Determine the kinetic energy of a satellite with a mass of \( m = 1000\,\text{kg} \) orbiting the Earth at an altitude of \( h = 270\,\text{km} \) above the surface.
\[ m = 1000\,\text{kg}, \quad M = 6 \times 10^{24}\,\text{kg}, \quad R = 6.4 \times 10^6\,\text{m}, \quad G = 6.67 \times 10^{-11}\,\text{Nm}^2/\text{kg}^2 \] \[ h = 270\,\text{km} = 270 \times 10^3\,\text{m} \]
The gravitational force acting on a satellite in a circular orbit is equal to the centripetal force required for that orbit:
\[ \frac{GMm}{r^2} = \frac{mv^2}{r} \] \[ \Rightarrow v^2 = \frac{GM}{r} \]
where \( r = R + h \) represents the orbital radius.
The kinetic energy (\( K \)) of the satellite is given by:
\[ K = \frac{1}{2}mv^2 = \frac{1}{2}m\frac{GM}{r} \]
Step 1: Calculate the orbital radius:
\[ r = R + h = 6.4 \times 10^6\,\text{m} + 0.27 \times 10^6\,\text{m} = 6.67 \times 10^6\,\text{m} \]
Step 2: Substitute the orbital radius into the kinetic energy formula:
\[ K = \frac{1}{2}m\frac{GM}{r} \]
Step 3: Insert the given numerical values into the formula:
\[ K = \frac{1}{2} \times 1000\,\text{kg} \times \frac{(6.67 \times 10^{-11}\,\text{Nm}^2/\text{kg}^2)(6 \times 10^{24}\,\text{kg})}{6.67 \times 10^6\,\text{m}} \]
Step 4: Simplify the expression:
\[ \frac{GM}{r} = \frac{6.67 \times 6}{6.67} \times 10^{-11 + 24 - 6} = 6 \times 10^7\,\text{m}^2/\text{s}^2 \] \[ K = \frac{1}{2} \times 1000\,\text{kg} \times 6 \times 10^7\,\text{m}^2/\text{s}^2 = 3 \times 10^{10}\,\text{J} \]
The kinetic energy of the satellite is:
\[ \boxed{K = 3 \times 10^{10}\,\text{J}} \]
Therefore, the kinetic energy is 3 × 1010 J.