Question 14 Marks
Explain energy generation in stars through the process of nuclear fusion and explain proton. proton cycle.
Answer
View full question & answer→→ Sun continuously emits energy due to thermonuclear fusion. The interior of the Sun has a temperature of $1.5 \cdot 10^7 K$.
→ The thermonuclear fusion process in the Sun is known as proton-proton cycle.
→ This process is a multi-step process in which the hydrogen is burned into helium. Thus the fuel in the Sun is the hydrogen in its core.
→ The proton-proton cycle is represented by the following sets of reactions:
$
\begin{array}{l}
{ }_1^1 H+{ }_1^1 H \rightarrow{ }_1^2 H+e^{+}+v+0.42 MeV \ldots \text {(i) } \\
e^{+}+e^{-} \rightarrow Y+Y+1.02 MeV \ldots \text { (ii) } \\
{ }_1^2 H+{ }_1^1 H \rightarrow{ }_2^3 He+\gamma+5.49 MeV \ldots \text { (iii) } \\
{ }_2^3 He+{ }_2^3 He \rightarrow{ }_2^4 He+{ }_1^1 H+{ }_1^1 H+12.86 MeV ...(iv)
\end{array}
$
→ In this reaction, the first three reactions must occur twice and in the fourth reaction two light helium nuclei unite to form ordinary helium nucleus.
→ If we consider the combination
2 (i) +2 (ii) +2 (iii) + (iv), the net effect is
$
4_1 H^1+2 e^{-} \rightarrow{ }_2 He^4+2 v+6 y+26.7 MeV
$
OR
$
4_1 H^1+4 e^{-} \rightarrow\left[{ }_2 He^4+2 e^{-}\right]+2 v+6 y+26.7 MeV
$
→ Thus four hydrogen atoms combine to form an $_2 He ^4$ atom with a release of 26.7 MeV of energy.
→ The thermonuclear fusion process in the Sun is known as proton-proton cycle.
→ This process is a multi-step process in which the hydrogen is burned into helium. Thus the fuel in the Sun is the hydrogen in its core.
→ The proton-proton cycle is represented by the following sets of reactions:
$
\begin{array}{l}
{ }_1^1 H+{ }_1^1 H \rightarrow{ }_1^2 H+e^{+}+v+0.42 MeV \ldots \text {(i) } \\
e^{+}+e^{-} \rightarrow Y+Y+1.02 MeV \ldots \text { (ii) } \\
{ }_1^2 H+{ }_1^1 H \rightarrow{ }_2^3 He+\gamma+5.49 MeV \ldots \text { (iii) } \\
{ }_2^3 He+{ }_2^3 He \rightarrow{ }_2^4 He+{ }_1^1 H+{ }_1^1 H+12.86 MeV ...(iv)
\end{array}
$
→ In this reaction, the first three reactions must occur twice and in the fourth reaction two light helium nuclei unite to form ordinary helium nucleus.
→ If we consider the combination
2 (i) +2 (ii) +2 (iii) + (iv), the net effect is
$
4_1 H^1+2 e^{-} \rightarrow{ }_2 He^4+2 v+6 y+26.7 MeV
$
OR
$
4_1 H^1+4 e^{-} \rightarrow\left[{ }_2 He^4+2 e^{-}\right]+2 v+6 y+26.7 MeV
$
→ Thus four hydrogen atoms combine to form an $_2 He ^4$ atom with a release of 26.7 MeV of energy.


