Answer
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Hint: You can start by calculating the average radius of satellite A when it moves from position 1 to position 2 by using the equation $a = \dfrac{{{r_1} + {r_2}}}{2}$. Then use the $\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{{{a^3}}}{{r_2^3}}$ to find the value of ${T_1}$. Then divide the time period of satellite A by half to reach the solution.
Complete step-by-step answer:
In the given problem we are given two satellites A and B. B is revolving around the earth with a radius ${r_2}$ and A is revolving around the earth with a radius ${r_1}$.
Given ${r_2} = 3{r_1}$
Let the average radius of satellite A (when it goes from position 1 to position 2) be$a$.
We know that a will be the average radius of satellite A, so
$a = \dfrac{{{r_1} + {r_2}}}{2}$
$a = \dfrac{{{r_1} + 3{r_1}}}{2}$
$a = 2{r_1}$
Kepler’s law are very important laws in physics, these laws are used to describe the motion of planets and some other celestial bodies.
Let’s take the time taken of the period of revolution of satellite A in the elliptical path as ${T_1}$
We know by Kepler’s law
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{{{a^3}}}{{r_2^3}}$
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{{{{(2{r_1})}^3}}}{{{{(3{r_1})}^3}}} = \dfrac{{8r_1^3}}{{27r_1^3}}$
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{8}{{27}}$
${T_1} = \sqrt {\dfrac{8}{{27}}} T$
If we see the movement of satellite A from position 1 to position 2 is half of the whole revolution so the time taken by the satellite in moving from position 1 to position 2 is $\dfrac{{{T_1}}}{2} = \dfrac{{\sqrt 2 }}{{3\sqrt 3 }}T$.
Hence, option C is the correct choice.
Note: In the problem there is no specific mention that the objects A and B are satellites. But in these types of questions, it is very important to figure out what the objects are. We figured it out in this case as in this case, the image provided in the problem has earth in the center and satellites revolve around the earth.
Complete step-by-step answer:
In the given problem we are given two satellites A and B. B is revolving around the earth with a radius ${r_2}$ and A is revolving around the earth with a radius ${r_1}$.
Given ${r_2} = 3{r_1}$
Let the average radius of satellite A (when it goes from position 1 to position 2) be$a$.
We know that a will be the average radius of satellite A, so
$a = \dfrac{{{r_1} + {r_2}}}{2}$
$a = \dfrac{{{r_1} + 3{r_1}}}{2}$
$a = 2{r_1}$
Kepler’s law are very important laws in physics, these laws are used to describe the motion of planets and some other celestial bodies.
Let’s take the time taken of the period of revolution of satellite A in the elliptical path as ${T_1}$
We know by Kepler’s law
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{{{a^3}}}{{r_2^3}}$
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{{{{(2{r_1})}^3}}}{{{{(3{r_1})}^3}}} = \dfrac{{8r_1^3}}{{27r_1^3}}$
$\dfrac{{T_1^2}}{{{T^2}}} = \dfrac{8}{{27}}$
${T_1} = \sqrt {\dfrac{8}{{27}}} T$
If we see the movement of satellite A from position 1 to position 2 is half of the whole revolution so the time taken by the satellite in moving from position 1 to position 2 is $\dfrac{{{T_1}}}{2} = \dfrac{{\sqrt 2 }}{{3\sqrt 3 }}T$.
Hence, option C is the correct choice.
Note: In the problem there is no specific mention that the objects A and B are satellites. But in these types of questions, it is very important to figure out what the objects are. We figured it out in this case as in this case, the image provided in the problem has earth in the center and satellites revolve around the earth.
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