26.11.2012 Views

Chapter 11 Gravity

Chapter 11 Gravity

Chapter 11 Gravity

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Substitute for cosθ and simplify to<br />

obtain:<br />

Substitute in equation (1) and<br />

simplify:<br />

General Problems<br />

r<br />

F<br />

C<br />

GMm<br />

=<br />

2 ⎛ 2 R ⎞<br />

4 ⎜<br />

⎜d<br />

+<br />

4 ⎟<br />

⎝ ⎠<br />

GMmd<br />

=<br />

2 ⎛ 2 R ⎞<br />

4 ⎜<br />

⎜d<br />

+<br />

4 ⎟<br />

⎝ ⎠<br />

3 / 2<br />

d<br />

2<br />

iˆ<br />

d<br />

R<br />

+<br />

4<br />

r GMm<br />

F iˆ<br />

GMmd<br />

= − + 2<br />

d<br />

2 ⎛ 2 R ⎞<br />

4 ⎜<br />

⎜d<br />

+<br />

4 ⎟<br />

⎝ ⎠<br />

=<br />

⎡<br />

⎢<br />

GMm ⎢<br />

− 1 2 ⎢ −<br />

d<br />

⎢ ⎧<br />

⎢<br />

⎨d<br />

⎣ ⎩<br />

2<br />

<strong>Gravity</strong><br />

2<br />

iˆ<br />

3 / 2<br />

3<br />

d<br />

4<br />

2<br />

R ⎫<br />

+<br />

4<br />

89 •• A neutron star is a highly condensed remnant of a massive star in the<br />

last phase of its evolution. It is composed of neutrons (hence the name) because<br />

the star’s gravitational force causes electrons and protons to ″coalesce″ into the<br />

neutrons. Suppose at the end of its current phase, the Sun collapsed into a neutron<br />

star (it can’t in actuality because it does not have enough mass) of radius 12.0 km,<br />

without losing any mass in the process. (a) Calculate the ratio of the gravitational<br />

acceleration at the surface of the Sun following its collapse compared to its value<br />

at the surface of the Sun today. (b) Calculate the ratio of the escape speed from<br />

the surface of the neutron-Sun to its value today.<br />

Picture the Problem We can apply Newton’s second law and the law of gravity<br />

to an object of mass m at the surface of the Sun and the neutron-Sun to find the<br />

ratio of the gravitational accelerations at their surfaces. Similarly, we can express<br />

the ratio of the corresponding expressions for the escape speeds from the two suns<br />

to determine their ratio.<br />

(a) Express the gravitational force<br />

acting on an object of mass m at the<br />

surface of the Sun:<br />

Solving for ag yields:<br />

GM<br />

F g = mag<br />

=<br />

R<br />

Sun<br />

2<br />

Sun<br />

Sun<br />

2<br />

Sun<br />

m<br />

⎬<br />

⎭<br />

iˆ<br />

3 / 2<br />

⎤<br />

⎥<br />

⎥<br />

iˆ<br />

⎥<br />

⎥<br />

⎥<br />

⎦<br />

GM<br />

a g = (1)<br />

R<br />

239

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!