4.6 • 3K Ratings
🗓️ 9 July 2019
⏱️ 17 minutes
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A geophysical look at the idea that Earth's early history had enormous destructive tides.
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0:00.0 | To me there's never been a more exciting or dramatic concept than the idea that in the |
0:08.3 | early days of planet Earth, when the moon was much closer and orbited much faster and exerted |
0:14.6 | much greater tidal forces, that catastrophic oceanic tidal waves, kilometers high, circled |
0:22.5 | the planet at thousands of kilometers per hour, destroying everything in their path, |
0:28.2 | multiple times every single day. Prehistoric supersonic monster tides is coming up right now, |
0:36.0 | unskeptoid. |
0:42.2 | You're listening to Skeptoid. I'm Brian Dunning from Skeptoid.com. Prehistoric supersonic monster tides. |
0:52.2 | It's a fact in the early days of Earth when the moon was newly formed. The two bodies were |
0:58.1 | much closer and orbited each other much faster, spinning like ice dancers pulled tight. Gradually |
1:04.9 | they've been slowing and pulling farther apart, leading to the distance we measure today, |
1:09.0 | and the relatively mellow tides we enjoy. The moon's gravity is what drives the tides on Earth, |
1:15.4 | so you may have heard, either on television or the internet, or your other pop culture, |
1:20.4 | data-spigot of choice, that in those earliest days, the tides were enormous, manifesting as a |
1:27.2 | titanic wall of crashing white water, kilometers high, an endless sweep of destruction, roaring across |
1:34.4 | the continents at supersonic speeds, obliterating everything every few hours. It's an image that puts |
1:42.4 | anything in Dante's inferno to shame. It's an image of such intensity, such drama, that you may wonder |
1:49.5 | if such cataclysmic violence was actually possible and actually real. Today we're going to deconstruct the |
1:56.1 | components of this geologic and oceanographic melee, and see if we can determine just what the |
2:02.7 | real conditions were, in comparison to this popularly depicted cataclysm. Let's go back in time, |
2:11.3 | some four and a half billion years ago. Earth and the other planets coalesced from the dust of |
2:17.3 | which the solar system was formed. The ejected material left over when a previous dying star exploded. |
2:24.7 | Gravity and angular momentum drew this material together into a rotating disc, which gradually |
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