Step 1: The energy equivalent \( E \) of mass \( m \) is given by Einstein's equation: \[ E = mc^2 \]
where:
- \( m = 1 \, {g} = 1 \times 10^{-3} \, {kg} \),
- \( c = 3 \times 10^8 \, {m/s} \).
Step 2: Substitute the values into the equation: \[ E = (1 \times 10^{-3}) \times (3 \times 10^8)^2 = 9 \times 10^{13} \, {J} \]
Thus, the energy equivalent of 1 g of substance is \( 9 \times 10^{13} \, {J} \).
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
In the travelling plane wave equation given by \( y = A \sin \omega \left( \frac{x}{v} - t \right) \), where \( \omega \) is the angular velocity and \( v \) is the linear velocity.
The dimension of \( \omega t \) is:
Kepler's second law (law of areas) of planetary motion leads to law of conservation of