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Ask a Spaceman!

AaS! 224: Can Life Survive on Locked Planets?

Ask a Spaceman!

Paul M. Sutter

Astrophysics, Science, Cosmos, Holes, Black, Astronomy, Natural Sciences, Universe, Cosmology, Space, Physics

4.8853 Ratings

🗓️ 21 May 2024

⏱️ 38 minutes

🧾️ Download transcript

Summary

How do planets get tidally locked? What are these systems typically like? Can life find a home in such a challenging environment? I discuss these questions and more in today’s Ask a Spaceman!

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Transcript

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0:00.0

The famed science fiction author Isaac Asimov called them Ribbon Worlds.

0:13.1

Planets forced to always show one face to their parent star.

0:18.0

The star side would be locked in perpetual day, its sun never dipping below the

0:23.5

horizon. Indeed, its sun never moving at all, fixed in place as if time itself stood still.

0:32.0

The far side would be trapped in perpetual night, a sky blazing with the light of a thousand stars, never

0:40.1

knowing the warmth of its own parent. And in between the two extremes, a special place.

0:48.4

A Terminator line, the boundary between night and day, a region of infinite twilight, or, depending on your perspective,

0:56.3

perpetual dusk, caught between the two poles of heat and cold, this ribbon that stretches

1:02.6

like a girdle around a planet might, might, just be a home for life, neither too hot in the

1:10.2

never-ceasing glare of the star, or too cold in its

1:13.8

infinite night. At the time that Asimov coined that term in the 1950s, astronomers still

1:20.7

believed that Mercury, the innermost and smallest planet of the solar system, was in such a state.

1:27.8

In speculation abounded about whether it could possibly support a strange form of life

1:33.1

in the narrow ribbon of its own Terminator.

1:36.1

But soon observations revealed that Mercury does indeed rotate just extremely slowly.

1:42.0

There are worlds in our solar system that are indeed locked this way, but they are

1:46.8

all satellites. Our own moon is like this, always presenting the same face to observers on

1:52.4

the surface of the Earth. Indeed, despite our intimacy with our nearest of cosmic neighbors,

1:58.2

it wasn't until the 1950s that we humans got our first

2:03.1

hazy glance at the far side of the moon. This frozen face is given a technical term, because

2:11.0

of course it is, and it's known as tidal locking. The source of tidal locking is, well, we actually have it a little easy here

2:19.9

because this is a rare case of the technical jargon term actually describing the physics.

...

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