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Hang on! Hang on!

Hang on! - PowerPoint Presentation

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Uploaded On 2017-07-16

Hang on! - PPT Presentation

Its going to be a WILD RIDE Journey to the Center of the Earth Imagine if you will You are a Geologist and have been given the task of traveling to the center of the Earth You have a specially designed Earthship that will take you to the core Your Earthship ID: 570561

crust core pressure mantle core crust mantle pressure layer stop rock earth lithosphere temperature solid depth outer dense asthenosphere

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Presentation Transcript

Slide1

Hang on!

It’s going to be a WILD RIDE!

Journey to the Center of the EarthSlide2
Slide3

Imagine if you will…..

You are a Geologist* and have been given the task of traveling to the center of the Earth. You have a specially designed Earthship that will take you to the core. Your Earthship,

Gaia One

, is equipped with instruments that will record changes in temperature and pressure as you travel through the crust, the mantle, and finally, the core.

So strap yourself in….

It’s going to get very, very HOT!

*

A scientist who studies the physical and chemical properties of rocks,

and the processes and forces that make and shape the Earth.Slide4

First stop – the CRUST

The first layer that Gaia One will travel through is the crust…

The crust is a layer of rock

that forms the outer skin of the Earth

2

types of crust:Oceanic crust – thinnest part of crust, composed mostly of dense igneous rock known as basalt.Continental crust - thicker than oceanic crust, especially beneath high mountains,

made up mostly of

a less dense igneous rock called

granite.

Earth's crust is made up of several elements: 32% iron

,

30% oxygen, 15% silicon,

14% magnesium, 3% sulfur, 2% nickel

,

and trace amounts of calcium, aluminum and other elements.Slide5
Slide6

First stop – the CRUST

Temperature in the crust…

First 20 meters rock is cool

After that, temperature rises one degree Celsius for every 40 meters in depth. Continues for several kilometers.

Temperature rise slows down to a more steady rate.

At the crust – mantle boundary, temperature is approximately 870 degrees CelsiusThe deeper you go into the Earth, the hotter it gets (temperature increases with depth)Slide7

First stop – the CRUST

Less Pressure in the

crust

…so it

is the least dense

.Pressure - the force pushing on a surface or area Pressure increases with depth, caused by the weight of the rock above. This pressure increase changes the density of the layers of Earth as you move toward the core.Slide8

Next stop – the MANTLE

At a depth between 5 and 40 kilometers beneath the surface

,

you cross a boundary called the Mohorovicic Discontinuity. Above you - the oceanic and continental crust Below you lies the mantle, a layer of hot rock The crust & uppermost part of the mantle are very similar

Together they

form a rigid layer called the

lithosphere

(

lithos

= ‘stone’)

The

lithosphere averages about 100 kilometers in thickness

Lithosphere broken into sections called

tectonic platesSlide9

Next stop – the MANTLE

Beneath the lithosphere, the rock begins to change

Hotter and under increasing pressure (more dense)

Like in the crust, temperature, pressure, & density increase with depth in the mantle Here, with this heat and pressure, rock is less rigid More like road tar softened by the heat of the sun It can bend like plastic This layer is called the asthenosphere (asthenes = ‘weak’) Slide10

Next stop – the MANTLE

The lithosphere floats on top of the asthenosphere

.

It is between

400 and 700 kilometers thick

. Below the asthenosphere, the mantle continues for almost another 3000 kilometers before reaching the solid iron core.Slide11

Final stop – the CORE

FINALLY! The CORE!

Core = the innermost part of the Earth

.

Composed of the metals iron and nickel. Two Parts - liquid outer core and solid inner core. The outer core is a layer of molten metal that surrounds the inner core. This layer is under extreme pressure, but still behaves like a

thick liquid

. Slide12

Final stop – the CORE

The

inner core is a dense ball of solid metal

.

The pressure is so great here that atoms of iron and nickel are squeezed so much that they cannot spread out to form a liquid.

The inner core spins, which generates the Earth’s magnetic field Together, the inner and outer core make up about one- third of Earth’s mass, but only about 15 % of its volume.Slide13

Easy

Peasy

– Can you do it?Slide14

The Earth’s structure can be divided up two different ways.

The first is based on the chemical properties of the layers. As we go deeper toward the core, the chemical elements that make up those layers increase in density. For example, the crust is made mainly of silicate minerals, whereas the core is made of iron and nickel. The silicates are much less dense than the metals.This separation occurred in the very early stages of the Earth’s formation, as heavier elements were pulled by gravity towards the center, and the lighter elements rose to the surface. Slide15

The second way we divide up the Earth is by the

physical properties of the layers, which is controlled by the effects of heat and pressure with depth. The inner core is solid. Even though the temperatures are greatest there, the intense pressure keeps the inner core solid. The outer core, with less pressure, behaves as a liquid due to the intense heat.The mesosphere, or mantle, acts as a highly viscous solid, which means it is capable of flow. Heat from the core rises, causing convection movement in the mantle. More on that later. On top of the mantle is the asthenosphere, a relatively low-viscosity layer on which the lithosphere rides. The asthenosphere behaves like a hot plastic or road tar. The outer component, the lithosphere, is solid and includes the oceanic and continental crust, along with the very uppermost part of the rigid mantle. Imagine a graham cracker on top of pudding. That is similar to how the lithosphere moves on the asthenosphere.Slide16

Snapshots from your trip…

“Moho”Slide17

Snapshots from your trip…

“Moho”Slide18

Snapshots from your trip…Slide19

Moving the plates….Slide20

The engine behind plate tectonicsSlide21

Divergent boundarySlide22

Convergent boundaries

Ocean - Continent

Ocean - Ocean

Continent - Continent