Great Ideas in Science: Lecture 9 – Earth as a Planet Professor Robert Hazen UNIV 301 Great Idea: Earth, one of the planets that orbits the Sun, formed.

Slides:



Advertisements
Similar presentations
Earth science The study of how the earth changes over time Includes:
Advertisements

Solar System Formation – Earth Formation Layers of the Earth Review.
April 18, 2006Astronomy Chapter 13 Cosmic Samples and the Origin of the Solar System What are some of the general patterns in the solar system? What.
Structure & Formation of the Solar System
1. L ist the 9 planets in our solar system. Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto (dwarf planet)
3 rd Grade. The Sun is a star. The Sun is the center of the solar system.
Geology 150 Earth Revealed Introduction. Evolution of the Earth Big Bang – 15 b.y. Solar Nebula Cooling and Condensation of tiny particles Repeat collisions.
THE PRIMORDIAL EARTH Hadean and Archean Eons Solar System Includes: Sun Planets Moons Asteroids Comets.
…and other cool space stuff!. The OUTER PLANETS Mercury Venus Earth Mars The Inner Planets The Outer Planets Jupiter Saturn Uranus Neptune Asteroid Belt.
Solar System 3 rd Grade Katonya Beaubouef. Solar System The sun and all the objects that orbit around it.
Vocabulary.  Our solar system includes the sun, the planets and many smaller objects.
Two Types of Planets. Why do planets look bright? Planets look bright to us because they are reflecting light from the sun. Planets, like satellites,
An Introduction to Astronomy Part VI: Overview and Origin of the Solar System Lambert E. Murray, Ph.D. Professor of Physics.
Seconds Remaining: What makes up the solar system?
The Terrestrial Planets
Formation of the Solar System
Space Ch 3 Notes. Bell Work 2/23/10 Draw a diagram showing the orbit of Earth and the orbit of Earth’s Moon. Label the Sun, Earth, the Moon, Earth’s orbit,
Formation of the Solar System Chapter 27 page 684-
Origin of the Solar System. Stars spew out 1/2 their mass as gas & dust as they die.
Chapter 27 The Solar System.
JOURNAL #17 – THE SOLAR SYSTEM 1.What is the order of the planets from the Sun outward? 2.If during a solar eclipse the moon must be between the Sun and.
Solar Nebula Theory How to make a solar system: 1.Start with nebula = a large cloud of dust and gas. 2.A nearby star explodes (supernova) or the nebula.
Ch 27 Review Planets & the Solar System. Name the inner planets.
Lecture 2: Understanding Earth
Our Solar System Cornell Notes Pg. 77. Our Solar System 8 planets revolve around our sun, as well as many other celestial bodies Heliocentric.
The History of the Earth. Origin of the Universe The universe began about 14.4 billion years ago The Big Bang Theory states that, in the beginning, the.
Lecture Outlines Physical Geology, 14/e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Plummer, Carlson &
The Solar System Chapter 23.
Earth and Other Planets Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great cloud of dust.
The Solar System Science Third Grade The solar system is the sun and the objects that orbit around it.
The Sun The center of our solar system A main sequence yellow star Is powered through Nuclear fusion. A reaction where 2 atoms of Hydrogen are forced together.
Review 2 What was the solar nebula? What was it made of? How did gravitational collapse affect the Solar nebula? How does conservation of energy and angular.
Big Bang theory Parts of our solar system Planet characteristics Galaxies Constellations Nebulas.
Our Solar Neighbourhood “protoplanet hypothesis” = model to explain the birth of solar systems 1. cloud of dust and gas begins to swirl 2. most material.
1.How do supernovas influence the formation of new solar systems? ANS: They provide the material and energy required to form a new Sun, and all the planets,
A Survey of the Solar System. Geocentric vs. Heliocentric.
The Planets and the Solar System
NEW CHAPTER Our Solar System CHAPTER the BIG idea Planets and other objects form a system around our Sun. Planets orbit the Sun at different distances.
Origins of the Planets and Moons Our sun was the center of a nebula (cloud of dust and gas). Planets formed when bits of matter first collided and aggregated.
Week 30 Review The Time for Excellence is Now!. Which tectonic plate is under the starred region? Eurasian.
A Journey to Our Planetary Neighbors
Our Solar System A Write On Activity EARTH AND SPACE SCIENCE Tennessee Standard: Content Standard: 7.0 Earth and Its Place in the Universe The student.
THE CREATION OF THE SOLAR SYSTEM By Gabriella Lopez.
The Earth and Other Planets
Chapter 19: Origin of the Solar System
HOW DID WE GET HERE?? EARTH AND THE ORIGIN OF LIFE.
Standard 1 Objective 2 Study Notes Astronomy 2. 1 _____ is the most likely destination for manned _________ and surface exploration because it has some.
The Inner Planets Chapter Terrestrial Planets Mercury, Venus, Earth, Mars Mostly solid rock with metallic cores Impact craters.
Intro to Our Solar System. Our Solar System Most of the planets in our solar system can be seen without a telescope. Uranus and Neptune are the only two.
The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.
What makes up the Solar System and what force is holding it in place? The Force of Gravity hold our Solar System in Place. Things that make up our Solar.
The Solar System.
NEW CHAPTER Our Solar System CHAPTER the BIG idea Planets and other objects form a system around our Sun. Planets orbit the Sun at different distances.
EXPLAIN THE NEBULAR HYPOTHESIS OF THE ORIGIN OF THE SOLAR SYSTEM. DESCRIBE HOW THE PLANETS FORMED DESCRIBE THE FORMATION OF THE LAND, THE ATMOSPHERE, AND.
Solar system planet gravity telescope comet asteroid meteor meteorite Lesson 3 Splash.
Planetary Chart PlanetAUMassTypeAtmosphereMoons Mercury Venus Earth Mars Inner Planets Jupiter Saturn Uranus Neptune *Pluto.
The Solar System Chapter 29 Review.
Inner Planets Inner and Outer Planets Galaxies Space.
Our Solar System Formed about five billion years ago from a giant cloud of gas and debris Gravity caused Earth and other planets to become layered according.
The Solar System By Gina Wike. Solar System Early Greeks thought that everything centered around the Earth. Copernicus thought differently. He said the.
1 Earth and Other Planets 3 November 2015 Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great.
The Principles of Planetary Geology By: Katie McCormick and Kyle Lennox.
(Textbook pages ) The Outer Planets
The Physical World Chapter 2.
EARLY HISTORY OF THE TERRESTRIAL PLANETS
Earth and Other Planets
Great Ideas in Science: Lecture 9 – Earth as a Planet
Solar System #17.
Notes: Our Solar System
Presentation transcript:

Great Ideas in Science: Lecture 9 – Earth as a Planet Professor Robert Hazen UNIV 301 Great Idea: Earth, one of the planets that orbits the Sun, formed 4.5 billion years ago from a great cloud of dust and gas.

Today: Key Ideas About Earth 1.Earth, one of the planets that orbits the Sun, formed 4.5 billion years ago from a great cloud of dust and gas. 2. The surface of our planet changes constantly; no feature is permanent. 3. The entire Earth is still changing, due to the slow convection of soft, hot rocks deep within the planet. 4. Earth materials move in cycles; a change in one cycle affects others.

Clues to the Origin of the Solar System Solar System = Objects gravitationally bound to the Sun

Clue #1: Planetary Orbits Features of solar system –All planets orbit in the same direction –All planets orbit in the same plane –Most planets rotate in the direction of orbit

Clue #2: Distribution of Mass Almost all mass is in the Sun (99.9%) Two types of planets –Terrestrial planets –Jovian planets Other objects –Moons, asteroids, comets

The Nebular Hypothesis

Terrestrial (Inner) Planets Mercury, Venus, Earth, Mars –Rocky and relatively small –Mercury and Venus too hot for life –Mars may have had life long ago

Terrestrial (Inner) Planets Mars Exploration –Multiple missions –Found evidence of water

Jovian (Outer) Planets Jupiter, Saturn, Uranus, Neptune

Jovian (Outer) Planets Jupiter, Saturn, Uranus, Neptune –Layered structure –No solid surface

Pluto and the Plutoids –Only 0.3% of Earth’s mass –Three moons –Captured comet or asteroid? –Is it a planet?

Asteroids, Comets, and Meteors Asteroids Small rocky bodies Orbit sun Asteroid belt Comets Dirty snowballs Highly elongated orbits Stardust and Deep Impact missions Meteors and Meteorites Meteor showers Original solar system material

The Formation of Earth The Great Bombardment

Differentiation Heat produced from collisions Dense material sank to center Lighter material rose to surface Layered structure –Core –Mantle –Crust

The Formation of the Moon “Big Splash” Large object impacted Earth Parts of mantle blown into orbit Moon formed from this material

The Formation of the Moon “Big Splash”

The Evolution of Earth’s Atmosphere 1.Volcanoes released N 2, CO 2, H 2, & H 2 O 2.Large impacts blew off most atmosphere 3.Hydrogen lost by gravitational escape 4.Living organisms introduced oxygen

Volcanoes and Earthquakes: Evidence of Earth’s Inner Forces Volcanoes: Magma breaks through surface

Volcanoes and Earthquakes: Evidence of Earth’s Inner Forces Earthquakes –Rocks breaks along fault –Energy transmitted as wave –Tsunamis

The Case of the Disappearing Mountains Young Old

Deep Time James Hutton at Jedburgh Scotland ca.1790

Deep Time 1.Sediments 2.Burial 3.Uplift 4.Sediments

Plate Tectonics Great Idea: Earth is constantly changing, due to the slow convection of soft, hot rocks deep within the planet.

Plate tectonics – 6 lines of evidence 1.Physiology: Similar shapes of continents

Plate tectonics – 6 lines of evidence 1.Physiology: Shape of continents 2.Seismology: Earth’s inner structure

Plate tectonics – 6 lines of evidence 1.Physiology: Shape of continents 2.Seismology: Earth’s inner structure 3.Geology: Distribution of rocks and fossils

Plate tectonics – 6 lines of evidence 1.Physiology: Shape of continents 2.Seismology: Earth’s inner structure 3.Geology: Distribution of rocks and fossils 4.Oceanography: Sea floor topography Bruce Heezen and Marie Tharp

Plate tectonics – 6 lines of evidence 1.Physiology: Shape of continents 2.Seismology: Earth’s inner structure 3.Geology: Distribution of rocks and fossils 4.Oceanography: Sea floor topography 5.Volcanology: Ages of Atlantic volcanoes <5

Plate tectonics – 6 lines of evidence 1.Physiology: Shape of continents 2.Seismology: Earth’s inner structure 3.Geology: Distribution of rocks and fossils 4.Oceanography: Sea floor topography 5.Volcanology: Ages of Atlantic volcanoes 6.Paleomagnetismof sea floor rocks

New Support for Plate Tectonics Measurements of the distance between continents North America and Europe are separating at ~5 cm per year

Earth’s Tectonic Plates

Plate Boundaries Three Main Boundary Types – Divergent – Convergent – Transform

Divergent Boundaries

Convergent Plate Boundaries Three Types: 1. Ocean-ocean

Convergent Plate Boundaries Three Types: 1. Ocean-ocean 2. Continent-continent

Convergent Plate Boundaries Three Types: 1. Ocean-ocean 2. Continent-continent 3. Ocean-continent

Transform Plate Boundary

Another Look at Volcanoes and Earthquakes Volcanoes Occur: 1. At Divergent Plate Boundaries 2. Close to Convergent Plate Boundaries 3. Above Hotspots

Another Look at Volcanoes and Earthquakes Earthquakes Occur at: 1.Transform Plate Boundaries 2.Convergent boundaries

Earth’s Geochemical Cycles Earth materials move in cycles; a change in one cycle affects the others. 1. Atoms recycle; they’re used over and over. Reservoirs (Aluminum can) Hydrologic cycle Atmospheric cycle Rock cycle 2. Energy flows through the system.

Geochemical Cycles Account for all the repositories of that substance. Document processes by which the substance moves from repository to another. Gold

ROCK CYCLE: Igneous Rocks Igneous Rocks –Solidify from hot liquid Types –Extrusive rocks solidify at the surface –Intrusive rocks solidify below surface

ROCK CYCLE: Sedimentary Rocks Rocks deposited layer by layer from weathered particles (sand, silt, etc.) or chemicals (i.e., coral).

ROCK CYCLE: Metamorphic Rocks Rocks formed by pressure and heat Examples –Slate –Schist –Gneiss –Quartzite –Marble

Atmospheric Cycle Air mass: Uniform temperature and moisture Weather: State of the atmosphere Climate: Long-term average of weather

The General Circulation of the Atmosphere Circulation powered by Sun –Air heated and rises –Cools and sinks Prevailing winds –Caused by earth’s rotation

Weather Five variables define state of atmosphere –Temperature –Air pressure –Humidity –Cloudiness –Prevailing winds

Climate Gradual change over long periods Influences on climate –Large bodies of water –Ocean currents –Mountain ranges –Position of tectonic plates –Solar output –Greenhouse gases

The Water (Hydrologic) Cycle The total amount of Earth’s water is constant; the same atoms cycle from one reservoir to another Total volume ~ 1.4 billion km 3 Oceans 97.3% Lakes and Rivers 0.01% Groundwater 0.6% Ice Caps & Glaciers 2.1% Atmosphere 0.001% All life %

How does water move among reservoirs?

Ocean Currents Redistribute heat across planet

Ice Ages As the ice caps and glaciers grow, the sea level drops. Cycle tied to Earth’s tilt and orbit

Two facts about water use A human requires about 2 liters of water per day to survive The average American uses about 6,000 liters of water per day

The Water Table The water table will drop when discharge exceeds recharge (like a bank) In the US we “mine” about 100,000,000 gallons of water every day (more than the recharge) Artificial recharge helps Urbanization and pollution hurt