THE UNIVERSE Part 3: Earth and Life.

Slides:



Advertisements
Similar presentations
A journey to the stars.
Advertisements

ASTR Spring 2008 Joel E. Tohline, Alumni Professor 247 Nicholson Hall [Slides from Lecture26]
Structure & Formation of the Solar System
Solar System. What is the Solar System? Consists of a star, (like the sun) and all of the planets, moons and other bodies that travel around it. Planets.
The Evolution of Stars - stars evolve in stages over billions of years 1.Nebula -interstellar clouds of gas and dust undergo gravitational collapse and.
How all the stuff in the solar system was created.
View from the top of the Flatirons (Boulder, CO)
How our Solar System (and Moon) came to be…. Learning Objectives Be able to explain – How our solar system and moon came to be.
Solar Nebula Theory 4:30.
CH 25.5 Solar System Formation
THE LIFE CYCLES OF STARS. In a group, create a theory that explains: (a)The origin of stars Where do they come from? (b)The death of stars Why do stars.
Solar Nebula Hypothesis
Earths Place in the Universe. Standard 2a and 2b Students know the solar system is located in an outer edge of the disc- shaped Milky Way Galaxy, which.
23.1 The Solar System The Solar System.
The Earth and Other Planets
Chapter 20 – The Formation of the Solar System
ACTIVITY 1. For distances to stars and galaxies, astronomers use a unit called a light- year. A light-year is the distance that light travels in a year.
Earth’s Place in the Universe. Cosmology Simply put, the study of the Universe (and everything in it… including us), its origin, present state, and its.
The Solar System Chapter The Solar System 99.85% of the mass of our solar system is contained in the Sun 99.85% of the mass 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?
How was Earth formed?. Big Bang Theory 13.7 billion years ago 13.7 billion years ago Creation of all matter Creation of all matter Hydrogen and Helium.
 There was nothing Billion Years Ago  Energy expanded out from a single point called a singularity.  Really HOT  No matter yet (no atoms)
The Life Cycle of Stars.
Formation of the Solar System Carin Miranda SMS
 A star begins its formation in a cloud of hydrogen and helium gas referred to as a nebula.
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.
FORMATION OF THE SOLAR SYSTEM The Stellar Nebula Hypothesis.
The solar system Topic # 2 Term # 2 The Local System.
Introduction to The Sun Our sun is a star located at the center of our Solar System. It is a huge, spinning ball of hot gas and nuclear reactions that.
Origins and Our Solar System
Nebular Theory of Solar System Formation
Space.
Survey of the Solar System
Our Solar System.
Regular Features of the Solar System
Our Solar System and Its Origin
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.
Looking at the History….of EVERYTHING….
Planet Types Terrestrial Planet Gas Planet Inner Four Planets
Solar System Formation
Formation of a Solar System
How was Earth formed?.
A Note Taking Experience.
Any theory about the origin of the solar system must explain why all of the planets’ orbits lie more or less in a plane and all of the planets orbit the.
Formation of Our Solar System
Chapter 1 Earth Science Review.
Solar System Formation
Mesosaurus: Warm Up: describe what you think this map represents
Origin of the Earth.
Comparative Planetology II: The Origin of Our Solar System
Any theory about the origin of the solar system must explain why all of the planets’ orbits lie more or less in a plane and all of the planets orbit the.
Jeopardy Q $100 Q $100 Q $100 Q $100 Q $100 Q $200 Q $200 Q $200
Origin of the Universe.
The Life Cycle of a Star.
The Earth.
Jupiter’s Interior:.
3A Objectives Describe the nebular theory in detail.
Section 1: Formation of the Solar System
The Solar System.
Do-NOW 9/23 PLEASE COLLECT YOUR INBS FROM THE BOTTOM SHELF!
Earth’s Structure and Motion
NEBULAR THEORY.
Stellar Evolution Chapter 30.2.
Star Formation CH. 5.
Do Now: What do you already know about the different kinds of planets in our solar system? Do you already know something specific about them? Write.
Topic # 2 Term # 2 The Local System
04/07/2019 The Earth and Beyond.
Celestial Objects in Space
Presentation transcript:

THE UNIVERSE Part 3: Earth and Life

Earth & Life Our solar system was once a large cloud of gases and heavy metals. This suggests that our region of space was once the host of another star that underwent a supernova. Gradually, over time, these gases and heavy metals began to collide and form a protostar. This protostar would eventually become our Sun, paving the way for the formation of our solar system

Earth & Life The solar system forms in four stages: The gas and metal cloud begins to collapse and spin The speed of rotation allows some material to collide and form a protoplanetary disk The material in this protoplanetary disk begins to clump together and form the planets The protostar undergoes the transformation into the sun as gravitational force increases

Earth & Life Not all planets in our solar system are the same structurally. We place the planets into two classes: Rocky Planets Gas Giants

Earth & Life Rocky planets, true to their name, consist of a series of rocky layers. The core of these planets is very dense due to the effects of…………… pulling in heavier metals. Gradually, the outer layers become less dense until you reach the outer mantle and crust. The mantle is composed of light silicon based rocks, while the crust is composed of lighter elements such as sodium, aluminium and magnesium.

Earth & Life Gas Giants differ from rocky planets in that their layers are primarily composed of gaseous and liquid gas elements such as hydrogen and helium. The core of these planets is very dense, composed of some rocky elements and metallic hydrogen Large amounts of liquid hydrogen and helium compose the middle layer, while the outer layer is composed of gaseous hydrogen and helium.

Interestingly, our planet is perfectly tailored to supporting human life…

Earth & Life But how did life first begin on our planet? Several different theories for the origins on life have been put forward… Abiogenesis Panspermia

Earth & Life Abiogenesis is the process where, under prehistoric conditions, elements such as hydrogen, carbon and oxygen were subjected to electrical voltages in the form of lightning to generate the building blocks of life. These included Amino Acids and Carbohydrates.

Earth & Life Panspermia is the theory that life on our planet developed from organisms that ‘arrived’ here on top of asteroids. These organisms, also known as tardigrades, were extremely resilient, allowing them to survive the vacuum of space. Eventually, these organisms would evolve to give those that we know today

Earth & Life The atmosphere of the earth is perfectly suited for sustaining life The earth’s orbit around the sun places it in a habitable zone The earths tides allowed prehistoric organisms to adapt to living on land Important elements in our atmosphere help to drive metabolic reactions in organisms