An external galaxy; a spiral like our own.. Which way does it rotate?

Slides:



Advertisements
Similar presentations
Galaxies & the Universe
Advertisements

ASTRONOMİ VE UZAY BİLİMİ Astronomy and Space Science Astrophysics.
ASTRONOMİ VE UZAY BİLİMİ
SPIRAL GALAXIESSPIRAL GALAXIES Galaxies are made up of millions or billions of stars. Some may also contain gas and dust which could produce stars from.
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
Bell Question 11/09/11 1.Describe the life cycle of a star the size of our sun. (5 pts.)
Dark Matter, Dark Energy, and the Fate of the Universe.
The Milky Way Galaxy part 2
Particle Astrophysics & Cosmology SS Chapter 7 Dark Matter.
Physics 133: Extragalactic Astronomy and Cosmology Lecture 10; February
Galaxies Types Dark Matter Active Galaxies Galaxy Clusters & Gravitational Lensing.
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.
The Milky Way Galaxy 19 April 2005 AST 2010: Chapter 24.
Dark Stuff – an interlude Toby Burnett. How do we measure mass? Weigh? Count the number of atoms? Gravitational effect?
Measurement of the rotation of the galaxy UGC 9242 by Nicole Vogt, Martha Haynes and Terry Herter using the Palomar 5m telescope. This image shows the.
Particle Astrophysics & Cosmology SS Chapter 8 Structure Formation.
GALAXY FORMATION AND EVOLUTION - 2. DISCOVER Magazine’s 2007 Scientist of the Year David Charbonneau, of the Harvard-Smithsonian Canter for Astrophysics.
Galaxies. Our Galaxy (CP Fig 19.1a) Our Galaxy (CP Fig 19.1b)
Galaxy Formation Models Cold Dark Matter is the dominant component of galaxies and is key to their formation and evolution. CDM models have been wonderful.
The Milky Way. Structure of the Milky Way The Milky Way.
Chapter 14 Our Galaxy The Milky Way Revealed Our Goals for Learning What does our galaxy look like? How do stars orbit in our galaxy?
The Milky Way Galaxy.
By: Flavio Gutierrez. What is a Galaxy? Massive Consists of: Stars Dust Dark matter Contains Planets Stars Moon en.wikipedia.org.
By Enrique V. Zepeda 10/01/2012. Introduction First galaxies formed due to fluctuations of density in some areas of the early universe. Two theories or.
Galaxies Chapter 13:. Galaxies Contain a few thousand to tens of billions of stars, Large variety of shapes and sizes Star systems like our Milky Way.
Where in the universe are we?. What is the universe? Everything that exists is part of the universe. Our universe is a large expanse of dust, gas, stars,
Overview of Astronomy AST 200. Astronomy Nature designs the Experiment Nature designs the Experiment Tools Tools 1) Imaging 2) Spectroscopy 3) Computational.
Walter Orlov The Hidden Galaxy The Basic Idea. The rotation curves of spiral galaxies are not only flat.
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?
The Milky Way Galaxy.
Galaxies Nimisha G. Kantharia National Centre for Radio Astrophysics Tata Institute of FundamentalResearch Pune.
Notes 10 - Galaxies Mrs. Gordon Saturday, October 03, 2015Saturday, October 03, 2015Saturday, October 03, 2015Saturday, October 03, 2015.
Ch Star Groups.
YSS - Intro. to Observational Astrophysics (ASTR 205) Class #13 Dark Matter, Dark Energy, and the Fate of the Universe (Chapter 16) Professor: José Maza.
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.
Origins Lecture 10; May Previously… on Origins: Is Earth a special/unique place? What does the question mean? How do we find planets? What are.
Lecture 1: Introduction to Cosmology Astronomy 5: The Formation and Evolution of the Universe Sandra M. Faber Spring Quarter 2007 UC Santa Cruz.
Lecture Outlines Astronomy Today 7th Edition Chaisson/McMillan © 2011 Pearson Education, Inc. Chapter 23.
The Milky Way Galaxy. HW #9 – MasteringAstro “Stars and Galaxies” Available now Tuesday April 17 th Due BEFORE CLASS Tuesday April 24 th Observing logs.
People once thought that earth was Today we know its shape as a.
Announcements 4th test is finished! Please pick up graded work Homework 12 due Monday (requires internet use) Second project is due in two weeks Please.
Galaxies GALAXIES Stars are not randomly sprinkled throughout the universe. Most astronomers agree that there are about 100 billion galaxies in the universe,
What is a Galaxy and, how many different kinds are there Joson Anjo C. Casillan VII- Amorsolo.
Dark Matter Facts Only 20% of all known matter is the matter we can see, or “normal matter.” The other 80% is Dark Matter, which is also around us just.
Astronomy 404/CSI 769 Extragalactic Astronomy
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.
LECTURE 23, NOVEMBER 23, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
ASTR112 The Galaxy Lecture 2 Prof. John Hearnshaw 2. Constituents of the Galaxy 3. Structure of the Galaxy 4. The system of galactic coordinates 5. Stellar.
10.2 Galaxies Galaxies are a collection of stars, gas and dust held together by gravity Our star, the sun, is one of 100 million stars in the Milky Way.
Lecture 6: Weighing Galaxies --Dark Matter Astronomy 5: The Formation and Evolution of the Universe Sandra M. Faber Spring Quarter 2007 UC Santa Cruz.
Stellar Birth By: Scott M & Jeremy B By: Scott M & Jeremy B.
The origins of the planets Star nurseries in the constellation Sagittarius.
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.
Stars are formed from _______ ___ and ____ coming together due to _______. All stars begin with the _______ ______. What happens then depends on the ____.
ASTR Fall Semester Joel E. Tohline, Alumni Professor Office: 247 Nicholson Hall [Slides from Lecture18]
Astronomy 1143 – Spring 2014 Lecture 21: The Evidence for Dark Matter.
Spiral Galaxy - Canis Venitici We can only see about 1/6 (ca 6000ly) of the way to the Galctic Centre due to scattering by gas and dust in the disk.
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 Big Bang.  Cosmology – The study of the structure and evolution of the universe.  Big Bang Theory – The universe was very hot and small. Billions.
The Milky Way Galaxy. What are each of these?
Dark Energy and Dark Matter International Conference on General Relativity: Centennial Overviews and Future Perspectives December 21 (Mon) ~ December 23.
What Are the Spiral Nebulae?. Two Questions (~1920) We see spiral nebulae in the night sky. It is apparent that they are flat. 1. Are they small objects.
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.
Lecture 32- Properties of the Milky Way (cont)
Galaxies and the Universe
Title: 30.1 Galaxies and The Universe
Galaxies.
Star Notes.
Structure, Types, Known Galaxies
Presentation transcript:

An external galaxy; a spiral like our own.

Which way does it rotate?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve? WRONG!

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

An edge-on spiral; we can measure its rotation

An external galaxy; a spiral like our own. How does it rotate? i.e. what is rotation curve?

We believe that only 10% of the mass of this object is baryonic matter (in the form of stars, stellar remnants, interstellar gas, interstellar dust) and the other 90% is “dark matter”

Vera Rubin showed that 90 % of a typical galaxy’s mass is “ dar k matter ”

Except for the closest few galaxies, they are all moving away from us (fast!)

Last 4 lectures - cosmology monday wednesay friday monday 3/6