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The source of energy of stars is nuclear...

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about `10^(7) `. Energy released in the process of fusion is due to mass defect. It is also called `Q`-value. `Q = Delta mc^(2), Delta m =` mass defect.
In a nuclear reaction
`._(1)H^(2) + ._(1)H^(2) rarr ._(2)He^(3) + ._(0)n^(1)`
If the masses of ._(1)H^(2)` and `._(2)He^(3)` are 2.014741 and 3.016977 amu, respectively. then the `Q`-value of the reaction is nearly.

A

`0.00352 MeV`

B

`3.27 MeV`

C

`0.82 MeV`

D

`2.45 MeV`

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To solve the problem, we need to calculate the Q-value of the nuclear fusion reaction given by: \[ _{1}H^{2} + _{1}H^{2} \rightarrow _{2}He^{3} + _{0}n^{1} \] ### Step-by-Step Solution: 1. **Identify the masses involved in the reaction:** - Mass of deuterium (\( _{1}H^{2} \)) = 2.014741 amu - Mass of helium-3 (\( _{2}He^{3} \)) = 3.016977 amu - Mass of neutron (\( _{0}n^{1} \)) = 1.008987 amu 2. **Calculate the total mass of the reactants:** - Since there are two deuterium nuclei, the total mass of the reactants is: \[ \text{Total mass of reactants} = 2 \times \text{mass of deuterium} = 2 \times 2.014741 = 4.029482 \text{ amu} \] 3. **Calculate the total mass of the products:** - The products of the reaction are one helium-3 nucleus and one neutron: \[ \text{Total mass of products} = \text{mass of helium-3} + \text{mass of neutron} = 3.016977 + 1.008987 = 4.025964 \text{ amu} \] 4. **Calculate the mass defect (\( \Delta m \)):** - The mass defect is the difference between the total mass of the reactants and the total mass of the products: \[ \Delta m = \text{Total mass of reactants} - \text{Total mass of products} \] \[ \Delta m = 4.029482 - 4.025964 = 0.003518 \text{ amu} \] 5. **Convert mass defect to energy (Q-value):** - The Q-value can be calculated using the formula: \[ Q = \Delta m \times c^2 \] - To convert the mass defect from amu to MeV, we use the conversion factor \( 1 \text{ amu} \approx 931 \text{ MeV} \): \[ Q = 0.003518 \text{ amu} \times 931 \text{ MeV/amu} \approx 3.27 \text{ MeV} \] ### Final Answer: The Q-value of the reaction is approximately **3.27 MeV**. ---

To solve the problem, we need to calculate the Q-value of the nuclear fusion reaction given by: \[ _{1}H^{2} + _{1}H^{2} \rightarrow _{2}He^{3} + _{0}n^{1} \] ### Step-by-Step Solution: 1. **Identify the masses involved in the reaction:** - Mass of deuterium (\( _{1}H^{2} \)) = 2.014741 amu ...
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The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. Fusion reaction takes place at about

The source of energy of stars is nuclear fusion. Fusion reaction occurs at very high temperature, about 10^(7) . Energy released in the process of fusion is due to mass defect. It is also called Q -value. Q = Delta mc^(2), Delta m = mass defect. Mass equivalent to the energy 931 MeV is

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In the nuclear raction ._1H^2 +._1H^2 rarr ._2He^3 +._0n^1 if the mass of the deuterium atom =2.014741 am u , mass of ._2He^3 atom =3.016977 am u , and mass of neutron =1.008987 am u , then the Q value of the reaction is nearly .

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