Answer:
a).
b).
Explanation:
Using the conservation of energy and the kinetic energy of the satellite around the asteroid can model the motion in




a).



b).



Answer:
50joules
Explanation:
See the explanation from the image I have provided above.
Most of the mass is located in the nucleus as suggested by Rutherford's gold foil experiment.
Initial velocity, u = 0
Final velocity, v = 60 m/s (at take off)
Duration of the acceleration, t = 4 s
Calculate average acceleration.
a = (v - u)/t
= (60 m/s)/(4 s)
= 15 m/s²
Calculate the distance traveled during acceleration.
s = ut + (1/2)*a*t²
= 0.5*(15 m/s²)*(4 s)²
= 120 m
Answer: 120 m
The hotter star will be 16 times more luminous - luminosity depends on two things - the size of the star and the temperature of the star. The hotter a star is, the more energy it will give out. This will give rise to greater luminosity.