1. The Size and Structure of the Milky Way Galaxy We live in a new class of astronomical object

2. First… an advertisement for 29:52 “Exploration of the Solar System” The other half of astronomy

3. Observations indicate the shape and size of the Milky Way Galaxy

4. Structure of the Milky Way Disk Bulge Galactic center Galactic halo Question: what simple observation Is consistent with a part of this picture?

5. A view of the Milky Way with an artist’s touch

6. Next topic: the motion of the Sun in the Milky Way (leads to something extremely interesting) How does the Sun move in the Milky Way?

7. Next topic: the motion of the Sun in the Milky Way (leads to something extremely interesting) How does the Sun move in the Milky Way? V=220 km/sec The sun moves in response to the gravitational force of All the rest of the mass in the galaxy

8. How is the mass distributed? How could we tell?

9. Force of Gravity acts on the Sun and all objects in the Galaxy Gravity has magnitude and direction

10. Sun responds to net force by moving on circular path around the galactic center

11. Mass distributions like 1,2, and 3 give circular orbits with V(R) A plot of V versus R is called a rotation curve

12. The Observed Case for the Milky Way No sign of the “root-R falloff”

13. Significance of the Rotation Curve for the Milky Way Rotation curve stays high outside the bulk of the stars Mass indicated by the rotation curve exceeds that in stars Most of the mass of the Milky Way is in an unknown form of “Dark Matter”

14. The New View of the Milky Way Dadark matter halo

15. Dark Matter: A Major Problem for Contemporary Physics and Astronomy Stars are a small fraction of the mass of major galaxies The dark matter problem becomes more pronounced as you go out in the universe The form of the dark matter is unknown; probably not what you studied in chemistry Possibly/probably an unknown form of elementary particle

16. At the Very Center

17. What do we see at the galactic center (radio and infrared wavelengths? Strong radio source (synchrotron radiation) At infrared wavelengths, can see stars orbiting very vast around Sgr A http://antwrp.gsfc.nasa.gov/apod/ap001 220.htmlhttp://antwrp.gsfc.nasa.gov/apod/ap001 220.html Ten years of observations speeded up

18. The Orbit of Star S2

19. Star S2 passes about as close to Sagittarius A* as the planet Pluto passes to the Sun. Indicates supermassive object in a very small region Andrea Ghez paper