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The ratio of energy required to raise a ...

The ratio of energy required to raise a satellite to a height `h` above the earth surface to that required to put it into the orbit is

A

`R:h`

B

`h:R`

C

`R:2h`

D

`2h:R`

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The correct Answer is:
To find the ratio of energy required to raise a satellite to a height \( h \) above the Earth's surface to that required to put it into orbit, we will follow these steps: ### Step 1: Calculate the Energy Required to Raise the Satellite (E1) The gravitational potential energy \( U \) at a distance \( r \) from the center of the Earth is given by: \[ U = -\frac{GMm}{r} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( m \) is the mass of the satellite. 1. **Initial Energy at Earth's Surface (r)**: \[ U_i = -\frac{GMm}{r} \] 2. **Final Energy at Height \( h \) (r + h)**: \[ U_f = -\frac{GMm}{r + h} \] 3. **Energy Required to Raise the Satellite (E1)**: \[ E_1 = U_f - U_i = \left(-\frac{GMm}{r + h}\right) - \left(-\frac{GMm}{r}\right) \] \[ E_1 = \frac{GMm}{r} - \frac{GMm}{r + h} \] \[ E_1 = GMm \left(\frac{1}{r} - \frac{1}{r + h}\right) \] \[ E_1 = GMm \left(\frac{(r + h) - r}{r(r + h)}\right) = \frac{GMmh}{r(r + h)} \] ### Step 2: Calculate the Energy Required to Put the Satellite into Orbit (E2) The kinetic energy \( K \) required to put the satellite into orbit is given by: \[ E_2 = \frac{1}{2} mv^2 \] where \( v \) is the orbital velocity. The orbital velocity at height \( h \) is given by: \[ v = \sqrt{\frac{GM}{r + h}} \] Thus, \[ E_2 = \frac{1}{2} m \left(\sqrt{\frac{GM}{r + h}}\right)^2 = \frac{1}{2} m \frac{GM}{r + h} = \frac{GMm}{2(r + h)} \] ### Step 3: Find the Ratio of E1 to E2 Now we can find the ratio \( \frac{E_1}{E_2} \): \[ \frac{E_1}{E_2} = \frac{\frac{GMmh}{r(r + h)}}{\frac{GMm}{2(r + h)}} \] Cancelling \( GMm \) and \( (r + h) \): \[ \frac{E_1}{E_2} = \frac{2h}{r} \] ### Final Result Thus, the ratio of energy required to raise a satellite to a height \( h \) above the Earth's surface to that required to put it into orbit is: \[ \frac{E_1}{E_2} = \frac{2h}{r} \]
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