Composition Until 30 years ago, we thought all matter was “baryonic” matter (protons, neutrons, electrons). Now: 4.6% is baryonic matter 95% is non-baryonic.

Slides:



Advertisements
Similar presentations
Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 6. Dark matter.
Advertisements

What is dark matter?. 96% of the universe is missing In fact, all of the stuff we can detect in the universe: –All of the matter –All of the energy –Only.
Week 10 Dark Matter Reading: Dark Matter: 16.1, 16.5d (4 pages)
Dark Matter Mike Brotherton Professor of Astronomy, University of Wyoming Author of Star Dragon and Spider Star.
Dark Matter Da yang Jacob Daeffler. What do we mean by dark matter? Material whose presence can be inferred from its effects on the motions of stars and.
Dark Matter, Dark Energy, and the Fate of the Universe.
Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe.
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 17.
PRESENTATION TOPIC  DARK MATTER &DARK ENERGY.  We know about only normal matter which is only 5% of the composition of universe and the rest is  DARK.
© 2010 Pearson Education, Inc. Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe.
Chapter 23: Our Galaxy Our location in the galaxy Structure of the galaxy Dark matter Spiral arm formation Our own supermassive black hole.
Announcements Homework 14 due Wednesday (5 questions) Monty Python Challenge offer good through this Wednesday! Final exam in SL 228 next Monday or Tuesday.
The latest experimental evidence suggests that the universe is made up of just 4% ordinary matter, 23% cold dark matter and 73% dark energy. These values.
Fritz Zwicky and Dark Matter Wes Donehower. The “Missing Mass” Problem In 1933, Zwicky was studying galaxies and he estimated their total mass by measuring.
Class 23 : The mass of galaxies and the need for dark matter How do you measure the mass of a galaxy? What is “dark matter” and why do we need it?
Copyright © 2010 Pearson Education, Inc. Dark Matter and Dark Energy.
GALAXY FORMATION AND EVOLUTION - 2. DISCOVER Magazine’s 2007 Scientist of the Year David Charbonneau, of the Harvard-Smithsonian Canter for Astrophysics.
The Milky Way. Structure of the Milky Way The Milky Way.
Dark Matter Masses of Galaxies Gravity and Light Black Holes What is Dark Matter?
Astro-2: History of the Universe Lecture 5; April
Dark Matter begin. Definition Dark Matter is matter that we cannot see. It neither emits nor reflects any light. If we can’t see it, how do we know it.
Dark Matter Friday, October 17. The Sun goes around the center of the Milky Way Galaxy on a nearly circular orbit.
THE UNSEEN EFFECT OF DARK MATTER Max Ehrhardt Physics 335 Final Presentation 12/1/04.
Dark Matter, Dark Energy, and the Fate of the Universe
Components of the Milky Way The light from galaxies is centrally concentrated. But is the mass also centrally concentrated? Does Mass follow Light in Galaxies?
Galaxy Mass Star Number/Density Counting stars in a given volume
Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe
Dark Matter, Dark Energy, How Come Some People Think We Need It and Others Don’t and the Fate of the Universe.
YSS - Intro. to Observational Astrophysics (ASTR 205) Class #13 Dark Matter, Dark Energy, and the Fate of the Universe (Chapter 16) Professor: José Maza.
North America at night from space. Light can be: broken up into component colors broken up into component colors absorbed absorbed reflected reflected.
Lecture 12 Astronomy /27/07. Looking Back Through Time Recall that looking at distant objects is the same as looking backwards through time The.
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
The Universe  What do we know about it  age: 14.6 billion years  Evolved from Big Bang  chemical composition  Structures.
Lecture 18 : Weighing the Universe, and the need for dark matter Recap – Constraints on the baryon density parameter  B The importance of measuring the.
Dark Matter. Zwicky’s Coma In 1933 Fred Zwicky measured the speed of Coma cluster galaxies. –Too fast for the visible stars –Cluster would fly apart Either.
Cosmology Olber’s Paradox Big Bang Development of the Universe.
So, how’s it gonna end? The Big Bang started the universe expanding fast, but gravity should have put on the brakes. Expansion should slow down after.
Origins: Dark Matter & Dark Energy WWK: Students will understand the theories of Dark Matter & Dark Energy and how they’re thought to affect the Universe.
Chapter 22 Dark Matter, Dark Energy, and the Fate of the Universe.
Dark Matter The Portion of the Universe You Have to Appreciate to “See” By Andre Bosman and Barbara Anderson.
GALAXIES By Christopher Wrobleski & Patrick Bradford Poole.
Astronomy 1143 – Spring 2014 Lecture 30: Dark Matter Revisted…..
A Quick Look At The History of Dark Matter Dan Hooper Fermilab/University of Chicago Cosmology Short Course For Museum and Planetarium Staff September.
Lecture 39: Dark Matter review from last time: quasars first discovered in radio, but not all quasars are detected in the radio first discovered in radio,
More to the universe than meets the eye
DARK MATTER IN THE UNIVERSE? PRESENTED BY L. KULL AT THE R.H.FLEET SCIENCE CENTER December 14,2005.
Physics 55 Monday, December 5, Course evaluations. 2.General relativity with applications to black holes, dark matter, and cosmology. 3.Hubble’s.
Dark Matter cannot be seen directly with telescopes; it neither emits nor absorbs light; estimated to constitute 84.5% of the total matter in the universe.
14 Dark Matter Join me on the Dark Side. 14 Goals Why do we think there is dark matter? Where do we think it is? How much is there?
Astronomy 1143 – Spring 2014 Lecture 21: The Evidence for Dark Matter.
Dark Matter By Joel Tome Period 3. What is Dark Matter? ►T►T►T►The mass in galaxies and galactic clusters inferred to exist: bbbby rotational properties.
LUMINOUS MATTER  luminous = »The matter that astronomers see in the Universe (stars, dust clouds, etc.) makes up less than 1/2 of one percent of.
Yale Summer Class: Observational Astronomy. Class #13 Dark Matter, Dark Energy, and the Fate of the Universe Professor: José Maza July 6, 2009 Professor:
© 2010 Pearson Education, Inc. Dark Universe: Dark Matter Dark Energy and the Fate of the Universe.
Dark Matter and Energy What are our eyes missing?.
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.
Public Star Party Organized by Institute for Astronomy, University of Hawaii. Contact person: Prof. Jim Heasley. When? Tonight between 8:30 and 10 pm.
Dark Matter, Dark Energy
Dark Matter, Dark Energy, and the Fate of the Universe.
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.
2. April 2007J.Wicht : Dark Matter2 Outline ● Three lecturers spoke about Dark Matter : – John Ellis, CMB and the Early Universe – Felix Mirabel, High-Energy.
Wormholes. The simplest example The r = 2m singularity is more complicated than previously mentioned… Has solution (the Schwarzschild metric):
Masses of Galaxies Measure mass by: motion within a galaxy
The Dark Universe Susan Cartwright.
dark matter and the Fate of the Universe
Dark matter and dark energy
Dark Matter Background Possible causes Dark Matter Candidates
Dark Matter, Dark Energy, and the Fate of the Universe
Homework #10 is due Wednesday, April 25, 9:00 pm. Review session Wednesday, April 25, 7:15 pm.
Dark Matter In the 1970s, using spectral analysis, it was discovered that spiral galaxies were not rotating like they looked like they should be. If you.
Presentation transcript:

Composition Until 30 years ago, we thought all matter was “baryonic” matter (protons, neutrons, electrons). Now: 4.6% is baryonic matter 95% is non-baryonic matter

Non-Baryonic Matter 23% is Dark Matter- composed of sub-atomic particles that interact weakly with ordinary matter. 72% is Dark Energy - this amount would explain a flat, accelerating universe… which is what we observe. ??% are neutrinos - like electrons, but without a charge.

Dark Matter Measure mass of galaxies and stars by how fast objects orbit them. Galaxies have more mass than stars, gas and dust within them. Also, gravitational lensing shows too much mass in galaxies.

Dark Matter Gravitational pull, but does not emit or absorb light. Could be… 1.Brown Dwarfs: small stars too small to shine, but still have large gravity. - called MACHOS (massive compact halo objects). If so, than missing mass is baryonic.

Dark Matter 2.Supermassive Black Holes: May power quasars. May be detected through lensing. 3.New Forms of Matter: Called WIMPS (Weakly Interacting Massive Particles)… non- baryonic matter.

Dark Energy New cosmological constant… first used by Einstein to keep universe static… now used to explain acceleration. Cosmological Constant = energy from vacuum of space. Quantum fluctuations. Something from nothing? Consistent with observations