Answers to PROBLEM SET #6
APAS 1200

1. Estimate the radius of the Earth if it were collapsed to the density of a Neutron Star.

kg/m3

Volume Earth = 6x1024kg/2x1018kg/m3 = 3x106m3

1.33pr3 = 3x106m3

r = 100m

2. Why is it that a white dwarf can be formed without the violence of a supernova explosion, but a neutron star cannot?

The electron degeneracy of a white dwarf is built up slowly in the center of a star. The only way to reach neutron degeneracy is through the sudden collapse of electron degeneracy.

3. Calculate the thermal luminosity of a neutron star with a 10km radius and a surface temperature of 5000K. Compare to the Sun.

L=sAT4=5.7x10-8x4px(104)2x(5000)4=4.5x1016W

Lns = 10-10Lsun

4. An 8km radius neutron star is spinning 1000 times per second. Calculate the speed of a point on its equator. Compare to the speed of light.

Circumference = 2pr = 50km

At 1000 per second, v = 50,000km/s

V = .16c

5. Given that the Schwarzschild radius for the Sun is 3km, and radius is proportional to mass, calculate the Schwarzschild radius of a 100kg human and a 1011 solar mass galaxy.

Rhuman = 3000m x 100kg / 2x1030kg = 1.5x10-25 m

Rgalaxy = 3km x 1011 = 3x1011 km

6. Using Newtons Laws, and the formula for the Schwarzschild radius, calculate the acceleration due to gravity at the surface of a one solar mass black hole. Redo for a 1012 solar mass black hole.

a = 1.5x1013x1012/1024 = 15m/s2 = 1.5 x gravity of Earth