turns that keeps it aiming our way.

Over the eons, Earth’s gravity created tides in the lunar surface. That slowed the Moon’s rotation. Eventually, it slowed enough that the same side always faces our way. So the Moon turns on its axis at the same rate at which it orbits Earth. By the time it’s moved a quarter of the way around us, it’s also completed a quarter turn on its axis, and so on.

The Moon, of course, creates tides in Earth’s oceans, which are slowing its rotation. So if Earth and Moon are around long enough, then just as the same hemisphere of the Moon always faces Earth, the same hemisphere of Earth will always face the Moon.

Script by Damond Benningfield

  continue reading

28 episodes

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