The escape velocity \( v_{\text{escape}} \) for a celestial body is given by:
\[ v_{\text{escape}} = \sqrt{\frac{2GM}{R}}, \]where \( G \) is the gravitational constant, \( M \) is the mass of the body, and \( R \) is its radius.
Given that the escape velocity on the planet is \( v \):
\[ v = \sqrt{\frac{2GM}{R}}. \]For the moon:
Substitute these values into the escape velocity formula for the moon:
\[ v_{\text{moon}} = \sqrt{\frac{2G \cdot \frac{M}{144}}{\frac{R}{16}}} = \sqrt{\frac{2GM \cdot 16}{144R}} = \sqrt{\frac{2GM}{9R}} = \frac{1}{3} \sqrt{\frac{2GM}{R}} = \frac{v}{3}. \]Thus, the escape velocity on the moon is:
\[ \frac{v}{3}. \]
In the given circuit the sliding contact is pulled outwards such that the electric current in the circuit changes at the rate of 8 A/s. At an instant when R is 12 Ω, the value of the current in the circuit will be A.
Let A be a 3 × 3 matrix such that \(\text{det}(A) = 5\). If \(\text{det}(3 \, \text{adj}(2A)) = 2^{\alpha \cdot 3^{\beta} \cdot 5^{\gamma}}\), then \( (\alpha + \beta + \gamma) \) is equal to: