Energy and Human Ambitions on a Finite Planet, 2021a
Energy and Human Ambitions on a Finite Planet, 2021a
Energy and Human Ambitions on a Finite Planet, 2021a
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15 Nuclear <str<strong>on</strong>g>Energy</str<strong>on</strong>g> 270<br />
56<br />
3. How many neutr<strong>on</strong>s does the isotope Fe c<strong>on</strong>tain?<br />
12 13<br />
4. Use the informati<strong>on</strong> in the boxes for C <str<strong>on</strong>g>and</str<strong>on</strong>g> C in Figure 15.4<br />
to determine the weighted composite mass of a natural blend of<br />
carb<strong>on</strong>—showing work—<str<strong>on</strong>g>and</str<strong>on</strong>g> compare this to the number in the<br />
left-most box for carb<strong>on</strong> in the same figure.<br />
5. In Figure 15.4, what are the <strong>on</strong>ly mass numbers, A, for which no<br />
stable nuclei exist?<br />
6. What are the <strong>on</strong>ly three l<strong>on</strong>g-lived radioactive isotopes in the<br />
porti<strong>on</strong> of the Chart of the Nuclides appearing in Figure 15.4, <str<strong>on</strong>g>and</str<strong>on</strong>g><br />
which <strong>on</strong>e lives the l<strong>on</strong>gest (how l<strong>on</strong>g)?<br />
7. Cosmic rays impinging <strong>on</strong> our atmosphere generate radioactive<br />
14<br />
C from<br />
14 N nuclei. 78 14<br />
These C atoms so<strong>on</strong> team up with oxygen 78: Nitrogen is the principal c<strong>on</strong>stituent in<br />
to form CO 2 , so that plants absorbing CO 2 from the air will have Earth’s atmosphere.<br />
about <strong>on</strong>e in a trilli<strong>on</strong> of their carb<strong>on</strong> atoms in this form. Animals<br />
eating these plants 79 will also have this fracti<strong>on</strong> of carb<strong>on</strong> in their 79: . . . <str<strong>on</strong>g>and</str<strong>on</strong>g>/or eating the animals that eat<br />
bodies, until they die <str<strong>on</strong>g>and</str<strong>on</strong>g> stop cycling carb<strong>on</strong> into their bodies. At these plants<br />
14<br />
this point, the fracti<strong>on</strong> of carb<strong>on</strong> atoms in the form of C in the The wording is l<strong>on</strong>g because without c<strong>on</strong>text,<br />
it’s just math. The real learning is in<br />
body declines, with a half life of 5,715 years. If you dig up a human<br />
skull, <str<strong>on</strong>g>and</str<strong>on</strong>g> discover that <strong>on</strong>ly <strong>on</strong>e-eighth of the usual <strong>on</strong>e-trilli<strong>on</strong>th<br />
the applicati<strong>on</strong> of math to the world.<br />
14<br />
of carb<strong>on</strong> atoms are C, how old do you deem the skull to be?<br />
8. If a friend creates a nucleus whose half-life is 4 hours <str<strong>on</strong>g>and</str<strong>on</strong>g> gives it<br />
to you at no<strong>on</strong>, what is the probability that it will not have decayed<br />
by no<strong>on</strong> the following day?<br />
235 238<br />
9. In close analog to the half-lives of U <str<strong>on</strong>g>and</str<strong>on</strong>g> U, let’s say two<br />
elements have half lives of 4.5 billi<strong>on</strong> years <str<strong>on</strong>g>and</str<strong>on</strong>g> 750 milli<strong>on</strong> years. 80<br />
If we start out having the same number of each (1:1 ratio), what<br />
will the ratio be after 4.5 billi<strong>on</strong> years? Express as x:1, where x is<br />
the larger of the two.<br />
10. C<strong>on</strong>trol rods in nuclear reactors tend to c<strong>on</strong>tain 10 B, which has<br />
a high neutr<strong>on</strong> absorpti<strong>on</strong> cross secti<strong>on</strong>. 81 What happens to this<br />
nucleus when it absorbs a neutr<strong>on</strong>, <str<strong>on</strong>g>and</str<strong>on</strong>g> is the result stable? If not,<br />
track the decay chain until it l<str<strong>on</strong>g>and</str<strong>on</strong>g>s <strong>on</strong> a stable nucleus.<br />
80: ...afactorof6different<br />
81: ...asindicated by the orange lower-half<br />
of the corresp<strong>on</strong>ding box in Figure 15.4<br />
14<br />
11. If some<strong>on</strong>e managed to create a B nucleus, what would its fate<br />
be? Track the decay chain <strong>on</strong> Figure 15.4—indicating the type of<br />
decay at each step—until it reaches stability, <str<strong>on</strong>g>and</str<strong>on</strong>g> indicate how<br />
l<strong>on</strong>g each step is likely to take.<br />
12. A particular nuclide is found to have lost 3 neutr<strong>on</strong>s <str<strong>on</strong>g>and</str<strong>on</strong>g> 1 prot<strong>on</strong><br />
after a decay chain. What combinati<strong>on</strong> of α <str<strong>on</strong>g>and</str<strong>on</strong>g> β decays could<br />
account for this result?<br />
13. How would you qualitatively describe the overall sense from<br />
Figure 15.8 in terms of where 82 <strong>on</strong> the chart <strong>on</strong>e is likely to see α<br />
82: Regi<strong>on</strong> descripti<strong>on</strong>s can include references<br />
to the mass range (e.g., low mass<br />
or high mass), above or below the stable<br />
elements (prot<strong>on</strong>-rich or neutr<strong>on</strong>-rich).<br />
© 2021 T. W. Murphy, Jr.; Creative Comm<strong>on</strong>s Attributi<strong>on</strong>-N<strong>on</strong>Commercial 4.0 Internati<strong>on</strong>al Lic.;<br />
Freely available at: https://escholarship.org/uc/energy_ambiti<strong>on</strong>s.