Karol
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1. Homework Statement
Calculate the time the moon rotates once around the earth, and show that you have to add 4 hours to that since the moon & the Earth rotate around their center of mass. hint: use the reduced mass: \overline{m}=\frac{m_{1}m_{2}}{m_{1}+m_{2}}
mass of moon: m=0.0734E24[kg]
mass of earth: 81 times mass of moon: M=81m
radius of earth: Re=6.37E6[m]
distance centers earth-moon: 60Re
gravity constant: G=6.673E-11
(1) F=\frac{GMm}{r^{2}}
(2) F=\frac{mV^{2}}{r} (3) V=\frac{2r\pi}{T}
xc.m.=\frac{m_{1}x_{1}+m_{2}x_{2}}{m_{1}+m_{2}}
maybe: the momentum in the center of mass coordinate system: (4)\vec{p_{1}}=m1\vec{V_{1}}=\overline{m}\vec{V_{12}}, while V12 is the relative velocity between them, and \overline{m}=\frac{m_{1}m_{2}}{m_{1}+m_{2}} is the reduced mass.
the revolution time when the Earth is "stuck" in place and the moon rotates only: using equations: (1)=(2), (3): \Rightarrow \frac{mV^{2}}{60R^{e}}=\frac{81Gm^{2}}{(60R_{e})^{2}} \Rightarrow T=2,357,028[sec]=27.28[days], and the relative velocity is: V12=1018.8[m/sec].
the distance of the center of their mass from center of earth: xc.m.=\frac{60R_{e}m}{82m}=4,660,976[m]
now, in the coordinate system of the moving center of gravity, i find the moon's tangential velocity, knowing that the relative velocity V12 is the same in all coordinate systems: according to equation (4) above: V1=\frac{\overline{m}V_{12}}{m_{1}}=1006.3[m/sec]
now, the revolution time of the moon round the distance to center of mass (3): \frac{2\pi(60R_{e}-x_{c.m.})}{1006.3}=2,357,187[sec]
this is only 159[sec] more, not 4 hours!
Calculate the time the moon rotates once around the earth, and show that you have to add 4 hours to that since the moon & the Earth rotate around their center of mass. hint: use the reduced mass: \overline{m}=\frac{m_{1}m_{2}}{m_{1}+m_{2}}
mass of moon: m=0.0734E24[kg]
mass of earth: 81 times mass of moon: M=81m
radius of earth: Re=6.37E6[m]
distance centers earth-moon: 60Re
gravity constant: G=6.673E-11
Homework Equations
(1) F=\frac{GMm}{r^{2}}
(2) F=\frac{mV^{2}}{r} (3) V=\frac{2r\pi}{T}
xc.m.=\frac{m_{1}x_{1}+m_{2}x_{2}}{m_{1}+m_{2}}
maybe: the momentum in the center of mass coordinate system: (4)\vec{p_{1}}=m1\vec{V_{1}}=\overline{m}\vec{V_{12}}, while V12 is the relative velocity between them, and \overline{m}=\frac{m_{1}m_{2}}{m_{1}+m_{2}} is the reduced mass.
The Attempt at a Solution
the revolution time when the Earth is "stuck" in place and the moon rotates only: using equations: (1)=(2), (3): \Rightarrow \frac{mV^{2}}{60R^{e}}=\frac{81Gm^{2}}{(60R_{e})^{2}} \Rightarrow T=2,357,028[sec]=27.28[days], and the relative velocity is: V12=1018.8[m/sec].
the distance of the center of their mass from center of earth: xc.m.=\frac{60R_{e}m}{82m}=4,660,976[m]
now, in the coordinate system of the moving center of gravity, i find the moon's tangential velocity, knowing that the relative velocity V12 is the same in all coordinate systems: according to equation (4) above: V1=\frac{\overline{m}V_{12}}{m_{1}}=1006.3[m/sec]
now, the revolution time of the moon round the distance to center of mass (3): \frac{2\pi(60R_{e}-x_{c.m.})}{1006.3}=2,357,187[sec]
this is only 159[sec] more, not 4 hours!