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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
Final Solution: The energy required to launch the spaceship out of the solar system is approximately $2.93 \times 10^{11} \, \text{J}$.
More Questions from Class 11 Physics Gravitation Additional Exercises
- Q8.22: As you have learnt in the text, a geostationary satellite orbits the earth at a height of nearly 36,000 km from the surface of the earth. What is the potential due to earth’s gravity at the site of this satellite ? (Take the potential energy at infinity to be zero). Mass of the earth = $6.0 \times 10^{24}$ kg, radius = 6400 km.
- Q8.23: A star 2.5 times the mass of the sun and collapsed to a size of 12 km rotates with a speed of 1.2 rev. per second. (Extremely compact stars of this kind are known as neutron stars. Certain stellar objects called pulsars belong to this category). Will an object placed on its equator remain stuck to its surface due to gravity ? (mass of the sun = $2 \times 10^{30}$ kg).
- Q8.25: A rocket is fired ‘vertically’ from the surface of mars with a speed of 2 km s$^{–1}$. If 20% of its initial energy is lost due to martian atmospheric resistance, how far will the rocket go from the surface of mars before returning to it ? Mass of mars = $6.4 \times 10^{23}$ kg; radius of mars = 3395 km; G = $6.67 \times 10^{-11}$ N m$^2$ kg$^{–2}$.
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