Cosmology Slides.

Slides:



Advertisements
Similar presentations
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL Revision Lecture.
Advertisements

LECTURE 27, DECEMBER 9, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
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.
Origin & Evolution of the Universe
When Galaxies Collide. It is not uncommon for galaxies to gravitationally interact with each other, and even collide!
Chapter 26: Cosmology Why is the sky dark? The expanding universe Beginning of the universe: The Big Bang Cosmic microwave background The early universe.
Chapter 28 Cosmology The Creation and Fate of the Universe.
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.
Einstein’s Universe Tuesday, February 5. Einstein – Newton smackdown! gravityspace Two different ways of thinking about gravity and space.
Lecture 20 Hubble Time – Scale Factor ASTR 340 Fall 2006 Dennis Papadopoulos.
AST101 Lecture 25 Why is the Night Sky Dark?. Olber’s Paradox Suppose the universe is infinite In whatever direction you look, you will see a star The.
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 Overview David Spergel. Lecture Outline  THEME: Observations suggest that the simplest cosmological model, a homogenuous flat universe describes.
19 The Big Bang Evidence The Science of Creation.
1.Homogeneity 2.Isotropy 3.Universality 4.Cosmological Principle Matter is distributed evenly throughout the universe on the largest scales (~ 300 Mpc).
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 26 Cosmology Cosmology.
Cosmology Physics466 Olbers Paradox Cosmological principle Expansion of the Universe Big Bang Theory Steady State Model Dark Matter Dark Energy Structure.
Hubble Diagram: Distribution of Galaxies. Hubble’s Law: v = H o d Velocity increases with distance.
1 In the beginning God created the heavens and the earth. 2 Now the earth was formless and empty, darkness was over the surface of the deep, and the Spirit.
The Evolution of the Universe Nicola Loaring. The Big Bang According to scientists the Universe began ~15 billion years ago in a hot Big Bang. At creation.
Contemporary science issues Lesson 16: Has the universe always been there? © 2006 Gatsby Technical Education Projects.
Please press “1” to test your transmitter.
The Standard Model of Cosmology Chad A. Middleton, Ph.D. Mesa State College October 11, 2007 “The most incomprehensible thing about the world is that it.
Cosmology: The Study of the Universe as a Whole Physics 360 Geol 360 Astronomy John Swez.
Midterm exam: date: March 17, 2006, 8:15 a.m. date: March 17, 2006, 8:15 a.m. location: Conrad Naber Hall location: Conrad Naber Hall bring pocket calculator.
Geometry of the Universe
Beginnings The First Americans. The First Arrivals The first people began to arrive on this continent as early as 20,000 years ago But Where did they.
Cosmology The Origin and Future of the Universe Part I Olbers’ Paradox.
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
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.
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 3. Cosmological concepts and Olbers’ paradox.
General Relativity and the Expanding Universe Allan Johnston 4/4/06.
The Fate of the Universe
Dark Energy Wednesday, October 29 Midterm on Friday, October 31.
The moon!! The stars!!  She's a greek goddess and she rides a chariot across the sky trailing stars and her 2 sons are with her, Thanatos and Hypnos.
Big Bang Theory – A History 1927: Belgian priest Georges Lemaître proposes that the universe began with the explosion of a "primeval atom". Einstein develops.
Hubble’s galaxy classes Spheroid Dominates Disk Dominates.
10B The Big Bang Where do we come from, where are we going?
Origins Lecture 15; May Previously on Origins Time of history/humans vs. time of “god” –What was there before time? –Does this make sense? The.
The 6 Days of Creation Genesis 1.
The BIG Bang. Hubble Telescope  This image is taken of galaxies that are billions of light-years away. Light takes a very long time to travel to Earth.
Ch. 22 Cosmology - Part 1 The Beginning. Beginnings ???? - Newton suggested that for the stars not to have coalesced, the universe must be infinite and.
Beginnings The First Americans. The First Arrivals The first people began to arrive on this continent as early as 12,000 – 30,000 years ago But Where.
Fate of the Universe 1)Fate of the Universe 2)Shape of the Universe 3)Large Scale Structure November 25, 2002 Final Exam will be held in Ruby Diamond Auditorium.
The Meaning of Einstein’s Equation*
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
Cosmology (Chapter 14) NASA. Student Learning Objectives Describe the Big Bang theory Analyze possible fates of our universe.
The Expanding Universe
Announcements Final exam is Monday, May 9, at 7:30 am. –Students with last names A-K go to 225 CB. –Students with last names L-Z go to 300 CB. –All students.
Universe Tenth Edition Chapter 25 Cosmology: The Origin and Evolution of the Universe Roger Freedman Robert Geller William Kaufmann III.
Lecture 27: The Shape of Space Astronomy Spring 2014.
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.
The Mass of the Galaxy Can be determined using Kepler’s 3 rd Law –Solar System: the orbital velocities of planets determined by mass of Sun –Galaxy: orbital.
The Fate of the Universe. The fate depends on the rate of expansion and the density Density greater than critical value – gravity will halt expansion.
The Genesis Account of Creation The Bible starts with God’s revelation of how He prepared the earth for mankind, the creatures He made in His image and.
Lecture 23: The Acceleration of the Universe Astronomy 1143 – Spring 2014.
Chapter 20 Cosmology. Hubble Ultra Deep Field Galaxies and Cosmology A galaxy’s age, its distance, and the age of the universe are all closely related.
The Science of Creation
Genesis 1:1 – 2:3. Genesis 1:1 – 2:3 Genesis 1:1 – 2:3 7 days vs 13.7 billion years.
Ch. 14 Cosmology (or “The Whole Enchilada”)
Beginnings The First Americans.
Pop-quiz #9 Which of the following statements is TRUE?
Expansion of the Universe
Lectures on galaxies and cosmology
Cosmology.
The Last Epoch.
Cosmology: The Origin and Evolution of the Universe
Presentation transcript:

Cosmology Slides

Iroquois Myth The heavens were around for a lot longer than the Earth, according to a creation myth told by the Iroquois people of North America. One of the heavenly inhabitants, the Great Spirit, punished his daughter for becoming pregnant by throwing her through a hole formed when he ripped up a giant tree. To keep her from perishing, though, he ordered the Great Turtle to dive down into the water, bring up some mud and wait for the daughter to land on its back. When she landed, she gathered up the mud and created the Earth as an island carried on the Great Turtle's back. http://www.brighthub.com/science/space/articles/11499.aspx

Genesis – The Bible In the beginning God created the heavens and the earth.2 Now the earth was formless and empty, darkness was over the surface of the deep, and the Spirit of God was hovering over the waters. 3 And God said, "Let there be light," and there was light. 4 God saw that the light was good, and he separated the light from the darkness. 5 God called the light "day," and the darkness he called "night." And there was evening, and there was morning--the first day.

Other Creation Myths In ancient Greece, In the beginning there was an empty darkness. The only thing in this void was Nyx, a bird with black wings. With the wind she laid a golden egg and for ages she sat upon this egg. Finally life began to stir in the egg and out of it rose Eros, the god of love. One half of the shell rose into the air and became the sky and the other became the Earth. Eros named the sky Uranus and the Earth he named Gaia. Then Eros made them fall in love. . The ancient Babylonians' view of the universe was detailed in the Enuma Elish, a creation myth inscribed on a series of seven clay tablets. In the story, a battle among the gods leads Marduk, the god of spring, to kill Tiamat, goddess of the sea. He splits her body in two, and one half becomes the Earth, the other, the sky. The slain Tiamat's saliva becomes the rain. http://www.cs.williams.edu/~lindsey/myths/myths_16.html

Flat Earth http://4.bp.blogspot.com/_x0tbqXdMlkc/TU-VuLfkVAI/AAAAAAAAAGQ/7SkmfXEsN3U/s1600/flat_earth-edit.jpg http://2.bp.blogspot.com/-sCIpfNH9Fw8/TpNwd_CQ6AI/AAAAAAAAACk/dwexLhz2rhg/s1600/falling-off-flat-earth.jpg

Cosmological Principle Seen on a sufficiently large scale, the universe looks the same for all observers. The universe is the same whoever you are and wherever you are. two testable structural consequences of the cosmological principle are homogeneity and isotropy. Homogeneity : the same in all locations: “the gravy is smooth if you ignore the lumps”. Galaxies violate the cosmological principle Isotropy: the same in all directions. Get the same results no matter where you look. Allows Universe to be treated as a whole, with average energy densities, speeds, pressures, temperatures – Allows science to work http://en.wikipedia.org/wiki/Cosmological_principle

Olber’s Paradox The paradox is that a static, infinitely old universe with an infinite number of stars distributed in an infinitely large space would be bright rather than dark. http://en.wikipedia.org/wiki/Olbers%27_paradox#History

Quantifying Olber’s Paradox

Animation of Olber’s Paradox http://en.wikipedia.org/wiki/File:Olber%27s_Paradox_-_All_Points.gif

Einstein’s Field Equations the Ricci curvature tensor – curvature of space – related to amount of mass in the universe the scalar curvature also related to the curvature of space The metric tensor - defines notions such as distance, volume, curvature, angle, future and past. the stress–energy tensor . describes the density and flux of energy and momentum in spacetime, generalizing the stress tensor of Newtonian physics. It is an attribute of matter, radiation, and non-gravitational force fields. The stress-energy tensor is the source of the gravitational field in the Einstein field equations of general relativity, just as mass is the source of such a field in Newtonian gravity. The Cosmological Constant – put in by Einstein as a modification of his original theory of general relativity to achieve a stationary universe. Einstein abandoned the concept after the observation of the Hubble redshift indicated that the universe might not be stationary, as he had based his theory on the idea that the universe is unchanging.[1] http://en.wikipedia.org/wiki/Einstein_field_equations#Mathematical_form

Hubble Diagram

Difference in types of redshift

CMB http://en.wikipedia.org/wiki/File:Firas_spectrum.jpg

Other forms of Wiens Law

Stellar Parallax http://en.wikipedia.org/wiki/File:Stellarparallax2.svg

Extragalactic Distance Measures http://en.wikipedia.org/wiki/Cosmic_distance_ladder#Main_sequence_fitting

Rotation Curve of Spiral Galaxy http://en.wikipedia.org/wiki/Galaxy_rotation_problem#History_and_description_of_the_problem

Dark Matter Halos http://www.nasa.gov/mission_pages/hubble/science/dark-matter-core.html

Expected Dark Matter Halo in Milky way http://news.nationalgeographic.com/news/2012/04/120419-dark-matter-sun-missing-stars-milky-way-space-science/

Einstein’s Field Equations the Ricci curvature tensor – curvature of space – related to amount of mass in the universe the scalar curvature also related to the curvature of space The metric tensor - defines notions such as distance, volume, curvature, angle, future and past. the stress–energy tensor . describes the density and flux of energy and momentum in spacetime, generalizing the stress tensor of Newtonian physics. It is an attribute of matter, radiation, and non-gravitational force fields. The stress-energy tensor is the source of the gravitational field in the Einstein field equations of general relativity, just as mass is the source of such a field in Newtonian gravity. The Cosmological Constant – put in by Einstein as a modification of his original theory of general relativity to achieve a stationary universe. Einstein abandoned the concept after the observation of the Hubble redshift indicated that the universe might not be stationary, as he had based his theory on the idea that the universe is unchanging.[1] http://en.wikipedia.org/wiki/Einstein_field_equations#Mathematical_form

Curvature of Space http://preposterousuniverse.com/writings/encyc/ The circle represents very roughly the region favored by current observations of distant supernovae, the cosmic microwave background, and the dynamics of galaxies. http://preposterousuniverse.com/writings/encyc/