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+ <meta name="description" content="The plane of the satellite's orbit is divided into sectors with a common vertex in the center of the planet of mass M and the same small solution angles d \varphi. Find the change in the satellite's speed as it passes through each sector, if its speed is in the pericenter v_p, and the distance from the satellite to the center of the planet is in the pericenter r_p.">
+ <meta name="author" content="Aliaksandr Melnichenka">
+ <meta name="date" content="2023-10" scheme="YYYY-MM">
+ <meta property="og:title" content="The plane of the satellite's orbit is divided into sectors with a common vertex in the center of the planet of mass M and the same small solution angles d \varphi. Find the change in the satellite's speed as it passes through each sector, if its speed is in the pericenter v_p, and the distance from the satellite to the center of the planet is in the pericenter r_p.">
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+ <title>The plane of the satellite's orbit is divided into sectors with a common vertex in the center of the planet of mass M and the same small solution angles d \varphi. Find the change in the satellite's speed as it passes through each sector, if its speed is in the pericenter v_p, and the distance from the satellite to the center of the planet is in the pericenter r_p.</title>
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+ <header style="text-align:center;">
+ <h2>Solutions of Savchenko Problems in Physics</h2>
+ <p class="author">
+ Aliaksandr Melnichenka <br/>
+ October 2023
+ </p>
+ </header>
+
+ <h3 id="back-link"><a href="../../#2.6">$\leftarrow$Back</a></h3>
+
+ <h3> Statement </h3>
+ <p>
+ $2.6.42^*.$ The plane of the satellite's orbit is divided into sectors with a common vertex in the center of the planet of mass $M$ and the same small solution angles $d \varphi$. Find the change in the satellite's speed as it passes through each sector, if its speed is in the pericenter $v_p$, and the distance from the satellite to the center of the planet is in the pericenter $r_p$.
+</p>
+<center>
+ <figure>
+ <img src="2.6.42.png"
+ loading="lazy" width="120" />
+ <figcaption>
+ For problem $2.6.42^*$
+ </figcaption>
+ </figure>
+</center>
+<p>
+ </p>
+
+ <h3>Solution</h3>
+ <p>
+
+</p>
+<center>
+ <figure>
+ <img src="2.6.42_1.png"
+ loading="lazy" width="300" />
+ <figcaption>
+ Change in speed over a short period of time
+ </figcaption>
+ </figure>
+</center>
+<p>
+
+For a short time, $dt$, the body moves along the arc of the circle of arc $d\varphi$ with radius-curvature of the trajectory $R_n$.</p><p>
+Newton's second law for an external force, the gravitational force
+$$ma=\frac{GmM}{R_n^2}$$
+By definition of acceleration
+$$a=\frac{dv}{dt}\Rightarrow \frac{dv}{dt}=\frac{GM}{R_n^2}\quad (1)$$
+In a small amount of time
+$$R_n=v_ndt\quad (2)$$
+By definition the arc length of the circle corresponding to the angle $d\varphi$
+$$dR=d\varphi \cdot R_n\quad (3)$$
+After substituting $(2)$ and $(3)$ into $(1)$
+$$\frac{dv}{dR}v_n=\frac{GM}{R_n^2}\Rightarrow \frac{dv}{d\varphi}v_n=\frac{GM}{R_n}$$
+After the transformation, we can get a change in the satellite's speed
+$$\boxed{dv=\frac{GM\cdot d\varphi}{R_nv_n}}$$
+ </p>
+
+ <h4>Answer</h4>
+ <p>
+ $dv=\gamma Md\varphi/(v_{\mathrm{n}}r_{\mathrm{n}})$. The vector $dv$ is directed towards the centre of the planet
+ </p>
+ <p style="text-align: right; font-style: italic; font-size: 14;">
+ Almaskhan Arsen<br>
+ </p>
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