Earth's Composition and Structure PDF

Summary

This document explores Earth's composition and structure, discussing topics ranging from Earth's surface to its interior layers. It also presents information on the Earth's atmosphere, magnetic field, and the solar system. The content touches upon various elements, convection, and the role of seismic waves in understanding Earth's interior.

Full Transcript

Earth’s Composition and Structure: A Journey to the Center of the Earth Earth’s Surface Our experience with Earth is limited to its surface. Yet Earth has a complicated interior. Earth is characterized by… – An internally generated magnetic fie...

Earth’s Composition and Structure: A Journey to the Center of the Earth Earth’s Surface Our experience with Earth is limited to its surface. Yet Earth has a complicated interior. Earth is characterized by… – An internally generated magnetic field. The Black Canyon of the Gunnison, CO – A layered interior Solid and liquid layers. – A gaseous envelope. i.e. atmosphere The Solar System Human perceptions have changed. – Early history – Planets as moving lights. – 1600s – 1st telescopes saw hazy spheres. – Today – A complex, evolving system. – Structure – History Space probes have photographed and analyzed planets. Scientists have hypothesized likely origins of the solar system. Earth and the Solar System What would solar system visitors notice? – Magnetic field. – Atmosphere. – Surface features. Continents. Oceans. Polar ice caps. Evidence of humanity? – Structures. » Dams. » Great Wall of China. » Cities. » Roads / canals. – Electric lights. The Celestial Neighborhood Interstellar space: a ~vacuum with a virtual absence of matter. The amount of matter greatly increases approaching the Sun. The Sun ejects matter outward into space as the solar wind. Solar wind: – Magnetically & electrically charged particles. – Stream outward in all directions. – Consists of… Protons (+ charge). Electrons (– charge). Only a small percentage of the solar wind impinges upon Earth. Five Key Characteristics About Earth’s Structure: 1. Earth has a dipole magnetic field that deflects solar wind and protects earth’s surface from solar radiation 2. Earth has a stratified atmosphere, mainly composed of nitrogen (N2) and oxygen (O2) 3. Earth is made of a variety of minerals, glasses, melts, fluids and volatiles, all left behind during birth of the solar system 4. The Earth has layers: a thin silicate crust, a thick iron- & magnesium silicate mantle, and a thick metallic core 5. Physically, the earth can be divided into a rigid outer lithosphere and a plastic/ductile asthenosphere Earth’s Magnetic Field Geodynamo - The Earth’s magnetic field is produced by the geodynamo -Flow in the liquid iron outer core creates a magnetic field Magnetic field - region affected by force emanating from a magnet - grows stronger as separating distance decreases - attracts or repels magnetically charged or moving electrically charged objects - compasses work because Earth is a large magnet Earth’s Magnetic Field Magnetic field - Like a bar magnet, Earth’s magnetic field is a dipole, (has both a N and S pole) - Solar wind contains electromagnetic particles that are deflected by earth’s field. These particles distort the shape of earth’s magnetic field in space - Van Allen belts – two belts in the inner magnetic field where high energy cosmic rays are trapped. Protects us from solar radiation! Northern & Southern Lights Form because of our dipole magnetic field! Aurorae Some ions escape Van Allen belts. – These ions are pulled to the magnetic poles. – The ions create light in the upper atmosphere. Spectacular aurora follow solar flares. – Aurora borealis – Northern lights. – Aurora australis – Southern lights. Earth’s Atmosphere Distinct layers of gas surround the solid portion of the earth. o Composition is ~uniform regardless of altitude o 78% N2 o 21% O2 o All others ~1% o Ar, CO2, CH4, H2O, Ne, CO, SO2 o Some other Planets have atmospheres too! o None have N2 & O2 as dominant gasses o Earth was oxygen-free until ~2.5 Ga Earth’s Atmosphere o Pressure decreases with increasing altitude o Reflects # of molecules/volume o Lower pressure = less molecules/volume o Air pressure @ sea level = 14.7 lb/in2 = 1 bar o Pressure is caused by the weight of overlying material o Upper atmosphere has less material above it o Pressure is lower o 99% of atmosphere is below 50 km, the rest is between 50 and 500 km. Earth’s Atmosphere o Earth’s Atmosphere is divided into distinct layers based on altitude o Exosphere (very thin ~500 km) o Atmosphere merges with space o Thermosphere (>90 km) o Where space shuttles orbit o Mesosphere (50-90 km) o Meteors burn up here o Stratosphere (12-50 km) o Stable air; good for jets o Tropopause (11-12 km) o Troposphere (0-11 km) o Mixing layer o All weather is limited to this layer o “Tropo” = Greek for “turning” Earth’s Atmosphere o Troposphere o A well-mixed layer dominated by convection of air masses o Convection o Method of heat transfer in a fluid o Think lava lamp! o Cold is more dense = sinks o Hot is less dense = rises o This process results in circular convection cells o Also causes pressure gradients which create wind! o Also applies to the interior of the Earth …this guy likes convection Earth’s Components o Earth’s surface = ~30% land, ~70% water o unlike any other known planet o Hydrosphere = includes oceans, lakes, seas, rivers, & groundwater o Cryosphere = glaciers, snow, and sea ice o Earth’s surface is not flat; it has topography o Ignoring oceans, Earth’s surface is dominated by two distinct elevations: o Most land is 0-2 km above sea level o Most of the sea floor is 3-5 km below sea level Earth’s Components o Earth’s elemental composition reflects mostly heavier elements not blown away by solar wind during formation of the solar system o Most abundant elements o Fe, O, Si, Mg o Most common minerals consist 35% of silica (SiO2) mixed in varying proportions with other elements such as Fe, Mg, Al, 30% 10% Ca, K, Na o Felsic = more silica (less Fe/Mg) 10% & less dense o E.g. Granite o Mafic = less silica (more Fe/Mg) 15% & more dense Bulk Earth composition o E.g. Gabbro / Basalt o Range: Felsic / Intermediate / Mafic / Ultramafic Earth Materials Elements combine in a variety of Earth materials. – Organic compounds – Carbon-containing compounds. Most are residue from once-living creatures. Include wood, peat, lignite, coal, and oil. Geologically rare (decomposes in contact with oxygen). Earth Materials Elements combine in a variety of Earth materials. – Minerals – Inorganic crystalline solids. Comprise rocks and, hence, most of the Earth. Most rocks on Earth are silicates (based on Si and O). – Glasses – Non-crystalline mineral-like matter. Cool too quickly to form structure – Rocks – Aggregates of minerals. There are many types. Igneous – Cooled from a liquid (melt). Sedimentary – Debris cemented from pre-existing rock. Metamorphic – Rock altered by pressure and temperature. Earth Materials Metals – Solids made of metallic elements. Melts – Rocks that have been heated to a liquid. – Magma – Molten rock beneath the surface. – Lava – Molten rock at the surface. Volatiles – Materials that turn into gas at surface temps. – H2O, CO2, CH4, and SO2 – Volatiles are released from volcanic eruption. A Layered Earth We live on the thin outer skin of Earth. Early perceptions about Earth’s interior were wrong. – Open caverns filled with magma, water, and air. – Furnaces and flames. We now know that Earth is comprised of layers. – The Crust. – The Mantle. – The Core. Outer Core. Inner Core. Some basic rules of physics give some clues… From Milton’s “Paradise Lost” Earth’s Density Earth’s Density gives us clues about its internal structure Density = Mass/Volume Measures how much mass is in a given volume. Expressed in units of mass/volume e.g. g/cm3 Ice floats…why? Estimates of earth’s mass and volume give a whole earth density of ~5.5 g/cm3 Typical rocks at the surface of the Earth have a density of 2.0-2.5 g/cm3 What does this require of the density of material in the Earth’s interior? Earth’s Density Earth’s shape as a clue to the internal structure of the Earth If density increased gradually and uniformly towards the center, a significant portion of Earth’s mass would be near the outer edges…. Then centrifugal force (not centripetal) would cause the planet to flatten into a disk. This has (obviously) not happened… Earth’s Layers Earth’s shape as a clue to the layering of the earth If the Earth consisted of a thin solid shell over a thick liquid center, then the surface would rise and fall with tides like the ocean – This does not happen; only the oceans rise and fall. Thus, the Crust does not float over a liquid interior A Layered Earth Earthquake clues - Earthquake energy transmitted as seismic waves that pass through Earth. – Seismic waves have been used to probe the interior. Wave velocity changes with density. Velocity changes give depth of layer changes. Changes with depth. – Pressure. – Temperature. More on this in Chapter 10 and Interlude D! Earth’s Interior Layers The Earth (and other planets) have layered interiors. – Crust Continental Oceanic – Mantle Upper Lower – Core Outer – Liquid Inner – Solid © W. W. Norton The Crust The outermost “skin” of Earth with variable thickness. – Thickest under mountain ranges (70 km – 40 miles). – Thinnest under mid-ocean ridges (3 km – 2 miles). The Mohorovičić discontinuity or “Moho” is the lower boundary. – Separates the crust from the upper mantle. – Discovered in 1909 by Andrija Mohorovicic. – Marked by a change in the velocity of seismic P waves. Two Types of Crust Continental crust – Underlies the continents. – Avg. rock density about 2.7 g/cm3. – Avg. thickness 35-40 km. – Felsic composition. Avg. rock type = Granite Oceanic crust – Underlies the ocean basins. – Density about 3.0 g/cm3. – Avg. thickness 7-10 km. – Mafic composition Avg. rock type = Basalt/Gabbro Two Types of Crust Crustal density controls surface position. – Continental crust Less dense; “floats higher.” – Oceanic crust More dense: “floats lower.” Crustal Composition 98.5% of the crust is comprised of just 8 elements. Oxygen is (by far!) the most abundant element in the crust. – This reflects the importance of silicate (SiO2-based) minerals. – As a large atom, oxygen occupies ~93% of crustal volume. Bulk Earth Composition 35% 10% 30% 10% 15% Earth’s Mantle Solid rock layer between the crust and the core. 2,885 km thick, the mantle is 82% of Earth’s volume. Mantle composition = ultramafic rock called peridotite. Below ~100-150 km, the rock is hot enough to flow. It convects: hot mantle rises, cold mantle sinks. Three subdivisions: upper, transitional, and lower. The Core An iron-rich sphere with a radius of 3,471 km. 2 components with differing seismic wave behavior. – Outer core Liquid iron-nickel-sulfur 2,255 km thick Density – 10-12 g/cm3 – Inner core Solid iron-nickel alloy Radius of 1,220 km. Density – 13 g/cm3 Flow in the outer core generates the magnetic field. Lithosphere-Asthenosphere The Crust, Mantle, Core boundaries – defined by composition …but sometimes we want to divide the layers of the Earth by their behavior or physical properties Lithosphere – The brittle portion of Earth’s interior. – Behaves as a non-flowing, rigid material. – The material that moves as tectonic plates. – Made of 2 components: crust and upper mantle. Asthenosphere – The ductile portion of Earth’s interior. – Shallower under oceanic lithosphere. – Deeper under continental lithosphere. – Flows as a soft solid. Boundaries Between Layers The Crust-Mantle boundary = Moho – defined by seismic discontinuity indicating significant change in composition. Lithosphere-Asthenosphere boundary = Brittle-ductile transition – Defined by a significant change in rock physical properties (viscosity) – Also defined as the depth below which earthquakes do not occur. Lithosphere ≠ Crust

Use Quizgecko on...
Browser
Browser