Earth Formation by Tega Jessa One of the oldest questions for mankind is how the Earth was formed. However, no one has an exact answer. First by the best estimates it occurred over 4 billion years ago before any life appeared. So there are no eyewitness accounts and other pieces of evidence. The best we can do is look at the geologic record and the stars to get our answers. While we may not have the entire picture we have a good idea and it all starts with how stars are born. magma cause volcanic activity that released gases. These would lead to the creation of the atmosphere and the oceans starting the water cycle. The formation of the Earth was only the beginning and we still see the Earth changing year by years through erosion and plate tectonics. However in learning more about the formation of the Earth we are able to better understand what makes life possible on our planet. Just like the formation of the Earth and other planets, stars take a long time to be born. Stars are essentially formed from clouds of gas in space. We know these as nebulas. You can basically consider them to be star forges. Over time gravity causes the atoms of gases and space dust to start coming together and gathering. Over time this gather of gases gains more mass and with it stronger gravity. This is a process that can take millions of years. In time the gravity causes the gases, mainly hydrogen to fuse in a nuclear reaction and a star is formed. The formation of the Earth occurred after this initial phase happened for our Sun. After the Sun was formed we know from observations and other indirect evidence that there were left over gases and heavier elements. The gravity of the Sun helped to flatten these leftovers into a disk and start to fuse them together. This created the planetesimals and planetoids which would later make up the planets. Over time these planetesimals would collide creating even bigger masses. It was in this method that the Earth was eventually formed. Now we need to know that fusion eventually creates heavier elements such as carbon and iron. These elements were to compose a significant part of young Earth. The pressure and heat from radioactive decay of elements and the aftershocks of massive collisions caused the Earth to be molten. Over time the surface of the Earth cooled and became the Crust. However the molten layers that remained became our mantle and the core. The currents of this massive underground ocean of The Earth – Part 1 (ART 7.1) Layers of the Earth by Fraser Cain The solid surface we stand on is just one of the layers of the Earth. In fact, it’s the only one we can survive on. If you could dig down through the Earth’s layers, you would find temperatures and pressure rising to the point that rock melts and beyond. Let’s take a look at the Earth layers, starting with the inside. The very center of the Earth is known as the core. This is actually comprised of a solid inner core with a radius of 1,220 km, and then a liquid outer core that extends out to 3,400 km. Scientists think that during the Earth‘s formation, the heaviest elements – like iron – sunk down to the center of the Earth and helped to form this core. We know that the Earth’s core rotates, generating a magnetic field that protects us from the Sun‘s solar wind. Nobody really knows how hot it is down there, but scientists think it’s probably 3,000-5,000 Kelvin. page 1 of 5 Outside the core is the mantle,; the thickest part of the Earth’s interior layers. This is a vast underground ocean… of liquid rock! The lave we see pouring out of volcanoes comes from the mantle. The heat released from the Earth’s core drives convection in the mantle, and the crust‘s tectonic plates serve to stir up the mantle as well. Hotter material rises, and relatively cooler blobs of rock sink down through the mantle. The outermost layer of the Earth is the crust – the cooled and hardened part of the Earth. That’s what you’re standing on right now! The depth of the crust varies from 5 km underneath the oceans and 30 km thick underneath the continents. You might be surprised to know that the Earth’s crust only accounts for about 1% of the entire volume of the Earth. planet and accumulate at the core. The core is believed to have two parts: a solid inner core, with a radius of 1,220 km, and then a liquid outer core that extends to a radius of 3,400 km. The core is through to be 80% iron, as well as nickel and other dense elements like gold, platinum and uranium. The inner core is solid, but the outer core is a hot liquid. Scientists think that movements of metal, like currents in the oceans, create the magnetic field that surrounds the Earth. This magnetic field extends out from the Earth for thousands of kilometers, and redirects the solar wind blowing from the Sun. Without this magnetic field, the solar wind would blow away the lightest parts of our atmosphere, and make our environment more like cold, dead Mars. Although the Earth’s crust is cool, the inside of the Earth is hot. The mantle is only about 30 km beneath our feet, and it’s hot enough to melt rock. At the core of the Earth, temperatures are thought to rise to 3,000 to 5,000 Kelvin. Since the core is thousands of kilometers beneath our feet, how can scientists know anything about it? One way is to just calculate. The average density of the Earth is 5.5 grams per cubic cm. The Earth’s surface is made of less dense materials, so the inside must have something much more dense than rock. The second part is through seismology. When earthquakes rock the surface of the Earth, the planet rings like a bell, and the shockwaves pass through the center of the Earth. Monitoring stations around the planet detect how the waves bounce, and scientists are able to use this to probe the interior of the Earth. Core of the Earth Earth’s Mantle by Fraser Cain Scientists believe that deep down inside the Earth, there’s a huge ball of liquid and solid iron. This is the Earth’s core, and it protects us from the dangerous radiation of space. by Fraser Cain The ground under your feet might seem solid, but you’re standing on a relatively thin crust of rock above a vast ocean of rock. This molten rock is the Earth‘s mantle, and it comprises the largest part of the Earth‘s volume. When the Earth first formed, 4.6 billion years ago, it was a hot ball of molten rock and metal. And since it was mostly liquid, heavier elements like iron and nickel were able to sink down into the The Earth – Part 1 (ART 7.1) The crust we stand on is only about 30 km thick. Out in the oceans, it’s even thinner, getting down to 5 km in places. Beneath this crust is the mantle page 2 of 5 of the Earth; a region that extends down a depth of almost 2,900 km. Although the mantle is largely hidden from our view, we do see it in places where cracks open up, allowing the molten rock to escape. These are volcanoes, of course, and the liquid rock we see pouring out is the same as you’d find in the mantle. The Earth’s mantle is mostly composed of silicate rocks that are rich in iron and magnesium. Although it’s mostly solid, it’s hot enough that it can flow over long timescales. The upper mantle flows more easily than the lower mantle because of the increasing temperature and pressures as you descend into the Earth. The Earth’s tectonic plates float on top of the mantle. In some places, the plates are sliding under one another, returning rock back to the interior of the Earth. In other places, the plates are spreading apart, and fresh volcanic material is welling up to fill the cracks. Inside the mantle, convection is slowly taking place – like in a lava lamp. Hotter material, heated by the core of the Earth rises slowly to the surface of the mantle. Material cools near the crust and then sinks back down to the core, to repeat the process all over again. It’s believed that this convection helps drive the motions of Earth’s tectonic plates. Earth’s Crust by Fraser Cain You might not realize it, but you’re standing on a thin shell of solid rock encasing a vast quantity of molten rock. This is the Earth‘s crust, and it’s the part of the planet that has cooled down enough to solidify. But just a few kilometers below your feet, it’s molten rock, extending for thousands of kilometers down to the planet‘s superheated iron core. Here on solid ground, on the continental shelves, the crust of the Earth is about 30 km thick. In the mid-ocean, the thickness of the crust can be as little as 5 km. The entire crust occupies just 1% of the Earth‘s volume. The crust is composed of a variety of igneous, metamorphic and sedimentary rocks gathered together into tectonic plates. These plates float above the Earth’s mantle, and it’s believed that convection of rock in the mantle causes the plates to slide around. On average, rocks in the crust last about 2 billion years before they slide underneath another plate and are returned to the Earth’s mantle. New rocks are formed in the mid-ocean regions where new material wells out of the Earth in between spreading plates. In comparison, rocks in the oceans are only 200 million years old. The temperature of the crust increases as you go deeper into the Earth. It starts out cool, but can get up to 400 degrees C at the boundary between the crust and the mantle. Scientists really know very little about internal structure of the Earth. The crust is the only part that we have any information about. And we’ve barely explored it at all. The deepest hole ever dug was the Russian Kola Superdeep Borehole. Started in 1970, the hole eventually reached a depth of 12.3 km. They eventually had to quit because temperatures in the hole became too hot to go any further. Other plans are in the works to bore into the crust in the ocean, where the thickness is much less. The Earth – Part 1 (ART 7.1) page 3 of 5 The crust of the Earth is not one single piece but is made up of interacting pieces called the tectonic plates. This is because the crust sort of floats on top of the lower layer of the earth made of rock and magma called the mantle. The convection of magma in the mantle create the current that causes plate tectonics forcing different plate to crash or pull away creating seismic activity. Crust of the Earth by Tega Jessa We know about the crust of the Earth than any other part of the Earth‘s structure. It is mainly because this is the layer that we live on and it the region most easily within our reach. Thought it is only the “peel’ of the earth we have been able to learn a lot about the Earth from investigating it. We know how old the earth is by dating the rocks and classifying the different kinds that rose to the surface from the interior of the earth. We know the fault lines and boundaries of tectonic plates and where and how the effect the formation of volcanoes and other geothermal activity. Scientist believe that the crust was the last part of the earth to be formed. It is theorized that over 4 billion years ago the Earth was a molten ball. The denser elements sank to the center of the planet and became the core. The lighter elements rose and stratified forming the mantle. The last layer the crust was formed when the molten exterior of the Earth finally cooled. The Earth’s crust can be divided into two distinct categories. The first is the oceanic crust and the second is the continental crust. Each has a unique composition that is different from the other and the mantle below. The oceanic crust is most made up of basalt, diabase, gabbro. The continental crust is made mostly of granite. The thickness of the crust also varies depending on whether it is the continental or oceanic crust. The continental crust can be anywhere from 30 km to 50 km thick and the oceanic crust can be 5 to 10 km thick. The Earth – Part 1 (ART 7.1) The crust is also the source of many of the minerals and other substances that we use in industry and other fields. The continental crust is especially known for the wide variety of minerals in its composition. Tectonic Plates by Jerry Coffey The lithosphere is the rigid outermost shell of a rocky planet. The lithosphere is broken up into what are called tectonic plates. The Earth has eight major and many minor plates. The lithospheric plates ride on the asthenosphere. These plates move in relation to one another at one of three types of plate boundaries: convergent, or collisional boundaries; divergent boundaries, also called spreading centers; and transform boundaries. Earthquakes, volcanoes, mountainbuilding, and oceanic trench formation occur along plate boundaries. The lateral movement of the plates is typically 50–100 mm annually. The reason that tectonic plates are able to move is the Earth‘s lithosphere has a higher strength and lower density than the underlying asthenosphere. Their movement is dictated by heat dissipation from the Earth’s mantle. Lateral density variations in the mantle result in convection, which is transferred into tectonic plate motion through some combination of frictional drag, downward suction at the subduction zones, and variations in topography and density of the crust that result in differences in gravitational forces. Tectonic plates consist of lithospheric mantle overlain by one of two types of crust material: oceanic crust (sima) and continental crust (sial). Average oceanic lithosphere is typically 100 km thick; its thickness is a function of its age: as time passes, it conductively cools and becomes thicker. page 4 of 5 Because it is formed at mid-ocean ridges and spreads outwards, its thickness is a function of its distance from the mid-ocean ridge where it was formed. For a typical distance oceanic lithosphere must travel before being subducted, the thickness varies…6 km thick at mid-ocean ridges to greater than 100 km at subduction zones; for shorter or longer distances, the subduction zone thickness becomes smaller or larger, respectively. Typical continental lithosphere is typically 200 km thick, though this also varies considerably between basins, mountain ranges, and stable cratonic interiors of continents. The two types of crust also differ in thickness, with continental crust being considerably thicker than oceanic. The difference being 35 km vs. 6 km. The tectonic plates have played a major role in the formation of the Earth as we know it and will continue to do so for the entire existence of this planet. At the same time those plates have wreaked havoc on human dwellings and lifestyle by causing earthquakes, tsunamis, etc. Ah, mother Earth is our sustenance and our bane. The Earth – Part 1 (ART 7.1) page 5 of 5