Respuesta :
(a) 0.49
The potential energy of a satellite in orbit is given by
[tex]U=-\frac{GMm}{R+h}[/tex]
where G is the gravitational constant, M is the Earth's mass, m is the satellite's mass, R is the Earth's radius and h is the altitude of the satellite.
The potential energy of satellite A is
[tex]U_A=-\frac{GMm_A}{R+h_A}[/tex]
The potential energy of satellite B is
[tex]U_B=-\frac{GMm_B}{R+h_B}[/tex]
So the ratio of the potential energy of satellite B to that of satellite A is
[tex]\frac{U_B}{U_A}=\frac{m_B}{m_A}\frac{R+h_A}{R+h_B}[/tex]
The two satellites have same mass, [tex]m_A = m_B = m[/tex], so the equation becomes
[tex]\frac{U_B}{U_A}=\frac{R+h_A}{R+h_B}[/tex]
where
[tex]R=6370 km\\h_A = 7580 km\\h_B = 22000 km[/tex]
Substituting into the equation,
[tex]\frac{U_B}{U_A}=\frac{6370 km+7580 km}{6370 km+22000km}=0.49[/tex]
(b) 0.49
The kinetic energy of a satellite in orbit is given by
[tex]K=-\frac{1}{2}U[/tex]
where U is the potential energy.
The kinetic energy of satellite A is
[tex]K_A=-\frac{1}{2}U_A[/tex]
The kinetic energy of satellite B is
[tex]K_B=-\frac{1}{2}U_B[/tex]
So the ratio of the kinetic energy of satellite B to that of satellite A is
[tex]\frac{K_B}{K_A}=\frac{U_B}{U_A}[/tex]
and we already found the value of this ratio in part (a), so this ratio is also equal to 0.49.
(c) Satellite A
The total energy of a satellite in orbit is sum of potential energy and kinetic energy:
[tex]E=U+K=U-\frac{1}{2}U=\frac{1}{2}U[/tex]
We can write therefore the total energy of satellite A as
[tex]E_A=\frac{1}{2}U_A[/tex]
and the total energy of satellite B as
[tex]E_B=\frac{1}{2}U_B[/tex]
The ratio of the total energy of satellite B to that of satellite A is therefore
[tex]\frac{E_B}{E_A}=\frac{U_B}{U_A}=0.49[/tex]
which implies that satellite A has greater total energy then satellite B.
(d) by [tex]1.32 \cdot 10^8 J[/tex]
In order to find the difference between the total energies of the two satellite, we must calculate the exact value for each satellite. Using m = 18.2 kg and [tex]M=5.98\cdot 10^{24}kg[/tex] (Earth's mass), we find:
[tex]E_A = \frac{1}{2}U_A = \frac{1}{2}\frac{GMm}{R+h_A}=\frac{1}{2}\frac{(6.67\cdot 10^{-11})(5.98\cdot 10^{24}kg)(18.2 kg)}{6370\cdot 10^3 m+7580\cdot 10^3 m}=2.60\cdot 10^8 J[/tex]
[tex]E_B = \frac{1}{2}U_B = \frac{1}{2}\frac{GMm}{R+h_B}=\frac{1}{2}\frac{(6.67\cdot 10^{-11})(5.98\cdot 10^{24}kg)(18.2 kg)}{6370\cdot 10^3 m+22000\cdot 10^3 m}=1.28\cdot 10^8 J[/tex]
So the difference between the two energies is
[tex]\Delta E=2.60\cdot 10^{8}J-1.28\cdot 10^8 J=1.32 \cdot 10^8 J[/tex]
The ratio of the potential energies of satellite A to that of Satellite B is [tex]\frac{513}{1000}[/tex].
Solution for Question A
Since the altitudes are given, it is the orbital radii that enter the equations is given as: rₐ = (7580 + 7580 )Km = 15,160Km while [tex]r_{b}[/tex] = (7580 + 22000) km = 29,580Km.
[tex]\frac{Q_{b} }{Q_{a} }[/tex] = [tex]\frac{-GmM/Rb}{-GmM/Ra}[/tex]
= [tex]\frac{Ra}{Rb}[/tex] = 15,160/29,580
= 0.513 or [tex]\frac{513}{1000}[/tex]
(b) the ratio of kinetic energies is
[tex]\frac{X_{b} }{X_{a} }[/tex] = [tex]\frac{-GmM/2Rb}{-GmM/2Ra}[/tex]
= [tex]\frac{Ra}{Rb}[/tex] = 15,160/29,580
= 0.513 or [tex]\frac{513}{1000}[/tex]
(C) Which satellite has the greater total energy?
The satellite with the greatest energy is B because It has the largest value of r.
(D) To get the variance between the energy levels of each mass we say:
Δ E = Eb - Ea; where E is energy.
= [tex]\frac{-GmM}{2}[/tex] [tex](\frac{1}{rb}) - (\frac{1}{ra})[/tex]
Therefore, Δ E = 1.1 x 10¹³J
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