At the Center of the Galaxy!. Galaxy Centers are Mysterious and Wild Below is a picture of where the Galaxy center is with respect to the horizon (for.

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

Chapter 21: The Milky Way. William Herschel’s map of the Milky Way based on star counts In the early 1800’s William Herschel, the man who discovered the.
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 15 The Milky Way Galaxy.
ASTR100 (Spring 2008) Introduction to Astronomy The Milky Way Prof. D.C. Richardson Sections
14.2 Galactic Recycling Our Goals for Learning How does our galaxy recycle gas into stars? Where do stars tend to form in our galaxy?
A105 Stars and Galaxies  Milky Way Homework (#11) due today  Projects Due Nov. 30  For next week: Units 74, 75, 76, 78, 79  “rooftop” tonight, 8 PM,
© 2010 Pearson Education, Inc. The Milky Way. © 2010 Pearson Education, Inc. Dusty gas clouds obscure our view because they absorb visible light. This.
Lecture Outline Chapter 15: Our Galaxy © 2015 Pearson Education, Inc.
AST101 The Evolution of Galaxies. Virgo Cluster Collisions of Galaxies Outside of Clusters (the field), most galaxies are spiral or irregular In dense.
QUASARS Monsters of the ancient Universe Professor Jill Bechtold Steward Observatory Tucson Amateur Astronomers, Dec. 6, 2002.
The Milky Way PHYS390 Astrophysics Professor Lee Carkner Lecture 19.
15 The Milky Way More than just a candy bar.. 15.
Galaxies and the Foundation of Modern Cosmology III.
The Milky Way II What do halo stars tell us about our galaxy’s history? How did our galaxy form?
11 Black Holes and General Relativity Stuff that warps your mind.
The Milky Way Center, Shape Globular cluster system
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 Immanuel Kant (1724 – 1804) German philosopher The infinitude of creation is great enough to make a world, or a Milky Way of worlds,
The Milky Way Galaxy.
Our Galaxy The Milky Way. 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.
The Milky Way Our Galaxy Please press “1” to test your transmitter.
The Milky Way Galaxy Chapter 12:. 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.
What’s Brewing in the Teapot? M7 M6 M8 M22 Caty Pilachowski IU Astronomy.
© 2010 Pearson Education, Inc. Chapter 19 Our Galaxy.
The Galactic Centre: a hidden treasure How can we study the Galactic centre? How can we study the Galactic centre? What is do we find there? What is do.
30 Galaxies and the Universe Section 30.1: The Milky Way Galaxy
GALAXIES. A GALAXY IS A massive group of stars held together by their mutual gravity.
The Milky Way Galaxy.
The Milky Way Appears as a band of light stretching across the sky There are dark regions along the band, giving the appearance of a lack of stars This.
Ch. 14. The Milky Way Ch. 14. Ch. 14 OUTLINE Shorter than book 14.1 The Milky Way Revealed 14.2 Galactic Recycling (closely related to Ch. 13) 14.3 The.
Galaxies Astronomy 100. What is a “star cluster”? stars formed together at same time stars may be gravitationally bound together two types: open (galactic)
Galaxies are collections of stars (between 200 billion and 400 billion) that all rotate (orbit) around a massive central point.
 Einstein views Gravity NOT as a force, but as a bending of spacetime  It still affects how things move, but not as an attractive force  It is.
Galaxies Miss Scillieri 6 th Grade Science Memorial School.
Location and Motion of the Solar System. Where are we? Our solar system is located in the outer reaches of the Milky Way Galaxy, which is a spiral galaxy.
Tour of the Invisible Universe From the Moon to Beyond.
Copyright © 2012 Pearson Education, Inc. Chapter 14 Our Galaxy.
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.
Chapter 14 The Milky Way Galaxy What do you think? Where in the Milky Way is the solar system located? How fast is the Sun moving in the Milky Way? How.
Introduction to Galaxies 5/23/2013. BR: Milky Way Scale The Milky Way has a diameter of approximately 8.25 x 10 9 AU (8.25 billion AU). 206,265 AU = 3.26.
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.
15.4 Quasars and Other Active Galactic Nuclei Our Goals for Learning What are quasars? What is the power source for quasars and other active galactic nuclei?
ASTR112 The Galaxy Lecture 7 Prof. John Hearnshaw 11. The galactic nucleus and central bulge 11.1 Infrared observations (cont.) 11.2 Radio observations.
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.
Galaxies GALAXIES Stars are not randomly sprinkled throughout the universe. Most astronomers agree that there are about 100 billion galaxies in the universe,
Chapter 19 Our Galaxy.
Earth & Space Science March 2015
Supermassive Black Holes Preserving a Galactic Treasure.
“OUR GALAXY” Definition of a Galaxy: a huge group of individual stars, star clusters, dust, and gas bound together by gravity.
UNIT 1 The Milky Way Galaxy.
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.
AST101 Lecture 19 Discovery of the Galaxy. Northern Milky Way.
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.
Copyright © 2010 Pearson Education, Inc. Chapter 14 The Milky Way Galaxy Lecture Outline.
The Milky Way Galaxy. What are each of these?
© 2017 Pearson Education, Inc.
Galaxies.
More than just a candy bar.
Chapter 19 Our Galaxy.
Multiwavelength Images
Chapter 15 Our Galaxy.
Milky Way Orbits of stars in the Milky Way Rotation curves
Our Milky Way Galaxy.
Pop-quiz #5 Which of the following statements is FALSE?
The Milky Way Galaxy.
Types of galaxies.
Presentation transcript:

At the Center of the Galaxy!

Galaxy Centers are Mysterious and Wild Below is a picture of where the Galaxy center is with respect to the horizon (for our latitude of 40 o North). Note the constellations of Sagittarius and Scorpius. This visible photograph shows the Galactic center. In this photo it would appear there is not much going on. WRONG. The dust and gas block our view!

Dust Emission! Dust radiates at about 4000 nm (visible is nm). The Galaxy center is bright in this “dust shine”. Most features are supernova remnants. The channeled look of the gas suggests that magnetic fields are at work.

Zooming in on a Radio Image of Sgr A radio infrared

Sgr A is the most central object in our Galaxy. This is a spiral swirl of gas around an intense radio source. The arms of the swirl are streaming into the center. It is thought that this is where a 3 million solar mass black hole lives.

The center of less than 4 AU in diameter. The emitted light suggests that there are many stars in the disk. These stars are so packed that they are 1000 AU apart (whereas stars near the sun are 330,000 AU apart. Though material around Sgr A is moving fast, the center is not moving, suggesting that it is very massive. Stars in this disk are orbiting about every 2.8 years (until they are sucked in to the black hole). Suggests a Black Hole in Center Evaluating the Black Hole Hypothesis

The location of the Black Hole