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.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL 6. Dark matter.
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.
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:
Week 10 Dark Matter Reading: Dark Matter: 16.1, 16.5d (4 pages)
Dark Matter, Dark Energy, and the Fate of the Universe.
Chapter 16 Dark Matter 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.
The Hidden Lives of Galaxies Jim Lochner, USRA & NASA/GSFC.
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.
The Milky Way. Structure of the Milky Way The Milky Way.
The Milky Way Galaxy.
M 51. M 51 Galaxy merger simulation.
Chapter 20: Galaxies So far we have talked about “small” things like stars, nebulae and star clusters. Now it’s time to get big!
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.
Ch. 4 Sec. 5 The Expanding Universe Discover activity- How Does the Universe Expand pg What happens to the distances between galaxies that are.
Galaxies and 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.
North America at night from space. Light can be: broken up into component colors broken up into component colors absorbed absorbed reflected reflected.
The Standard Model Part II. The Future of the Universe Three possible scenarios: Expand forever (greater than escape velocity) Expand to a halt (exactly.
Cosmic Chemistry: Cosmogony Dark Matter—More Than Meets the Eye Student Text Supplement.
COSMOLOGY SL - summary. STRUCTURES Structure  Solar system  Galaxy  Local group  Cluster  Super-cluster Cosmological principle  Homogeneity – no.
Lecture 18 : Weighing the Universe, and the need for dark matter Recap – Constraints on the baryon density parameter  B The importance of measuring the.
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.
1 The Milky Way Galaxy We live on the quiet outskirts of a galaxy of approximately 100 Billion stars. This galaxy, the Milky Way, is roughly disk-shaped.
The Milky Way Galaxy Structure & Evolution Ohio University - Lancaster Campus slide 2 of 35 Spring 2009 PSC 100.
GALAXIES By Christopher Wrobleski & Patrick Bradford Poole.
Astronomy 1143 – Spring 2014 Lecture 22 The Nature of Dark Matter: MACHOs and WIMPs.
Orbits and Masses of astronomical objects Using gravity and orbits to to measure masses Masses of planets, stars and galaxies Dark matter.
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,
Test #3 Same types of questions Bring a calculator Study the other exam reviews.
More to the universe than meets the eye
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.
The Milky Way Galaxy Comprehend the Milky Way Galaxy and the Sun’s Place In It Comprehend the Four Components of the Galaxy Comprehend Other Planetary.
Physics 55 Monday, December 5, Course evaluations. 2.General relativity with applications to black holes, dark matter, and cosmology. 3.Hubble’s.
Life Cycle of Stars Mr. Weaver.
1 “It really sucks!”. 2 Newton Isaac Newton ( ) was a British scientist who first explained how gravity works. His ideas were inspired by seeing.
Astronomy 1143 – Spring 2014 Lecture 21: The Evidence for Dark Matter.
Dark Matter Mathematics Janet Moore NASA Educator Ambassador Janet Moore NASA Educator Ambassador.
Galaxies: Our Galaxy: the Milky Way. . The Structure of the Milky Way Galactic Plane Galactic Center The actual structure of our Milky Way is very hard.
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:
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 Masses of Galaxies. Remember Hubble’s ‘Tuning Fork’
Black Holes and Gravity 1)Type II Supernova 2)Neutron Stars 3)Black Holes 4)More Gravity April 7, 2003
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.
Dark Matter, Dark Energy
Masses of Galaxies Measure mass by: motion within a galaxy
The Masses of Galaxies: Dark Matter
Discussion Most bright galaxies are spirals. What do you think causes these galaxies to have a spiral pattern?
Lecture 18 : Weighing the Universe, and the need for dark matter
Rotational Mathematics
Introduction to Galaxies Types of Galaxies The Milky Way Dark Matter
Dark Matter, Dark Energy And The Fate Of The Universe
Chapter 23 Our Galaxy.
Galaxies and the Universe
Dark Matter, Dark Energy, and the Fate of the Universe
Section 5 – pg 622 The Expanding Universe
12-3,4 Evolution of Stars.
Homework #10 is due Wednesday, April 25, 9:00 pm. Review session Wednesday, April 25, 7:15 pm.
Stars and Galaxies.
Presentation transcript:

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 have a system where most of the mass is in the center, like the solar system with the Sun having 99.8% of the mass, the closer a planet is, the faster it moves.

Spiral galaxies look like most of the mass is near the center in the nucleus, so nearer stars to the center should rotate faster.

Astronomers found that stars near the center of spiral galaxies were rotating slower than stars farther out, implying that most of the mass was not in the bright center.

There had to be some other invisible mass changing the rotation speed of stars. This got the name “Dark Matter”. Several explanations for this “Dark Matter” have come forward. Neutrinos MACHOs WIMPs/Sparticles Dark Energy

Neutrinos are subatomic particles given off during nuclear fusion Neutrinos are subatomic particles given off during nuclear fusion. They don’t react with much of anything, and thus are nearly impossible to detect. Right now buzillions of them are traveling through you, and the Earth from the Sun. If they weigh something, they could account for the missing mass.

MACHOs are massive compact halo objects, implying they are objects with mass that don’t give off light (in the halo or outskirts of a galaxy). These things could be planets, black holes, or neutron stars.

WIMPS are weakly interacting massive particles, meaning they are massive subatomic particles that don’t react with other matter. They have yet to be “discovered”. String theory predicts a similar particle called a “sparticle”.

Dark Energy is an undefined source of matter/energy that is causing the entire Universe to expand faster than it should be. There are no explanations of what it is or what causes it.