ML2 T–1
M–2L3 T–2
M–2L2 T–1
M–1L3 T–2
The universal gravitational constant, denoted as G, is used in Newton's law of universal gravitation. According to the law, the force F of attraction between two masses m_1 and m_2 separated by a distance r is given by:
F = \frac{G \cdot m_1 \cdot m_2}{r^2}
Where:
Hence, rearranging for G, we get:
G = \frac{F \cdot r^2}{m_1 \cdot m_2}
Substitute the dimensions of each term:
Thus, the dimensions of G will be:
G = \frac{[MLT^{-2}] \cdot [L^2]}{[M^2]} = [M^{-1}L^3T^{-2}]
This matches the correct answer, which is:
Correct Answer: M^{-1}L^3T^{-2}
This dimensional formula is crucial in understanding how the gravitational constant balances the units in gravitational force calculations. It demonstrates the relationship between force, distance, and mass in the context of gravitational interactions.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)