The total mechanical energy \( E \) of a satellite in a circular orbit is given by the sum of its kinetic energy and gravitational potential energy:
\[ E = K + U \]
where:
The kinetic energy \( K \) of the satellite is given by:
\[ K = \frac{1}{2} m v^2 \]
Substituting \( m = 10 \) kg and \( v = 200 \) m/s:
\[ K = \frac{1}{2} \times 10 \times (200)^2 \]
\[ K = 5 \times 40000 = 200000 \text{ J} \]
The gravitational potential energy \( U \) for an object in orbit is given by:
\[ U = -\frac{GMm}{r} \]
where:
For a circular orbit, the gravitational force provides the centripetal force required for the satellite’s circular motion:
\[ \frac{GMm}{r^2} = \frac{m v^2}{r} \]
Solving for \( r \):
\[ r = \frac{GM}{v^2} \]
Substituting this into the potential energy equation:
\[ U = -\frac{1}{2} m v^2 \]
Thus, the total energy is:
\[ E = K + U = \frac{1}{2} m v^2 - \frac{1}{2} m v^2 = -\frac{1}{2} m v^2 \]
Substituting \( m = 10 \) kg and \( v = 200 \) m/s:
\[ E = -\frac{1}{2} \times 10 \times (200)^2 \]
\[ E = -5 \times 40000 = -200000 \text{ J} \]
\[ E = -200 \text{ kJ} \]
The total energy of the satellite is \(-200\) kJ.
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.)