Hubble Diagram: Distribution of Galaxies. Hubble’s Law: v = H o d Velocity increases with distance.

Slides:



Advertisements
Similar presentations
Relativity H2: Concepts and postulates of special relativity.
Advertisements

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.
Theory of Special Relativity
Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
Chapter 18: Relativity and Black Holes
PHY306 1 Relativity Principle of relativity  not a new idea! Basic concepts of special relativity  …an idea whose time had come… Basic concepts of general.
Special and General Relativity
Origin & Evolution of the Universe
Chapter 26: Cosmology Why is the sky dark? The expanding universe Beginning of the universe: The Big Bang Cosmic microwave background The early 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.
Extragalactic Astronomy & Cosmology First-Half Review [4246] Physics 316.
The Mathematics of General Relativity, Black holes, and Cosmology Chad A. Middleton Brown Bag Seminar Mesa State College February 12, 2010.
The Nature of the Universe The universe began 13.8 billion years ago with the “big bang”. At this moment in time, all of the matter and energy in the.
Galileo simply described this as the fact that an observer in motion sees things differently from a stationary observer We use this as a part of our everyday.
The Life Cycles of Stars and our Sun. Your Questions 1.Have you ever heard of the sun song by the group They Might be Giants?
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.
How do we transform between accelerated frames? Consider Newton’s first and second laws: m i is the measure of the inertia of an object – its resistance.
SPECIAL RELATIVITY -Postulates of Special Relativity -Relativity of time –> time dilation -Relativity of length –> length contraction © 2005.
Chapter 22: Black Holes Einstein’s relativity: –Special –General –Relativity and black holes Evidence of black holes Properties of black holes Long-time.
The Big Bang: Fact or Fiction? The Big Bang Fact or fiction? Dr Cormac O’Raifeartaigh.
Quiz 1 Each quiz sheet has a different 5-digit symmetric number which must be filled in (as shown on the transparency, but NOT the same one!!!!!) Please.
Julia Sickels - jns5224 Sam Fisher - sef5176 Alyssa Hawras - aoh5295.
Special Relativity Speed of light is constant Time dilation Simultaneity Length Contraction Spacetime diagrams.
Stationary Elevator with gravity: Ball is accelerated down.
What can electromagnetic waves tell us about the movement of planets, stars, and galaxies?
Origin of the Universe Have you ever heard of a little thing called the “Big Bang?”
Please press “1” to test your transmitter.
Modern Physics: Part 2. ALL Galaxies have redshifts – farther from us greater redshifts! Many other scientists made observations similar to Slipher’s.
Theory on the Formation of the Universe
Chapter 26 Relativity. General Physics Relativity II Sections 5–7.
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.
Special Relativity Space and Time. Spacetime Motion in space is related to motion in time. Special theory of relativity: describes how time is affected.
Physics Mrs. Coyle -Gravitational Field -Satellites -Einstein’s View of Gravity.
Intro to Cosmology! OR What is our Universe?. The Latest High Resolution Image of the Cosmic Microwave Background Radiation Low Energy RegionHigh Energy.
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
Quiz 1, Astro 1140, AU15, Pradhan – Curve: +10% A B C D E.
General Relativity and the Expanding Universe Allan Johnston 4/4/06.
Black Holes Formation Spacetime Curved spacetime Event horizon Seeing black holes Demo: 1L Gravity Well - Black Hole.
Lecture 27: Black Holes. Stellar Corpses: white dwarfs white dwarfs  collapsed cores of low-mass stars  supported by electron degeneracy  white dwarf.
Extragalactic Astronomy & Cosmology Lecture GR Jane Turner Joint Center for Astrophysics UMBC & NASA/GSFC 2003 Spring [4246] Physics 316.
Announcements Exam 3 is scheduled for Wednesday April 8. Will be pushed back to Monday April 13 Tentatively will cover the rest of Chapter 4, all of Chapters.
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.
Principle of Equivalence: Einstein 1907 Box stationary in gravity field Box falling freely Box accelerates in empty space Box moves through space at constant.
The “Big Bang” Theory Birth of the Universe. The Big Bang Theory First and foremost – THIS IS A THEORY! – It is up to you whether you want to believe.
The Meaning of Einstein’s Equation*
General Relativity and Cosmology The End of Absolute Space Cosmological Principle Black Holes CBMR and Big Bang.
To do: Run through the ppt on Big Bang and Cosmology (resources.faulkes-telescope.com > GCSE Astronomy > Class Exercises > Cosmology Complete the following.
Cosmology (Chapter 14) NASA. Student Learning Objectives Describe the Big Bang theory Analyze possible fates of our universe.
Cosmology -- the Origin and Structure of the Universe Cosmological Principle – the Universe appears the same from all directions. There is no preferred.
Universe Tenth Edition Chapter 25 Cosmology: The Origin and Evolution of the Universe Roger Freedman Robert Geller William Kaufmann III.
Visual Guide to Special and General Relativity. This is about to get weird…
Special Relativity By Jackson Andrews.
Astronomy 1020 Stellar Astronomy Spring_2016 Day-34.
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.
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.
Black Hole. Special Relativity Einstein’s special theory of relativity has two parts. –All objects moving at constant velocity have the same laws of physics.
The Big Bang Theory.
Einstein’s Universe Dr Martin Hendry Dept of Physics and Astronomy,
Astrophysics and Cosmology
Einstein’s postulates
Chapter S2 Space and Time
Albert Einstein and the Theory of Relativity
BIG BANG THEORY.
Einstein’s Theory of Relativity
Pop-quiz #1 Which of the following statements is TRUE:
Lesson 13: Gravitational Force
Cosmology: The Origin and Evolution of the Universe
Origin of Universe - Big Bang
BIG BANG THEORY.
Principle of Equivalence: Einstein 1907
Presentation transcript:

Hubble Diagram: Distribution of Galaxies

Hubble’s Law: v = H o d Velocity increases with distance

Expanding Universe Hubble’s law  Universe is expanding Universe had a beginning ! How long ago? Age of the universe: 1/H o (units of time) Big Bang !! How does one determine distances? Redshift

Cosmic Microwave Background (CMB): Universal and Uniform Radiation

CMB Properties The entire universe is filled with extremely uniform radiation CMB radiation corresponds to a fixed temperature of 2.73 K ( o C or o F) Blackbody: uniform temperature oven CMB radiation is also isotropic  same in all directions But with extremely slight variations immediately following the Big Bang due to matter

Distribution of Matter in Galaxy Stars rotate about the center of galaxy Velocity determined by gravity: mass M c and distance R c from the center KE = PE ½ m star v 2 = G M c m star / R c Velocity v should decrease with radius R c Surprise !

Evidence of Dark Matter: Rotation Curves of Galaxies

Dark Matter Halo Rotation curves are flat out to distances beyond observable galaxies Ergo: Galaxies have “dark matter” haloes What is dark matter?

Einstein’s Theory of Relativity Is there a maximum velocity in nature ? If no, then one can travel or convey information over infinite distances in infinitesimally short time – Action at a distance as presupposed by Newton But, do not observe instantaneous action implying infinite speed But if yes, then what is the limiting velocity?

The Two Postulates of Relativity 1. Speed of light is the maximum speed in nature, and is constant regardless of the speed of the source or the observer 2. All physical laws are the same everywhere, and should have the same form (equations) when describing the same phenomenon (first proposed by Galileo)  Principle of Relativity Changes our concept of space and time

Consequences of Relativity Special Theory of relativity  constant velocities Can not simply add velocities v1 + v2 v = (v1 + v2) / (1 + v1v2 / c 2 ) E = m c 2  Energy and mass are equivalent (example: atomic energy, A- and H-bombs) No object with mass can attain the speed of light; its inertial mass becomes infinite m = m(rest) / (1 – v 2 /c 2 ) 1/2 Light is bent by gravity of a massive object such as the Sun

Relativity (Contd.) General Theory of Relativity  Accelerating objects and gravity Why are astronauts in the orbiting space shuttle weightless ? They are continuously falling towards the Earth at the same rate as the floor of the space shuttle (e.g. like a freely falling elevator) Gravity  Acceleration (equivalent) Basic idea: F = ma  W = mg

Relativity (Contd.) Space and time are equivalent (simultaneity is relative, not absolute) Example: Two observers, one on a moving train and the other stationary on the ground observe “simultaneous” flashes of light at different times  difference in space due to motion is “converted” to difference in time Time ‘flows’ slower in a moving frame of reference (astronauts live slightly longer!), or near a massive object such as a black hole

Time Dilation and Space Contraction A time interval in a moving frame of reference (platform moving with velocity v) gets longer as t’ = t / [ 1 – (v/c ) 2 ] 1/2 But the space interval gets shorter as x’ = x [ 1 – (v/c) 2 ] 1/2