JEE MAIN - Physics (2023 - 13th April Morning Shift - No. 3)

A planet having mass $$9 \mathrm{Me}$$ and radius $$4 \mathrm{R}_{\mathrm{e}}$$, where $$\mathrm{Me}$$ and $$\mathrm{Re}$$ are mass and radius of earth respectively, has escape velocity in $$\mathrm{km} / \mathrm{s}$$ given by:

(Given escape velocity on earth $$\mathrm{V}_{\mathrm{e}}=11.2 \times 10^{3} \mathrm{~m} / \mathrm{s}$$ )

33.6
11.2
16.8
67.2

Explanation

The escape velocity on a planet is given by the following formula:

$$v_{esc} = \sqrt{\frac{2GM}{R}}$$

where $v_{esc}$ is the escape velocity, $G$ is the gravitational constant, $M$ is the mass of the planet, and $R$ is the radius of the planet.

For Earth, we are given that $v_e = 11.2 \times 10^3$ m/s. We know that the mass of the planet in question is $9M_e$ and its radius is $4R_e$. Let's find the escape velocity of this planet:

$$v_{esc} = \sqrt{\frac{2G(9M_e)}{4R_e}}$$

Divide both sides by the Earth's escape velocity formula:

$$\frac{v_{esc}}{v_e} = \frac{\sqrt{\frac{2G(9M_e)}{4R_e}}}{\sqrt{\frac{2GM_e}{R_e}}}$$

Simplify:

$$\frac{v_{esc}}{11.2 \times 10^3 \text{ m/s}} = {\sqrt{\frac{9}{4}}}$$

$$\frac{v_{esc}}{11.2 \times 10^3 \text{ m/s}} = \frac{3}{2}$$

Now, solve for $v_{esc}$:

$$v_{esc} = 11.2 \times 10^3 \text{ m/s} \times \frac{3}{2}$$

$$v_{esc} = 16.8 \times 10^3 \text{ m/s}$$

Converting this to km/s, we get:

$$v_{esc} = 16.8 \text{ km/s}$$

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