Physics of the Cosmos Sections 37.4 – 37.5. Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL:

Slides:



Advertisements
Similar presentations
E4 Cosmology. Newton’s Universe Infinite (in space and time) Static.
Advertisements

E4 Cosmology. Newton’s Universe Infinite (in space and time) Static.
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.
OPTION E - ASTROPHYSICS E4 Cosmology Olber’s Paradox.
Origin & Evolution of the Universe
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 Evidence for the Big Bang Student Resource Sheet 5 Science and Religion in Schools: Unit 4a.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 22 "In the beginning the Universe was created. This has made a lot of people very angry and been.
Cosmology Past, present and future of the universe Is space flat or curved? Where is the center? What lies beyond our limit of vision? What is the universe.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 22 "In the beginning the Universe was created. This has made a lot of people very angry and been.
Cosmology Astronomy 315 Professor Lee Carkner Lecture 24.
The Big Bang Astrophysics Lesson 18. Learning Objectives To know:-  What is the big bang theory  What is the evidence supporting it including:-  Cosmological.
History of the Universe. If the universe was 1 year old...
Why is the sky dark at night? Distant galaxies are receding from us with a speed proportional to distance.
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.
UNIT NINE: Matter and Motion in the Universe  Chapter 26 The Solar System  Chapter 27 Stars  Chapter 28 Exploring the Universe.
Contemporary science issues Lesson 16: Has the universe always been there? © 2006 Gatsby Technical Education Projects.
Theory on the Formation of the Universe
Cosmology The Origin and Future of the Universe Part I Olbers’ Paradox.
Professor Martin Hendry University of Glasgow.
Expansion of the Universe Natural consequence of the basic field equations of the General Theory of Relativity (GTR) When GTR was first developed in the.
Astrophysics Cosmology - the study of the nature of the universe.
Cosmology Olber’s Paradox Big Bang Development of the Universe.
Stars – Temperature Hotter objects emit shorter wavelengths Cooler objects emit longer wavelengths –Ex. Sun is a “medium hot” (5800 K or about 5500 C)
Physics of the Cosmos Secs Reminders Lab D1-LFA: Light from Atoms due 4 (this will be the last lab for the semester) In-class Quiz.
Exploring the Universe
CO-The Big Bang Theory LO-Describe the events leading to the formation of the Universe. 1.
The Big Bang Theory Not this one…. The Theory The Big Bang describes how: – a massive explosion created the universe – the cooling and expansion of.
The Expanding Universe. The Hubble Law The Hubble constant H o is one of the most important numbers in cosmology because it may be used to estimate the.
The Universe and Galaxies The universe is vast in size and very very old.
Welcome to Astronomy!. Prove that the following equation is valid by means of resolution:  xp(x)v  xq(x)   x  p(x)vq(x)  Why can ’ t you do this.
Our Universe. The universe is everything that exists including all matter and energy The universe is 13.7 billion years old. No one knows if the universe.
Galaxy Formation and the Hubble Law Assigned reading: Chapter 16 REMINDER: HW7 due Monday, plus Quiz.
The Expanding Universe
THE BIG BANG THEORY The Expanding Universe. Review Human demonstration.
Evidence for the Big Bang Theory Christianity, Science & Belief.
The UniverseSection 3 Section 3: Origin of the Universe Preview Key Ideas Bellringer What Is the Universe? What Happened at the Beginning? Predicting the.
Key Areas covered The temperature of stellar objects is related to the distribution of emitted radiation over a wide range of wavelengths. The wavelength.
The Expanding Universe  When light or sound moves toward or away from an observer, its frequency/wavelength changes (Known as Doppler effect)  Can be.
s/redshift.
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,
Astronomy: Big Bang EQ: How did the universe begin? ** Copy all pink and yellow words. p. 89.
Option D. 3. Universe was born around 13.8 billion years ago in process called Big Bang In the beginning, all matter & energy in the entire universe was.
The Big Bang Theory.
Types of Stars (review)  Cepheid variables Cepheid variables are stars of variable luminosity. The luminosity increases sharply and falls of gently with.
© 2017 Pearson Education, Inc.
The Science of Creation
The Science of Creation
Key Areas covered The temperature of stellar objects is related to the distribution of emitted radiation over a wide range of wavelengths. The wavelength.
The Big Bang The Big Bang
BIG BANG THEORY.
The Science of Creation
Stars Notes Ch. 28.
Cosmology.
Expansion of the Universe
Astronomy-Part 2 Notes Origins of the Universe
Big Bang.
Contemporary science issues
Cosmology.
The Universe A journey through time.
Physics of the Cosmos.
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.
Physics of the Cosmos.
The Big Bang Theory Picture is a gamma burst—there are obviously no pictures of the Big Bang, but we can imagine what it looked like.
Key Areas covered The temperature of stellar objects is related to the distribution of emitted radiation over a wide range of wavelengths. The wavelength.
The Big Bang The Big Bang
Cosmology.
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.
A galaxy like the Milky Way contains about 10 billion stars.
BIG BANG THEORY.
Presentation transcript:

Physics of the Cosmos Sections 37.4 – 37.5

Reminders Today: In-class Quiz #6 addressing Chapter 37 and questions from prior quiz and test. LAB B2-WNL: Wave Nature of Light due 4pm. Weekly Reflection #13 will be sent out after class today; due Tuesday evening after fall break. The Mallard-based reading quiz due prior to class on Tuesday after fall break.

Review The time since the beginning of the universe is 1/H years or about 13.8 billion years. The Big Bang started off immensely hot! Radiation dominated the early universe. Matter dominance occurs after radiation “cools” enough for matter to condense per the relationship E=mc 2.

Matter Dominance (today) The universe is composed mostly of matter. Most of the past 13.8 billion years has been dominated by matter. Our “horizon” is 13.8 billion light years away. During this period, the rate of expansion has been slowing (but for some recent findings!) In the past, H was much higher.

Radiation Dominance (early) The nature of the radiation was that of a black body radiator at an extremely high temperature. The visible remnant of the early universe (radiation) is black body-like with a large red shift.

Wien’s Law

Stefan-Boltzmann Law

Expansion and Olber’s Paradox Why is the night sky dark? If the universe is infinite and without boundary, every line of sight should intersect a star and the sky should be intensely bright. Consider the mathematics: – Apparent brightness is proportional to 1/r 2 – The volume of thin layers of space is proportional to r 2 – These two effects offset one another!

Some Faulty Explanations The universe consists only of the Milky Way – a spinning Island Universe – but today we know that the Milky Way is only one of hundreds of billions of galaxies filling space. Absorption of starlight by dust between the clouds. But, no, these clouds would heat up if they absorbed all that radiation and would soon start glowing themselves.

Resolving Olber’s Paradox The paradox is resolved by the fact that the universe is expanding, distant objects are moving faster with increasing distance, and red shifts are greater with more distant objects. Ergo, the most distant objects are red shifted into longer wavelengths that we cannot see.

Echo of the Big Bang Work of Arno Penzias and Robert Wilson detecting cosmic microwave background radiation. Colleagues at Princeton University made an earlier prediction that microwave “echo” should exist as a consequence of the Big Bang.

Cosmic Background Radiation Black body radiator at T = 2.725K and the work of COBE – a perfect match! During the earliest stages of the cosmos, the universe was radiation dominated. This radiation is just now reaching us from the “horizon” of the universe and is red shifted so it appears as a cold black body radiator.