Lecture 31 – Structure of the Milky Way. Let’s check our answer

Slides:



Advertisements
Similar presentations
Chapter 15: The Milky Way Galaxy
Advertisements

Slide 1 Andromeda galaxy M31Milky Way galaxy similar to M31.
Chapter 15 The Milky Way Galaxy.
Copyright © 2010 Pearson Education, Inc. Dark Matter and Dark Energy.
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.
Where Is Our Solar System Located Within Our Galaxy? (C) Copyright all rights reserved
The Size and Structure of the Milky Way Galaxy We live in a new class of astronomical object.
The Milky Way Galaxy Shape & Size Structure & Contents Stellar Populations Gas & Dust Motion of Stars & Gas The Galactic Center Formation.
Unit 6 Galaxies *Basic Galaxy Info. *Types of Galaxies -Characteristics of The Milky Way (Spiral Galaxies) *Red Shift & Hubble’s Law.
THE MILKY WAY Our Home Galaxy GALAXIES 3 Main Types Spiral/Barre d Elliptical Irregular.
Galaxies are collections of stars (between 200 billion and 400 billion) that all rotate (orbit) around a massive central point.
The Expanding Universe. The Doppler Effect  Relative motion affects wavelength affects wavelengthaffects wavelength  Cars  Trains  Stars!  Galaxies!
The Nature of Galaxies Chapter 17. Other Galaxies External to Milky Way –established by Edwin Hubble –used Cepheid variables to measure distance M31 (Andromeda.
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.
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.
Electromagnetic Spectrum
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.
What is the Milky Way? WHERE ARE WE IN THE MILKY WAY? How do we know?
What does our galaxy look like?
An Expanding Universe Redshift, Blueshift and the Doppler Effect.
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.
Stars & Galaxies in Motion 6:30 Wednesday, October 15 Next Planetarium Show: tonight, 6:30 pm.
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.
10.2 Galaxies Our star, the sun, is one of billion stars in the Milky Way galaxy, and there are 125 billion galaxies in the universe! See pages.
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.
Milky Way: Galactic Structure and Dynamics Milky Way has spiral structure Galactic Bulge surrounds the Center Powerful radio source Sagittarius A at Center.
The Milky Way Galaxy. What are each of these?
NOTES: The Galactocentric Perspective The Milky Way: Herschel The slab universe Kapteyn The red blood cell universe Harlow Shapley We.
The Milky Way And other galaxies.
Galaxies and the universe
© 2017 Pearson Education, Inc.
Universe Fact File WebPages on slides.
Lecture 30- The Structure of the Milky Way Galaxy
Galaxies and the Universe
Galactic Structure.
Lecture 32- Properties of the Milky Way (cont)
Formation of the Universe
The Universe Chapter 25.3.
Galaxies and the Universe
The Milky Way, Deep Space, and Beyond!
Origin of the Universe.
How Can We Find the Center of Our Galaxy?
Spiral Arms.
Milky Way Orbits of stars in the Milky Way Rotation curves
Properties of light.
The Sun and Light Years.
Our Milky Way Galaxy.
Redshift Ms. Griswold 5/14/2014.
GALAXIES OF STARS & OUR UNIVERSE
GALAXIES OF STARS & OUR UNIVERSE
Chapter 14 Spiral Galaxy.
Chapter 14 Our Galaxy.
Galaxies.
Unit 11- Characteristics of the Universe
The Universe Chapter 25.3.
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.
20.2 The Milky Way and Other Galaxies
Lecture 33- What’s the Milky Way made of?
Science behind fissures
Properties of light Optics Unit.
The Milky Way Our home galaxy.
Lesson 5 Splash galaxy Milky Way spectrum expansion redshift big bang
Galaxies.
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.
Shapes, composition and motion of stars and galaxies
Today’s Agenda… Bellringer: How are comets and meteorites different? Which one do we refer to as a shooting star? Review yesterday’s topics Notes on Galaxies.
Presentation transcript:

Lecture 31 – Structure of the Milky Way. Let’s check our answer Are there other objects in the sky which resemble the MW?

M31 The Andromeda Galaxy

M104 The Sombrero Galaxy

The Sky is filled with objects with the same shape and size of the Milky Way. The term for these objects is spiral galaxy. So we figured out the structure of the MW pretty well from the inside, and there is a universe filled with similar objects

Next topic: motions of stars in galaxies There are internal motions In galaxies, a “procession of stars”. How can we tell?

The Doppler Effect (p104) If a source of waves is in motion with respect to an observer, the observer measures a different wavelength than was emitted

The Doppler Effect: Say it in equations W-W0 V W0 c DEMO

How the Doppler Effect effects spectral lines

Results for the motion of the Sun in the Milky Way Doppler shifts measured for many objects outside the Milky Way, or not a part of the galactic disk. The Sun is moving on an orbit around the galactic center at a speed of V=220 km/sec The motion of our orbit is in the direction of Cygnus

An independent proof that the Sun is moving on an orbit in the Milky Way DEMO VLBI observations