02.06.2013 Views

Untitled - Kelly Walsh High School

Untitled - Kelly Walsh High School

Untitled - Kelly Walsh High School

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Nuclear Chemistry 299<br />

Don’t Forget!<br />

If you want to calculate the energy in joules, the mass must be in units of kilograms.<br />

A joule is a kgm 2 /s 2 .<br />

20-5 Fission and Fusion<br />

Nuclear fission is the breakdown of a nucleus into two or more smaller nuclei<br />

with the release of energy. The most useful fission process involves the decay of<br />

U-235 when hit by a neutron:<br />

1 235<br />

0n 92U l<br />

Notice that the reaction consumes one neutron, but the reaction releases three<br />

neutrons. Those three neutrons are then free to initiate additional fission reactions.<br />

This type of situation in which there is a multiplier effect is a chain reaction.<br />

We can use isotopes that undergo chain reaction in both the production of<br />

bombs and in nuclear power plants. U-235 is fissionable, but U-238 is not. There<br />

is a certain minimum quantity of fissionable matter needed to support a chain<br />

reaction, the critical mass.<br />

Nuclear reactors are useful in the production of electricity, but they are not<br />

without their problems. These problems include disposal of nuclear wastes,<br />

accidents, and sabotage. The eventual answer may lie in nuclear fusion.<br />

Fusion is the combining of lighter nuclei into a heavier one. Such reactions can<br />

release a great deal of energy. Isotopes of hydrogen fuse into helium and power<br />

the sun. For the past few decades, scientists have been investigating the fusion<br />

process as a way of providing the world with energy. One of the more promising<br />

fusion reactions is:<br />

2<br />

1H 3 1H 142 91<br />

56Ba 36Kr 3 1 0n l<br />

4<br />

2He 1 0n In this reaction, two isotopes of hydrogen fuse into helium and a neutron. Three<br />

major problems in this reaction have arisen—time, temperature, and containment.<br />

The nuclei must be held together long enough (~1 s) at high enough temperatures<br />

to provide the activation energy for the reaction (~40,000,000 K). At<br />

this temperature, every substance is a gas or plasma so containment is proving<br />

to be the biggest obstacle. Scientists are conducting major investigations into the

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!