2. Chapter 14 The Milky Way Galaxy

3. 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 many stars are in the Milky Way Galaxy?

4. A B Which is a picture of the Milky Way? A is what we see from Earth inside the Milky Way while B is what the Milky Way “might” look like if we were far away looking back at our own galaxy from some other galaxy.

5. Enormous clouds of dust obscure our view of most of the stars in our Galaxy The Milky Way is composed of all the stars in our galaxy, nearly 400 billion. All the stars you can see in the sky are in our Galaxy.

6. Interstellar dust hides the true extent of the Milky Way This dust makes it difficult to determine distances to stars (using the variable star period-luminosity relationship) because dust impedes our accurate measurement of brightness. This dust makes it nearly impossible to “see” what is at the center of our galaxy.

7. Distance measurements to globular clusters define the location of the galactic center. Globular clusters form a sphere around the center of the Milky Way. In 1917, Harlow Shapley determined distances to globular clusters by finding variable stars and used the period-luminosity relationship. The center of this distribution shows the location of the galactic center.

8. The center of the distribution of globular clusters shows the location of the Milky Way’s center. globular clusters galactic nucleus nuclear bulge spiral arms disk note position of the Sun, just over half way out.

9. Looking for 21-cm wavelengths of light … –emitted by interstellar hydrogen –as we look along the disk of the Milky Way (from inside), we see 21-cm photons Doppler shifted varying amounts –this allows the interstellar hydrogen to be mapped Radio observations help map the galactic disk

10. A Map of the Milky Way Based on 21-cm wavelength light mapping

11. Spiral Galaxy M83 observed in both visible light and radio wavelengths.

12. Do galaxies look like they spin? If so, in which sense?

13. Differential Rotation of the Galaxy The Sun orbits at 230 km/s or about 500,000 mph

14. The Galaxy’s Rotation Curve

15. Most of the matter in the Galaxy has not yet been identified According to Kepler’s Third Law, the farther a star is from the center, the slower it should orbit Observations show that speed actually increases with distance from the center This could be due to gravity from extra mass we cannot see - called D ARK M ATTER.

16. The galactic nucleus is also still poorly understood because dust obscures our view The center is located near the constellation of Sagittarius.

17. Infrared wave- lengths from the center can penetrate dust reasonably well.

18. Radio wavelengths from the center can penetrate dust reasonably well.

19. What exactly is at the Center? ???????? We observe gas flying around the center at enormous speeds of 200 km/s It would take about a million times the mass of the Sun to keep it from flying out of the center. A black hole? We observe supermassive black holes in the center of other galaxies. New X-ray telescopes are being designed to look carefully at exactly what the gas at the center is doing.

20. What did you think? Where in the Milky Way is the solar system located? The solar system is about 28,000 ly from the center of the Galaxy near the Orion spiral arm. How fast is the Sun moving in the Milky Way? The Sun orbits the center of the Milky Way Galaxy at a speed of 828,000 km per hour. How many stars are in the Milky Way Galaxy? The Milky Way has more than 200 billion stars.

21. Self-Check 1: Draw and label diagrams of the Milky Way from top and side views, showing the major components. Indicate the approximate dimensions of the components and note the location of the Sun in each diagram. 2: Describe the galactic distribution of general interstellar material, nebulae, and open and globular star clusters. Specify the defining physical characteristics of each. 3: Define differential rotation and discuss the observations used to establish the rotation curve of the galaxy and its value in probing the structure of the Milky Way. 4: Discuss the “missing mass” problem. 5: Describe what might be at the center of the galaxy.