Presentation is loading. Please wait.

Presentation is loading. Please wait.

Gerald-rhemann-4apr-02.

Published byMargaret Chase Modified over 5 years ago

Similar presentations

Presentation on theme: "Gerald-rhemann-4apr-02."— Presentation transcript:

1 Gerald-rhemann-4apr-02

2

3 http://sydfish. wordpress

4

5 http://boojum. as. arizona

6 ARE most white dwarf stars in the plane of the disk or in the bulge
ARE most white dwarf stars in the plane of the disk or in the bulge? Do the ages and masses of white dwarf stars change with distance from the bulge?

7

8 IRAS_allsky

Download ppt "Gerald-rhemann-4apr-02."

Similar presentations

Astronomy Review. What is gravity? The attractive force between two masses.

Astronomy Review. What is gravity? The attractive force between two masses.
$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.
The Milky Way. Structure of the Milky Way The Milky Way.

The Milky Way. Structure of the Milky Way The Milky Way.
GALACTIC UNIVERSE.

GALACTIC UNIVERSE.
Stars and Galaxies. Gravitational Pull-Key Terms Mass- the amount of atoms inside an object. Mass does not change. Weight- the pull of gravity on the.

Stars and Galaxies. Gravitational Pull-Key Terms Mass- the amount of atoms inside an object. Mass does not change. Weight- the pull of gravity on the.
Chapter 14 Our Galaxy. 14.1 The Milky Way Revealed Our Goals for Learning What does our galaxy look like? How do stars orbit in our galaxy?

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 Shape & Size Structure & Contents Stellar Populations Gas & Dust Motion of Stars & Gas The Galactic Center Formation.

The Milky Way Galaxy Shape & Size Structure & Contents Stellar Populations Gas & Dust Motion of Stars & Gas The Galactic Center Formation.
MILKY WAY GALAXY By: Lauren Reich 3/30/12 www.NASA.gov.

MILKY WAY GALAXY By: Lauren Reich 3/30/12
$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.

$100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300 $400 $500 $100 $200 $300.
Galaxies Chapter 16. Topics Types of galaxies Dark Matter Distances to galaxies Speed of galaxies Expansion of the universe and Hubble’s law.

Galaxies Chapter 16. Topics Types of galaxies Dark Matter Distances to galaxies Speed of galaxies Expansion of the universe and Hubble’s law.
What is the Andromeda Galaxy? The nearest galaxy from our Milky Way. 2.3M light year away. Considered that it has structure similar to our Milky Way. ↓

What is the Andromeda Galaxy? The nearest galaxy from our Milky Way. 2.3M light year away. Considered that it has structure similar to our Milky Way. ↓
THE MILKY WAY Our Home Galaxy GALAXIES 3 Main Types Spiral/Barre d Elliptical Irregular.

THE MILKY WAY Our Home Galaxy GALAXIES 3 Main Types Spiral/Barre d Elliptical Irregular.
Clusters Small collection of stars… thousands to millions 2 Types: 1. Open 2. Globular.

Clusters Small collection of stars… thousands to millions 2 Types: 1. Open 2. Globular.
MILKY WAY Period 1 Caitlin and Hiromi Period 1 Caitlin and Hiromi.

MILKY WAY Period 1 Caitlin and Hiromi Period 1 Caitlin and Hiromi.
Where does our Sun plot on the H-R Diagram? Temperature.

Where does our Sun plot on the H-R Diagram? Temperature.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.

Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 14 The Milky Way Galaxy.
Try This!  How did our solar system form? Solar System Formation  Early universe – hot cloud of mostly hydrogen and helium  Gases clump to form nebula.

Try This!  How did our solar system form? Solar System Formation  Early universe – hot cloud of mostly hydrogen and helium  Gases clump to form nebula.
Galaxies CHAPTER 4 SECTION 3. Milky Way galaxy  The Sun and our solar system are located in the Milky Way galaxy.  Milky Way is shaped like a disk with.

Galaxies CHAPTER 4 SECTION 3. Milky Way galaxy  The Sun and our solar system are located in the Milky Way galaxy.  Milky Way is shaped like a disk with.
Goal to understand the scale of the universe

Goal to understand the scale of the universe
Galaxies and Stars.

Galaxies and Stars.

Similar presentations

Ads by Google