Monday, 24 November 2014

Nov. 24 – Fusion

Here is the schedule for the rest of the week:
  • Monday - last lesson, extra help rm 245
  • Tuesday - Review
  • Wednesday - Wellness
  • Thursday - Guest speaker, extra help rm 146
  • Friday - Review

  • Monday, Dec. 1 Test
First we wrapped up our discussion of fission by discussing the pros and cons of nuclear power.


Advantages and disadvantages of nuclear power
Pros: 
  • does not produce CO2, clean
  • produces large amount of energy for small amount of fuel (high energy density)
  • large reserves of nuclear fuel

Cons: 
  • warms up nearby lakes
  • spent fuel is still radioactive
  • dangerous to mine
  • waste material from mining


Then we discussed fusion

Fusion

Lighter elements fuse together to form heavier elements

The sun fuses 4 H —> He in what is called the proton-proton chain.


The best fusion reactor we have is the sun.



Hydrogen mass: 1.008 amu  = 1.6738 e -27 kg
Helium mass: 4.002 amu  = 6.6455 e -27 kg

The mass of 4 H does not add up to 1 He.  This was called the “mass defect”.
The missing mass is converted into energy. 



E = energy
m = mass
c = speed of light, 3.00 e 8 m/s

Ex) How much energy is produced from the “mass defect”?

The mass lost is given by:
m = 4m(Hydrogen) – m(He) 
m = 4(1.6738 e -27 kg) – (6.6455 e -27 kg) = 4.97 e -29 kg
This missing mass is converted into energy
E = mc²
E =  (4.97 e -29 kg)(3.00 e 8 m/s)² = 4.47 e -12 J

Remember that this is for the producing of ONE He nucleus.

Ex) How much energy is produced from fusing 4g of helium (about 1 mole)?

4 grams of He is about 1 mole, which is 6.02 e 23 He nuclei.  So the total energy is this number times the result from above.

E(total) = E x 1 mole
E(total) = (4.47 e -12 J)(6.02 e 23) = 2.69 e 12 J
This is a massive amount of energy!
A small amount of mass can be converted into a large amount of energy.

If we can do this in a fusion reactor we can produce useful energy with the only fuel being hydrogen!
Watch this video:


Homework

Complete these handouts



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