Question

The proton-proton mechanism that accounts for energy production in the sun releases $$26.7\,MeV$$  energy for each event. In this process, protons fuse to form an alpha particle $$\left( {^4He} \right).$$  At what rate $$\frac{{dm}}{{dt}}$$  hydrogen being consumed in the core of the sun by the $$p-p$$  cycle? Power of sun is $$3.90 \times {10^{26}}W.$$

A. $$1.6 \times {10^{10}}kg/s$$
B. $$2.3 \times {10^9}kg/s$$
C. $$6.2 \times {10^{11}}kg/s$$  
D. $$5.5 \times {10^{10}}kg/s$$
Answer :   $$6.2 \times {10^{11}}kg/s$$
Solution :
The rate $$\frac{{dm}}{{dt}}$$  can be calculate as;
Power, $$P = \frac{{dE}}{{dt}} = \frac{{dE}}{{dm}} \times \frac{{dm}}{{dt}} = \frac{{\Delta E}}{{\Delta m}} \times \frac{{dm}}{{dt}}$$
$$\therefore \frac{{dm}}{{dt}} = \frac{{\Delta m}}{{\Delta E}}P\,.......\left( {\text{i}} \right)$$
We known that $$26.2\,MeV = 4.20 \times {10^{ - 12}}J$$     of thermal energy is produced when four protons are consumed. This is $$\Delta E = 4.20 \times {10^{ - 12}}J$$    for $$\Delta m = 4 \times \left( {1.67 \times {{10}^{ - 27}}kg} \right).$$
Substituting these values in equation (i), we have
$$\eqalign{ & \frac{{dm}}{{dt}} = \frac{{\Delta m}}{{\Delta E}}P = \frac{{4\left( {1.67 \times {{10}^{ - 27}}} \right)}}{{4.20 \times {{10}^{ - 12}}}} \times \left( {3.90 \times {{10}^{26}}} \right) \cr & = 6.2 \times {10^{11}}kg/s \cr} $$

Releted MCQ Question on
Modern Physics >> Atoms or Nuclear Fission and Fusion

Releted Question 1

The equation
$$4_1^1{H^ + } \to _2^4H{e^{2 + }} + 2{e^ - } + 26MeV$$       represents

A. $$\beta $$ -decay
B. $$\gamma $$ -decay
C. fusion
D. fission
Releted Question 2

Fast neutrons can easily be slowed down by

A. the use of lead shielding
B. passing them through water
C. elastic collisions with heavy nuclei
D. applying a strong electric field
Releted Question 3

In the nuclear fusion reaction
$$_1^2H + _1^3H \to _2^4He + n$$
given that the repulsive potential energy between the two nuclei is $$ \sim 7.7 \times {10^{ - 14}}J,$$    the temperature at which the gases must be heated to initiate the reaction is nearly
[Boltzmann’s Constant $$k = 1.38 \times {10^{ - 23}}J/K$$    ]

A. $${10^7}K$$
B. $${10^5}K$$
C. $${10^3}K$$
D. $${10^9}K$$
Releted Question 4

The binding energy per nucleon of deuteron $$\left( {_1^2H} \right)$$ and helium nucleus $$\left( {_2^4He} \right)$$  is $$1.1\,MeV$$  and $$7\,MeV$$  respectively. If two deuteron nuclei react to form a single helium nucleus, then the energy released is

A. $$23.6\,MeV$$
B. $$26.9\,MeV$$
C. $$13.9\,MeV$$
D. $$19.2\,MeV$$

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