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Q8.24:
A spaceship is stationed on Mars. How much energy must be expended on the spaceship to launch it out of the solar system ? Mass of the space ship = 1000 kg; mass of the sun = $2 \times 10^{30}$ kg; mass of mars = $6.4 \times 10^{23}$ kg; radius of mars = 3395 km; radius of the orbit of mars = $2.28 \times 10^8$ km; G = $6.67 \times 10^{-11}$ N m$^2$ kg$^{–2}$.

Solution :

Given Variables & Initial Setup

To launch a spaceship out of the solar system, we must provide sufficient energy to overcome the gravitational potential energy exerted by both the Sun and Mars. The total energy required ($E$) is the negative of the total mechanical energy of the spaceship in its current position.

  • Mass of spaceship ($m$) = $1000 \, \text{kg}$
  • Mass of Sun ($M_S$) = $2 \times 10^{30} \, \text{kg}$
  • Mass of Mars ($M_M$) = $6.4 \times 10^{23} \, \text{kg}$
  • Radius of Mars ($R_M$) = $3395 \times 10^3 \, \text{m} = 3.395 \times 10^6 \, \text{m}$
  • Radius of Mars' orbit ($r$) = $2.28 \times 10^8 \, \text{km} = 2.28 \times 10^{11} \, \text{m}$
  • Gravitational constant ($G$) = $6.67 \times 10^{-11} \, \text{N m}^2 \text{kg}^{-2}$

Step 1: Calculating the Potential Energy at the Surface of Mars

The total energy ($E_{total}$) is the sum of the potential energy due to the Sun ($U_S$) and the potential energy due to Mars ($U_M$), plus the kinetic energy ($K$) of the spaceship due to Mars' orbital motion. [Per the Law of Conservation of Energy, $E_{launch} = -E_{total}$].

Potential energy due to Mars ($U_M$):

$U_M = -\frac{GM_Mm}{R_M}$ $U_M = -\frac{(6.67 \times 10^{-11})(6.4 \times 10^{23})(1000)}{3.395 \times 10^6}$ $U_M \approx -1.258 \times 10^{10} \, \text{J}$

Step 2: Calculating Potential Energy due to the Sun

The spaceship is at the distance of Mars from the Sun.

$U_S = -\frac{GM_Sm}{r}$ $U_S = -\frac{(6.67 \times 10^{-11})(2 \times 10^{30})(1000)}{2.28 \times 10^{11}}$ $U_S \approx -5.851 \times 10^{11} \, \text{J}$

Step 3: Accounting for Kinetic Energy of the Spaceship

The spaceship possesses kinetic energy due to the orbital velocity ($v_o$) of Mars. [Per the principle of orbital mechanics, $v_o = \sqrt{\frac{GM_S}{r}}$].

$K = \frac{1}{2}mv_o^2 = \frac{1}{2}m\left(\frac{GM_S}{r}\right)$ $K = \frac{(1000)(6.67 \times 10^{-11})(2 \times 10^{30})}{2 \times 2.28 \times 10^{11}}$ $K \approx 2.925 \times 10^{11} \, \text{J}$

Step 4: Total Energy Required

The total mechanical energy $E_{total} = U_M + U_S + K$. The energy required to escape ($E_{expended}$) is $-E_{total}$.

$E_{total} = (-0.1258 \times 10^{11}) + (-5.851 \times 10^{11}) + (2.925 \times 10^{11})$ $E_{total} = -2.9268 \times 10^{11} \, \text{J}$

Energy to be expended:

$E_{expended} = -(-2.9268 \times 10^{11} \, \text{J})$ $E_{expended} \approx 2.93 \times 10^{11} \, \text{J}$

Visualization of Gravitational Well

Mars To Escape

Final Solution: The energy required to launch the spaceship out of the solar system is approximately $2.93 \times 10^{11} \, \text{J}$.


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