A Short Look at Earth History. Formation of Sun Formation of Universe: 13 billion years Formation of Galaxy: 11 billion Years Formation of Solar System:

Slides:



Advertisements
Similar presentations
Big Bang to Earth's Formation Concept Map
Advertisements

Planets of the Solar System The Moon and Other Bodies
Solar System.
Planet Earth.
Lesson9a - Formation Comets and their effect.
The Universe. The Milky Way Galaxy, one of billions of other galaxies in the universe, contains about 400 billion stars and countless other objects. Why.
Introduction To Physical Geology. The Science Geology is typically broken up into two fields of study –Physical Geology –Historical Geology.
The Terrestrial Planets Astronomy 311 Professor Lee Carkner Lecture 9.
A Short Look at Earth History The big perspective of ‘us in the universe’ E&ES 199.
1 Chapter 2 Creation of Oceans. 2 Supporting Evidence for the Big Bang Edwin Hubble discovered spreading of galaxies. Cosmic background radiation (the.
Astro 10-Lecture 6: Formation and Structure of the Solar System What are the properties of the solar system? How are these properties explained by theories.
The Solar System.
How our Solar System (and Moon) came to be…. Learning Objectives Be able to explain – How our solar system and moon came to be.
An Introduction to Astronomy Part VI: Overview and Origin of the Solar System Lambert E. Murray, Ph.D. Professor of Physics.
Origin of the Solar System. Stars spew out 1/2 their mass as gas & dust as they die.
Solar System.
Formation of the Solar System
Our Solar System.
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.
Astronomy 100: Formation and Structure of the Solar System What are the properties of the solar system? How are these properties explained by theories.
Chapter 27 The Solar System.
Chapter 27: Planets of the solar system
What Do You Know about our Solar System???. Is Pluto bigger, smaller or the same size as the Earth's moon? a) Smaller b) Bigger c) The same size MOON.
CH 25.5 Solar System Formation
Copyright © 2014 All rights reserved, Government of Newfoundland and Labrador Earth Systems 3209 Unit: 1 Introduction to Earth Science – The Evolution.
Survey of the Solar System
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.
Formation of The Earth. Composition of the Sun The Most Unusual Element Administratium (Ad) No protons: Atomic Number Zero One neutron 27 Assistant neutrons.
Hadean Eon & the formation of Earth
Earth and Space Science Mrs. Jones Science Class.
Formation of Our Solar System Modified presentation originally created by the Lunar and Planetary Institute Image: Lunar and Planetary Laboratory:
Chapter Four The Moon: The Earth’s Closest Neighbor.
Unit 2 THE PLANETS BY MRS. D FOR ELL STUDENTS. What is the Milky Way?  The Milky Way is galaxy that contains our solar system.
Survey of the Solar System. Introduction The Solar System is occupied by a variety of objects, all maintaining order around the sun The Solar System is.
23.1 The Solar System The Solar System.
 Formation of Universe: billion years  Big Bang Theory  Formation of Galaxy: 11 billion Years  Formation of Solar System: 4.6 billion years.
The Origin of the Solar System. In the beginning, we started out looking like this, just a huge cloud of gas in space….
A Short Look at Earth History. Formation of Sun Formation of Universe: 13 billion years Formation of Galaxy: 11 billion Years Formation of Solar System:
Rare Earth Hypothesis That occurrence of Earth-like planets with complex life forms in the universe is rare. So many geologic and astronomical conditions.
Chapter 4 Exploring Our Evolving Solar System. Comparing the Planets: Orbits The Solar System to Scale* – The four inner planets are crowded in close.
HOW DID WE GET HERE?? EARTH AND THE ORIGIN OF LIFE.
Comparative Planetology II: The Origin of Our Solar System Chapter Eight.
The Sun is our closest star. Is a member of the Milky Way galaxy. Is a medium size star and it’s a class G2. It is believed to be about 4.6 billion.
Formation of the Solar System. The Age of the Solar System We can estimate the age of the Solar System by looking at radioactive isotopes. These are unstable.
Planets of the Solar system Section 4 Key Ideas Identify the basic characteristics that make the outer planets different from terrestrial planets. Compare.
© 2016 Cengage Learning. All Rights Reserved. 1 Oceanography, An Invitation to Marine Science | 9e Tom Garrison The Origin of the Ocean.
Formation of Our Solar System
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.
CH 25.5 Solar System Formation Objectives: How did our solar system form? What evidence supports our ideas?
The Planets Mrs. Cothery’s 7 th grade class. The Solar System  Our solar system is made up of eight individual and unique planets and is nearly five.
 There was nothing Billion Years Ago  Energy expanded out from a single point called a singularity.  Really HOT  No matter yet (no atoms)
Chapter 27 Formation of the Solar System The sun and all of the planets and other bodies that revolve around the sun.
Fig. 2-CO, p. 40. Fig. 2-1, p. 41 Fig. 2-2, p. 42.
Planets of the Solar System Section 1 Section 1: Formation of the Solar System Preview Key Ideas The Nebular Hypothesis Formation of the Planets Formation.
27-1OBJECTIVES Explain the nebular hypothesis of the origin of the solar system Describe how the planets formed Describe the formation of the land, the.
Solar System PowerPoint By Kayley. Stars and our Sun A star is a huge ball of gas that is very hot and that gives off heat, light, and other energy that.
Origin of the Universe  Where did Earth, the solar system, & the stars come from? Where did life come from?  Our universe came into existence suddenly.
EARTH’S FORMATION. UNIVERSE The Universe Organization: Organization: Universe Universe Galaxies Galaxies Stars Stars Solar Systems Solar Systems Planets.
EARTH’S FORMATION.
Survey of the Solar System
Over geologic time, oceans formed, continents grew due to constructive and destructive forces, and the composition of the atmosphere changed. The.
Chapter 9.
The study of everything on and in the Earth (including the oceans and the atmosphere), and everything outside of it (the universe). - four major branches.
Formation of a Solar System
Section 1: Formation of the Solar System
Mesosaurus: Warm Up: describe what you think this map represents
Notes: Our Solar System
Origins of the Earth, Oceans, and Life
Section 1: Formation of the Solar System
Presentation transcript:

A Short Look at Earth History

Formation of Sun Formation of Universe: 13 billion years Formation of Galaxy: 11 billion Years Formation of Solar System: 4.6 billion years Sun is probably a third generation star Probably takes million years for planets to form

Formation of Planets Planets made of same material as Sun, minus elements that remain mostly in gases Inner Rocky Planets: iron and magnesium silicates Outer gas giants and moons: water ice If a protoplanet gets big enough, it can hold everything (Jupiter, Saturn) Very far from sun: methane, ammonia, nitrogen ice

Our Solar System May Not Be Typical Over 200 extrasolar planets known Barely can detect Jupiter-size planets, don't yet have technology to see small planets Many have very eccentric orbits Some have gas giants very close in to sun ("hot Jupiters")

Formation of Earth Planets formed by accretion of smaller objects = impact Very tiny objects hold together by atomic forces Objects kilometers across hold together by gravity How do objects the size of a refrigerator hold together? As planets get bigger, gravity gets stronger, impacts get more violent Big impacts throw out ejecta, trap heat Magma ocean Formation of core early in earth history as iron sinks

Formation of Moon It's very hard to account for the Moon: –Very big compared to its parent planet –Orbits nearly in plane of earth's orbit, not over equator. Co-creation with Earth? Fission? Capture?

Collision A collision takes no finesse at all Can explain why moon orbits in earth's orbital plane Can explain why moon's composition differs from earth Models of solar system evolution suggest that last stage is mega-collisions Impact would have melted most of earth and moon Earth would have been incandescent for about 10,000 years.

Unstable Early Earth May have been several moon-forming events 1000-km impactors can melt crust 100-km impactors create temporary atmosphere of vaporized rock, vaporize oceans Life not possible until large impacts cease To have life on Earth, we need Jupiter? –Sweeps up debris and reduces impacts –Stabilizes orbits of other planets To have life on Earth, we need Moon? –Stabilizes changes in earth's axis tilt

Conditions on Early Earth Oldest existing earth materials: 4.1 billion years old Oldest rocks: 3.9 billion years old Oxygen-poor atmosphere (present oxygen is created by life) Faint Early Sun: perhaps 30 per cent less bright Evidence for liquid water from very early on Atmosphere and sun must have evolved in tandem Carbonate-Silicate Cycle: life not essential but liquid water is.

Life What Is It? "Life is what dies when you stomp on it"-- Dave Barry A self-replicating chemical system

How Did Life Originate? Certainly not as complex as anything now alive Lots of candidates for first self-replicators Role of minerals as catalysts and templates? Simplest organisms are extremophiles At least since 3 billion years, probably much earlier

Major Events in the History of Life Oxygen levels in atmosphere –Plants release waste oxygen –Eventually organisms developed a way to utilize oxygen Sex: Who Needs It? We are a team: Mitochondria Snowball Earth: what survived and how? Cambrian "Explosion"

Mass Extinctions

Causes ? Climate Change Disease Mountain-building Sea Level Change Competing Organisms Over-specialization Volcanism Meteor Impact

Average Global Temperature

Plate Tectonics Very early earth may have had thin, unstable crust Large areas of continental crust existed by 2.5 billion years Plate tectonics since at least two billion years Wilson Cycle and Supercontinents –Supercontinents –Dispersal –Reassembly –Rodinia 800 million years –Pangaea 250 million years

Humans Australopithecus > 2 m.y. Homo erectus 1-2 m.y. Homo ergaster 1-2 m.y. Homo habilis < 1 m.y. Homo neanderthalensis 500,000-30,000 yr. Homo sapiens<100,000 years

Earth History e=related