Chapter 14: The Milky Way Galaxy The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

Galaxies & the Universe
LECTURE 21, NOVEMBER 16, 2010 ASTR 101, SECTION 3 INSTRUCTOR, JACK BRANDT 1ASTR 101-3, FALL 2010.
Astro1010-lee.com UVU Survey of Astronomy Chapter 21 Our Milky Way.
Galaxy Classification
Our Galaxy `. Interstellar dust obscures our view at visible wavelengths along lines of sight that lie in the plane of the galactic disk.
Introduction to Astrophysics Lecture 13: The Milky Way Galaxy.
Chapter 20 Dark Matter, Dark Energy, and the Fate of the Universe.
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 17.
The Milky Way Galaxy Astronomy 315 Professor Lee Carkner Lecture 16.
Chapter 23: Our Galaxy Our location in the galaxy Structure of the galaxy Dark matter Spiral arm formation Our own supermassive black hole.
The Mass of the Galaxy We can use the orbital velocity to deduce the mass of the Galaxy (interior to our orbit): v orb 2 =GM/R. This comes out about 10.
The Milky Way Galaxy 19 April 2005 AST 2010: Chapter 24.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 23 Our Galaxy CHAPTER 23 Our Galaxy.
The Milky Way Galaxy Astronomy 315 Professor Lee Carkner Lecture 17.
Stellar Kinematics Astronomy 315 Professor Lee Carkner Lecture 18.
9B The Milky Way Our Galactic Home. 9B 9B Goals Structure of our Galaxy. Its size and shape. How do stars and things move through it? Mass and Dark Matter.
The Milky Way Center, Shape Globular cluster system
Chapter 31 Galaxies & the Universe Review & Recap It does this by precisely measuring the speed of gas and stars around a black hole. This provides clues.
The Milky Way I AST 112 Credit: Stephane Vetter.
Levels of organization: Stellar Systems Stellar Clusters Galaxies Galaxy Clusters Galaxy Superclusters The Universe Everyone should know where they live:
The Milky Way Galaxy.
Virtually all galaxies show a flat rotation curve.
M 51. M 51 Galaxy merger simulation.
Chapter 21 Section 4 Star Systems And Galaxies. Done By Nick White And Gina Heath.
Galaxies. Galaxies A galaxy is a huge region of space that contains hundreds of billions of stars, planets, glowing nebulae, dust, empty space, and possibly.
Galaxies Read Your Textbook: Foundations of Astronomy
 Students will be able to determine the size and shape of our galaxy.  Students will be able to distinguish the different kinds of variable stars. 
GALAXIES From: Jim Lochner, USRA & NASA/GSFC
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.
Chapter 22 Dark Matter, Dark Energy, 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…
The Nature of Galaxies Chapter 17. Other Galaxies External to Milky Way –established by Edwin Hubble –used Cepheid variables to measure distance M31 (Andromeda.
Galaxies GALAXY -comes from the ancient Greeks and their word for “milk”- galactos.
January 2nd 2013 Objective Warm-Up
Galactic Nucleus. Mass of the Galaxy The orbit of clusters can be used to estimate the mass of the galaxy. –Same used for planets and binary stars The.
Planets, Solar Systems, and Galaxies…..Oh my!
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.
“OUR GALAXY” Definition of a Galaxy: a huge group of individual stars, star clusters, dust, and gas bound together by gravity.
Quiz #10 What would really happen to you if you were to fall all the way into the Event Horizon of a black hole? We know the gravity is unbelievably strong.
Harry Kroto ifa.hawaii.edu Harry Kroto 2004
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Our Milky Way Galaxy. The Milky Way Almost everything we see in the night sky belongs to the Milky Way. We see most of the Milky Way as a faint band of.
Dark Matter and Rotational Motion e.t. revised feb 09.
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?
Universe Tenth Edition
Milky Way: Galactic Structure and Dynamics Milky Way has spiral structure Galactic Bulge surrounds the Center Powerful radio source Sagittarius A at Center.
Our Galaxy Chapter Twenty-Five. Guiding Questions 1.What is our Galaxy? How do astronomers know where we are located within it? 2.What is the shape and.
Chapter 28 Our Solar System. Big Idea: Using the laws of motion and gravitation, astronomers can understand the orbits and the properties of the planets.
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?
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.
The Milky Way. The Milky Way: Our Home Galaxy What are the different components of the Milky Way? How do we see those components? What does a map of each.
Formation of the Solar System and The Universe. Our Solar System Sun is the center of a huge rotating system of: Sun is the center of a huge rotating.
NOTES: The Galactocentric Perspective The Milky Way: Herschel The slab universe Kapteyn The red blood cell universe Harlow Shapley We.
Formation of the Solar System and The Universe
News flash ALMA observes a protoplanetary disk around the young star HL Tauri. This is the first time we can DIRECTLY actually observe a planetary system.
© 2017 Pearson Education, Inc.
Formation of the Solar System and The Universe
Discussion Most bright galaxies are spirals. What do you think causes these galaxies to have a spiral pattern?
The Milky Way Our home galaxy, full of stars, gas and mysterious dark matter We decompose it into a disk and a halo and a few other parts.
Dark Matter Join me on the Dark Side.
WHAT IS….. DARK MATTER??.
Our Milky Way Galaxy.
Dark Matter Join me on the Dark Side.
The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud of gas and dust, shrinks under its.
Section 5 – pg 622 The Expanding Universe
Formation of Our Solar System
Dust Dust cloud The disk Lots of dust in spiral galaxies The bulge
The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud of gas and dust, shrinks under its.
Presentation transcript:

Chapter 14: The Milky Way Galaxy The scenario for the formation of galaxies is very reminiscent of the formation process for solar systems. Giant cloud of gas and dust, shrinks under its own gravity, rotation produces a flattened disk. The halo objects probably formed first and retained their spherical distribution and didn’t get pulled into the disk.

Chapter 14: The Milky Way Galaxy Spectroscopic radio astronomy allows astronomers to look through our galaxy and see the Doppler velocities of hydrogen through its 21 cm spin-flip line. With this information astronomers can recreate the 3 dimensional structure of our galaxy including the number of spiral arms, etc. This is what we think our galaxy looks like.

Chapter 14: The Milky Way Galaxy Astronomers still can’t explain well why we have spiral arms in galaxies. The stars, gas, and dust in the galaxy all obey Kepler’s laws of planetary motion. Thus the inner matterial rotates faster than the outer matterial. If spiral arms were tied to the galaxy then after a few 100,000,000 years they would all be wound up and loose their shape.

Chapter 14: The Milky Way Galaxy The density wave theory says that a compression front moves through the disk and compresses the gas and dust to start the star formation process. In this model new matterial is being constantly fed into the density regions as old matterial leaves.

Chapter 14: The Milky Way Galaxy Since matterial orbiting the galaxy must obey Kepler’s laws, if we could measure the distance and orbital period of matterial as a function of distance from the center, we could determine the amount of mass inside that distance. When we reach the “edge” of the galaxy, we expect the rotation speed to diminish, but instead it keeps on increasing as if there is some “invisible” (dark) matter.

Chapter 14: The Milky Way Galaxy One attempt to detect dark matter is to look for gravitational lensing. Even if the matter is dark it should disturb the space-time continuum and produce gravity like any other matter. While we have seen several such events, they could only account for about 1/2 the dark matter.