(b) Find the period and angular frequency of the orbital motion. · OlympiadBench #984

Physics · mechanics

Problem

(b) Find the period TT and angular frequency ω\omega of the orbital motion. Given constants: 3. The circular restricted three-body problem In general, there is no exact solution of the three-body problem, in which three masses move under their mutual gravitational attraction. However, it is possible to make some progress by adding some constraints to the motion. Two-body problem Let's start with the motion of two masses, M1M_{1} and M2M_{2}. Assume both masses move in circular orbits about their center of mass. Consider the inertial frame whose origin coincides with the center of mass of the system. Context question: (a) Express the equations of motion of M1M_{1} and M2M_{2} in terms of the gravitational constant GG and the position vectors r1→\overrightarrow{r_{1}} and r2→\overrightarrow{r_{2}} which point from the origin to M1M_{1} and M2M_{2}, respectively. Context answer: d2dt2r1→=GM2∣r2→−r1→∣3(r2→−r1→)d2dt2r2→=GM1∣r1→−r2→∣3(r1→−r2→)\begin{aligned} & \frac{d^{2}}{d t^{2}} \overrightarrow{r_{1}}=\frac{G M_{2}}{\left|\overrightarrow{r_{2}}-\overrightarrow{r_{1}}\right|^{3}}\left(\overrightarrow{r_{2}}-\overrightarrow{r_{1}}\right) \\ & \frac{d^{2}}{d t^{2}} \overrightarrow{r_{2}}=\frac{G M_{1}}{\left|\overrightarrow{r_{1}}-\overrightarrow{r_{2}}\right|^{3}}\left(\overrightarrow{r_{1}}-\overrightarrow{r_{2}}\right) \end{aligned}

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