1. The Life Cycles of Stars and our Sun

2. Your Questions 1.Have you ever heard of the sun song by the group They Might be Giants?

3. `Fun websites’: http://www.asu.edu/clas/hst/www/ahah/ Appreciating Hubble at Hyper-speed http://www.stsci.edu/outreach/

4. 1. How are distances between galaxies and between galaxy clusters calculated? The Hubble Flow v = H o d (H o = 71 km/s/Mpc) d d 1 2 1.Observer 1 sees both galaxies at distance d with speed v 2.Observer 2 sees the furthest galaxy at distance 2d, with speed 2v v v

5. 2. Elaborate on the difference between the Dark Matter theory and the MOdified Newtonian Dynamics theory (MOND).

6. Describing Motion Motion is when the position of an object changes in time If position does not change, the object is at rest The describe motions we need to monitor position and time The rate at which an objects covers a given amount of space in a given amount of time is called speed v = d/t (when you add a direction to speed, it is called velocity)

7. Acceleration An acceleration is a change in velocity. Acceleration occurs when either the magnitude or direction of the velocity (or both) are altered. Uniform Circular Motion is Accelerated Motion

8. Acceleration and Force An object in constant velocity (or at rest) has no force acting on it. Or: if an object is being accelerated, there must be a net force acting on it (Newton’s first law) Acceleration is caused by force but also related to the mass of the object (Newton ’ s second law) Force = Mass x Acceleration F = m·a Or a = F/m

9. The gravitational force on an object near the surface of Earth is: F grav = m·g (g = 9.8m/s 2 )

10. Gravity We can summarize the universal law of gravitation with the following statements: –Every mass attracts every other mass through the force of gravity. –If mass #1 exerts force on mass #2, and mass#2 exerts force on mass#1, the force must depend o both masses, namely: –The force of attraction is directly proportional to the product of the two masses. –The force of attraction is inversely proportional to the square of the distance between the masses.

11. The Law of Gravity d M1M1 M2M2 G = 6.67x10 -11 m 3 /kg/s 2 Near Earth’s surface

12. … so why don’t planets just fall into the sun? M1M1 M2M2

13. … because they miss it! M1M1 M2M2 v This is the concept of an orbit: M 2 is being attracted by M1, which causes an acceleration, but has sufficient tangential velocity that the `fall’ becomes an orbit FgFg FgFg

14. The same is true for galaxies: Their stars rotate around their center of mass. If you know the distance of your star from the center, R, and its speed, v, you can calculate the mass of the galaxy contained within the radius R: R M(<R) = v 2 R / G And the acceleration: a= v 2 / R For the sun: M(<8kpc) = 9x10 10 M sun a = 2.5x10 -8 cm/s 2

15. …and when you reach the edges of galaxies… The `flat rotation curve’ seen beyond the visible edges of galaxies does not agree with the expectation that the galaxy `ends’. In this case one would expect a trend: v ~ R (-1/2)

16. 1.DM: F g = ma = GMm/r 2, a= GM/r 2 (gravitational force) F c = m v 2 / r (centripetal force) Flat rotation curves imply `unseen’ mass in galaxies 2. MOND: F = m  (a/a o ) a = GMm/r 2 a o = 1.2 10 -8 cm s -2 Flat rotation curves stem from very small accelerations at the edges of galaxies, where the Newtonian dynamics is modified to imply: a= (Gma o ) (1/2) / R and v ~ const.

17. Current difficulties for MOND: 1.Gravitational lensing: (still in progress; recent MOND covariant formulation) 2. Density profiles of galaxy clusters