K.J.Healey
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The non generated one is just for :
G = 6.667428*10^-11 _m^3 _kg^-1 _s^-2
G = 6.667428*10^-11 _m^3 _kg^-1 _s^-2
The discussion centers on the hypothetical scenario of dropping a ball through a tunnel that passes through the Earth's center. Participants agree that, neglecting air resistance and heat, the ball would oscillate indefinitely, with a calculated travel time of approximately 42 minutes for a one-way trip. The gravitational force decreases linearly as the ball descends, leading to a unique oscillation period that mirrors that of a satellite in orbit. The mathematical analysis involves concepts such as simple harmonic motion and the gravitational force equation, resulting in a period of about 84 minutes for a complete oscillation.
PREREQUISITESThis discussion is beneficial for physicists, engineering students, and anyone interested in gravitational physics and oscillatory motion. It provides insights into theoretical models of motion through gravitational fields and the complexities involved in real-world applications.
Since I don't use Mathematica I can't comment on your use of it, but your potential energy term is incorrect.K.J.Healey said:Heres how i did it in mathematica:
<br /> F= -G m M /r[t]{}^{\wedge}2<br />
<br /> -\frac{G m M}{r(t)^2}<br />
<br /> U=\text{Integrate}[F,r[t]]<br />
<br /> \frac{G m M}{r(t)}<br />
<br /> \rho = \text{ME}/((4/3)*\text{Pi}*\text{RE}{}^{\wedge}3)<br />
<br /> \frac{3 \text{ME}}{4 \pi \text{RE}^3}<br />
M=\rho *(4/3)*\text{Pi}*r[t]{}^{\wedge}3<br />
<br /> \frac{\text{ME} r(t)^3}{\text{RE}^3}<br />
T=(1/2)m (r'[t]){}^{\wedge}2<br />
<br /> \frac{1}{2} m r'(t)^2<br />
<br /> L=T-U<br />
<br /> \frac{1}{2} m r'(t)^2-\frac{G m \text{ME} r(t)^2}{\text{RE}^3}<br />