17
The Life Cycles of Stars The Life Cycles of Stars and our Sun and our Sun

The Life Cycles of Stars and our Sun

  • Upload
    miette

  • View
    25

  • Download
    0

Embed Size (px)

DESCRIPTION

The Life Cycles of Stars and our Sun. Your Questions. Have you ever heard of the sun song by the group They Might be Giants?. `Fun websites’:. http://www.asu.edu/clas/hst/www/ahah/ Appreciating Hubble at Hyper-speed. http://www.stsci.edu/outreach/. - PowerPoint PPT Presentation

Citation preview

Page 1: The Life Cycles of Stars and our Sun

The Life Cycles of StarsThe Life Cycles of Starsand our Sunand our Sun

Page 2: The Life Cycles of Stars and our Sun

Your Questions 1. Have you

ever heard of the sun song by the group They Might be Giants?

Page 3: The Life Cycles of Stars and our Sun

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

http://www.stsci.edu/outreach/

Page 4: The Life Cycles of Stars and our Sun

1. How are distances between galaxies and between galaxy clusters calculated? The Hubble Flow

v = Ho d (Ho = 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

Page 5: The Life Cycles of Stars and our Sun

2. Elaborate on the difference between the Dark Matter theory and the MOdified Newtonian Dynamics theory

(MOND).

Page 6: The Life Cycles of Stars and our Sun

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)

Page 7: The Life Cycles of Stars and our Sun

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

Page 8: The Life Cycles of Stars and our Sun

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

Page 9: The Life Cycles of Stars and our Sun

The gravitational force on an object nearthe surface of Earth is:

Fgrav = m·g (g = 9.8m/s2)

Page 10: The Life Cycles of Stars and our Sun

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.

Page 11: The Life Cycles of Stars and our Sun

The Law of Gravity

221

d

MMGFg =

d

M1M2

G = 6.67x10-11 m3/kg/s2

2

21

2

9.8m/s=

=

=

dM

Gg

gMFg

Near Earth’s surface

Page 12: The Life Cycles of Stars and our Sun

… so why don’t planets just fall into the sun?

M1M2

Page 13: The Life Cycles of Stars and our Sun

… because they miss it!

M1M2

v

This is the concept of an orbit: M2 is being attracted by M1, which causes an acceleration, but has sufficient tangential velocity that the `fall’ becomes an orbit

Fg Fg

Page 14: The Life Cycles of Stars and our Sun

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) = v2 R / G

And the acceleration: a= v2 / R

For the sun:M(<8kpc) = 9x1010 Msun

a = 2.5x10-8 cm/s2

Page 15: The Life Cycles of Stars and our Sun

…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)

Page 16: The Life Cycles of Stars and our Sun

1. DM: Fg = ma = GMm/r2 , a= GM/r2 (gravitational force) Fc = m v2 / r (centripetal force) Flat rotation curves imply `unseen’ mass in galaxies

2. MOND: F = m (a/ao) a = GMm/r2

ao = 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= (Gmao)(1/2) / R and v ~ const.

Page 17: The Life Cycles of Stars and our Sun

Current difficulties for MOND:

1. Gravitational lensing: (still in progress; recent MOND covariant formulation)

2. Density profiles of galaxy clusters