yego.me
💡 Stop wasting time. Read Youtube instead of watch. Download Chrome Extension

Everything You Need to Know About Planet Earth


5m read
·Nov 2, 2024

Planet Earth is the home of every lifeform known to us in the universe. Its age is about 1/3 of the age of the universe, and admitted, it is a thing of beauty. A slightly squashed sphere with a heavy metal core and a lighter surface crust, wrapped in a thin sliver of sweet air to breathe, with vast oceans, fertile plains, magnificent mountains, fresh water rivers, streams, lakes, and aquifers, orbiting a star which warms us and gives us energy.

But how did our home come into existence, and what's it made of? 4.6 billion years ago, Earth was created from the remnants of dead stars that collected in a giant, dirty gas cloud. The gas cloud became denser in its center and formed an accretion disk. Small particles started clumping together and building larger and larger objects until they formed the objects we call "Planets" today. This process took 10 to 20 million years and is still not very well understood.

At about this time, when the solar system was young and chaotic, a giant object, about as big as Mars, collided with our home. The impact was violent, and if the object had been more massive, it might have destroyed Earth. Materials from Earth were smashed out into orbit and formed the Moon, which is the biggest satellite in relation to its planet in the solar system. At this time, Earth was a hot hell, constantly being hit by asteroids, with seas of lava and a toxic atmosphere. But something was about to change drastically.

Earth cooled down. Water from the inside of the Earth wandered to the surface and rained down on Earth, only to vaporize again and become clouds. Millions of asteroids brought more and more water to our planet. All the water on Earth has about this volume compared to Earth. Today, the surface of Earth is 71% water and 29% land. 97.5% is saline water, while only 2.5% is fresh water. The fresh water is 69% ice and snow, 30% are ground waters, and only about 1% make up the remaining ground waters. But even this small part is mostly frozen. Only a tiny part of our water is actually lakes and rivers, and an even tinier part is bound in living things.

So, gradually the Earth cooled down, and the surface formed a thin crust. But inside the Earth, hot rock continues to swirl about, moving the crust from below and breaking it apart. This process is called "Plate Tectonics", and is happening right now. We'll make a whole video about it in the future. For now, let's just say that the crust of Earth consisted of separate giant plates that move around. As they meet, they crumble and create mighty mountains or violently plunge back down, deeper into Earth, creating deep trenches. That's the way the highest place on Earth was formed: Mt. Everest, and the deepest: the Mariana Trench.

From our perspective, Earth's mountains and trenches are mighty indeed, but when you look at the Earth in cross-section, you can see how tiny they actually are. The part we stand on is the crust, which is about 50 kilometers thick, though it can vary between 5 and 70 kilometers. By the way, the deepest hole ever drilled by man is 12.262 kilometers deep.

After the crust comes the mantle. It's a silicate rocky shell and about 2,900 kilometers thick. The mantle consists of the upper mantle and the lower mantle. The upper mantle has different regions, too. Its upper part, which is viscous and carries the crust, is called the "Lithosphere." After that, there comes the "Asthenosphere," which consists of less mobile, mostly solid material. The lower mantle reaches deep down to the outer core of Earth.

Earth's outer core is a liquid layer of iron and nickel, about 2,266 kilometers thick. Temperatures vary from 4,000℃ (7,232℉) to 5,700℃ (10,292℉). And in the center is the inner core. It's mostly solid, a ball made of an iron-nickel alloy with a radius of about 1,200 kilometers. 70% of the size of the moon, and about the temperature of the surface of the Sun. It is slowly growing at an estimated rate of about 1mm/year. Now, for some perspective, this small layer of crystallized melt products of former molten mantle is where we live.

Then, there's Earth's magnetic field. It's an invisible phenomenon that diverts high-energy particles coming from the Sun and other sources, allowing for a stable environment with comparatively little radiation impact on Earth. But why is it there? Actually, we don't really know a terrible lot about that. We know it has something to do with the core of Earth. Inside this metal sphere, large electrical currents flow in complicated patterns. They cause a magnetic field that sort of stabilizes itself according to the laws of electrodynamics. This entire system is called the "Dynamo." But, don't let us fool you into thinking we have it all figured out.

Speaking of breathtaking information, what about the airy stuff that surrounds us? By volume, dry air consists mostly of Nitrogen, Oxygen, Argon, Carbon, a variable amount of water vapor, and small amounts of other gases. Humans are very dependent on the lowest layer of the atmosphere: the Troposphere - where the weather is. It's 12 kilometers thick on average. Above that is the Stratosphere, which is where the ozone layer protects us from the sun's most aggressive type of light. Above that is the Mesosphere - the coolest place on Earth, with an average temperature around -85℃ (-121℉).

At about 80 kilometers up, the Thermosphere starts. The transition to space is a fluent one, without clear borders, but humans decided that space starts here. At about 100 kilometers, Earth stops, and space begins, though the atmosphere extends a bit further. In this region, we find the Ionosphere, the aurora borealis, and the ISS, and the outermost layer is the Exosphere, stretching up to 10,000 kilometers. It merges fluently with outer space, where there's no atmosphere at all. The atoms and molecules in this area are so far apart that they can travel hundreds of kilometers without colliding with each other.

OK. Humans, in their present form, have only been around for 200,000 years - that's 0.004% of Earth's history. Not long, really. And here we are now, living in a thin, moist layer on a small, wet rock. We call this rock: Earth. It is the product of the universe's deepest workings, the result of a constant process of creation and destruction, happening all over the universe, all the time, helped by chance, the laws of the universe, and random events. We are really lucky.

More Articles

View All
Introduction to integral calculus | Accumulation and Riemann sums | AP Calculus AB | Khan Academy
So I have a curve here that represents ( y ) is equal to ( f(x) ), and there’s a classic problem that mathematicians have long thought about: how do we find the area under this curve, maybe under the curve and above the x-axis, and let’s say between two b…
2016 Breakthrough Junior Challenge with Priscilla Chan | National Geographic
The Breakthrough Junior Challenge is a video competition in which we invite you to submit creative and exciting explanations of ideas in math and science. Last year, Ryan Chester won the first Breakthrough Junior Challenge prize. “Make a video about scie…
Two-sample t test for difference of means | AP Statistics | Khan Academy
Kaito grows tomatoes in two separate fields. When the tomatoes are ready to be picked, he is curious as to whether the sizes of his tomato plants differ between the two fields. He takes a random sample of plants from each field and measures the heights of…
How A Ponzi Scheme Works
So you may have heard about Ponzi schemes in the news. Everybody knows they’re illegal, but you might not understand how they work. So Ben is here to show us. To start off, Ben gets a few people to invest their money with him. At the end of the year, he …
The Dred Scott case and citizenship | Citizenship | High school civics | Khan Academy
In this video, I want to give you a very brief overview of Dred Scott vs. Sanford, a Supreme Court decision made in 1857 that had major consequences on the definition of citizenship in the United States. This case was tied up with so many of the questions…
Planning Our Route to Mars | MARS: How to Get to Mars
Before we get through the first half of this century, humans will be living and working on Mars. We can do it with the kinds of technology we either have today or know how to build today. Let’s think about how we go about this thing, okay? This journey to…