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If the escape velocity of a planet is 3 ...

If the escape velocity of a planet is 3 times that of the earth and its radius is 4 times that of the earth, then the mass of the planet is (Mass of the earth = `6 xx 10^24 kg`)

A

`1.62 xx 10^22 kg `

B

`0.72 xx 10^22 kg `

C

`2.16 xx 10^26 kg `

D

`1.22 xx 10^22 kg `

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The correct Answer is:
To find the mass of the planet given that its escape velocity is 3 times that of Earth and its radius is 4 times that of Earth, we can follow these steps: ### Step 1: Understand the formula for escape velocity The escape velocity \( v_e \) from a celestial body is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}} \] where \( G \) is the gravitational constant, \( M \) is the mass of the body, and \( R \) is its radius. ### Step 2: Write the escape velocity for Earth and the planet Let: - \( v_{eE} \) be the escape velocity of Earth, - \( M_E \) be the mass of Earth, - \( R_E \) be the radius of Earth. For Earth: \[ v_{eE} = \sqrt{\frac{2GM_E}{R_E}} \] For the planet: - The escape velocity \( v_{eP} \) is given as \( 3v_{eE} \), - The mass of the planet is \( M_P \), - The radius of the planet is \( R_P = 4R_E \). Thus, the escape velocity for the planet can be expressed as: \[ v_{eP} = \sqrt{\frac{2GM_P}{R_P}} = \sqrt{\frac{2GM_P}{4R_E}} = \frac{1}{2} \sqrt{\frac{2GM_P}{R_E}} \] ### Step 3: Set the escape velocities equal Since \( v_{eP} = 3v_{eE} \), we can substitute the expressions we have: \[ 3v_{eE} = \frac{1}{2} \sqrt{\frac{2GM_P}{R_E}} \] Substituting \( v_{eE} \): \[ 3 \sqrt{\frac{2GM_E}{R_E}} = \frac{1}{2} \sqrt{\frac{2GM_P}{R_E}} \] ### Step 4: Square both sides Squaring both sides to eliminate the square roots gives: \[ 9 \left(\frac{2GM_E}{R_E}\right) = \frac{1}{4} \left(\frac{2GM_P}{R_E}\right) \] ### Step 5: Simplify the equation Cancelling \( \frac{2G}{R_E} \) from both sides (assuming \( R_E \neq 0 \)): \[ 9M_E = \frac{1}{4}M_P \] ### Step 6: Solve for \( M_P \) Multiplying both sides by 4 gives: \[ M_P = 36M_E \] ### Step 7: Substitute the mass of Earth Given \( M_E = 6 \times 10^{24} \, \text{kg} \): \[ M_P = 36 \times (6 \times 10^{24}) = 216 \times 10^{24} \, \text{kg} \] ### Step 8: Convert to scientific notation \[ M_P = 2.16 \times 10^{26} \, \text{kg} \] ### Final Answer The mass of the planet is \( 2.16 \times 10^{26} \, \text{kg} \). ---

To find the mass of the planet given that its escape velocity is 3 times that of Earth and its radius is 4 times that of Earth, we can follow these steps: ### Step 1: Understand the formula for escape velocity The escape velocity \( v_e \) from a celestial body is given by the formula: \[ v_e = \sqrt{\frac{2GM}{R}} \] where \( G \) is the gravitational constant, \( M \) is the mass of the body, and \( R \) is its radius. ...
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