To solve the problem, we need to determine the number of triple alpha processes per second, denoted as \( n \times 10^{42} \, \text{s}^{-1} \).
Firstly, calculate the energy released in a single triple alpha process. The reaction is:
\[ ^4\text{He} + ^4\text{He} + ^4\text{He} \rightarrow ^{12}\text{C} + Q \]
The masses of the participating isotopes are:
- Mass of \( ^4\text{He} \) = 4.0026 u
- Mass of \( ^{12}\text{C} \) = 12 u
The initial total mass of the three \( ^4\text{He} \) nuclei:
\[ 3 \times 4.0026 \, \text{u} = 12.0078 \, \text{u} \]
The mass defect \(\Delta m\) is the difference in mass before and after the reaction:
\[ \Delta m = 12.0078 \, \text{u} - 12 \, \text{u} = 0.0078 \, \text{u} \]
The energy released \( Q \) can be calculated using \( E= \Delta m \times 931.5 \, \text{MeV/u} \):
\[ Q = 0.0078 \times 931.5 \, \text{MeV} = 7.2617 \, \text{MeV} \]
Convert the energy to joules (1 MeV = \( 1.60218 \times 10^{-13} \) J):
\[ Q = 7.2617 \times 1.60218 \times 10^{-13} \, \text{J} = 1.163 \times 10^{-12} \, \text{J} \]
Now, find the rate \( n \) using the given power output of the star:
Power \( P = 5.808 \times 10^{30} \, \text{W} \). Since power is energy per unit time,
\[ P = n \times 10^{42} \times 1.163 \times 10^{-12} \, \text{J/s} \]
\[ 5.808 \times 10^{30} = n \times 10^{42} \times 1.163 \times 10^{-12} \]
Solve for \( n \):
\[ n = \frac{5.808 \times 10^{30}}{1.163 \times 10^{-12} \times 10^{42}} \]
\[ n \approx \frac{5.808}{1.163} \times 10^{24} \]
\[ n \approx 5.0 \]
Thus, the value of \( n \) is 5. The computed value fits within the expected range of 5,5, confirming the solution is correct.
The given triple alpha process is:
\( ^4\text{He} + ^4\text{He} + ^4\text{He} \rightarrow ^{12}\text{C} + Q \)
The power generated by the star is given as:
\( \text{Power} = \frac{N}{t} Q \),
where \( \frac{N}{t} \) is the number of reactions per second.
The energy released per reaction (\( Q \)) is:
\( Q = (3m_{\text{He}} - m_{\text{C}})c^2 \)
Substituting the given values:
\( Q = (3 \times 4.0026 - 12) \times (3 \times 10^8)^2 \)
\( Q = 7.266 \, \text{MeV} \)
Convert \( Q \) into joules:
\( Q = 7.266 \times 1.602 \times 10^{-13} \, \text{J} \)
\( Q = 1.163 \times 10^{-12} \, \text{J} \)
Rearranging the power equation:
\( \frac{N}{t} = \frac{\text{Power}}{Q} \)
Substitute the values:
\( \frac{N}{t} = \frac{5.808 \times 10^{30}}{1.163 \times 10^{-12}} \)
Simplify:
\( \frac{N}{t} = 5 \times 10^{42} \, \text{s}^{-1} \)
Final Answer: The rate of conversion of \( ^4\text{He} \) to \( ^{12}\text{C} \) is:
\( n = 5 \, (\text{where } \frac{N}{t} = n \times 10^{42} \, \text{s}^{-1}) \).
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,

In a nuclear fission process, a high mass nuclide (A ≈ 236) with binding energy 7.6 MeV/Nucleon dissociated into middle mass nuclides (A ≈ 118), having binding energy of 8.6 MeV/Nucleon. The energy released in the process would be ____ MeV.
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 : \(A_2 \rightleftharpoons 2A\)