Bell Ringer! What objects in the night sky did Hubble look at to see the red shift that gave us evidence for an expanding universe? What rule did Hubble.

Slides:



Advertisements
Similar presentations
Olber’s paradox Why isn't the night sky as uniformly bright as the surface of the Sun? If the Universe has infinitely many stars, then it should be uniformly.
Advertisements

The Life-Cycle of a Star
Dark Matter. Either dark matter exists or we do not understand how gravity operates across galaxy-sized distances. We have many reasons to have confidence.
Life Cycle of a Star.
Thursday, April 8 th Agenda  Finish Section 18.1: The Universe  Origin of the universe, red shift, big bang theory  In-Class Assignments Section 18.1.
Dark Energy. Conclusions from Hubble’s Law The universe is expanding Space itself is expanding Galaxies are held together by gravity on “small” distance.
Newton’s Hypothesis The universe is infinite, static and uniform. Proven to be incorrect by Olber’s Paradox. Olber theorised that if this was correct then.
The Big Bang Theory (Part III) The End of it All Mike Stuckey Warren East High School.
The Age of the Universe. The universe is expanding !!  The visible universe is made up of clusters of stars, held together in galaxies by their mutual.
Objectives Distinguish the different models of the universe.
What is the Lifecycle of a Star? Chapter Stars form when a nebula contracts due to gravity and heats up (see notes on formation of the solar system).
Review for Exam 3.
Stars start out as a Nebula –
30.3 Big Bang Theory. Doppler Effect Doppler effect = apparent shift in the wavelengths of energy emitted by an energy source moving away from or towards.
Cosmology. Some important questions Did the universe have a beginning or has it always existed? Will the universe end? If it ends, what will happen at.
The Universe Pictures by the Hubble Space Telescope.
Bell Ringer 8/25 You may write this week’s bell ringers on the same paper as last week’s bell ringers, just be sure to include the correct DATE!! In your.
Stellar Life Stages Star Birth and Death.
Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe
A black hole is a region of space with such a strong gravitational field that not even light can escape.
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
Astrophysics Cosmology - the study of the nature of the universe.
Cosmology Olber’s Paradox Big Bang Development of the Universe.
Introduction to Cosmology. Types of Universes If you were to make a universe, would you give it a finite size, or make it infinite? In a finite universe,
How It All Began…. Chapter 1: The Big Bang Chapter 2: The Galaxies Chapter 3: The Fate of the Universe.
Dark Energy. Expanding Universe Galaxies in the universe are spreading out over time. –Hubble’s law From Einstein’s general relativity this happens as.
Chapter 12 Space Exploration. Section 12.1 page 428 Explaining the Early Universe GALAXY – collection of stars, planets, gas and dust held together by.
Stars. Before the first star  Early Universe, Matter is cooling  Finally Forms first atoms - H  This is 400,000 years a.b.b.  Early Universe, Matter.
The Big Bang Theory. Warm Up: Use your textbook on page 532 to describe the Big Bang Theory. What are 2 pieces of evidence for the Big Bang Theory?
THEORIES OF UNIVERSE FORMATION. Studying Space Cosmology – the study of the origin, structure, and future of the universe Astronomers study planets, stars,
A Note Taking Experience.
Olber’s Paradox Why is the night sky dark?. Night Sky.
Origins of the Universe. How did it all get here? How did it all get here? MANY THEORIES!!!! MANY THEORIES!!!! Big Bang Theory Big Bang Theory Steady.
The Life Cycle of Stars. Cycle for all stars Stage One- Born in vast, dense clouds of gas, mostly hydrogen along with small amounts of helium, and dust.
Bell Ringer 10/13 Why do we celebrate Columbus Day?
Cosmology- the study of the origin, evolution and composition of the universe.
Earth, Stars, and the Universe Earth tends to be hotter at the equator because the sun’s energy is perpendicular to the earth and therefore more concentrated.
The UniverseSection 3 Section 3: Origin of the Universe Preview Key Ideas Bellringer What Is the Universe? What Happened at the Beginning? Predicting the.
The Shape and Fate of the Universe Assumptions in cosmology Olber’s paradox Expansion of the Universe Curvature of the Universe Fate of the Universe.
Cosmology. Formation of a Star 1.Stars form from clouds of interstellar dust and gas, which consist mainly of the elements hydrogen and helium. 2.Where.
The life and death of stars Stars take millions of years to form. They then go through a stable period in their life and finally they die. Sometimes in.
Black Holes and Gravity 1)Type II Supernova 2)Neutron Stars 3)Black Holes 4)More Gravity April 7, 2003
Life Cycle of a Star Notes Write in Cornell Notes format.
AQA Science © Nelson Thornes Ltd P3 4 Summary Stars and space Corel 768 (NT)
The Expanding Universe  When light or sound moves toward or away from an observer, its frequency/wavelength changes (Known as Doppler effect)  Can be.
The Origin of the Universe Chapter 20.3 Notes. What is the Universe? The universe consists of all space, matter, and energy that exists—now, in the past,
Milky Way Galaxy. Galaxy A group of stars, dust and gases held together by gravity. 170 billion galaxies in the universe 200 billion stars in a galaxy.
The life cycle of a star u All stars go through four main stages u Nebulae u Protostar u Main sequence u Red giant.
Stars  To understand the life cycle of stars Thursday, June 23, 2016.
© 2010 Pearson Education, Inc. Chapter 14 Dark Matter and Dark Energy.
All existing matter and space considered as a whole; the cosmos believed to be at least 10 billion light years in diameter and contain a vast number of.
Lives of Stars.
Life Cycle of Stars Objectives
Astrophysics and Cosmology
Stars change over their life cycles.
The Big Bang The Big Bang
THE EXPANDING UNIVERSE
8 Space physics Topic overview
A Note Taking Experience.
Life Cycle of Stars 1st Step: Stars form from nebulas
dark matter and the Fate of the Universe
Origin of Universe Universe…all the space, time, energy and matter that exists Because things are so far from Earth, and light takes so long to travel.
Life Cycle of a Star.
Stars, Galaxies, and the Universe
The Universe.
The Big Bang The Big Bang
Theories of Universe Formation
Absorption lines of a galaxy shift toward the blue end of the spectrum when it moves toward Earth. The lines shift to the red end of the spectrum when.
The study of the origin and nature of The Universe
Presentation transcript:

Bell Ringer! What objects in the night sky did Hubble look at to see the red shift that gave us evidence for an expanding universe? What rule did Hubble come up with about a object’s movement in space?

Is the Universe Expanding Forever? It is not known whether the universe will continue expanding. Two opposing forces govern the expansion: the momentum of expansion outward, and the force of gravity inward.

Astronomers can determine the mass of objects they can see, but this total would not include objects that are difficult to see. Objects like white dwarves, black holes and other dead stars do not emit much light, but can be very massive. The existence of dark matter cannot be seen and the mass cannot be calculated. Until astronomers can better determine the mass of the universe, they will not know how strong the inward pull of gravity is.

Three Fates of the Universe Astronomers have calculated the amount of mass needed to exactly balance the expansion, called the critical density. What happens to the expansion depends on whether the true average density of the universe is equal to, higher than, or less than the critical density.

Fate 1: Open Universe If the average density is less than the critical density, gravity will not be strong enough to stop the expansion, creating an open universe.

Fate 2: Closed Universe If the average density is more than the critical density, gravity will slow down and eventually reverse the expansion, creating a closed universe.

Fate 3: Flat Universe If the average density is equal to the critical density, gravity will balance the expansion and the universe will reach a stable size, creating a flat universe. This is also called the Inflationary Model because the universe expanded at first and the reached a maximum size.