Step 1: Relation between power and velocity.
Since \(P = Fv = m a v\) and \(a = \frac{dv}{dt}\):
\[
P = m v \frac{dv}{dt}
\]
\[ $\Rightarrow$ v \, dv = \frac{P}{m} dt
\]
Integrate both sides from \(0\) to \(v\) and \(0\) to \(t\):
\[
\frac{v^2}{2} = \frac{P t}{m} $\Rightarrow$ v = \sqrt{\frac{2Pt}{m}}
\]
Step 2: Relate distance and time.
\[
s = \int_0^t v\, dt = \int_0^t \sqrt{\frac{2P}{m}} t^{1/2} dt = \sqrt{\frac{2P}{m}} \frac{2}{3} t^{3/2}
\]
Rearrange for \(P\):
\[
P = \frac{9m s^2}{8t^3}
\]
Step 3: Substitute values.
\(m = 600\ \text{kg},\ s = 600\ \text{m},\ t = 60\ \text{s}\)
\[
P = \frac{9 \times 600 \times 600^2}{8 \times 60^3} = \frac{9 \times 600 \times 360000}{8 \times 216000} = \frac{1.944 \times 10^9}{1.728 \times 10^6} = 1125\, \text{W} = 1.125\, \text{kW}
\]
Rounded: \(1.13\, \text{kW}\).
Step 4: Conclusion.
Hence, the power \(P = 1.13\, \text{kW}\).



At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/m³, which is dimensionally incorrect for a spectral density. The correct unit J/(m³·Hz) or J·s/m³ is used here for the solution.)