Solution:
The escape velocity is given by the formula: $$ v_e = \sqrt{\frac{2GM}{R}} $$ where:
$v_e$ is the escape velocity
$G$ is the gravitational constant
$M$ is the mass of the celestial body
$R$ is the radius of the celestial body
Let:
$M_p$ be the mass of the planet
$R_p$ be the radius of the planet
$M_e$ be the mass of the Earth
$R_e$ be the radius of the Earth
$v_{ep}$ be the escape velocity of the planet
$v_{ee}$ be the escape velocity of the Earth
Given:
$M_p = 16 M_e$
$R_p = 4 R_e$
Escape velocity of Earth: $$ v_{ee} = \sqrt{\frac{2GM_e}{R_e}} $$ Escape velocity of the planet: $$ v_{ep} = \sqrt{\frac{2GM_p}{R_p}} $$ Ratio: $$ \frac{v_{ep}}{v_{ee}} = \frac{\sqrt{\frac{2GM_p}{R_p}}}{\sqrt{\frac{2GM_e}{R_e}}} = \sqrt{\frac{M_p R_e}{M_e R_p}} $$ Substitute the given values: $$ \frac{v_{ep}}{v_{ee}} = \sqrt{\frac{16M_e R_e}{M_e 4R_e}} = \sqrt{\frac{16}{4}} = \sqrt{4} = 2 $$ Therefore, the ratio of the escape velocity of the planet to the escape velocity of Earth is 2:1.
The correct answer is (2) 2:1.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)
In mechanics, the universal force of attraction acting between all matter is known as Gravity, also called gravitation, . It is the weakest known force in nature.
According to Newton’s law of gravitation, “Every particle in the universe attracts every other particle with a force whose magnitude is,
On combining equations (1) and (2) we get,
F ∝ M1M2/r2
F = G × [M1M2]/r2 . . . . (7)
Or, f(r) = GM1M2/r2
The dimension formula of G is [M-1L3T-2].