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Hello guys, the following problem I've had is from Beer and Johnston, Dynamics:
At a distance R above the Earth's surface, a particle at rest is let go. Given the gravitational acceleration: a =-g\frac{R^2}{r^2} where r is the distance from the center of the Earth to the particle, R is the Earth radius and g is the gravitational acceleration at the surface, calculate (a) the velocity of the particle when it hits the Earth, (b) the time it takes to fall to the surface. (Earth radius = R = 6.380 km, g=9.81 m/seg^2) Results: V=7910 m/s, t=34.5 m = 2070 s
1.a =-g\frac{R^2}{r^2}
2.a = vdv/dr
3.v = dr/dt
4.a = dv/dt
Okay, so for (a) what I did was integrating the acceleration using 2. and get velocity as a function of r or the distance Earth center - particle from r to r_{0}, these being R to 2R, \int-gR^2/r^2 dr and I got V(r)=\sqrt{2gR^2(\frac{1}{R} -\frac{1}{2R})} since V_{0} is 0 because the particle is initially, at r=2R and t=0, at rest. For r=R, it gave me 7911 m/s which is the solution the book gives. Now as for the time, I tried integrating the indefinite integral of the acceleration again, to get the time, by using 3. dt=dr/v, which is \int-gR^2/r^2 dr and gives V(r)=\sqrt{2gR^2/r}+C that didn't work, because when I integrate V, I have the constant, and to get that constant I did V(r=2R)=0, because it is at rest, that gave me C=-7911, and that's is impossible because I tried V(r=R) which should be 7911, but it gave me 3277, so I don't know what I'm doing wrong. I tried the other way, by doing V(r=R)=7911, but the constant didn't correspond to V(r=2R)=0.
The result is 34.5 m or 2070 s. I also tried integrating the acceleration over time, by using 4., but that got me nowhere, since I would have to use double integrals because r varies. Though I'm not really sure about this last part.
Homework Statement
At a distance R above the Earth's surface, a particle at rest is let go. Given the gravitational acceleration: a =-g\frac{R^2}{r^2} where r is the distance from the center of the Earth to the particle, R is the Earth radius and g is the gravitational acceleration at the surface, calculate (a) the velocity of the particle when it hits the Earth, (b) the time it takes to fall to the surface. (Earth radius = R = 6.380 km, g=9.81 m/seg^2) Results: V=7910 m/s, t=34.5 m = 2070 s
Homework Equations
1.a =-g\frac{R^2}{r^2}
2.a = vdv/dr
3.v = dr/dt
4.a = dv/dt
The Attempt at a Solution
Okay, so for (a) what I did was integrating the acceleration using 2. and get velocity as a function of r or the distance Earth center - particle from r to r_{0}, these being R to 2R, \int-gR^2/r^2 dr and I got V(r)=\sqrt{2gR^2(\frac{1}{R} -\frac{1}{2R})} since V_{0} is 0 because the particle is initially, at r=2R and t=0, at rest. For r=R, it gave me 7911 m/s which is the solution the book gives. Now as for the time, I tried integrating the indefinite integral of the acceleration again, to get the time, by using 3. dt=dr/v, which is \int-gR^2/r^2 dr and gives V(r)=\sqrt{2gR^2/r}+C that didn't work, because when I integrate V, I have the constant, and to get that constant I did V(r=2R)=0, because it is at rest, that gave me C=-7911, and that's is impossible because I tried V(r=R) which should be 7911, but it gave me 3277, so I don't know what I'm doing wrong. I tried the other way, by doing V(r=R)=7911, but the constant didn't correspond to V(r=2R)=0.
The result is 34.5 m or 2070 s. I also tried integrating the acceleration over time, by using 4., but that got me nowhere, since I would have to use double integrals because r varies. Though I'm not really sure about this last part.