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| <meta name="date" content="2023-10" scheme="YYYY-MM"> | | <meta name="date" content="2023-10" scheme="YYYY-MM"> |
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| <h2>Solutions of Savchenko Problems in Physics</h2> | | <h2>Solutions of Savchenko Problems in Physics</h2> |
| <p class="author"> | | <p class="author"> |
| Aliaksandr Melnichenka <br/> | | Aliaksandr Melnichenka <br/> |
| October 2023 | | October 2023 |
| </p> | | </p> |
| </header> | | </header> |
| | | |
| <h3 id="back-link"><a href="../../#2.6">$\leftarrow$Back</a></h3> | | <h3 id="back-link"><a href="../../#2.6">$\leftarrow$Back</a></h3> |
| | | |
| <h3> Statement </h3> | | <h3> Statement </h3> |
| <p> | | <p> |
| $2.6.52^*.$ Two touching each other globular blocks of mass $m$ and radius $r$ each move in a circular orbit around a planet of mass $M$. The centers of the boulders are located at the same radius, the distance from their point of contact to the center of planet $R$. With what force does one block press on another? At what radius of the orbit will the mutual attraction of the lumps cease to hold them together? The radius of the planet is $R_0 \gg r$. Take the density of the boulders to be equal to the average density of the planet. | | $2.6.52^*.$ Two touching each other globular blocks of mass $m$ and radius $r$ each move in a circular orbit around a planet of mass $M$. The centers of the boulders are located at the same radius, the distance from their point of contact to the center of planet $R$. With what force does one block press on another? At what radius of the orbit will the mutual attraction of the lumps cease to hold them together? The radius of the planet is $R_0 \gg r$. Take the density of the boulders to be equal to the average density of the planet. |
| </p> | | </p> |
| <center> | | <center> |
| <figure> | | <figure> |
| <img src="statement.png" | | <img src="statement.png" |
| loading="lazy" width="200" /> | | loading="lazy" width="200" /> |
| <figcaption> | | <figcaption> |
| For problem $2.6.52^*$ | | For problem $2.6.52^*$ |
| </figcaption> | | </figcaption> |
| </figure> | | </figure> |
| </center> | | </center> |
| <p> | | <p> |
| </p> | | </p> |
| | | |
| <h3>Solution</h3> | | <h3>Solution</h3> |
| <p> | | <p> |
| | | |
| </p> | | </p> |
| <center> | | <center> |
| <figure> | | <figure> |
| <img src="draw.png" | | <img src="draw.png" |
| loading="lazy" width="250" /> | | loading="lazy" width="250" /> |
| <figcaption> | | <figcaption> |
| Forces acting on the system | | Forces acting on the system |
| </figcaption> | | </figcaption> |
| </figure> | | </figure> |
| </center> | | </center> |
| <p> | | <p> |
| | | |
| Newton's second law for two bodies: | | Newton's second law for two bodies: |
| $$\left\{\begin{matrix} | | $$\left\{\begin{matrix} |
| F_1+N-F_0=m\omega^2(R-r) \\ | | F_1+N-F_0=m\omega^2(R-r) \\ |
| F_1-N+F_0=m\omega^2(R+r) | | F_1-N+F_0=m\omega^2(R+r) |
| \end{matrix}\right.$$ | | \end{matrix}\right.$$ |
| Dividing one equation by the other, we get | | Dividing one equation by the other, we get |
| $$\frac{F_1+N-F_0}{F_1-N+F_0}=\frac{R-r}{R+r}$$ | | $$\frac{F_1+N-F_0}{F_1-N+F_0}=\frac{R-r}{R+r}$$ |
| Transforming the obtained expression, we obtain | | Transforming the obtained expression, we obtain |
| $$N=F_0-\frac{F_1(R+r)-F_2(R-r)}{2R}$$ | | $$N=F_0-\frac{F_1(R+r)-F_2(R-r)}{2R}$$ |
| The forces of gravitational attraction of the clumps between themselves and the planet | | The forces of gravitational attraction of the clumps between themselves and the planet |
| $$\left\{\begin{matrix} | | $$\left\{\begin{matrix} |
| F_0=G\frac{m^2}{4r^2}\\ | | F_0=G\frac{m^2}{4r^2}\\ |
| F_1=G\frac{mM}{(R-r)^2} \\ | | F_1=G\frac{mM}{(R-r)^2} \\ |
| F_2=G\frac{mM}{(R+r)^2} | | F_2=G\frac{mM}{(R+r)^2} |
| \end{matrix}\right.$$ | | \end{matrix}\right.$$ |
| Substituting into the expression for $\vec{N}$ | | Substituting into the expression for $\vec{N}$ |
| $$N=G\frac{m^2}{4r^2}-\frac{GmM}{2R}\left(\frac{R+r}{(R-r)^2}-\frac{R-r}{(R+r)^2}\right)$$ | | $$N=G\frac{m^2}{4r^2}-\frac{GmM}{2R}\left(\frac{R+r}{(R-r)^2}-\frac{R-r}{(R+r)^2}\right)$$ |
| After mathematical transformations we obtain | | After mathematical transformations we obtain |
| $$\boxed{N=G\frac{m^2}{4r^2}-\frac{GmM}{R}\frac{3R^2r+r^3}{(R^2-r^2)^2}}$$ | | $$\boxed{N=G\frac{m^2}{4r^2}-\frac{GmM}{R}\frac{3R^2r+r^3}{(R^2-r^2)^2}}$$ |
| The mutual attraction will stop binding them together at the moment when the force $N$ becomes equal to $0$ | | The mutual attraction will stop binding them together at the moment when the force $N$ becomes equal to $0$ |
| $$G\frac{m^2}{4r^2}-\frac{GmM}{R}\frac{3R^2r+r^3}{(R^2-r^2)^2}=0$$ | | $$G\frac{m^2}{4r^2}-\frac{GmM}{R}\frac{3R^2r+r^3}{(R^2-r^2)^2}=0$$ |
| After some minor adjustments | | After some minor adjustments |
| $$\frac{m}{M}=\frac{4r^3}{R}\frac{3R^2+r^2}{(R^2-r^2)^2} \quad (1)$$ | | $$\frac{m}{M}=\frac{4r^3}{R}\frac{3R^2+r^2}{(R^2-r^2)^2} \quad (1)$$ |
| Let's write an expression for the relation between mass $m$ and $M$ and density $\rho$ | | Let's write an expression for the relation between mass $m$ and $M$ and density $\rho$ |
| $$\left\{\begin{matrix} | | $$\left\{\begin{matrix} |
| m=\rho\cdot \frac{4}{3}\pi r^3\\ | | m=\rho\cdot \frac{4}{3}\pi r^3\\ |
| M=\rho\cdot \frac{4}{3}\pi R_0^3 | | M=\rho\cdot \frac{4}{3}\pi R_0^3 |
| \end{matrix}\right.$$ | | \end{matrix}\right.$$ |
| Dividing one equation by the other, we get | | Dividing one equation by the other, we get |
| $$\frac{m}{M}=\frac{r^3}{R_0^3}$$ | | $$\frac{m}{M}=\frac{r^3}{R_0^3}$$ |
| Let's put the obtained expression in $(1)$ | | Let's put the obtained expression in $(1)$ |
| $$\frac{r^3}{R_0^3}=\frac{4r^3}{R}\frac{3R^2+r^2}{(R^2-r^2)^2}$$ | | $$\frac{r^3}{R_0^3}=\frac{4r^3}{R}\frac{3R^2+r^2}{(R^2-r^2)^2}$$ |
| Given that $r \ll R$, we can neglect the summands of order $r^2$ | | Given that $r \ll R$, we can neglect the summands of order $r^2$ |
| $$\frac{r^3}{R_0^3}=\frac{4r^3}{R}\cdot\frac{3R^2}{R^4}$$ | | $$\frac{r^3}{R_0^3}=\frac{4r^3}{R}\cdot\frac{3R^2}{R^4}$$ |
| From where we get expressing $R$ through $R_0$ | | From where we get expressing $R$ through $R_0$ |
| $$\boxed{R=\sqrt[3]{12} R_0}$$ | | $$\boxed{R=\sqrt[3]{12} R_0}$$ |
| </p> | | </p> |
| | | |
| <h4>Answer</h4> | | <h4>Answer</h4> |