Let \( g_0 \) be the acceleration due to gravity at the earth's surface. The acceleration due to gravity at a height \( h \) above the surface is given by:
\( g_h = \frac{g_0}{(1 + \frac{h}{R_e})^2} \)
The acceleration due to gravity at a depth \( d = \alpha h \) below the surface is given by:
\( g_d = g_0 \left(1 - \frac{\alpha h}{R_e}\right) \)
According to the problem, \( g_h = g_d \). Therefore:
\[\frac{g_0}{(1 + \frac{h}{R_e})^2} = g_0 \left(1 - \frac{\alpha h}{R_e}\right)\]
We can cancel \( g_0 \) from both sides and solve the resulting equation:
\[\frac{1}{(1 + \frac{h}{R_e})^2} = 1 - \frac{\alpha h}{R_e}\]
For simplicity, let's approximate \((1+\frac{h}{R_e})^2\) using binomial expansion, considering \( h \ll R_e \):
\((1 + \frac{h}{R_e})^2 \approx 1 + \frac{2h}{R_e}\)
Thus, the equation simplifies to:
\[\frac{1}{1 + \frac{2h}{R_e}} \approx 1 - \frac{\alpha h}{R_e}\]
Expanding the left side using binomial approximation again:
\[1 - \frac{2h}{R_e} \approx 1 - \frac{\alpha h}{R_e}\]
Equating coefficients of \(\frac{h}{R_e}\):
\[2 = \alpha\]
Thus, the value of \(\alpha\) is \(2\), which fits within the given range of \(2,2\).
\(g(1 - \frac{2h}{R}) = g(1 - \frac{d}{R})\)
\(⇒ 2h = d\)
\(⇒ α = 2\)
So, the answer is 2.
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].