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Escape Velocity. According to Newton’s law of gravitation,
Chapter 3, Problem 25E(choose chapter or problem)
Escape Velocity. According to Newton’s law of gravitation, the attractive force between two
objects varies inversely as the square of the distances between them. That is, \(F_{g}=G M_{1} M_{2} / r^{2}\), where \(M_{1}\) and \(M_{2}\) are the masses of the objects, 𝑟 is the distance between them (center to center), \(F_{g}\) is the attractive force, and 𝐺 is the constant of proportionality. Consider a projectile of constant mass 𝑚 being fired vertically from Earth (see Figure 3.12). Let 𝑡 represent time and y the velocity of the projectile.
(a) Show that the motion of the projectile, under Earth’s gravitational force, is governed by the
equation
\(\frac{d v}{d t}=-\frac{g R^{2}}{r^{2}}\),
where 𝑟 is the distance between the projectile and the center of Earth, 𝑅 is the radius of Earth, 𝑀 is the mass of Earth, and \(g=G M / R^{2}\).
(b) Use the fact that \(dr/dt=v\) to obtain
\(v \frac{d v}{d r}=-\frac{g R^{2}}{r^{2}}\).
(c) If the projectile leaves Earth’s surface with velocity \(v_{0}\), show that
\(v^{2}=\frac{2 g R^{2}}{r}+v_{0}^{2}-2 g R\).
(d) Use the result of part (c) to show that the velocity of the projectile remains positive if and only if \(v_{0}^{2}-2 g R>0\). The velocity \(v_{e}=\sqrt{2 g R}\) is called the escape velocity of Earth.
(e) If \(g=9.81 \mathrm{~m} / \mathrm{sec}^{2}\) and \(R=6370 \mathrm{~km}\) for Earth, what is Earth’s escape velocity?
(f) If the acceleration due to gravity for the Moon is \(g_{m}=g / 6\) and the radius of the Moon is \(R_{m}=1738\) km, what is the escape velocity of the Moon?
Equation Transcription:
Text Transcription:
F_{g}=GM_{1}M_{2 r^{2}
M_{1}
M_{2}
F_{g}
\frac{d v}{d t}=-\frac{g R^{2}}{r^{2}}
g=G M / R^{2}
dr/dt=v
v {dv}over{dr}=-{gR^{2}}{r^{2}}
v_{0}
v^{2}={2gR^{2}}over{r}+v_{0}^{2}-2gR
v_{0}^{2}-2gR>0
v_{e}=\sqrt{2 g R}
g=9.81 m/sec^{2}
R=6370 \mathrm{~km}
g_{m}=g/6
R_{m}=1738
Questions & Answers
QUESTION:
Escape Velocity. According to Newton’s law of gravitation, the attractive force between two
objects varies inversely as the square of the distances between them. That is, \(F_{g}=G M_{1} M_{2} / r^{2}\), where \(M_{1}\) and \(M_{2}\) are the masses of the objects, 𝑟 is the distance between them (center to center), \(F_{g}\) is the attractive force, and 𝐺 is the constant of proportionality. Consider a projectile of constant mass 𝑚 being fired vertically from Earth (see Figure 3.12). Let 𝑡 represent time and y the velocity of the projectile.
(a) Show that the motion of the projectile, under Earth’s gravitational force, is governed by the
equation
\(\frac{d v}{d t}=-\frac{g R^{2}}{r^{2}}\),
where 𝑟 is the distance between the projectile and the center of Earth, 𝑅 is the radius of Earth, 𝑀 is the mass of Earth, and \(g=G M / R^{2}\).
(b) Use the fact that \(dr/dt=v\) to obtain
\(v \frac{d v}{d r}=-\frac{g R^{2}}{r^{2}}\).
(c) If the projectile leaves Earth’s surface with velocity \(v_{0}\), show that
\(v^{2}=\frac{2 g R^{2}}{r}+v_{0}^{2}-2 g R\).
(d) Use the result of part (c) to show that the velocity of the projectile remains positive if and only if \(v_{0}^{2}-2 g R>0\). The velocity \(v_{e}=\sqrt{2 g R}\) is called the escape velocity of Earth.
(e) If \(g=9.81 \mathrm{~m} / \mathrm{sec}^{2}\) and \(R=6370 \mathrm{~km}\) for Earth, what is Earth’s escape velocity?
(f) If the acceleration due to gravity for the Moon is \(g_{m}=g / 6\) and the radius of the Moon is \(R_{m}=1738\) km, what is the escape velocity of the Moon?
Equation Transcription:
Text Transcription:
F_{g}=GM_{1}M_{2 r^{2}
M_{1}
M_{2}
F_{g}
\frac{d v}{d t}=-\frac{g R^{2}}{r^{2}}
g=G M / R^{2}
dr/dt=v
v {dv}over{dr}=-{gR^{2}}{r^{2}}
v_{0}
v^{2}={2gR^{2}}over{r}+v_{0}^{2}-2gR
v_{0}^{2}-2gR>0
v_{e}=\sqrt{2 g R}
g=9.81 m/sec^{2}
R=6370 \mathrm{~km}
g_{m}=g/6
R_{m}=1738
ANSWER:
Solution:-
Step1
(a)We have to show that the motion of the projectile.Earth’s gravitational force, is where r is the distance between the projectile and the center of Earth, R is the radius of Earth, M is the mass of Earth, and g = .
We have
According to Newton’s law of gravitation, the attractive force between two objects varies inversely as the square of the distances between them.
That is,
where and are the masses of the objects, r is the distance between them (center to center), is the attractive force, and G is the constant of proportionality.
(since,
Therefore, where r is the distance between the projectile and the center of Earth, R is the radius of Earth, M is the mass of Earth.
Step2
(b) Use the fact that dr/dt = v to obtain .
Therefore,
Step3
(c) If the projectile leaves Earth’s surface with velocity v0, we have to show that