Finding energy produced in nuclear fusion

In summary, the proposed fusion reactor has a possible reaction of H(2,1) + H(3,1) -> He(4,2) + n(1,0). Using the given atomic masses, 150kg of isotopes of hydrogen could produce 5.07 x 10^16 J of energy through this reaction. The equation E=mc^2 can be used to calculate this energy by finding the mass difference and multiplying it by c^2.
  • #1
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Homework Statement


In a proposed fusion reactor, one possible reaction is H(2,1) + H(3,1) -> He(4,2) + n(1,0)

How much energy might 150kg of the appropriate amount of isotopes of hydrogen produce?

Values given
Ar of H(2,1) = 2.014102
Ar of H(3,1) = 3.016050
Ar of He(4,2) = 4.002602
Ar of n(1,0) = 1.008665

Homework Equations


E=mc^2?


The Attempt at a Solution


The correct answer is 5.07 x 10^16 J but I can't seem to get it. Any help is appreciated thanks.
 
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  • #2
Start by figuring out the mass difference between the two sides of the reaction and multiply by c^2. Then figure out how many times you have to run that reaction to use up 150kg of H(2,1) + H(3,1).
 
  • #3


I would approach this problem by first understanding the concept of energy produced in nuclear fusion. In a fusion reaction, two atoms combine to form a heavier atom, releasing a large amount of energy in the process. This energy is a result of the conversion of mass into energy according to Einstein's famous equation, E=mc^2.

To solve this problem, we can use the equation E=mc^2, where E is the energy produced, m is the mass of the reactants, and c is the speed of light. We also need to convert the given atomic masses (Ar) into kilograms (kg) by multiplying them by the mass of one atomic unit (1.6605 x 10^-27 kg).

So, for the given reaction, the mass of the reactants (m) is equal to the sum of the masses of H(2,1) and H(3,1), which is (2.014102 x 1.6605 x 10^-27 kg) + (3.016050 x 1.6605 x 10^-27 kg) = 6.677 x 10^-27 kg.

Substituting this value into the equation E=mc^2, we get E= (6.677 x 10^-27 kg) x (299792458 m/s)^2 = 5.99 x 10^-11 J.

However, this is the energy produced by just one fusion reaction. The given problem asks for the energy produced by 150kg of the reactants. So, we need to multiply our answer by the number of fusion reactions that can occur in 150kg of the reactants.

To do this, we need to calculate the number of moles of the reactants in 150kg. This can be done by dividing the mass (in kg) by the molar mass (in kg/mol) of each reactant. The molar masses can be calculated by dividing the given atomic masses (Ar) by the Avogadro's number (6.022 x 10^23 mol^-1).

So, for H(2,1), the molar mass is (2.014102/6.022 x 10^23) = 3.34 x 10^-27 kg/mol. Similarly, for H(3,1), the molar mass is (3.016050/6.022 x 10^23
 

Related to Finding energy produced in nuclear fusion

1. How does nuclear fusion produce energy?

Nuclear fusion is a process in which two or more atomic nuclei fuse together to form a heavier nucleus. This fusion releases an enormous amount of energy, which is the same process that powers the sun and other stars.

2. What elements are involved in nuclear fusion?

Nuclear fusion typically involves light elements such as hydrogen and helium. These elements have the highest binding energies, making them the most efficient for energy production through fusion reactions.

3. How is the energy released in nuclear fusion harnessed?

The energy released in nuclear fusion is in the form of high-energy particles, such as neutrons and photons. These particles can be captured and converted into usable energy through various methods, such as heating water to produce steam to power turbines.

4. What are the potential benefits of using nuclear fusion as an energy source?

Nuclear fusion has the potential to provide a nearly limitless source of clean energy. It produces no greenhouse gases or long-lived radioactive waste, and the fuel sources are abundant and widely available.

5. What are the challenges and limitations of using nuclear fusion for energy production?

One of the main challenges of nuclear fusion is achieving and maintaining the extremely high temperatures and pressures required for the fusion reactions to occur. Additionally, the technology for harnessing and controlling fusion reactions is still in its early stages of development, making it a long-term goal for energy production.

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