To determine the radius of the fourth stationary orbit relative to the third orbit in Bohr's atom model, we need to understand the relation between the orbit radius and the principal quantum number.
According to Bohr's model, the radius \(r_n\) of the \(n\)-th orbit is given by the formula:
\(r_n = n^2 \cdot r_1\)
where \(r_1\) is the radius of the first stationary orbit, and \(n\) is the principal quantum number.
Given:
The radius of the third orbit is \(R\). Therefore, we have:
\(r_3 = 3^2 \cdot r_1 = 9 \cdot r_1 = R\)
From this, we can find \(r_1\):
\(r_1 = \frac{R}{9}\)
We want to find the radius of the fourth orbit, \(r_4\):
\(r_4 = 4^2 \cdot r_1 = 16 \cdot r_1\)
Substituting the value of \(r_1\), we get:
\(r_4 = 16 \cdot \frac{R}{9} = \frac{16}{9} R\)
Thus, the radius of the fourth stationary orbit is \(\frac{16}{9} R\).
Therefore, the correct answer is: \(\frac{16}{9} R\).
This matches the given correct answer option, confirming our solution is accurate.
According to Bohr’s theory, the radius of an electron’s orbit is given by:
\[ r \propto \frac{n^2}{Z} \]
where \(n\) is the principal quantum number and \(Z\) is the atomic number. Since the electron is in hydrogen (\(Z = 1\)), we get:
\[ \frac{r_4}{r_3} = \frac{4^2}{3^2} = \frac{16}{9} \]
Thus, \(r_4 = \frac{16}{9}R\).
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 : \(A_2 \rightleftharpoons 2A\)