Dark Matter and Energy What are our eyes missing?.

Slides:



Advertisements
Similar presentations
Measuring Our Rotation Measuring rotation in our galaxy is hard because we are inside it. One method for measuring circular rate of rotation at our radius:
Advertisements

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.
Chapter 23: Dark Matter & The Fate Of The Universe.
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.
Astronomy 100 Tuesday, Thursday 2:30 - 3:45 pm Tom Burbine
Dark Matter and the Fate of the Universe
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.
Black Holes. Outline Escape velocity Definition of a black hole Sizes of black holes Effects on space and time Tidal forces Making black holes Evaporation.
Astro-2: History of the Universe Lecture 4; April
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 17.
Evolution of Dark Matter How ideas have changed. Outline Timeline –Hints –People –Some Explanations right and wrong.
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.
Survey of the Universe Greg Snow U Nebraska Lincoln CROP.
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.
ASTR100 (Spring 2008) Introduction to Astronomy The Case for Dark Matter Prof. D.C. Richardson Sections
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.
DARK MATTER Matthew Bruemmer. Observation There are no purely observational facts about the heavenly bodies. Astronomical measurements are, without exception,
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 18.
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?
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.
The Dark Side of the Universe What is dark matter? Who cares?
1 Galaxies The Andromeda Galaxy - nearest galaxy similar to our own. Only 2 million light years away! Galaxies are clouds of millions to hundreds of billions.
Energy! (gamma photons and neutrinos) 100sec100,000 years Too hot for matter to form 13 P3 4.1 Galaxies C* Describe how the Universe changed after the.
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.
Dark Matter in Galaxies and Clusters AST 112. Matter Galaxies appear to be made up of stars, gas and dust Reasonable to think that’s the end of the story…
YSS - Intro. to Observational Astrophysics (ASTR 205) Class #13 Dark Matter, Dark Energy, and the Fate of the Universe (Chapter 16) Professor: José Maza.
1 Martin L. Perl SLAC National Accelerator Laboratory and Kavli Institute for Particle Astrophysics and Cosmology at Stanford.
North America at night from space. Light can be: broken up into component colors broken up into component colors absorbed absorbed reflected reflected.
The Universe  What do we know about it  age: 14.6 billion years  Evolved from Big Bang  chemical composition  Structures.
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.
Chapter 16 Dark Matter, Dark Energy, and the Fate of the Universe.
Dark Matter and Dark Energy By: Matt Tanaka And Bryent Kaneshiro.
DARK MATTER AND DARK ENERGY This powerpoint will show you the basics of dark matter and dark energy Their place in the universe By Jordan Ilori.
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.
Space and Unsolved Mysteries. Black Holes Form from the death of a very large star ( more than 25 solar masses). A supernova occurs followed by a black.
Dark Matter & Energy By: Conwa and Luke. Dark Matter Matter in the universe that is invisible. It can be detected by its gravity. 25% of the universe.
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,
The Universe. Galaxies are believed to have formed from mergers of smaller galaxies and star clusters. Galaxy Formation and Evolution.
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.
Physics 55 Monday, December 5, Course evaluations. 2.General relativity with applications to black holes, dark matter, and cosmology. 3.Hubble’s.
DCMST May 22 nd, 2007 Dark matter and dark energy Gavin Lawes Wayne State University.
Dark Matter Rotation Curves Creative Commons Jan Oort 1932 – Studied velocities of nearby stars within the Milky Way galaxy (our galaxy) Found higher.
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.
HOMEWORK: PAGE 381 # 1, 5, 7, UNSOLVED MYSTERIES.
Yale Summer Class: Observational Astronomy. Class #13 Dark Matter, Dark Energy, and the Fate of the Universe Professor: José Maza July 6, 2009 Professor:
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.
Dark Energy By Chris Malafis & Amit Sheth. Discovery Two competing groups from different observatories were trying to prove the deceleration of the expansion.
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,
The Milky Way Galaxy. What are each of these?
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. Dark Matter I.What Is It? A. Dark matter is a type of ______________ hypothesized to account for a large part of the total.
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
dark matter and the Fate of the Universe
Galaxies.
The “Dark Matter” Problem…!
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.
Presentation transcript:

Dark Matter and Energy What are our eyes missing?

What are Dark Matter and Energy? Mostly concepts, not particular things Mostly concepts, not particular things Dark matter emits no light, but has mass and volume. Dark matter emits no light, but has mass and volume. Dark energy is, in a sense, reverse gravity (repellant force). Dark energy is, in a sense, reverse gravity (repellant force). Empty spaces Empty spaces Einstein’s Cosmological Constant Einstein’s Cosmological Constant Dark Matter makes up most of our universe (around 88%). Dark Matter makes up most of our universe (around 88%). Result deduced from the Omega value Result deduced from the Omega value We know of their existence through experimental data results and theory. We know of their existence through experimental data results and theory. Both are extremely important to science, especially in astrophysics. Both are extremely important to science, especially in astrophysics. Dark Matter Not Dark Matter

Reasons and Proof for Existence Motions/Rotations of astronomical objects Motions/Rotations of astronomical objects Observable on many different scales(galaxies, galactic clusters, superclusters) Observable on many different scales(galaxies, galactic clusters, superclusters) Acceleration of the universe Acceleration of the universe CMB(Cosmic Microwave Background) CMB(Cosmic Microwave Background) Gravitational Wells Gravitational Wells Photon energy is higher coming out Photon energy is higher coming out Structure of the universe Structure of the universe Model of gravity effect on the universe

Where are Dark Matter and Energy? Dark matter can be in several forms Dark matter can be in several forms MACHOS(Massive Compact Halo Objects) MACHOS(Massive Compact Halo Objects) Huge particles located near or in galactic halos Huge particles located near or in galactic halos Brown dwarfs and black holes Brown dwarfs and black holes WIMPS(Weakly Interacting Massive Particles) WIMPS(Weakly Interacting Massive Particles) Thought to be mostly useless Thought to be mostly useless Currently favored possibility Currently favored possibility Neutrinos Neutrinos Ordinary matter Ordinary matter Not nearly enough to account for all the gravitational effects Not nearly enough to account for all the gravitational effects Understanding of gravity Understanding of gravity Perhaps we just do not have a proper grasp of the concepts and laws of gravity Perhaps we just do not have a proper grasp of the concepts and laws of gravity Dark energy is more of a force, like gravity, and thus has no “location” Dark energy is more of a force, like gravity, and thus has no “location”

Experiments and Research Fritz Zwicky Fritz Zwicky Studied the mass of galaxies (specifically in the Virgo and Coma clusters) Studied the mass of galaxies (specifically in the Virgo and Coma clusters) First calculation: Luminosity First calculation: Luminosity Second calculation: Spread in Velocities Second calculation: Spread in Velocities Second result 400 times larger than the first Second result 400 times larger than the first Jan Oort Jan Oort Measured perpindicular motions of nearby stars relative to the desk of our galaxy Measured perpindicular motions of nearby stars relative to the desk of our galaxy Could measure the mass of the disk by the gravitational pull on the stars Could measure the mass of the disk by the gravitational pull on the stars Resulted in twice the mass he expected Resulted in twice the mass he expected Both agreed that visible mass only makes up 10% or so of the mass needed to keep the galaxies from flying apart Both agreed that visible mass only makes up 10% or so of the mass needed to keep the galaxies from flying apart

What might new findings mean for us? Study of the location of galactic bodies Study of the location of galactic bodies Theories about the origin and behavior of the universe Theories about the origin and behavior of the universe Possible, though perhaps unlikely, “real world” application Possible, though perhaps unlikely, “real world” application Redefinition of the way people think of forces as a whole Redefinition of the way people think of forces as a whole

References igations/MassGalaxyDM.html igations/MassGalaxyDM.html igations/MassGalaxyDM.html igations/MassGalaxyDM.html tml tml tml tml tutorial/dm0.html tutorial/dm0.html